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	<updated>2026-04-29T17:19:18Z</updated>
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	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Proton_Calorimetry/Experimental_Runs/2018/FebScintSheets&amp;diff=1311</id>
		<title>Proton Calorimetry/Experimental Runs/2018/FebScintSheets</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Proton_Calorimetry/Experimental_Runs/2018/FebScintSheets&amp;diff=1311"/>
		<updated>2018-02-14T12:31:37Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Added header for raw data&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;The thickness of 50 scintillator sheets provided by Nuvia were measured using a digital caliper.&lt;br /&gt;
&lt;br /&gt;
== Measurements ==&lt;br /&gt;
&lt;br /&gt;
The measurements were added to an excel spreadsheet and converted to a comma delimited file for analysis using a python script. &lt;br /&gt;
*All of these files can be found at:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;/unix/pbt/wikiData/data/ScintillatorSheetThickness&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Before painting and any measurements were made, the sheets were divided into a group of 30x2mm sheets and a group of 20x3mm sheets. However, the 2mm group was found to be split evenly between an average thickness of 2mm and an average thickness of 2.6mm. These regimes are displayed in the histograms below.&lt;br /&gt;
&lt;br /&gt;
The data can be summarised in the following histograms:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;image400px&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&amp;gt;&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotal.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotal.png]&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotalPaint.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotalPaint.png]&lt;br /&gt;
&amp;lt;br /&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;image400px&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&amp;gt;&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotal.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotal.png]&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotalPaint.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotalPaint.png]&lt;br /&gt;
&amp;lt;br /&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Raw Data ==&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!Sheet number (before painting /after Painting if applicable)&lt;br /&gt;
!Pre-painting Raw measurements (mm)&lt;br /&gt;
!Post-painting Raw measurements (mm)&lt;br /&gt;
!Pre-painting average thickness (mm)&lt;br /&gt;
!Post-painting average thickness (mm)&lt;br /&gt;
!Notes&lt;br /&gt;
|-&lt;br /&gt;
| 1 || 2.60,2.63,2.64,2.60,2.63,2.62,2.62,2.57 || 2.59,2.63,2.65,2.63,2.68,2.66,2.69,2.72 || 2.61 || 2.66 ||&lt;br /&gt;
|-&lt;br /&gt;
| 2 || 2.56,2.58,2.59,2.56,2.58,2.53,2.56,2.58 || 2.65,2.64,2.62,2.63,2.65,2.59,2.65,2.67 || 2.57 || 2.64 ||&lt;br /&gt;
|-&lt;br /&gt;
| 3 || 2.60,2.57,2.59,2.55,2.57,2.55,2.56,2.57 || 2.61,2.62,2.62,2.57,2.60,2.58,2.60,2.61 || 2.57 || 2.60 ||&lt;br /&gt;
|-&lt;br /&gt;
| 4 || 2.68,2.66,2.61,2.64,2.59,2.63,2.59,2.56 || 2.59,2.59,2.57,2.63,2.60,2.64,2.62,2.64 || 2.62 || 2.61 || Described as &amp;quot;Lumpy&amp;quot; after painting&lt;br /&gt;
|-&lt;br /&gt;
| 5 || 2.60,2.58,2.57,2.58,2.57,2.56,2.56,2.54 || 2.62,2.65,2.57,2.62,2.62,2.63,2.61,2.61 || 2.57 || 2.62 ||&lt;br /&gt;
|-&lt;br /&gt;
| 6 || 2.55,2.55,2.54,2.54,2.54,2.49,2.52,2.52 || 2.62,2.62,2.58,2.58,2.60,2.52,2.55,2.57 || 2.53 || 2.58 || Excess paint seen along one edge&lt;br /&gt;
|-&lt;br /&gt;
| 7 || 1.91,1.90,1.89,1.91,1.89,1.90,1.89,1.89 || 1.91,1.94,1.94,1.92,1.93,1.93,1.93,1.95 || 1.90 || 1.93 ||&lt;br /&gt;
|-&lt;br /&gt;
| 8 || 2.67,2.68,2.73,2.70,2.77,2.70,2.75,2.79 || 2.67,2.71,2.77,2.71,2.80,2.73,2.77,2.81 || 2.72 || 2.75 ||&lt;br /&gt;
|-&lt;br /&gt;
| 9 || 2.73,2.75,2.79,2.69,2.74,2.66,2.67,2.71 || 2.77,2.78,2.81,2.71,2.78,2.68,2.69,2.73 || 2.72 || 2.74 ||&lt;br /&gt;
|-&lt;br /&gt;
| 10 || 1.91,1.92,1.91,1.93,1.93,1.95,1.95,1.94 || 1.95,1.97,2.00,1.96,2.00,1.95,1.96,1.98 || 1.93 || 1.97 ||&lt;br /&gt;
|-&lt;br /&gt;
| 11 || 2.60,2.65,2.68,2.58,2.62,2.54,2.56,2.59 || 2.57,2.59,2.63,2.60,2.66,2.62,2.67,2.71 || 2.60 || 2.63 || Possible scratch along one face&lt;br /&gt;
|-&lt;br /&gt;
| 12 || 2.57,2.55,2.52,2.54,2.51,2.51,2.51,2.47 || 2.56,2.59,2.62,2.52,2.57,2.49,2.53,2.53 || 2.52 || 2.55 ||&lt;br /&gt;
|-&lt;br /&gt;
| 13 || 1.92,1.91,1.91,1.94,1.92,1.96,1.94,1.95 || 2.01,1.98,1.96,1.99,1.96,2.00,1.97,1.95 || 1.93 || 1.98 ||&lt;br /&gt;
|-&lt;br /&gt;
| 14 || 1.96,1.97,1.98,1.99,2.00,1.99,2.00,2.03 || 2.05,2.06,2.07,2.04,2.05,2.01,2.00,1.99 || 1.99 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 15 || 1.88,1.88,1.92,1.89,1.90,1.90,1.91,1.91 || 1.92,1.95,1.95,1.92,1.93,1.93,1.93,1.95 || 1.90 || 1.94 ||&lt;br /&gt;
|-&lt;br /&gt;
| 16 || 2.57,2.54,2.52,2.57,2.52,2.56,2.52,2.50 || 2.62,2.59,2.54,2.60,2.55,2.60,2.55,2.53 || 2.54 || 2.57 ||&lt;br /&gt;
|-&lt;br /&gt;
| 17 || 1.98,1.97,1.98,1.98,1.97,1.98,1.96,1.96 || 2.01,2.02,2.04,2.04,2.03,2.04,2.03,2.04 || 1.97 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 18 || 1.95,1.93,1.92,1.94,1.91,1.94,1.93,1.92 || 1.98,1.98,1.99,2.00,2.00,2.01,2.01,2.02 || 1.93 || 2.00 ||&lt;br /&gt;
|-&lt;br /&gt;
| 19 || 1.97,1.96,1.97,1.98,1.98,1.99,2.00,2.01 || 2.06,2.04,2.03,2.06,2.03,2.07,2.03,2.05 || 1.98 || 2.05 || Two lumps near to edge measured 2.04mm of thickness 2.48 mm and 2.17 mm&lt;br /&gt;
|-&lt;br /&gt;
| 20 || 2.50,2.47,2.45,2.52,2.49,2.57,2.56,2.54 || 2.55,2.57,2.63,2.50,2.61,2.50,2.58,2.58 || 2.51 || 2.56 ||&lt;br /&gt;
|-&lt;br /&gt;
| 21 || 1.94,1.94,1.97,1.93,1.97,1.92,1.94,1.97 || 2.06,2.05,2.05,2.01,2.02,1.99,2.00,2.00 || 1.95 || 2.02 || Lump near to edge measured 2.01mm, 2.69mm (Next to drilled hole)&lt;br /&gt;
|-&lt;br /&gt;
| 22 || 1.92,1.90,1.90,1.92,1.90,1.92,1.91,1.89 || 1.96,1.96,1.97,1.94,1.94,1.93,1.94,1.93 || 1.91 || 1.95 ||&lt;br /&gt;
|-&lt;br /&gt;
| 23 || 2.60,2.61,2.59,2.59,2.62,2.56,2.59,2.63 || 2.66,2.64,2.60,2.63,2.65,2.59,2.61,2.62 || 2.60 || 2.63 || Possible fingerprints left from handling sheet without gloves&lt;br /&gt;
|-&lt;br /&gt;
| 24 || 2.58,2.61,2.60,2.61,2.59,2.60,2.60,2.57 || 2.66,2.64,2.61,2.63,2.65,2.61,2.65,2.65 || 2.59 || 2.64 ||&lt;br /&gt;
|-&lt;br /&gt;
| 25 || 2.50,2.50,2.54,2.48,2.55,2.49,2.53,2.55 || 2.59,2.60,2.58,2.57,2.56,2.55,2.53,2.59 || 2.52 || 2.57 ||&lt;br /&gt;
|-&lt;br /&gt;
| 26 || 1.98,2.00,2.01,1.96,1.99,1.94,1.95,1.97 || 2.03,2.00,1.99,2.03,1.99,2.05,2.02,2.01 || 1.97 || 2.01 ||&lt;br /&gt;
|-&lt;br /&gt;
| 27 || 2.01,2.00,2.00,1.98,1.99,1.97,1.96,1.98 || 2.02,2.01,2.00,2.03,2.04,2.04,2.04,2.05 || 1.99 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 28 || 1.93,1.94,1.96,1.93,1.96,1.93,1.94,1.97 || 2.02,2.00,2.03,1.98,2.01,1.99,1.98,1.99 || 1.94 || 2.00 ||&lt;br /&gt;
|-&lt;br /&gt;
| 29 || 1.91,1.90,1.91,1.98,1.89,1.89,1.88,1.89 || 1.96,1.95,1.95,1.96,1.95,1.97,1.94,1.95 || 1.91 || 1.95 ||&lt;br /&gt;
|-&lt;br /&gt;
| 30 || 2.13,2.09,2.08,2.10,2.05,2.09,2.07,2.05 || 2.12,2.09,2.09,2.14,2.12,2.18,2.15,2.15 || 2.08 || 2.13 ||&lt;br /&gt;
|-&lt;br /&gt;
| 1 (31) || 2.84,2.81,2.78,2.81,2.78,2.79,2.78,2.77 || 2.81,2.81,2.81,2.83,2.80,2.90,2.86,2.84 || 2.79 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 2 (32) || 2.86,2.79,2.79,2.81,2.78,2.82,2.79,2.79 || 2.88,2.82,2.83,2.84,2.80,2.84,2.81,2.81 || 2.80 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 3 (33) || 2.77,2.76,2.76,2.77,2.75,2.74,2.74,2.75 || 2.83,2.80,2.81,2.81,2.80,2.79,2.78,2.79 || 2.75 || 2.80 ||&lt;br /&gt;
|-&lt;br /&gt;
| 4 (34) || 2.79,2.78,2.79,2.79,2.77,2.78,2.77,2.78 || 2.84,2.88,2.85,2.82,2.83,2.83,2.81,2.83 || 2.78 || 2.84 ||&lt;br /&gt;
|-&lt;br /&gt;
| 5 (35) || 2.79,2.81,2.90,2.79,2.82,2.78,2.77,2.78 || 2.98,2.88,2.85,2.88,2.83,2.85,2.84,2.83 || 2.80 || 2.87 ||&lt;br /&gt;
|-&lt;br /&gt;
| 6 (36) || 2.81,2.83,2.86,2.82,2.84,2.87,2.84,2.85 || 2.88,2.89,2.92,2.87,2.89,2.93,2.90,2.91 || 2.84 || 2.90 || Difference in the paint down one edge, by eye&lt;br /&gt;
|-&lt;br /&gt;
| 7 (37) || 2.80,2.78,2.76,2.78,2.74,2.78,2.75,2.75 || 2.85,2.83,2.84,2.84,2.82,2.80,2.81,2.80 || 2.77 || 2.82 ||&lt;br /&gt;
|-&lt;br /&gt;
| 8 (38) || 2.79,2.74,2.78,2.76,2.77,2.77,2.75,2.76 || 2.81,2.81,2.82,2.80,2.80,2.82,2.81,2.81 || 2.77 || 2.81 ||&lt;br /&gt;
|-&lt;br /&gt;
| 9 (39) || 2.80,2.82,2.86,2.80,2.81,2.80,2.79,2.78 || 2.86,2.89,2.93,2.87,2.89,2.87,2.85,2.85 || 2.81 || 2.88 || Lump near to edge measured 2.87mm of height 2.89 mm&lt;br /&gt;
|-&lt;br /&gt;
| 10 (40) || 2.78,2.79,2.81,2.79,2.81,2.80,2.79,2.80 || 2.86,2.86,2.86,2.85,2.84,2.86,2.85,2.86 || 2.80 || 2.86 ||&lt;br /&gt;
|-&lt;br /&gt;
| 11 (41) || 2.76,2.74,2.74,2.73,2.74,2.75,2.74,2.75 || 2.78,2.77,2.78,2.76,2.77,2.79,2.76,2.77 || 2.74 || 2.77 ||&lt;br /&gt;
|-&lt;br /&gt;
| 12 (42) || 2.78,2.77,2.79,2.79,2.78,2.82,2.78,2.77 || 2.80,2.82,2.88,2.82,2.84,2.83,2.81,2.80 || 2.78 || 2.82 ||&lt;br /&gt;
|-&lt;br /&gt;
| 13 (43) || 2.78,2.75,2.76,2.75,2.76,2.74,2.75,2.77 || 2.85,2.83,2.83,2.82,2.82,2.83,2.81,2.81 || 2.76 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 14 (44) || 2.72,2.71,2.70,2.71,2.70,2.71,2.72,2.73 || 2.78,2.77,2.76,2.77,2.76,2.77,2.77,2.77 || 2.71 || 2.77 ||&lt;br /&gt;
|-&lt;br /&gt;
| 15 (45) || 2.79,2.76,2.80,2.78,2.80,2.77,2.78,2.83 || 2.90,2.88,2.83,2.82,2.82,2.82,2.82,2.85 || 2.79 || 2.84 ||&lt;br /&gt;
|-&lt;br /&gt;
| 16 (46) || 2.77,2.77,2.77,2.76,2.77,2.79,2.79,2.80 || 2.83,2.84,2.84,2.80,2.83,2.82,2.81,2.83 || 2.78 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 17 (47) || 2.78,2.77,2.78,2.75,2.78,2.77,2.77,2.79 || 2.84,2.82,2.82,2.83,2.80,2.84,2.83,2.83 || 2.77 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 18 (48) || 3.03,2.98,2.94,3.07,2.98,3.17,3.07,3.03 || 3.00,3.04,3.11,3.02,3.15,3.05,3.14,3.22 || 3.03 || 3.09 ||&lt;br /&gt;
|-&lt;br /&gt;
| 19 (49) || 2.81,2.81,2.80,2.80,2.81,2.80,2.80,2.81 || 2.85,2.85,2.84,2.86,2.85,2.86,2.86,2.85 || 2.80 || 2.85 ||&lt;br /&gt;
|-&lt;br /&gt;
| 20 (50) || 2.75,2.74,2.77,2.73,2.74,2.73,2.71,2.72 || 2.77,2.75,2.78,2.77,2.78,2.80,2.77,2.81 || 2.74 || 2.78 ||&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Proton_Calorimetry/Experimental_Runs/2018/FebScintSheets&amp;diff=1310</id>
		<title>Proton Calorimetry/Experimental Runs/2018/FebScintSheets</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Proton_Calorimetry/Experimental_Runs/2018/FebScintSheets&amp;diff=1310"/>
		<updated>2018-02-14T12:31:02Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Pushed first copy&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;The thickness of 50 scintillator sheets provided by Nuvia were measured using a digital caliper.&lt;br /&gt;
&lt;br /&gt;
== Measurements ==&lt;br /&gt;
&lt;br /&gt;
The measurements were added to an excel spreadsheet and converted to a comma delimited file for analysis using a python script. &lt;br /&gt;
*All of these files can be found at:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;/unix/pbt/wikiData/data/ScintillatorSheetThickness&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Before painting and any measurements were made, the sheets were divided into a group of 30x2mm sheets and a group of 20x3mm sheets. However, the 2mm group was found to be split evenly between an average thickness of 2mm and an average thickness of 2.6mm. These regimes are displayed in the histograms below.&lt;br /&gt;
&lt;br /&gt;
The data can be summarised in the following histograms:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;image400px&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&amp;gt;&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotal.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotal.png]&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotalPaint.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/AveThickTotalPaint.png]&lt;br /&gt;
&amp;lt;br /&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;image400px&amp;quot; style=&amp;quot;text-align: center;&amp;quot;&amp;gt;&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotal.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotal.png]&lt;br /&gt;
[http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotalPaint.png http://www.hep.ucl.ac.uk/pbt/wikiData/images/ScintilatorSheetThickness/RangeTotalPaint.png]&lt;br /&gt;
&amp;lt;br /&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{|class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!Sheet number (before painting /after Painting if applicable)&lt;br /&gt;
