Generator level study of gamma +MET using Sherpa
description
Transcript of Generator level study of gamma +MET using Sherpa
28th March, 2009 India-CMS meeting, Delhi 1
Generator level study of gamma +MET using
Sherpa
Sandhya Jain
Satyaki Bhattacharya
University of Delhi, Delhi
28th March, 2009 India-CMS meeting, Delhi 2
Introduction In 1998, Large extra dimension (LED) were proposed as a solution to hierarchy
problem by ADD.
It builds up saying that gravity can propagate in extra dimensions giving rise to
a relation given as, Mpl^2 = Md^(n+2) * R ^n
where, R is the size of compactified Extra-Dimension,
Md and n are the parameters of the theory.
Gravitational field in extra-dimensions is carried by a particle called graviton
whose signatures can be found at LHC.
For a direct graviton production, MET becomes a signature.
So, I am interested in looking for + MET as the signal for the direct graviton
production at LHC.
28th March, 2009 India-CMS meeting, Delhi 3
Sherpa- A Monte Carlo Event Generator
produces events that are qualified to be put into detector
simulations used by various experiments.
versatile to inbuilt matrix element and phase space generator
AMEGIC ++ & PHASIC ++ which calculate and integrate tree
level amplitudes. This feature makes Sherpa to be used as cross
section integrator and parton level event generator as well.
provides the implementation of CKKW merging, which provides
the improved description of multi jet production processes .
28th March, 2009 India-CMS meeting, Delhi 4
Feynman Diagrams contributing at tree level
q q
q q
28th March, 2009 India-CMS meeting, Delhi 5
Cross-section Vs n at Md = 2TeV
As n increases, the x-section decreases.
28th March, 2009 India-CMS meeting, Delhi 6
28th March, 2009 India-CMS meeting, Delhi 7
Cuts used
pt of > 100 GeV
Md = 1TeV, 2TeV
Ecms = 10.0 TeV
CMSSW 2_2_4 is being used for this studies.
28th March, 2009 India-CMS meeting, Delhi 8
Graviton Distributions
Energy Distribution (Md = 1TeV) Energy Distribution (Md = 2TeV)
28th March, 2009 India-CMS meeting, Delhi 9
Pt Distribution (2TeV)Pt Distribution (1TeV)
28th March, 2009 India-CMS meeting, Delhi 10
Pl Distribution (1 TeV) Pl Distribution (2 TeV)
28th March, 2009 India-CMS meeting, Delhi 11
Mass Distribution (1TeV) Mass Distribution (2TeV)
28th March, 2009 India-CMS meeting, Delhi 12
Eta distribution(1TeV) Eta distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 13
Phi distribution(1TeV) Phi distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 14
Photon Distributions
Energy distribution(1TeV) Energy distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 15
Pt distribution(1TeV) Pt distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 16
Pl distribution(1TeV) Pl distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 17
Eta distribution(2Tev)Eta distribution(1TeV)
28th March, 2009 India-CMS meeting, Delhi 18
Phi distribution(1TeV) Phi distribution(2TeV)
28th March, 2009 India-CMS meeting, Delhi 19
Photon pl / graviton pl(1TeV) Photon pl / graviton pl(2TeV)
28th March, 2009 India-CMS meeting, Delhi 20
Photon pt / graviton pt(2TeV)Photon pt / graviton pt(1TeV)
28th March, 2009 India-CMS meeting, Delhi 21
delta phi (1TeV) delta phi (2TeV)
28th March, 2009 India-CMS meeting, Delhi 22
cos(theta) (1TeV) cos(theta) (2TeV)
28th March, 2009 India-CMS meeting, Delhi 23
Summary & Future Plans Till the time of last meeting, I was looking at the photon
reconstruction at CMS using CMSSW (keeping in mind a search with
photon in the final state).
I have just started looking at the generator level plots of MET+
gamma (signal).
I have presented my initial results with CMSSW_2_1_10 in the QCD
photons group while at CERN in January.
As my next step, I would like to do a study of Z gamma at generator
level where Z -> bar, which is a background to this process.
Then, would like to proceed with the simulation and reconstruction.