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Revision: 1.12
Committed: Fri Jun 27 13:16:33 2008 UTC (16 years, 10 months ago) by beaucero
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Branch: MAIN
Changes since 1.11: +6 -3 lines
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# User Rev Content
1 vuko 1.1 \section{Signal and Background Modeling}
2     \label{sec:gen}
3     \subsection{Monte Carlo generators}
4     The signal and background samples for the full detector simulation
5 vuko 1.11 are generated with the leading order (LO) event generators
6 ymaravin 1.9 {\sl PYTHIA}~\cite{Sjostrand:2003wg}, {\sl ALPGEN} and {\sl COMPHEP}.
7     To accommodate next-to-leading (NLO) effects, constant $k$-factors are applied.
8     Additionally, the cross section calculator {\sl MCFM}~\cite{Campbell:2005}
9     is used to determine the NLO differential cross section for the $\WZ$
10     production. To estimate the uncertainty on the cross-section
11     due to the choice of the PDF, we use NLO event generator
12     {\sl MC@NLO 3.1}~\cite{Frixione:2002ik} together with CTEQ6M PDF set.
13    
14     \subsection{Signal definition}
15    
16     The goal of this analysis is to study the associative production of the on-shell
17     $W$ and $\Z$ bosons that decay into three leptons and a neutrino. In the
18     following we refer to a lepton to as either a muon or an electron, unless
19     specified otherwise. The leptonic final state $\ell^+ \ell^- \ell^\pm \nu$ also receives a
20     contribution from the $W\gamma^*$ production, where the $\gamma^*$ stands for a
21     virtual photon through the $WW\gamma$ vertex. In this analysis, we
22 ymaravin 1.10 restrict this contribution by requiring the $\ell^+\ell^-$ invariant mass to be
23 ymaravin 1.9 consistent with the nominal $\Z$ boson mass. As CMS detector has a very
24     good energy resolution for electrons and muons, the mass window
25     is set to be $\pm$ 10 GeV around 91 GeV.
26    
27 ymaravin 1.10 Using {\sl MCFM} we estimate the total NLO $\WZ$ cross-section to be
28 beaucero 1.5 \begin{equation}
29 ymaravin 1.10 \sigma_{NLO} ( pp \rightarrow W^+\Z; \sqrt{s}=14~{\rm TeV}) = 30.5~{\rm pb},
30 beaucero 1.5 \end{equation}
31     \begin{equation}
32 ymaravin 1.10 \sigma_{NLO} ( pp \rightarrow W^-\Z; \sqrt{s}=14~{\rm TeV}) = 19.1~{\rm pb}.
33 beaucero 1.5 \end{equation}
34    
35 ymaravin 1.10 The LO and NLO distributions of the \Z boson transverse momentum are
36     shown in Fig.~\ref{fig:LOvsNLO} with the case of $W^+$ on the left and $W^-$
37     on the right side. The NLO/LO ratio, $k$-factor, is also presented on the figure,
38     and it is increasing with $p_T(\Z)$. The $p_T$ dependence of the $k$-factor
39     becomes important when a proper NLO description of the $\Z$ boson transverse
40     momentum must be obtained, $e.g$ to measure the strength of the $WWZ$ coupling.
41     As the focus of this analysis is to prepare for the cross-section measurement,
42     we take a $p_{T}$-averaged value of the $k$-factor, equal to 1.84.
43 beaucero 1.5
44     \begin{figure}[!bt]
45     \begin{center}
46     \scalebox{0.8}{\includegraphics{figs/LOvsNLOZPtWminuns.eps}\includegraphics{figs/LOvsNLOZPtWplus.eps}}
47 ymaravin 1.10 \caption{$p_T(Z)$ distribution for LO (solid black histogram) and NLO (dashed black histogram)
48     in $W^-\Z$ events (left) and $W^+\Z$ events (right). The ratio NLO/LO is also given as a red
49     solid line.
50 beaucero 1.5 }
51     \label{fig:LOvsNLO}
52     \end{center}
53     \end{figure}
54 vuko 1.1
55 vuko 1.2 %# for bbll:
56     %#CS NLO ((Z/gamma*->l+l-)bb) = 830pb = 345 pb * 2.4, where:
57     %#- 345 pb is LO CS calculated with precision of ~0.15%
58     %#- 2.4 is MCMF calculated k-factor with precision ~30% (!)