!Pre-painting Raw measurements (mm)&lt;br /&gt;
!Post-painting Raw measurements (mm)&lt;br /&gt;
!Pre-painting average thickness (mm)&lt;br /&gt;
!Post-painting average thickness (mm)&lt;br /&gt;
!Notes&lt;br /&gt;
|-&lt;br /&gt;
| 1 || 2.60,2.63,2.64,2.60,2.63,2.62,2.62,2.57 || 2.59,2.63,2.65,2.63,2.68,2.66,2.69,2.72 || 2.61 || 2.66 ||&lt;br /&gt;
|-&lt;br /&gt;
| 2 || 2.56,2.58,2.59,2.56,2.58,2.53,2.56,2.58 || 2.65,2.64,2.62,2.63,2.65,2.59,2.65,2.67 || 2.57 || 2.64 ||&lt;br /&gt;
|-&lt;br /&gt;
| 3 || 2.60,2.57,2.59,2.55,2.57,2.55,2.56,2.57 || 2.61,2.62,2.62,2.57,2.60,2.58,2.60,2.61 || 2.57 || 2.60 ||&lt;br /&gt;
|-&lt;br /&gt;
| 4 || 2.68,2.66,2.61,2.64,2.59,2.63,2.59,2.56 || 2.59,2.59,2.57,2.63,2.60,2.64,2.62,2.64 || 2.62 || 2.61 || Described as &amp;quot;Lumpy&amp;quot; after painting&lt;br /&gt;
|-&lt;br /&gt;
| 5 || 2.60,2.58,2.57,2.58,2.57,2.56,2.56,2.54 || 2.62,2.65,2.57,2.62,2.62,2.63,2.61,2.61 || 2.57 || 2.62 ||&lt;br /&gt;
|-&lt;br /&gt;
| 6 || 2.55,2.55,2.54,2.54,2.54,2.49,2.52,2.52 || 2.62,2.62,2.58,2.58,2.60,2.52,2.55,2.57 || 2.53 || 2.58 || Excess paint seen along one edge&lt;br /&gt;
|-&lt;br /&gt;
| 7 || 1.91,1.90,1.89,1.91,1.89,1.90,1.89,1.89 || 1.91,1.94,1.94,1.92,1.93,1.93,1.93,1.95 || 1.90 || 1.93 ||&lt;br /&gt;
|-&lt;br /&gt;
| 8 || 2.67,2.68,2.73,2.70,2.77,2.70,2.75,2.79 || 2.67,2.71,2.77,2.71,2.80,2.73,2.77,2.81 || 2.72 || 2.75 ||&lt;br /&gt;
|-&lt;br /&gt;
| 9 || 2.73,2.75,2.79,2.69,2.74,2.66,2.67,2.71 || 2.77,2.78,2.81,2.71,2.78,2.68,2.69,2.73 || 2.72 || 2.74 ||&lt;br /&gt;
|-&lt;br /&gt;
| 10 || 1.91,1.92,1.91,1.93,1.93,1.95,1.95,1.94 || 1.95,1.97,2.00,1.96,2.00,1.95,1.96,1.98 || 1.93 || 1.97 ||&lt;br /&gt;
|-&lt;br /&gt;
| 11 || 2.60,2.65,2.68,2.58,2.62,2.54,2.56,2.59 || 2.57,2.59,2.63,2.60,2.66,2.62,2.67,2.71 || 2.60 || 2.63 || Possible scratch along one face&lt;br /&gt;
|-&lt;br /&gt;
| 12 || 2.57,2.55,2.52,2.54,2.51,2.51,2.51,2.47 || 2.56,2.59,2.62,2.52,2.57,2.49,2.53,2.53 || 2.52 || 2.55 ||&lt;br /&gt;
|-&lt;br /&gt;
| 13 || 1.92,1.91,1.91,1.94,1.92,1.96,1.94,1.95 || 2.01,1.98,1.96,1.99,1.96,2.00,1.97,1.95 || 1.93 || 1.98 ||&lt;br /&gt;
|-&lt;br /&gt;
| 14 || 1.96,1.97,1.98,1.99,2.00,1.99,2.00,2.03 || 2.05,2.06,2.07,2.04,2.05,2.01,2.00,1.99 || 1.99 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 15 || 1.88,1.88,1.92,1.89,1.90,1.90,1.91,1.91 || 1.92,1.95,1.95,1.92,1.93,1.93,1.93,1.95 || 1.90 || 1.94 ||&lt;br /&gt;
|-&lt;br /&gt;
| 16 || 2.57,2.54,2.52,2.57,2.52,2.56,2.52,2.50 || 2.62,2.59,2.54,2.60,2.55,2.60,2.55,2.53 || 2.54 || 2.57 ||&lt;br /&gt;
|-&lt;br /&gt;
| 17 || 1.98,1.97,1.98,1.98,1.97,1.98,1.96,1.96 || 2.01,2.02,2.04,2.04,2.03,2.04,2.03,2.04 || 1.97 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 18 || 1.95,1.93,1.92,1.94,1.91,1.94,1.93,1.92 || 1.98,1.98,1.99,2.00,2.00,2.01,2.01,2.02 || 1.93 || 2.00 ||&lt;br /&gt;
|-&lt;br /&gt;
| 19 || 1.97,1.96,1.97,1.98,1.98,1.99,2.00,2.01 || 2.06,2.04,2.03,2.06,2.03,2.07,2.03,2.05 || 1.98 || 2.05 || Two lumps near to edge measured 2.04mm of thickness 2.48 mm and 2.17 mm&lt;br /&gt;
|-&lt;br /&gt;
| 20 || 2.50,2.47,2.45,2.52,2.49,2.57,2.56,2.54 || 2.55,2.57,2.63,2.50,2.61,2.50,2.58,2.58 || 2.51 || 2.56 ||&lt;br /&gt;
|-&lt;br /&gt;
| 21 || 1.94,1.94,1.97,1.93,1.97,1.92,1.94,1.97 || 2.06,2.05,2.05,2.01,2.02,1.99,2.00,2.00 || 1.95 || 2.02 || Lump near to edge measured 2.01mm, 2.69mm (Next to drilled hole)&lt;br /&gt;
|-&lt;br /&gt;
| 22 || 1.92,1.90,1.90,1.92,1.90,1.92,1.91,1.89 || 1.96,1.96,1.97,1.94,1.94,1.93,1.94,1.93 || 1.91 || 1.95 ||&lt;br /&gt;
|-&lt;br /&gt;
| 23 || 2.60,2.61,2.59,2.59,2.62,2.56,2.59,2.63 || 2.66,2.64,2.60,2.63,2.65,2.59,2.61,2.62 || 2.60 || 2.63 || Possible fingerprints left from handling sheet without gloves&lt;br /&gt;
|-&lt;br /&gt;
| 24 || 2.58,2.61,2.60,2.61,2.59,2.60,2.60,2.57 || 2.66,2.64,2.61,2.63,2.65,2.61,2.65,2.65 || 2.59 || 2.64 ||&lt;br /&gt;
|-&lt;br /&gt;
| 25 || 2.50,2.50,2.54,2.48,2.55,2.49,2.53,2.55 || 2.59,2.60,2.58,2.57,2.56,2.55,2.53,2.59 || 2.52 || 2.57 ||&lt;br /&gt;
|-&lt;br /&gt;
| 26 || 1.98,2.00,2.01,1.96,1.99,1.94,1.95,1.97 || 2.03,2.00,1.99,2.03,1.99,2.05,2.02,2.01 || 1.97 || 2.01 ||&lt;br /&gt;
|-&lt;br /&gt;
| 27 || 2.01,2.00,2.00,1.98,1.99,1.97,1.96,1.98 || 2.02,2.01,2.00,2.03,2.04,2.04,2.04,2.05 || 1.99 || 2.03 ||&lt;br /&gt;
|-&lt;br /&gt;
| 28 || 1.93,1.94,1.96,1.93,1.96,1.93,1.94,1.97 || 2.02,2.00,2.03,1.98,2.01,1.99,1.98,1.99 || 1.94 || 2.00 ||&lt;br /&gt;
|-&lt;br /&gt;
| 29 || 1.91,1.90,1.91,1.98,1.89,1.89,1.88,1.89 || 1.96,1.95,1.95,1.96,1.95,1.97,1.94,1.95 || 1.91 || 1.95 ||&lt;br /&gt;
|-&lt;br /&gt;
| 30 || 2.13,2.09,2.08,2.10,2.05,2.09,2.07,2.05 || 2.12,2.09,2.09,2.14,2.12,2.18,2.15,2.15 || 2.08 || 2.13 ||&lt;br /&gt;
|-&lt;br /&gt;
| 1 (31) || 2.84,2.81,2.78,2.81,2.78,2.79,2.78,2.77 || 2.81,2.81,2.81,2.83,2.80,2.90,2.86,2.84 || 2.79 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 2 (32) || 2.86,2.79,2.79,2.81,2.78,2.82,2.79,2.79 || 2.88,2.82,2.83,2.84,2.80,2.84,2.81,2.81 || 2.80 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 3 (33) || 2.77,2.76,2.76,2.77,2.75,2.74,2.74,2.75 || 2.83,2.80,2.81,2.81,2.80,2.79,2.78,2.79 || 2.75 || 2.80 ||&lt;br /&gt;
|-&lt;br /&gt;
| 4 (34) || 2.79,2.78,2.79,2.79,2.77,2.78,2.77,2.78 || 2.84,2.88,2.85,2.82,2.83,2.83,2.81,2.83 || 2.78 || 2.84 ||&lt;br /&gt;
|-&lt;br /&gt;
| 5 (35) || 2.79,2.81,2.90,2.79,2.82,2.78,2.77,2.78 || 2.98,2.88,2.85,2.88,2.83,2.85,2.84,2.83 || 2.80 || 2.87 ||&lt;br /&gt;
|-&lt;br /&gt;
| 6 (36) || 2.81,2.83,2.86,2.82,2.84,2.87,2.84,2.85 || 2.88,2.89,2.92,2.87,2.89,2.93,2.90,2.91 || 2.84 || 2.90 || Difference in the paint down one edge, by eye&lt;br /&gt;
|-&lt;br /&gt;
| 7 (37) || 2.80,2.78,2.76,2.78,2.74,2.78,2.75,2.75 || 2.85,2.83,2.84,2.84,2.82,2.80,2.81,2.80 || 2.77 || 2.82 ||&lt;br /&gt;
|-&lt;br /&gt;
| 8 (38) || 2.79,2.74,2.78,2.76,2.77,2.77,2.75,2.76 || 2.81,2.81,2.82,2.80,2.80,2.82,2.81,2.81 || 2.77 || 2.81 ||&lt;br /&gt;
|-&lt;br /&gt;
| 9 (39) || 2.80,2.82,2.86,2.80,2.81,2.80,2.79,2.78 || 2.86,2.89,2.93,2.87,2.89,2.87,2.85,2.85 || 2.81 || 2.88 || Lump near to edge measured 2.87mm of height 2.89 mm&lt;br /&gt;
|-&lt;br /&gt;
| 10 (40) || 2.78,2.79,2.81,2.79,2.81,2.80,2.79,2.80 || 2.86,2.86,2.86,2.85,2.84,2.86,2.85,2.86 || 2.80 || 2.86 ||&lt;br /&gt;
|-&lt;br /&gt;
| 11 (41) || 2.76,2.74,2.74,2.73,2.74,2.75,2.74,2.75 || 2.78,2.77,2.78,2.76,2.77,2.79,2.76,2.77 || 2.74 || 2.77 ||&lt;br /&gt;
|-&lt;br /&gt;
| 12 (42) || 2.78,2.77,2.79,2.79,2.78,2.82,2.78,2.77 || 2.80,2.82,2.88,2.82,2.84,2.83,2.81,2.80 || 2.78 || 2.82 ||&lt;br /&gt;
|-&lt;br /&gt;
| 13 (43) || 2.78,2.75,2.76,2.75,2.76,2.74,2.75,2.77 || 2.85,2.83,2.83,2.82,2.82,2.83,2.81,2.81 || 2.76 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 14 (44) || 2.72,2.71,2.70,2.71,2.70,2.71,2.72,2.73 || 2.78,2.77,2.76,2.77,2.76,2.77,2.77,2.77 || 2.71 || 2.77 ||&lt;br /&gt;
|-&lt;br /&gt;
| 15 (45) || 2.79,2.76,2.80,2.78,2.80,2.77,2.78,2.83 || 2.90,2.88,2.83,2.82,2.82,2.82,2.82,2.85 || 2.79 || 2.84 ||&lt;br /&gt;
|-&lt;br /&gt;
| 16 (46) || 2.77,2.77,2.77,2.76,2.77,2.79,2.79,2.80 || 2.83,2.84,2.84,2.80,2.83,2.82,2.81,2.83 || 2.78 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 17 (47) || 2.78,2.77,2.78,2.75,2.78,2.77,2.77,2.79 || 2.84,2.82,2.82,2.83,2.80,2.84,2.83,2.83 || 2.77 || 2.83 ||&lt;br /&gt;
|-&lt;br /&gt;
| 18 (48) || 3.03,2.98,2.94,3.07,2.98,3.17,3.07,3.03 || 3.00,3.04,3.11,3.02,3.15,3.05,3.14,3.22 || 3.03 || 3.09 ||&lt;br /&gt;
|-&lt;br /&gt;
| 19 (49) || 2.81,2.81,2.80,2.80,2.81,2.80,2.80,2.81 || 2.85,2.85,2.84,2.86,2.85,2.86,2.86,2.85 || 2.80 || 2.85 ||&lt;br /&gt;
|-&lt;br /&gt;
| 20 (50) || 2.75,2.74,2.77,2.73,2.74,2.73,2.71,2.72 || 2.77,2.75,2.78,2.77,2.78,2.80,2.77,2.81 || 2.74 || 2.78 ||&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1114</id>
		<title>Software/Geant4/Eclipse</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1114"/>
		<updated>2017-09-27T12:57:43Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: formatting&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Editing Geant4 input files in Eclipse.&lt;br /&gt;
&lt;br /&gt;
== Why use Eclipse ==&lt;br /&gt;
&lt;br /&gt;
Eclipse allows for editing files remotely using an environment that gives rudimentary debugging tools and a easy to use remote file explorer. Furthermore, this method allows support of remote file editing on an operating system that does not have native access to the bash terminal (i.e. windows).&lt;br /&gt;
&lt;br /&gt;
It should be noted that this tutorial is written with the C/C++ Oxygen version of the Eclipse IDE in mind, as the Remote System Explorer plug-ins are included in this package, but the tutorial should work for other packages. All of the current eclipse packages can be found [https://www.eclipse.org/downloads/eclipse-packages/ here].&lt;br /&gt;
&lt;br /&gt;
== Connecting via SSH ==&lt;br /&gt;
&lt;br /&gt;
Once you have downloaded, installed, and launched Eclipse, you will want to SSH into the plus1.hep.ucl.ac.uk server. This is done by the following steps:&lt;br /&gt;
&lt;br /&gt;
1) Open the Remote System Explorer (RSE). This is done by going to Window &amp;gt; Perspective &amp;gt; Open Perspective &amp;gt; Other, and then choosing Remote System Explorer.&lt;br /&gt;
&lt;br /&gt;
2) In the Panel containing the Remote Systems tab that appeared when the RSE was opened, define a new connection. This can be done by clicking the icon at the top of the panel, or right clicking on the panel and selecting New &amp;gt; Connection&lt;br /&gt;
&lt;br /&gt;
3) In the New Connection window that opened, select the &#039;SSH Only&#039; System type.&lt;br /&gt;
&lt;br /&gt;
4) In the Host name text box, enter the server address that you want to SSH into. For use with the pbt server, enter&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
PLUS1.HEP.UCL.AC.UK&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
and give the connection a name, for example &amp;lt;code&amp;gt;PLUS1&amp;lt;/code&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
5) In the Remote Systems panel opened earlier, you should see a new connection with then connection name you chose earlier. Opening the tree by going Stfp Files &amp;gt; Root, you will be prompted to enter a User ID and password. In their respective text boxes, enter your pbt User ID and Password. You are now connected remotely to the PLUS1 server.*&lt;br /&gt;
&lt;br /&gt;
* It should be noted that you cannot subsequently SSH from the PLUS1 server into another pc in the pbt cluster using this method. Alternative methods to do so are discussed in the [http://www.hep.ucl.ac.uk/pbt/wiki/Software/Geant4/Eclipse#Running_a_SSH_Shell_in_Eclipse Running a SSH Shell in Eclipse] section.&lt;br /&gt;
&lt;br /&gt;
== Using Eclipse ==&lt;br /&gt;
&lt;br /&gt;
=== Remote System Details ===&lt;br /&gt;
&lt;br /&gt;
You can open a panel that displays details about the remote systems you have connected to. This is done by going to Window &amp;gt; Show View &amp;gt; Remote System Details. You can use this window in a manner similar to the Remote Systems file explorer panel, except that the Remote System Details panel gives more detail about the files contained (for example the time stamp of the last time the directory/file was edited etc). You can use the buttons at the top right of this panel to navigate through the servers directories.&lt;br /&gt;
&lt;br /&gt;
=== Easier File management ===&lt;br /&gt;
&lt;br /&gt;
Instead of using a bash terminal, you can use the tree within the Remote Systems panel to move, copy, and open files. This is done by simple highlighting the file, right clicking, and selecting the required operation (copy/cut/delete etc.). It should be noted that this method of file management is significantly slower than performing the same action via a terminal.&lt;br /&gt;
&lt;br /&gt;
=== Running a SSH Shell in Eclipse ===&lt;br /&gt;
&lt;br /&gt;
You can also open a bash terminal in Eclipse. In the Remote Systems panel, under the SSH connection you have created, you will see a subdirectory called &#039;Ssh Shells&#039;. Right click this and select Launch Shell. This shell allows connection to internal pc&#039;s in the pbt cluster, as well as the ability to perform all other standard bash commands on the pbt server.&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1113</id>
		<title>Software/Geant4/Eclipse</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1113"/>
