WW scattering in ATLAS.
This page is probably in the wrong place but as far as I can tell it can be moved later.
Our goal is measure WW scattering vs CM energy from threshold down to as
low as possible.
We had a meeting on 29 September 2005 and this was the start of a workplan.
Work Plan
ATLAS note
Sarah has pretty much finished this except:
- The AtlFast data was lost in a disk crash, but can be regenerated. Simon Head will be asked regenerate it. This should be without pileup, since the pileup is unofficial/undocumented, and not a big effect anyway. We can just make a comment in the text. ACTION Sarah and Simon
- Text to be checked and finalised ACTION Jon, Brian and Sarah
Infrastructure
- Make accounts at Manchester for code sharing ACTION Brian and Jon
- Archive code from note and paper. ACTION Sarah, Jon
- We want a shared code repository which allows us to to co-develop in reasonable privacy but also allows the checked out version to build/link against the ATLAS code. Action: Pete
Action: Jon set up mailing list at UCL. Ok, this means ask Gordon to do it...
Theory
We need to check that we are generating W+W-, W+W+. We would also
like to generate WZ and ZZ.
We would also like to cross check with the Montreal code.
ACTION Brian and Jeff.
Trigger
(FLT, HLT, offline selection)
Document which trigger chains the signal should get through etc here.
ACTION Stathes
Selection cuts
Action: Sarah to document what she actually does in the full sim analysis
Hadronic W mass resolution
pile up, jet finder dependence.
subjet cuts
cal granularity?
How to run it practically - produce an ATHENA algorithm
which takes a jet (AOD?) and produces a y cut array.
Action: Pete
electron
muon
missing ET
top mass resolution
pileup and jet finder dependence
This works in
AtlFast & at hadron level. Not yet working in full simulation.
tag jets
how well are they modelled?
how well is the rate known?
How can it be checked?
hard pt
how well is it modelled?
can it be checked?
minijet veto
is it really useful?
how well is it understood?
use new underlying event models/tunes.
background generation
what samples do we need? which generators?
we need W+jet and ttbar samples with a ptmin of about 250
GeV. However,
to get decent luminosity will require a lot of CPU so we should put this in
as a standing request to the SM and exotics groups, but not sweat about generating it
ourselves just yet - there is a lot of work to do on the signal.
detector simulation
how much with
AtlFast, how much needs full simulation?
Signal Generation
Sarah and Stathes can both generate signal with the modified pythia routine.
Continuum is the best default but we can look at other scenrios too.
We'd also like some high PT hadronic Ws Foundation samples
Action: Sarah to ask SM and Exo convenors
Maybe we should we aim for someone to give a talk at next UK SM meeting (November 30).
--
JonButterworth - 29 Sep 2005