Proton Calorimetry/Meetings/2017/06/21: Difference between revisions

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Line 13: Line 13:
'''ABF''':
'''ABF''':
* Assembling photodiode circuit with Hamamatsu preamp.
* Assembling photodiode circuit with Hamamatsu preamp.
* Waiting on resistor value for preamp from Hamamatsu.


'''Suggestions needed for our Water Equivalent range telescope plastic scintillator detector.'''
'''Suggestions needed for our Water Equivalent range telescope plastic scintillator detector.'''


; SciRT : '''Sci'''ntillating '''R'''ange '''T'''elescope
; SciRT : '''Sci'''ntillating '''R'''ange '''T'''elescope

Latest revision as of 15:09, 21 June 2017

Minutes for UCL Proton Calorimetry Meeting, 21st June 2017 (D17, Physics & Astronomy, UCL)

Present

Simon Jolly, Laurent Kelleter, Anastasia Basharina-Freshville, Ruben Saakyan, Phil Allport

LK:

  • Looking further into nuclear build-up for energy variation:
    • Relative reduction becomes constant at beam energies above 200 MeV: "saturation".
    • RS suggests that nuclear interactions become important above 200 MeV: suggests to count numbers of all secondaries by species in the entrance region.
    • PA suggests using a liquid Hydrogen target to simplify the nuclear interactions.

ABF:

  • Assembling photodiode circuit with Hamamatsu preamp.
  • Waiting on resistor value for preamp from Hamamatsu.

Suggestions needed for our Water Equivalent range telescope plastic scintillator detector.

SciRT
Scintillating Range Telescope