		<updated>2017-09-27T12:57:25Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: undid last edit, applied change to correct link&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Editing Geant4 input files in Eclipse.&lt;br /&gt;
&lt;br /&gt;
== Why use Eclipse ==&lt;br /&gt;
&lt;br /&gt;
Eclipse allows for editing files remotely using an environment that gives rudimentary debugging tools and a easy to use remote file explorer. Furthermore, this method allows support of remote file editing on an operating system that does not have native access to the bash terminal (i.e. windows).&lt;br /&gt;
&lt;br /&gt;
It should be noted that this tutorial is written with the C/C++ Oxygen version of the Eclipse IDE in mind, as the Remote System Explorer plug-ins are included in this package, but the tutorial should work for other packages. All of the current eclipse packages can be found [https://www.eclipse.org/downloads/eclipse-packages/ here].&lt;br /&gt;
&lt;br /&gt;
== Connecting via SSH ==&lt;br /&gt;
&lt;br /&gt;
Once you have downloaded, installed, and launched Eclipse, you will want to SSH into the plus1.hep.ucl.ac.uk server. This is done by the following steps:&lt;br /&gt;
&lt;br /&gt;
1) Open the Remote System Explorer (RSE). This is done by going to Window &amp;gt; Perspective &amp;gt; Open Perspective &amp;gt; Other, and then choosing Remote System Explorer.&lt;br /&gt;
&lt;br /&gt;
2) In the Panel containing the Remote Systems tab that appeared when the RSE was opened, define a new connection. This can be done by clicking the icon at the top of the panel, or right clicking on the panel and selecting New &amp;gt; Connection&lt;br /&gt;
&lt;br /&gt;
3) In the New Connection window that opened, select the &#039;SSH Only&#039; System type.&lt;br /&gt;
&lt;br /&gt;
4) In the Host name text box, enter the server address that you want to SSH into. For use with the pbt server, enter&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
PLUS1.HEP.UCL.AC.UK&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
and give the connection a name, for example &amp;lt;code&amp;gt;PLUS1&amp;lt;/code&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
5) In the Remote Systems panel opened earlier, you should see a new connection with then connection name you chose earlier. Opening the tree by going Stfp Files &amp;gt; Root, you will be prompted to enter a User ID and password. In their respective text boxes, enter your pbt User ID and Password. You are now connected remotely to the PLUS1 server.*&lt;br /&gt;
&lt;br /&gt;
* It should be noted that you cannot subsequently SSH from the PLUS1 server into another pc in the pbt cluster using this method. Alternative methods to do so are discussed in the[http://www.hep.ucl.ac.uk/pbt/wiki/Software/Geant4/Eclipse#Running_a_SSH_Shell_in_Eclipse Running a SSH Shell in Eclipse] section.&lt;br /&gt;
&lt;br /&gt;
== Using Eclipse ==&lt;br /&gt;
&lt;br /&gt;
=== Remote System Details ===&lt;br /&gt;
&lt;br /&gt;
You can open a panel that displays details about the remote systems you have connected to. This is done by going to Window &amp;gt; Show View &amp;gt; Remote System Details. You can use this window in a manner similar to the Remote Systems file explorer panel, except that the Remote System Details panel gives more detail about the files contained (for example the time stamp of the last time the directory/file was edited etc). You can use the buttons at the top right of this panel to navigate through the servers directories.&lt;br /&gt;
&lt;br /&gt;
=== Easier File management ===&lt;br /&gt;
&lt;br /&gt;
Instead of using a bash terminal, you can use the tree within the Remote Systems panel to move, copy, and open files. This is done by simple highlighting the file, right clicking, and selecting the required operation (copy/cut/delete etc.). It should be noted that this method of file management is significantly slower than performing the same action via a terminal.&lt;br /&gt;
&lt;br /&gt;
=== Running a SSH Shell in Eclipse ===&lt;br /&gt;
&lt;br /&gt;
You can also open a bash terminal in Eclipse. In the Remote Systems panel, under the SSH connection you have created, you will see a subdirectory called &#039;Ssh Shells&#039;. Right click this and select Launch Shell. This shell allows connection to internal pc&#039;s in the pbt cluster, as well as the ability to perform all other standard bash commands on the pbt server.&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1112</id>
		<title>Software/Geant4/Eclipse</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1112"/>
		<updated>2017-09-27T12:56:19Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: re-titled link&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Editing Geant4 input files in Eclipse.&lt;br /&gt;
&lt;br /&gt;
== Why use Eclipse ==&lt;br /&gt;
&lt;br /&gt;
Eclipse allows for editing files remotely using an environment that gives rudimentary debugging tools and a easy to use remote file explorer. Furthermore, this method allows support of remote file editing on an operating system that does not have native access to the bash terminal (i.e. windows).&lt;br /&gt;
&lt;br /&gt;
It should be noted that this tutorial is written with the C/C++ Oxygen version of the Eclipse IDE in mind, as the Remote System Explorer plug-ins are included in this package, but the tutorial should work for other packages. All of the current eclipse packages can be found in the [https://www.eclipse.org/downloads/eclipse-packages/ Running a SSH Shell in Eclipse] section.&lt;br /&gt;
&lt;br /&gt;
== Connecting via SSH ==&lt;br /&gt;
&lt;br /&gt;
Once you have downloaded, installed, and launched Eclipse, you will want to SSH into the plus1.hep.ucl.ac.uk server. This is done by the following steps:&lt;br /&gt;
&lt;br /&gt;
1) Open the Remote System Explorer (RSE). This is done by going to Window &amp;gt; Perspective &amp;gt; Open Perspective &amp;gt; Other, and then choosing Remote System Explorer.&lt;br /&gt;
&lt;br /&gt;
2) In the Panel containing the Remote Systems tab that appeared when the RSE was opened, define a new connection. This can be done by clicking the icon at the top of the panel, or right clicking on the panel and selecting New &amp;gt; Connection&lt;br /&gt;
&lt;br /&gt;
3) In the New Connection window that opened, select the &#039;SSH Only&#039; System type.&lt;br /&gt;
&lt;br /&gt;
4) In the Host name text box, enter the server address that you want to SSH into. For use with the pbt server, enter&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
PLUS1.HEP.UCL.AC.UK&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
and give the connection a name, for example &amp;lt;code&amp;gt;PLUS1&amp;lt;/code&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
5) In the Remote Systems panel opened earlier, you should see a new connection with then connection name you chose earlier. Opening the tree by going Stfp Files &amp;gt; Root, you will be prompted to enter a User ID and password. In their respective text boxes, enter your pbt User ID and Password. You are now connected remotely to the PLUS1 server.*&lt;br /&gt;
&lt;br /&gt;
* It should be noted that you cannot subsequently SSH from the PLUS1 server into another pc in the pbt cluster using this method. Alternative methods to do so are discussed [http://www.hep.ucl.ac.uk/pbt/wiki/Software/Geant4/Eclipse#Running_a_SSH_Shell_in_Eclipse here].&lt;br /&gt;
&lt;br /&gt;
== Using Eclipse ==&lt;br /&gt;
&lt;br /&gt;
=== Remote System Details ===&lt;br /&gt;
&lt;br /&gt;
You can open a panel that displays details about the remote systems you have connected to. This is done by going to Window &amp;gt; Show View &amp;gt; Remote System Details. You can use this window in a manner similar to the Remote Systems file explorer panel, except that the Remote System Details panel gives more detail about the files contained (for example the time stamp of the last time the directory/file was edited etc). You can use the buttons at the top right of this panel to navigate through the servers directories.&lt;br /&gt;
&lt;br /&gt;
=== Easier File management ===&lt;br /&gt;
&lt;br /&gt;
Instead of using a bash terminal, you can use the tree within the Remote Systems panel to move, copy, and open files. This is done by simple highlighting the file, right clicking, and selecting the required operation (copy/cut/delete etc.). It should be noted that this method of file management is significantly slower than performing the same action via a terminal.&lt;br /&gt;
&lt;br /&gt;
=== Running a SSH Shell in Eclipse ===&lt;br /&gt;
&lt;br /&gt;
You can also open a bash terminal in Eclipse. In the Remote Systems panel, under the SSH connection you have created, you will see a subdirectory called &#039;Ssh Shells&#039;. Right click this and select Launch Shell. This shell allows connection to internal pc&#039;s in the pbt cluster, as well as the ability to perform all other standard bash commands on the pbt server.&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1111</id>
		<title>Software/Geant4/Eclipse</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1111"/>
		<updated>2017-09-27T12:54:29Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Edited link for SSH&amp;#039;ing into alternate PC&amp;#039;s on the cluster&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Editing Geant4 input files in Eclipse.&lt;br /&gt;
&lt;br /&gt;
== Why use Eclipse ==&lt;br /&gt;
&lt;br /&gt;
Eclipse allows for editing files remotely using an environment that gives rudimentary debugging tools and a easy to use remote file explorer. Furthermore, this method allows support of remote file editing on an operating system that does not have native access to the bash terminal (i.e. windows).&lt;br /&gt;
&lt;br /&gt;
It should be noted that this tutorial is written with the C/C++ Oxygen version of the Eclipse IDE in mind, as the Remote System Explorer plug-ins are included in this package, but the tutorial should work for other packages. All of the current eclipse packages can be found [https://www.eclipse.org/downloads/eclipse-packages/ here].&lt;br /&gt;
&lt;br /&gt;
== Connecting via SSH ==&lt;br /&gt;
&lt;br /&gt;
Once you have downloaded, installed, and launched Eclipse, you will want to SSH into the plus1.hep.ucl.ac.uk server. This is done by the following steps:&lt;br /&gt;
&lt;br /&gt;
1) Open the Remote System Explorer (RSE). This is done by going to Window &amp;gt; Perspective &amp;gt; Open Perspective &amp;gt; Other, and then choosing Remote System Explorer.&lt;br /&gt;
&lt;br /&gt;
2) In the Panel containing the Remote Systems tab that appeared when the RSE was opened, define a new connection. This can be done by clicking the icon at the top of the panel, or right clicking on the panel and selecting New &amp;gt; Connection&lt;br /&gt;
&lt;br /&gt;
3) In the New Connection window that opened, select the &#039;SSH Only&#039; System type.&lt;br /&gt;
&lt;br /&gt;
4) In the Host name text box, enter the server address that you want to SSH into. For use with the pbt server, enter&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
PLUS1.HEP.UCL.AC.UK&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
and give the connection a name, for example &amp;lt;code&amp;gt;PLUS1&amp;lt;/code&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
5) In the Remote Systems panel opened earlier, you should see a new connection with then connection name you chose earlier. Opening the tree by going Stfp Files &amp;gt; Root, you will be prompted to enter a User ID and password. In their respective text boxes, enter your pbt User ID and Password. You are now connected remotely to the PLUS1 server.*&lt;br /&gt;
&lt;br /&gt;
* It should be noted that you cannot subsequently SSH from the PLUS1 server into another pc in the pbt cluster using this method. Alternative methods to do so are discussed [http://www.hep.ucl.ac.uk/pbt/wiki/Software/Geant4/Eclipse#Running_a_SSH_Shell_in_Eclipse here].&lt;br /&gt;
&lt;br /&gt;
== Using Eclipse ==&lt;br /&gt;
&lt;br /&gt;
=== Remote System Details ===&lt;br /&gt;
&lt;br /&gt;
You can open a panel that displays details about the remote systems you have connected to. This is done by going to Window &amp;gt; Show View &amp;gt; Remote System Details. You can use this window in a manner similar to the Remote Systems file explorer panel, except that the Remote System Details panel gives more detail about the files contained (for example the time stamp of the last time the directory/file was edited etc). You can use the buttons at the top right of this panel to navigate through the servers directories.&lt;br /&gt;
&lt;br /&gt;
=== Easier File management ===&lt;br /&gt;
&lt;br /&gt;
Instead of using a bash terminal, you can use the tree within the Remote Systems panel to move, copy, and open files. This is done by simple highlighting the file, right clicking, and selecting the required operation (copy/cut/delete etc.). It should be noted that this method of file management is significantly slower than performing the same action via a terminal.&lt;br /&gt;
&lt;br /&gt;
=== Running a SSH Shell in Eclipse ===&lt;br /&gt;
&lt;br /&gt;
You can also open a bash terminal in Eclipse. In the Remote Systems panel, under the SSH connection you have created, you will see a subdirectory called &#039;Ssh Shells&#039;. Right click this and select Launch Shell. This shell allows connection to internal pc&#039;s in the pbt cluster, as well as the ability to perform all other standard bash commands on the pbt server.&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1110</id>
		<title>Software/Geant4/Eclipse</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;diff=1110"/>
		<updated>2017-09-27T12:53:00Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Added page with tutorial to using Eclipse to SSH into the pbt server&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Editing Geant4 input files in Eclipse.&lt;br /&gt;
&lt;br /&gt;
== Why use Eclipse ==&lt;br /&gt;
&lt;br /&gt;
Eclipse allows for editing files remotely using an environment that gives rudimentary debugging tools and a easy to use remote file explorer. Furthermore, this method allows support of remote file editing on an operating system that does not have native access to the bash terminal (i.e. windows).&lt;br /&gt;
&lt;br /&gt;
It should be noted that this tutorial is written with the C/C++ Oxygen version of the Eclipse IDE in mind, as the Remote System Explorer plug-ins are included in this package, but the tutorial should work for other packages. All of the current eclipse packages can be found [https://www.eclipse.org/downloads/eclipse-packages/ here].&lt;br /&gt;
&lt;br /&gt;
== Connecting via SSH ==&lt;br /&gt;
&lt;br /&gt;
Once you have downloaded, installed, and launched Eclipse, you will want to SSH into the plus1.hep.ucl.ac.uk server. This is done by the following steps:&lt;br /&gt;
&lt;br /&gt;
1) Open the Remote System Explorer (RSE). This is done by going to Window &amp;gt; Perspective &amp;gt; Open Perspective &amp;gt; Other, and then choosing Remote System Explorer.&lt;br /&gt;
&lt;br /&gt;
2) In the Panel containing the Remote Systems tab that appeared when the RSE was opened, define a new connection. This can be done by clicking the icon at the top of the panel, or right clicking on the panel and selecting New &amp;gt; Connection&lt;br /&gt;
&lt;br /&gt;
3) In the New Connection window that opened, select the &#039;SSH Only&#039; System type.&lt;br /&gt;
&lt;br /&gt;
4) In the Host name text box, enter the server address that you want to SSH into. For use with the pbt server, enter&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
PLUS1.HEP.UCL.AC.UK&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
and give the connection a name, for example &amp;lt;code&amp;gt;PLUS1&amp;lt;/code&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
5) In the Remote Systems panel opened earlier, you should see a new connection with then connection name you chose earlier. Opening the tree by going Stfp Files &amp;gt; Root, you will be prompted to enter a User ID and password. In their respective text boxes, enter your pbt User ID and Password. You are now connected remotely to the PLUS1 server.*&lt;br /&gt;
&lt;br /&gt;
* It should be noted that you cannot subsequently SSH from the PLUS1 server into another pc in the pbt cluster using this method. Alternative methods to do so are discussed [http://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Eclipse&amp;amp;action=submit#Running_a_SSH_Shell_in_Eclipse here].&lt;br /&gt;
&lt;br /&gt;
== Using Eclipse ==&lt;br /&gt;
&lt;br /&gt;
=== Remote System Details ===&lt;br /&gt;
&lt;br /&gt;
You can open a panel that displays details about the remote systems you have connected to. This is done by going to Window &amp;gt; Show View &amp;gt; Remote System Details. You can use this window in a manner similar to the Remote Systems file explorer panel, except that the Remote System Details panel gives more detail about the files contained (for example the time stamp of the last time the directory/file was edited etc). You can use the buttons at the top right of this panel to navigate through the servers directories.&lt;br /&gt;
&lt;br /&gt;
=== Easier File management ===&lt;br /&gt;
&lt;br /&gt;
Instead of using a bash terminal, you can use the tree within the Remote Systems panel to move, copy, and open files. This is done by simple highlighting the file, right clicking, and selecting the required operation (copy/cut/delete etc.). It should be noted that this method of file management is significantly slower than performing the same action via a terminal.&lt;br /&gt;
&lt;br /&gt;
=== Running a SSH Shell in Eclipse ===&lt;br /&gt;
&lt;br /&gt;
You can also open a bash terminal in Eclipse. In the Remote Systems panel, under the SSH connection you have created, you will see a subdirectory called &#039;Ssh Shells&#039;. Right click this and select Launch Shell. This shell allows connection to internal pc&#039;s in the pbt cluster, as well as the ability to perform all other standard bash commands on the pbt server.&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Tutorials/Advanced/High-Precision_Dosimetry&amp;diff=1100</id>
		<title>Software/Geant4/Tutorials/Advanced/High-Precision Dosimetry</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Tutorials/Advanced/High-Precision_Dosimetry&amp;diff=1100"/>
		<updated>2017-09-26T12:04:01Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Formatting and minor corrections to code.&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Introduction ==&lt;br /&gt;
&lt;br /&gt;
This tutorial is based on the [http://geant4-dna.org/ Geant4-DNA project] tutorials. We chose to show three of the examples:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; dnaphysics &amp;lt;/span&amp;gt;: This example simulates track structures in 100-micron side cube made of liquid water. The physics processes are defined using class &#039;&#039;&#039;G4EmDNAPhysics&#039;&#039;&#039;. [http://geant4-dna.in2p3.fr/styled-3/styled-8/index.html Here] you can find more information about the different physics process that are used to build class &#039;&#039;&#039;G4EmDNAPhysics&#039;&#039;&#039; . [http://geant4-dna.in2p3.fr/styled-3/styled-9/index.html Here] you can find how to build your own &#039;&#039;&#039;G4EmDNAPhysics&#039;&#039;&#039; class. Simulated is a an electron beam using class &#039;&#039;&#039;G4ParticleGun&#039;&#039;&#039;. The beam is shot from the center of the cube. The output of this tutorial is a root ntuple with type of particle, type of physics process, energy deposit, energy loss and step length for every simulation step.  &lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; dnageometry &amp;lt;/span&amp;gt;: This example simulates track structures of different charged particles within a simplified geometrical model of the DNA molecule in a cell nucleus. [http://www.chemguide.co.uk/organicprops/aminoacids/dna1.html Here] you can read more about the DNA structure. Simulated are 6109 DNA pairs with the following structures: double helix, nucleosome, chromatine fibres, chromatine fibre loops and chromosome territories. Proton beam is simulated using class &#039;&#039;&#039;G4ParticleGun&#039;&#039;&#039;. The physics processes are defined using class &#039;&#039;&#039;G4EmDNAPhysics&#039;&#039;&#039;. The output is a root ntuple with type of particle, type of physics process, energy deposit and step length for every simulation step. &lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; microbeam &amp;lt;/span&amp;gt;: This example simulates the cellular irradiation beam line installed on the [http://www.cenbg.in2p3.fr/-AIFIRA-Home-?lang=en AIFIRA] electrostatic accelerator facility located at [http://www.cenbg.in2p3.fr/ CENBG], Bordeaux-Gradignan, France. This accelerator is mainly used to investigate the effects of low dose irradiation on living cells. A realistic cell phantom is obtained from confocal microscopy and from ion beam anlysis techniques. Alpha particles of 3 MeV are incident on this phantom. The output among other things is the dose deposited in the cell cytoplasm and in the cell nucleus. &lt;br /&gt;
&lt;br /&gt;
== How to run the tutorials ==&lt;br /&gt;
&lt;br /&gt;
=== Connect to the HEP cluster ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
ssh -X username@plus1.hep.ucl.ac.uk &lt;br /&gt;
&lt;br /&gt;
username@plus1.hep.ucl.ac.uk&#039;s password: type your password here&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Setup your environment ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 ~]$ source /unix/pbt/software/scripts/pbt.sh&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Copy the code to your working directory ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 ~]$ cp -r /unix/pbt/tutorials/advanced/DNAProject .&lt;br /&gt;
  &lt;br /&gt;
[username@plus1 ~]$ cd DNAProject&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
 &lt;br /&gt;
== dnaphysics: ==&lt;br /&gt;
&lt;br /&gt;
=== Inside &amp;lt;code&amp;gt;/home/username/DNAProject/&amp;lt;/code&amp;gt; create a directory ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ mkdir dnaphysics_build  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Compile the code with &amp;lt;code&amp;gt;make&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;cmake&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ cd dnaphysics_build &lt;br /&gt;
&lt;br /&gt;
[username@plus1 dnaphysics_build]$ cmake -DGeant4_DIR=/unix/pbt/software/dev /home/username/DNAProject/dnaphysics &lt;br /&gt;
&lt;br /&gt;
[username@plus1 dnaphysics_build]$ make  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Run macro &amp;lt;code&amp;gt;dna.mac&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ ./dnaphysics dna.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== dnageometry: ==&lt;br /&gt;
&lt;br /&gt;
=== Inside &amp;lt;code&amp;gt;/home/username/DNAProject/&amp;lt;/code&amp;gt; create a directory ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ mkdir dnageometry_build  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Compile the code with &amp;lt;code&amp;gt;make&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;cmake&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ cd dnageometry_build &lt;br /&gt;
&lt;br /&gt;
[username@plus1 dnageometry_build]$ cmake -DGeant4_DIR=/unix/pbt/software/dev /home/username/DNAProject/dnageometry &lt;br /&gt;
&lt;br /&gt;
[username@plus1 dnageometry_build]$ make  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Run macro &amp;lt;code&amp;gt;dnageometry.mac&amp;lt;/code&amp;gt; === &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnageometry_build]$ ./dnageometry dnageometry.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== microbeam: ==&lt;br /&gt;
&lt;br /&gt;
=== Inside &amp;lt;code&amp;gt;/home/username/DNAProject/&amp;lt;/code&amp;gt; create a directory ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ mkdir microbeam_build  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Compile the code with &amp;lt;code&amp;gt;make&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;cmake&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DNAProject]$ cd microbeam_build &lt;br /&gt;
&lt;br /&gt;
[username@plus1 microbeam_build]$ cmake -DGeant4_DIR=/unix/pbt/software/dev /home/username/DNAProject/microbeam &lt;br /&gt;
&lt;br /&gt;
[username@plus1 microbeam_build]$ make  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Run macro microbeam.mac === &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 microbeam_build]$ ./microbeam microbeam.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== How to analyze the data ==&lt;br /&gt;
&lt;br /&gt;
=== dnaphysics ===&lt;br /&gt;
&lt;br /&gt;
This is a [http://geant4advancedexampleswg.wikispaces.com/DNAPhysics link] to the official dnaphysics tutorial explanation notes. We recommend to read it before proceeding with this tutorial. &lt;br /&gt;
&lt;br /&gt;
==== Root file ====&lt;br /&gt;
&lt;br /&gt;
The macro &amp;lt;code&amp;gt;dna.mac&amp;lt;/code&amp;gt; produces two root files &amp;lt;code&amp;gt;dna_t0.root&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;dna_t1.root&amp;lt;/code&amp;gt; with ntuples containing the following information for every step: &lt;br /&gt;
&lt;br /&gt;
* type of particle&lt;br /&gt;
* type of physics process&lt;br /&gt;
* x, y and z coordinates of the beginning of the step &lt;br /&gt;
* total energy deposit alo[eV]&lt;br /&gt;
* step length [nm]&lt;br /&gt;
* kinetic energy difference along the step [eV] &lt;br /&gt;
&lt;br /&gt;
You can open the first root file and see the different ntuples:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ root -l dna_t0.root&lt;br /&gt;
&lt;br /&gt;
root [1] new TBrowser&lt;br /&gt;
&lt;br /&gt;
Select ROOT Files, dna_t0.root and Folder dna&lt;br /&gt;
&lt;br /&gt;
Click on the different leafs &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
You can analyze the root files using &amp;lt;code&amp;gt;plot.C&amp;lt;/code&amp;gt; macro. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ root -l&lt;br /&gt;
&lt;br /&gt;
root [1] .x plot.C&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The macro produces two plots. The first plot shows the distribution of the different physics plrocesses. The second plot shows the trajectory of the incident particle. [http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DNAProject/dnaphysics/flags.txt Here] you can find the codes for &amp;lt;code&amp;gt;flagParticle&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;flagProcess&amp;lt;/code&amp;gt;. The root macro produces the following plots:  &lt;br /&gt;
&lt;br /&gt;
http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DNAProject/dnaphysics/plot.png&lt;br /&gt;
&lt;br /&gt;
==== Run with different settings ====&lt;br /&gt;
&lt;br /&gt;
You can change the type and the energy of the incident particle by modifying the macro dna.mac. Open the macro with editor pico: &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ pico dna.mac &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This is the content of the macro:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
#/control/execute vis.mac&lt;br /&gt;
/tracking/verbose 0&lt;br /&gt;
/run/verbose 2&lt;br /&gt;
#/dna/det/setMat G4_WATER_MODIFIED&lt;br /&gt;
/dna/det/setMat G4_WATER&lt;br /&gt;
/gun/particle e-&lt;br /&gt;
#/gun/particle proton&lt;br /&gt;
#/gun/particle hydrogen&lt;br /&gt;
#/gun/particle alpha&lt;br /&gt;
#/gun/particle alpha+&lt;br /&gt;
#/gun/particle helium&lt;br /&gt;
/gun/energy 1 keV&lt;br /&gt;
/run/initialize&lt;br /&gt;
/process/em/auger true&lt;br /&gt;
/run/beamOn 100&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== Visualisation ====&lt;br /&gt;
&lt;br /&gt;
There is an option to run dna.mac with visualisation (in &amp;lt;code&amp;gt;dna.mac&amp;lt;/code&amp;gt; uncomment line &amp;lt;code&amp;gt;/control/execute vis.mac&amp;lt;/code&amp;gt;). However, runing with visualisation is very slow and it is not recommended.  &lt;br /&gt;
&lt;br /&gt;
=== dnageometry ===&lt;br /&gt;
&lt;br /&gt;
This is a [http://geant4advancedexampleswg.wikispaces.com/DNAGeometry link] to the official dnageometry tutorial explanation notes.&lt;br /&gt;
&lt;br /&gt;
==== Root file ====&lt;br /&gt;
&lt;br /&gt;
The macro &amp;lt;code&amp;gt;dnageometry.mac&amp;lt;/code&amp;gt; produces a root file &amp;lt;code&amp;gt;dnageometry.root&amp;lt;/code&amp;gt; with ntuples. The ntuples contain information for those geant4 steps for which the deposited energy in the DNA backbone is different from zero: &lt;br /&gt;
&lt;br /&gt;
* type of particle&lt;br /&gt;
* type of physics process&lt;br /&gt;
* the two DNA strands &lt;br /&gt;
* x, y and z coordinates of the post step [nm]&lt;br /&gt;
* total energy deposit alo[eV]&lt;br /&gt;
* step length [nm]&lt;br /&gt;
 &lt;br /&gt;
You can analyze the root files using &amp;lt;code&amp;gt;plot.C&amp;lt;/code&amp;gt; macro. First, copy this macro to your directory, then run the root &lt;br /&gt;
macro. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ cp /home/username/DNAProject/dnageometry/plot.C .&lt;br /&gt;
&lt;br /&gt;
[username@plus1 dnaphysics_build]$ root -l&lt;br /&gt;
&lt;br /&gt;
root [1] .x plot.C&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The macro produces a plot that shows the position of the two DNA strands in two colors. The spheres represent the amino bases. The plot shows only the DNA pairs with deposited energy (see the ntuple deffinition in SteppingAction.cc).    &lt;br /&gt;
&lt;br /&gt;
http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DNAProject/dnageometry/plot.png&lt;br /&gt;
&lt;br /&gt;
You can modify root macro &amp;lt;code&amp;gt;plot.C&amp;lt;/code&amp;gt; and plot the other ntuples.&lt;br /&gt;
 &lt;br /&gt;
=== microbeam  ===&lt;br /&gt;
&lt;br /&gt;
This is a [http://geant4advancedexampleswg.wikispaces.com/MicrobeamExample link] to the official microbeam tutorial explanation notes.&lt;br /&gt;
&lt;br /&gt;
==== Root file  ====&lt;br /&gt;
&lt;br /&gt;
The macro &amp;lt;code&amp;gt;microbeam.mac&amp;lt;/code&amp;gt; produces root files &amp;lt;code&amp;gt;microbeam_t0.root&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;microbeam_t1.root&amp;lt;/code&amp;gt; with ntuples grouped in five folders.&lt;br /&gt;
&lt;br /&gt;
You can analyze the root ntuples using the &amp;lt;code&amp;gt;plot.C&amp;lt;/code&amp;gt; macro. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 dnaphysics_build]$ root -l&lt;br /&gt;
&lt;br /&gt;
root [1] .x plot.C&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DNAProject/microbeam/plot.png&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Tutorials/Advanced/Computed_Tomography&amp;diff=1099</id>
		<title>Software/Geant4/Tutorials/Advanced/Computed Tomography</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Software/Geant4/Tutorials/Advanced/Computed_Tomography&amp;diff=1099"/>
		<updated>2017-09-26T09:54:16Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Formatting changes and tweaks of information contained&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Introduction ==&lt;br /&gt;
&lt;br /&gt;
This tutorial is based on the GEANT4 DICOM example originally developed by Louis Archambault, Luc Beaulieu and Vincent Hubert-Tremblay. In this example a list of DICOM files (.dcm) are converted to ASCII files (.g4dcm) and binary files (.g4bin) that can be read by GEANT4. Each of these files corresponds to a Z Computed tomography (CT) slice. Then, the .g4dcm (.g4bin) files are merged into one volume.    &lt;br /&gt;
&lt;br /&gt;
The geometry is constructed by voxelizing this volume. There are four navigation algorithms used to create the voxel geometry: &amp;lt;code&amp;gt;G4RegularNavigation&amp;lt;/code&amp;gt;, &amp;lt;code&amp;gt;G4VNestedParameterisation&amp;lt;/code&amp;gt;, &amp;lt;code&amp;gt;G4SmartVoxel&amp;lt;/code&amp;gt;/&amp;lt;code&amp;gt;G4VoxelNavigation&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;G4PVReplica&amp;lt;/code&amp;gt;.   &lt;br /&gt;
&lt;br /&gt;
The material for this volume is constructed by converting the pixel values (Hounsfield numbers) from the DICOM images to densities using the [http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DICOM/CT2Density.dat Hounsfield scale]. Then, the densities are converted to material types according to this [http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DICOM/Materials.txt table].&lt;br /&gt;
&lt;br /&gt;
A simple monenergetic electron beam is simulated using &amp;lt;code&amp;gt;G4ParticleGun&amp;lt;/code&amp;gt; class. The output of the tutorial is a text file with dose deposition in several voxels. The dose is scored using classes &amp;lt;code&amp;gt;G4MutiFunctionalDetector&amp;lt;/code&amp;gt;, &amp;lt;code&amp;gt;G4VPrimitiveScorer&amp;lt;/code&amp;gt;, &amp;lt;code&amp;gt;G4PSDoseDeposit3D&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;G4THitsMap&amp;lt;/code&amp;gt;. &lt;br /&gt;
&lt;br /&gt;
http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DICOM/dicom.png&lt;br /&gt;
&lt;br /&gt;
This is one of the DICOM files used in the tutorial.&lt;br /&gt;
&lt;br /&gt;
== How to run the tutorial ==&lt;br /&gt;
&lt;br /&gt;
=== Create folder DICOMFolder ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
ssh -X username@plus1.hep.ucl.ac.uk &lt;br /&gt;
&lt;br /&gt;
username@plus1.hep.ucl.ac.uk&#039;s password: type your password here&lt;br /&gt;
&lt;br /&gt;
[username@plus1 ~]$ mkdir DICOMFolder &lt;br /&gt;
&lt;br /&gt;
[username@plus1 ~]$ cd DICOMFolder  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Setup your environment ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOMFolder]$ source /unix/pbt/software/scripts/pbt.sh&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Copy the code to your working directory and rename it ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOMFolder]$ cp -r /unix/pbt/tutorials/advanced/DICOM .&lt;br /&gt;
  &lt;br /&gt;
[username@plus1 DICOMFolder]$ mv DICOM DICOM_source&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Create build directory ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOMFolder]$ mkdir DICOM_build  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Compile the code with &amp;lt;code&amp;gt;make&amp;lt;/code&amp;gt; and &amp;lt;code&amp;gt;cmake&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOMFolder]$ cd DICOM_build &lt;br /&gt;
&lt;br /&gt;
[username@plus1 DICOM_build]$ cmake -DGeant4_DIR=/unix/pbt/software/dev /home/username/DICOMFolder/DICOM_source &lt;br /&gt;
&lt;br /&gt;
[username@plus1 DICOM_build]$ make  &lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Run Macro &amp;lt;code&amp;gt;run.mac&amp;lt;/code&amp;gt; ===&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ ./DICOM run.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Analyze the data ==&lt;br /&gt;
&lt;br /&gt;
This is a [http://geant4.web.cern.ch/geant4/UserDocumentation/Doxygen/examples_doc/html/ExampleDICOM.html link] to the official DICOM tutorial explanation notes. We recommend to read it before proceeding with this tutorial.&lt;br /&gt;
&lt;br /&gt;
=== Text files ===&lt;br /&gt;
&lt;br /&gt;
The macro &amp;lt;code&amp;gt;run.mac&amp;lt;/code&amp;gt; produces a text file &amp;lt;code&amp;gt;dicom.out&amp;lt;/code&amp;gt; which includes the dose deposition in several voxels.&lt;br /&gt;
&lt;br /&gt;
=== Run with different settings ===&lt;br /&gt;
&lt;br /&gt;
Chose among several voxelization algorithms:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; G4RegularNavigation &amp;lt;/span&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;code&amp;gt;G4RegularNavigation&amp;lt;/code&amp;gt; class is the default class for this tutorial. This algorithm skips frontiers between voxels when they have the same material i.e. &amp;quot;replacing group of voxels with a smaller number of larger voxels&amp;quot;.  &lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; G4NestedParameterization &amp;lt;/span&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
To run with this voxelization algorithm you need to set the variable &#039;&#039;&#039;DICOM_NESTED_PARAM&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ export DICOM_NESTED_PARAM=1&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
You can check if it is set correctly by typing in the command line&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ env&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, compile and run the code:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ make &lt;br /&gt;
&lt;br /&gt;
[username@plus1 DICOM_build]$ ./DICOM run.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;span style=&amp;quot;color:#ff0000&amp;quot;&amp;gt; G4SmartVoxel / G4VoxelNavigation &amp;lt;/span&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
Using smart voxels required a huge amount of memory. At &amp;lt;code&amp;gt;/home/username/DICOMFolder/DICOM_source/src/DicomRegularDetectorConstruction.cc&amp;lt;/code&amp;gt; set&lt;br /&gt;
 &lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
patient_phys-&amp;gt;SetRegularStructureId(0);&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
compile and run the code:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ make&lt;br /&gt;
&lt;br /&gt;
[username@plus1 DICOM_build]$ ./DICOM run.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Change the type, energy and position of the incident particle ===&lt;br /&gt;
&lt;br /&gt;
At &amp;lt;code&amp;gt;/home/username/DICOMFolder/DICOM_source/src/DicomPrimaryGeneratorAction.cc&amp;lt;/code&amp;gt; change the following lines:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
G4ParticleDefinition* particle = particleTable-&amp;gt;FindParticle(particleName=&amp;quot;e-&amp;quot;);&lt;br /&gt;
&lt;br /&gt;
fParticleGun-&amp;gt;SetParticleEnergy(100.*MeV);&lt;br /&gt;
&lt;br /&gt;
fParticleGun-&amp;gt;SetParticlePosition(G4ThreeVector(0.,0.,0.));&lt;br /&gt;
&amp;lt;/pre&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
You can chose among several particles like &amp;quot;gamma&amp;quot;, &amp;quot;e+&amp;quot;, &amp;quot;alpha&amp;quot; and &amp;quot;He3&amp;quot;. Then, compile and run the code&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ make&lt;br /&gt;
&lt;br /&gt;
[username@plus1 DICOM_build]$ ./DICOM run.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Visualisation ===&lt;br /&gt;
&lt;br /&gt;
Run the visualisation macro &amp;lt;code&amp;gt;vis.mac&amp;lt;/code&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ ./DICOM vis.mac&lt;br /&gt;
&amp;lt;/pre&amp;gt;&lt;br /&gt;
&lt;br /&gt;
which will produce &amp;lt;code&amp;gt;.prim&amp;lt;/code&amp;gt; file. You can open this file in DAWN&lt;br /&gt;
&lt;br /&gt;
&amp;lt;pre&amp;gt;&lt;br /&gt;
[username@plus1 DICOM_build]$ dawn g4_00.prim&lt;br /&gt;
&amp;lt;/pre&amp;gt; &lt;br /&gt;
&lt;br /&gt;
This will create 3D image showing the patient geometry and the incident electron beam. The image is big and it takes time to open:&lt;br /&gt;
&lt;br /&gt;
http://www.hep.ucl.ac.uk/pbt/RadiotherapyWorkbook/skins/common/images/DICOM/g4_03.eps&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=867</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=867"/>
		<updated>2017-07-10T12:15:57Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Radiation Units */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;&lt;br /&gt;
{| style = &amp;quot;width:30%;&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
| style = &amp;quot;text-align:left;&amp;quot;| for a given effect  &lt;br /&gt;
| style = &amp;quot;width:30%; text-align:right;&amp;quot;| (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, &#039;&#039;&#039;WR&#039;&#039;&#039;  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, &#039;&#039;&#039;E&#039;&#039;&#039; (Eq-2) is the sum of the tissue-weighted equivalent dose, &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; multiplied by the equivalent dose, &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; for all tissue types, &#039;&#039;&#039;T&#039;&#039;&#039;. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &lt;br /&gt;
{| style = &amp;quot;width:30%&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;E&#039;&#039;&#039; = &#039;&#039;&#039;&amp;amp;sum;&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ( &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; &amp;amp;times; &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ) &lt;br /&gt;
|style=&amp;quot;width:30%; text-align:right;&amp;quot; | (2)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=866</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=866"/>
		<updated>2017-07-10T12:15:27Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt;&lt;br /&gt;
{| style = &amp;quot;width:30%;&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;&lt;br /&gt;
| style = &amp;quot;text-align:left;&amp;quot;| for a given effect  &lt;br /&gt;
| style = &amp;quot;width:30%; text-align:right;&amp;quot;| (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, &#039;&#039;&#039;WR&#039;&#039;&#039;  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, &#039;&#039;&#039;E&#039;&#039;&#039; (Eq-1) is the sum of the tissue-weighted equivalent dose, &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; multiplied by the equivalent dose, &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; for all tissue types, &#039;&#039;&#039;T&#039;&#039;&#039;. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &lt;br /&gt;
{| style = &amp;quot;width:80%&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;E&#039;&#039;&#039; = &#039;&#039;&#039;&amp;amp;sum;&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ( &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; &amp;amp;times; &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ) &lt;br /&gt;
|style=&amp;quot;width:80%; text-align:right;&amp;quot; | (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=865</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=865"/>
		<updated>2017-07-10T12:10:56Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Radiation Units */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, &#039;&#039;&#039;WR&#039;&#039;&#039;  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, &#039;&#039;&#039;E&#039;&#039;&#039; (Eq-1) is the sum of the tissue-weighted equivalent dose, &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; multiplied by the equivalent dose, &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; for all tissue types, &#039;&#039;&#039;T&#039;&#039;&#039;. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &lt;br /&gt;
{| style = &amp;quot;width:80%&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;E&#039;&#039;&#039; = &#039;&#039;&#039;&amp;amp;sum;&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ( &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; &amp;amp;times; &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ) &lt;br /&gt;
|style=&amp;quot;width:80%; text-align:right;&amp;quot; | (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=864</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=864"/>
		<updated>2017-07-10T11:55:53Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Radiation Units */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, &#039;&#039;&#039;WR&#039;&#039;&#039;  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; multiplied by the equivalent dose, &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; for all tissue types, &#039;&#039;&#039;T&#039;&#039;&#039;. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &lt;br /&gt;
{| style = &amp;quot;width:80%&amp;quot;&lt;br /&gt;
|&#039;&#039;&#039;E&#039;&#039;&#039; = &#039;&#039;&#039;&amp;amp;sum;&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ( &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; &amp;amp;times; &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ) &lt;br /&gt;
|style=&amp;quot;width:80%; text-align:right;&amp;quot; | (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=863</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=863"/>
		<updated>2017-07-10T11:54:43Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Radiation Units */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, &#039;&#039;&#039;WR&#039;&#039;&#039;  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; multiplied by the equivalent dose, &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; for all tissue types, &#039;&#039;&#039;T&#039;&#039;&#039;. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &lt;br /&gt;
{|&lt;br /&gt;
|&#039;&#039;&#039;E&#039;&#039;&#039; = &#039;&#039;&#039;&amp;amp;sum;&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ( &#039;&#039;&#039;H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; &amp;amp;times; &#039;&#039;&#039;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&#039;&#039;&#039; ) &lt;br /&gt;
|style=&amp;quot;width:100px; text-align:right;&amp;quot; | (1)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=862</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=862"/>
		<updated>2017-07-10T11:43:09Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Linear energy transfer&#039;&#039;&#039; (&#039;&#039;&#039;LET&#039;&#039;&#039;) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The &#039;&#039;&#039;LET&#039;&#039;&#039; of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the &#039;&#039;&#039;LET&#039;&#039;&#039;, the more biologically potent the radiation. The &#039;&#039;&#039;LET&#039;&#039;&#039; for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Relative biological effectiveness&#039;&#039;&#039; (&#039;&#039;&#039;RBE&#039;&#039;&#039;) is the ratio of the dose of radiation of type x, &#039;&#039;&#039;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&#039;&#039;&#039; required to produce the same biological effect as a reference dose &#039;&#039;&#039;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&#039;&#039;&#039; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; &#039;&#039;&#039;RBE&#039;&#039;&#039; = &#039;&#039;&#039;&amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt;&#039;&#039;&#039; &amp;amp;frasl; &#039;&#039;&#039;&amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;&#039;&#039;&#039;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;RBE&#039;&#039;&#039; increases with &#039;&#039;&#039;LET&#039;&#039;&#039; until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;RBE&#039;&#039;&#039; of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; multiplied by the equivalent dose, H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;(H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&amp;amp;times;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;)  Eq-1 &amp;lt;!--will be fixed properly--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=861</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=861"/>
		<updated>2017-07-10T11:39:27Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Linear energy transfer (LET) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The LET of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the LET, the more biologically potent the radiation. The LET for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
Relative biological effectiveness (RBE) is the ratio of the dose of radiation of type x, R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt; required to produce the same biological effect as a reference dose R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; RBE = &amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt; &amp;amp;frasl; &amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
RBE increases with LET until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The RBE of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; multiplied by the equivalent dose, H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;(H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&amp;amp;times;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;)  Eq-1 &amp;lt;!--will be fixed properly--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=860</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=860"/>
		<updated>2017-07-10T11:38:53Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */ Neatened up equations&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3&amp;amp;times;10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt; m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;margin-left: auto; margin-right: auto; border: none;&amp;quot;&lt;br /&gt;
!|Electromagnetic Radiation&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
|rowspan=&amp;quot;6&amp;quot;|In order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;4&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Linear energy transfer (LET) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The LET of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the LET, the more biologically potent the radiation. The LET for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
Relative biological effectiveness (RBE) is the ratio of the dose of radiation of type x, R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt; required to produce the same biological effect as a reference dose R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60&lt;br /&gt;
&lt;br /&gt;
&amp;lt;blockquote&amp;gt; RBE = &amp;lt;sup&amp;gt;R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;&amp;lt;/sup&amp;gt; &amp;amp;frasl; &amp;lt;sub&amp;gt;R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;&amp;lt;/sub&amp;gt;         for a given effect  &amp;lt;/blockquote&amp;gt;&lt;br /&gt;
&lt;br /&gt;
RBE increases with LET until a critical point of &amp;amp;asymp;100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The RBE of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of &amp;amp;asymp;1; this value increases &amp;amp;asymp;10 - fold, however, when localised within the nucleus [8].&lt;br /&gt;
&amp;lt;br/&amp;gt;&amp;lt;br/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style = &amp;quot;float: right;&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
!Radiation type&lt;br /&gt;
!Radiation weighting factor&lt;br /&gt;
|-&lt;br /&gt;
|X-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Gamma-rays	&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Electrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Positrons&lt;br /&gt;
|1&lt;br /&gt;
|-&lt;br /&gt;
|Protons &amp;gt; 2 MeV&lt;br /&gt;
|2&lt;br /&gt;
|-&lt;br /&gt;
|Alpha particles&lt;br /&gt;
|20&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The &#039;&#039;&#039;radiation-absorbed dose&#039;&#039;&#039; is the total energy absorbed by tissue. It is given in &#039;&#039;&#039;rad&#039;&#039;&#039; or &#039;&#039;&#039;Gray (Gy)&#039;&#039;&#039;, 0.01 Gy = 1 rad. The &#039;&#039;&#039;equivalent dose&#039;&#039;&#039; is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The &#039;&#039;&#039;effective&#039;&#039;&#039; dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; multiplied by the equivalent dose, H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt; for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;(H&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;&amp;amp;times;W&amp;lt;sub&amp;gt;T&amp;lt;/sub&amp;gt;)  Eq-1 &amp;lt;!--will be fixed properly--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=792</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=792"/>
		<updated>2017-07-07T09:23:49Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */ subscripted some equations&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3*108 m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
Electromagnetic radiation in order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
Linear energy transfer (LET) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The LET of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the LET, the more biologically potent the radiation. The LET for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Relative biological effectiveness (RBE) is the ratio of the dose of radiation of type x, R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt; required to produce the same biological effect as a reference dose R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt; which is normally a high-energy x-ray beam (250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt;) or a gamma-ray from Cobalt-60&lt;br /&gt;
&lt;br /&gt;
RBE=R&amp;lt;sub&amp;gt;x&amp;lt;/sub&amp;gt;/R&amp;lt;sub&amp;gt;R&amp;lt;/sub&amp;gt;   for a given effect&lt;br /&gt;
&lt;br /&gt;
RBE increases with LET until a critical point of ≈100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The RBE of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of ≈1; this value increases ≈10-fold, however, when localised within the nucleus [8].&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Radiation weighting factor&lt;br /&gt;
X-rays	1&lt;br /&gt;
Gamma-rays	1&lt;br /&gt;
Electrons	1&lt;br /&gt;
Positrons	1&lt;br /&gt;
Protons &amp;gt; 2 MeV	2&lt;br /&gt;
Alpha particles	20&lt;br /&gt;
&lt;br /&gt;
The radiation-absorbed dose is the total energy absorbed by tissue. It is given in rad or Gray (Gy), 0.01 Gy = 1 rad. The equivalent dose is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The effective dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, WT multiplied by the equivalent dose, HT for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑_T▒〖H_T*W_T                         Eq-1〗&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=758</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=758"/>
		<updated>2017-07-06T12:20:15Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: /* Terminology in nuclear medicine */ table headings corrected from sub-atomic particle to radiation in column 1&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3*108 m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
Electromagnetic radiation in order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
Linear energy transfer (LET) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The LET of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the LET, the more biologically potent the radiation. The LET for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Radiation&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Relative biological effectiveness (RBE) is the ratio of the dose of radiation of type x, Rx required to produce the same biological effect as a reference dose RR which is normally a high-energy x-ray beam (250 kVp) or a gamma-ray from Cobalt-60&lt;br /&gt;
RBE=R_x/R_R   for a given effect&lt;br /&gt;
RBE increases with LET until a critical point of ≈100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The RBE of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of ≈1; this value increases ≈10-fold, however, when localised within the nucleus [8].&lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Radiation weighting factor&lt;br /&gt;
X-rays	1&lt;br /&gt;
Gamma-rays	1&lt;br /&gt;
Electrons	1&lt;br /&gt;
Positrons	1&lt;br /&gt;
Protons &amp;gt; 2 MeV	2&lt;br /&gt;
Alpha particles	20&lt;br /&gt;
&lt;br /&gt;
The radiation-absorbed dose is the total energy absorbed by tissue. It is given in rad or Gray (Gy), 0.01 Gy = 1 rad. The equivalent dose is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The effective dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, WT multiplied by the equivalent dose, HT for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑_T▒〖H_T*W_T                         Eq-1〗&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
	<entry>
		<id>https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=756</id>
		<title>Background/Radiobiology</title>
		<link rel="alternate" type="text/html" href="https://www.hep.ucl.ac.uk/pbt/pbtWiki/index.php?title=Background/Radiobiology&amp;diff=756"/>
		<updated>2017-07-06T12:16:09Z</updated>

		<summary type="html">&lt;p&gt;JordanSilverman: Formatted table 2&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Particulate Radiation&lt;br /&gt;
|-&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!Elementary Charge&lt;br /&gt;
!Relative Atomic Mass&lt;br /&gt;
|-&lt;br /&gt;
|Alpha (&#039;&#039;He&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +2 || 4&lt;br /&gt;
|-&lt;br /&gt;
|Proton (&#039;&#039;H&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Neutron (&#039;&#039;n&amp;lt;sup&amp;gt;0&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;indirectly ionising&#039;&#039;&#039; || 0 || 1&lt;br /&gt;
|-&lt;br /&gt;
|Electron (&#039;&#039;e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || -1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
|Positron (&#039;&#039;e&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;/&#039;&#039;&amp;amp;beta;&amp;lt;sup&amp;gt;+&amp;lt;/sup&amp;gt;&#039;&#039;) &amp;amp;mdash; &#039;&#039;&#039;directly ionising&#039;&#039;&#039; || +1 || 0.0005&lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;3&amp;quot;|Table 1: Examples of particulate radiation.  The charge and relative atomic mass of particulate radiation is also given &amp;lt;nowiki&amp;gt;[1,11]&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Radiation is energy that travels through space and matter. It is of two types: electromagnetic (EM) and particulate (Table 1). EM radiation is massless and moves through a vacuum at 3*108 m/s. It can be ionising or non-ionising. Particulate radiation is energy in the form of subatomic particles [1]&lt;br /&gt;
&lt;br /&gt;
Electromagnetic radiation in order of increasing frequency:&lt;br /&gt;
* Radio waves&lt;br /&gt;
* Microwaves&lt;br /&gt;
* Infrared&lt;br /&gt;
* Visible Light&lt;br /&gt;
* Ultraviolet&lt;br /&gt;
* X-rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
* Gamma rays &amp;amp;mdash; &#039;&#039;&#039;Indirectly ionising&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Background-sources-of-radiation.png|thumb|Figure 1: Sources and relative contribution of background radiation [http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ &amp;lt;nowiki&amp;gt;[23]&amp;lt;/nowiki&amp;gt;]|right|389px|link=http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/]]&lt;br /&gt;
&lt;br /&gt;
Directly ionising radiation strips electrons from atoms electrostatically. Indirectly ionising radiation causes electrons to be ejected from their atom by Compton scatter and the photoelectric effect. In the former, the fraction of the photon energy transferred to an outer electron is proportional to the cosine of the scatter angle. In the latter, all the photon energy is transferred to an inner electron. An electron must acquire an energy greater than its binding energy to be ejected [1].&lt;br /&gt;
The common sources of background radiation are given in Figure 1. The average exposure per year, per individual, is ≈2.4 mSv, which is equivalent to a fatal cancer risk of 0.012% for individuals aged between 30-60 [2,3]&lt;br /&gt;
&lt;br /&gt;
 &lt;br /&gt;
== Terminology in nuclear medicine ==&lt;br /&gt;
&lt;br /&gt;
Linear energy transfer (LET) describes how much energy (keV) a radiation-beam transfers to its surroundings per metre (Table 2). The LET of radiation increases with charge and mass, and decreases with kinetic energy [1].   The higher the LET, the more biologically potent the radiation. The LET for particulate radiation increases as it loses energy whilst traversing a medium [4].&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; style=&amp;quot;float: right; max-width: 500px; margin-left: 1em;&amp;quot;&lt;br /&gt;
!Sub-Atomic Particle&lt;br /&gt;
!LET (keV/&amp;amp;mu;m)&lt;br /&gt;
|-&lt;br /&gt;
| 1.25 MeV Co&amp;lt;sup&amp;gt;60&amp;lt;/sup&amp;gt; &amp;amp;gamma;-ray [5] || 0.25&lt;br /&gt;
|-&lt;br /&gt;
| 250 kV&amp;lt;sub&amp;gt;p&amp;lt;/sub&amp;gt; x-rays [6] || 2&lt;br /&gt;
|-&lt;br /&gt;
| 10 MeV proton [6] || 5.7&lt;br /&gt;
|-&lt;br /&gt;
| 20 keV &amp;amp;beta;-particle [7] || 10&lt;br /&gt;
|-&lt;br /&gt;
| 1 keV electrons [6] || 12.3 &lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV neutron [7] || 20&lt;br /&gt;
|-&lt;br /&gt;
| 5 MeV &amp;amp;alpha; particle [7] || 50 &lt;br /&gt;
|-&lt;br /&gt;
!colspan=&amp;quot;2&amp;quot;|Table 2: Linear energy transfer for a range of radiation types and energies. Alpha particles have the highest LET, and hence are most potent when inside the body, due to their low velocity and high mass. &lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
Relative biological effectiveness (RBE) is the ratio of the dose of radiation of type x, Rx required to produce the same biological effect as a reference dose RR which is normally a high-energy x-ray beam (250 kVp) or a gamma-ray from Cobalt-60&lt;br /&gt;
RBE=R_x/R_R   for a given effect&lt;br /&gt;
RBE increases with LET until a critical point of ≈100 keV/μm. The overkill region arises because the increasing dose has no further biological effect [1].&lt;br /&gt;
&lt;br /&gt;
The RBE of radiation may vary depending on its subcellular distribution: for example, when situated outside the cell, Auger electrons have an RBE of ≈1; this value increases ≈10-fold, however, when localised within the nucleus [8]. &lt;br /&gt;
&lt;br /&gt;
== Radiation Units ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Radiation weighting factor&lt;br /&gt;
X-rays	1&lt;br /&gt;
Gamma-rays	1&lt;br /&gt;
Electrons	1&lt;br /&gt;
Positrons	1&lt;br /&gt;
Protons &amp;gt; 2 MeV	2&lt;br /&gt;
Alpha particles	20&lt;br /&gt;
&lt;br /&gt;
The radiation-absorbed dose is the total energy absorbed by tissue. It is given in rad or Gray (Gy), 0.01 Gy = 1 rad. The equivalent dose is the absorbed dose multiplied by the radiation weighting factor, WR  and is given in roentgen-Equivalent-Man (rem) or Sievert (Sv), 0.01 Sv = 1 rem. The effective dose, E (Eq-1) is the sum of the tissue-weighted equivalent dose, WT multiplied by the equivalent dose, HT for all tissue types, T. It arises because the same equivalent dose of radiation has different biological effects on different tissues [1]. &lt;br /&gt;
E=∑_T▒〖H_T*W_T                         Eq-1〗&lt;br /&gt;
&lt;br /&gt;
== Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
The biological effects of ionising radiation are caused by the secondary electrons from an ionisation event, not the primary radiation beam [9]. These electrons deposit energy within tissues causing molecular damage and the formation of toxic chemical species. Although ionisation and free-radical production occur on a sub-second time scale, biological effects may take years to manifest. [10]. &lt;br /&gt;
&lt;br /&gt;
Free radicals such as hydroxyl (OH•) and hydrogen (H•) form when radiation interacts with water. Secondary and tertiary molecules including (O2•-) and hydrogen peroxide (H2O2) are then produced, and interact with endogenous nitrogen molecules such as nitric oxide (NO•) to produce reactive nitrogen species including nitrogen dioxide (NO2•) and peroxynitrite (ONOO-). These molecules may cause DNA damage, protein oxidation or lipid damage [2]. &lt;br /&gt;
 &lt;br /&gt;
Biological effects are classified as stochastic or deterministic. Stochastic effects are probabilistic: the likelihood of them developing increases with radiation dose. They are primarily caused by low-radiation doses and have no lower-bound threshold. Deterministic effects are dose-dependent: the severity of the biological effects increases with radiation dose; they have a lower-bound threshold and are primarily caused by high-dose radiation [1,11].&lt;br /&gt;
&lt;br /&gt;
== Biological Range ==&lt;br /&gt;
&lt;br /&gt;
Radiation type	Range in tissue&lt;br /&gt;
Auger electrons	0.02-10  μm [12]&lt;br /&gt;
Alpha	10-100 μm [13]&lt;br /&gt;
Beta	few mm-few cm [14]&lt;br /&gt;
Gamma	Many cm [14]&lt;br /&gt;
X-ray	&lt;br /&gt;
Neutron	&lt;br /&gt;
Table 3 - Range of radiation in tissue&lt;br /&gt;
Radiation with a large mass, high charge and/or low energy have the shortest range. &lt;br /&gt;
Different types of radiation have different ranges in tissue (Table 3). Short-range radiation is used therapeutically to target localised lesions as it transfers its’ energy to surrounding cells more effectively than long-range radiation. Long-range radiation is used in medical imaging. Short-range radiation is more biologically potent.  &lt;br /&gt;
&lt;br /&gt;
== Direct and Indirect Biological Effects ==&lt;br /&gt;
&lt;br /&gt;
Direct effects, following ionisation or atomic excitation, include the breakage of molecular bonds of DNA (deoxyribonucleic acid) or proteins, molecular degradation and intermolecular cross-linking. They occur within a picosecond of radiation exposure and are typically induced by high-LET radiation [2,15]. Indirect effects, due to low-LET radiation, occur over a longer period and are mediated by free radicals and reactive oxygen or nitrogen species [15]. The majority of DNA damage occurs due to indirect effects because water, the source of free radicals, contributes 70% of cellular composition [11]. However, direct DNA damage is more potent because radiation with a high-LET can induce multi-strand breaks [16]. Indirect effects may occur at a distance from the initial radiation site. In addition to DNA strand-breakages, base losses or changes also occur. &lt;br /&gt;
Non-irradiated cells may express radiation-induced biological effects secondary to the release of signals from directly-irradiated cells in their vicinity. This is termed the bystander effect and is distinct from the abscopal effect in which tumour cells distant from the primary radiation-site diminish in size. The latter is thought to be mediated by the immune system [17].&lt;br /&gt;
Although the number of DNA lesions is large for a given radiation dose (1000 single-strand breaks and 40 double-strand breaks per Gy [10]), the number of cell fatalities is low: most radiation-induced DNA changes are detected and repaired by enzymes. Persistent mutations can cause genetic and somatic effects, as well as cell death The consequence of an un-repaired mutation will depend, in part, on the biological function of the affected gene   [10].  &lt;br /&gt;
&lt;br /&gt;
== Cellular Radiosensitivity ==&lt;br /&gt;
&lt;br /&gt;
The radiosensitivity of a cell depends on several factors. First undifferentiated cells (those lacking a specific physiological role) are more radiosensitive than differentiated ones as the former give rise to the latter (Figure 2). Second, the stage of the cell cycle (G1, S, G2 and M): cells are least radiosensitive during the DNA replication (S-)phase because a large number of DNA repair molecules are present, and most radiosensitive during the (M)mitotic-stage. Third is the size of the nucleus: cells with larger nuclei are more radiosensitive. Fourth is the rate of the cell-cycle: cells that replicate more frequently are more radiosensitive as radiation-induced DNA damage is more likely to persist [11,18]. &lt;br /&gt;
&lt;br /&gt;
On a subcellular level, different organelles have different radiosensitivities: for example, both the cell membrane and nucleus are more radiosensitive than the cytoplasm [9,19].&lt;br /&gt;
&lt;br /&gt;
The effect of radiation on cells can be visualised on a cell-survival curve, which plots the proportion of cells that survive at a particular absorbed dose of radiation (Figure 3). &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The steepness of Figure 3b will increase in response to several factors including an elevated local cellular oxygen concentrations (as oxygen stabilises free radicals, prolonging their half-life) and radiation with a higher LET. The oxygen-enhancement ratio (OER) is the ratio of the radiation dose required to produce a particular biological effect in hypoxic cells, CH and oxygenated cells, CO; OER = CH/CO. Its value is ≈3 for low-LET radiation and ≈1 for high-LET radiation [10].&lt;br /&gt;
&lt;br /&gt;
== Chronic and Acute Effects ==&lt;br /&gt;
&lt;br /&gt;
Biological effects may be acute or chronic. Chronic effects arise following multiple low-dose radiation exposure events, primarily in slowly proliferating cells. The effects can be stochastic or deterministic and may manifest genetically (in future generations) or somatically (e.g: teratogenesis, reduced life expectancy); examples of deterministic effects along with their associated threshold-doses are given in Table 4. Stochastic effects include germ-cell mutations, and cancer: the likelihood of developing leukaemia or a solid cancer per 100 mSv is 1% [20].  &lt;br /&gt;
Biological effect	Chronic exposure	Total accumulated exposure threshold &lt;br /&gt;
Permanent sterility 	2-5 rad/week		250-300 rad&lt;br /&gt;
Cataract	¬---------	400 rad (over 2 months)&lt;br /&gt;
Radiation dermatitis	1-2 rad/day	2000 rad&lt;br /&gt;
Table 4 – Deterministic effects following a chronic exposure to radiation. For the effects to manifest, the accumulated dose over time must be, at least, equal to the threshold value given in the far-right column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
Acute effects arise shortly after exposure to a high radiation dose, primarily in rapidly proliferating cells, and include erythema, conjunctivitis and acute radiation sickness (ARS). Table 5 gives the acute radiation dose required to produce several different biological effects. ARS has a natural history that is divided into 4 stages (Fig.10). In the prodromal stage, non-specific symptoms such as nausea and vomiting arise. The latent phase may last several weeks. Haemopoetic symptoms such as prolonged coagulation time and a dampened immune response arise at 250-500 rad. Gastrointestinal effects including gut ulceration and loss of intestinal villi occur at 500-1000 rad. Neurovascular symptoms  include motor- and sensory-dysfunction, and reduced levels of consciousness develop at 5000-10,000 rad. Mild symptoms of ARS include fatigue, loss of appetite and sweating [11,21]. Figure 4 illustrates the consequences of, and relationship between the different components of ARS. &lt;br /&gt;
&lt;br /&gt;
Chronic exposures, per unit of radiation, are less biologically significant than acute exposures as the body is capable of repairing any damage incurred between exposure events [22].&lt;br /&gt;
&lt;br /&gt;
Biological effect	Acute threshold radiation dose&lt;br /&gt;
Generalised erythema (skin reddening) 	200-600 rad&lt;br /&gt;
Temporary hair loss	300-600 rad&lt;br /&gt;
Temporary sterility	50 rad&lt;br /&gt;
Permanent sterility	200-1000 rad (this effect is age dependent)&lt;br /&gt;
Cataract formation	200-700 rad&lt;br /&gt;
Vomiting 2 hours post-exposure	100-400 rad&lt;br /&gt;
Diarrhoea 1 hour post-exposure	600-800 rad&lt;br /&gt;
Headache 4 hours post-exposure 	600-800 rad&lt;br /&gt;
Fever 1 hour post-exposure 	400-600 rad&lt;br /&gt;
Table 5 – The threshold acute radiation doses for a variety of biological effects.&lt;br /&gt;
The biological effects highlighted in blue arise during the prodromal stage of ARS following an acute radiation threshold dose given in the right-hand column&lt;br /&gt;
&lt;br /&gt;
Data is obtained from: [1]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
# Bushberg JT, Seibert JA, Leidholdt EM, Boone JM. The Essential Physics of Medical Imaging. Lippincott Williams &amp;amp; Wilkins; 2011.&lt;br /&gt;
# Reisz JA, Bansal N, Qian J, Zhao W, Furdui CM. Effects of ionizing radiation on biological molecules--mechanisms of damage and emerging methods of detection. Antioxid Redox Signal 2014;21:260–92.&lt;br /&gt;
# ICRP. The 2007 Recommendations of the International Commission on Radiological Protection. ICRP publication 103. Ann ICRP 2007;37:1–332.&lt;br /&gt;
# Laney T, Kooy H. Proton and Charged Particle Radiotherapy. Lippincott Williams &amp;amp; Wilkins; 2008.&lt;br /&gt;
# V C on the BE of IRB, Sciences C on L, Studies D on E and L, Council NR. Health Effects of Exposure to Low Levels of Ionizing Radiation:: BEIR V. National Academies; 1990.&lt;br /&gt;
# International Atomic Energy Agency. Radiation Biology: A Handbook for Teachers and Students. IAEA; 2010.&lt;br /&gt;
# Dendy PP, Heaton B. Physics for Diagnostic Radiology, Third Edition. CRC Press; 1999.&lt;br /&gt;
# Howell RW, Narra VR, Sastry KS, Rao D V. On the equivalent dose for Auger electron emitters. Radiat Res 1993;134:71–8.&lt;br /&gt;
# Mayles P, Nahum A, Rosenwald J. Handbook of Radiotherapy Physics: Theory and Practice. vol. 8. CRC Press; 2007.&lt;br /&gt;
# Bailey D, Humm J, Todd-Pokropek A, Van-Aswegen A. Nuclear Medicine Physics: A Handbook for Teachers and Students. Vienna: International Atomic Energy Agency; 2014.&lt;br /&gt;
# Saha GB. Physics and Radiobiology of Nuclear Medicine. New York, NY: Springer New York; 2006.&lt;br /&gt;
# Welch MJ, Redvanly CS. Handbook of Radiopharmaceuticals: Radiochemistry and Applications. John Wiley &amp;amp; Sons; 2003.&lt;br /&gt;
# Hoskin PJ. Radiotherapy in Practice - Radioisotope Therapy. OUP Oxford; 2007.&lt;br /&gt;
# Australian Government - Department of Health. Ionising Radiation and Human Health 2012. http://www.health.gov.au/internet/publications/publishing.nsf/Content/ohp-radiological-toc~ohp-radiological-05-ionising (accessed November 22, 2015).&lt;br /&gt;
# Desouky O, Ding N, Zhou G. Targeted and non-targeted effects of ionizing radiation. J Radiat Res Appl Sci 2015;8:247–54.&lt;br /&gt;
# Powsner RA, Powsner ER. Essential Nuclear Medicine Physics. John Wiley &amp;amp; Sons; 2008.&lt;br /&gt;
# Multhoff G, Pockley A, Gaipl U, Rodel F. Radiation-induced effects and the immune system. Frontiers E-books; 2013.&lt;br /&gt;
# Bergonié J, Tribondeau L. Interpretation of Some Results of Radiotherapy and an Attempt at Determining a Logical Technique of Treatment / De Quelques Resultats de la Radiotherapie et Essai de Fixation d’une Technique Rationnelle. Radiat Res 1959;11:587–8.&lt;br /&gt;
# Pouget J-P, Santoro L, Raymond L, Chouin N, Bardiès M, Bascoul-Mollevi C, et al. Cell membrane is a more sensitive target than cytoplasm to dense ionization produced by auger electrons. Radiat Res 2008;170:192–200.&lt;br /&gt;
# Committee to Assess Health Risks from Exposure to Low Levels of Ionising radiation. Health Risks from Exposure to Low Levels of Ionizing Radiation:: BEIR VII Phase 2. National Academies Press; 2006.&lt;br /&gt;
# Campeau F, Fleitz J. Limited Radiography. Cengage Learning; 2009.&lt;br /&gt;
# Langland OE, Langlais RP, Preece JW. Principles of Dental Imaging. Lippincott Williams &amp;amp; Wilkins; 2002.&lt;br /&gt;
# World Nuclear Organisation. Nuclear Radiation and Health Effects 2015. http://www.world-nuclear.org/info/Safety-and-Security/Radiation-and-Health/Nuclear-Radiation-and-Health-Effects/ (accessed November 14, 2015).&lt;/div&gt;</summary>
		<author><name>JordanSilverman</name></author>
	</entry>
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