59     %# 830x0.173 (== XS x eff.) = 143.59pb
60    
61    
62 ymaravin 1.10 \subsection{Signal and background Monte Carlo samples}
63    
64     The signal Monte Carlo sample is produced using {\sl PYTHIA}
65 vuko 1.11 generator. The decay for the \W has been forced to $e\nu_e$,
66     $\mu\nu_{\mu}$ or $\tau\nu_{\tau}$ final state, while the \Z decays
67 ymaravin 1.10 into electrons or muons only.
68 beaucero 1.6
69 ymaravin 1.10 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
70     % YM changes implemented up to here
71 beaucero 1.6 The main background that we have to consider are all final states
72     having at least two isolated leptons from the same flavor and with
73     opposite charge. The third one can be a real isolated lepton or a misidentified
74     lepton. The probability to misidentify one isolated lepton is rather low, so
75 beaucero 1.7 this is why we can considerer safely starting from two
76 beaucero 1.6 leptons. Moreover we will apply a cut on the invariant mass of the two
77 beaucero 1.7 isolated leptons so most of the background that we have to study are:\\
78 beaucero 1.6 \begin{itemize}
79 vuko 1.11 \item $W+jets$: $W$ boson will give us one isolated leptons. The probability that 2 additional jets will be misidentified as isolated lepton is very low and the criteria on the lepton invariant mass will definitely reduce such background. This channel is nevertheless useful to study other background for which data sample are not available such as $Wb\bar{b}$. The sample studied for this analysis, has been produced using ALPGEN generator per jet multiplicity bin.
80 beaucero 1.7 \item $Z + jets$: $Z$ boson is common between signal and background. The third isolated lepton can come from a misidentified lepton. The cross section of production of this channel is around 35 time greater than the signal.The sample studied for this analysis, has been produced using ALPGEN generator per jet bin.
81     \item $t\bar{t}$: top quark will decay to \W$b$ pair where each $W$ can decay via an isolated leptons. This leptons will have opposite charged. Even though combining the two leptons, we will not obtain a peak around the \Z mass, the cross section of this process is around 15 time the cross section of the signal. The sample studied for this analysis, has been produced using ALPGEN generator per jet bin. The third lepton will come from a semi leptonic decay of a $b$ quark which will be isolated.
82     \item $Z + b\bar{b}$: the presence of $Z$ boson will select such events. Moreover due to the semi leptonic decay of a $b$ quark, a third lepton can be easily identified and consider as isolated. The sample used has been produced by COMPHEP generator.
83 beaucero 1.12 \item $ZZ$: the inclusive cross section production is smaller than the signal studied but due to branching fraction and if we consider $Z\rightarrow b\bar{b}$ decay, some events can pass the analysis selection. This process has be
84     en produced using PYTHIA generator.
85     \item $Z\gamma$: TO BE ADDED
86 beaucero 1.6 \end{itemize}
87 beaucero 1.5
88 beaucero 1.7 All the different sample studied are part of the CSA07 production and
89 vuko 1.11 have been generated using $\mathrm{CMSSW}\_1\_4_\_6$ and went through the full
90 beaucero 1.7 GEANT simulation of the CMS detector using the same release. The
91 vuko 1.11 digitization and reconstruction have been done using $\mathrm{CMSSW}\_1\_6_\_7$
92 beaucero 1.7 release with a misalignment/miscalibration of the detector expected
93     after 100~pb$^{-1}$ of data. All ALPGEN samples are mixed together in
94     ``Chowder soup''.
95    
96     The summary of all datasets used for signal and background is given in
97     table~\ref{tab:MC}. We use the RECO production level to access to
98     low-level detector information, such as reconstructed hits. This lets
99     us to use full granularity of the CMS sub-detectors to use a isolation
100     discriminants.
101    
102     Analysis of the samples is done using CMSSW$\_1\_6\_7$ CMS software release.
103     The information is stored in ROOT trees using a code in
104     CVS:/UserCode/Vuko/WZAnalysis, which is based on Physics Tools candidates.
105    
106     \begin{table}[!tb]
107     %\begin{tabular}{llllll} \hline
108     %Sample & Generator & Sample name & Events & $\sigma \cdot \epsilon
109     %\cdot k$ & k-factor \\ \hline WZ & Pythia &
110     %/WZ/CMSSW\_1\_6\_7-CSA07-1195663763/RECO & 58897 & 0.585 pb & 1.92 \\
111     %$Zb\bar{b}$ & COMPHEP &
112     %/comphep-bbll/CMSSW\_1\_6\_7-CSA07-1198677426/RECO & 143.59 pb & 2.4
113     %\\ ``Chowder'' & ALPGEN &
114     %/CSA07AllEvents/CMSSW\_1\_6\_7-CSA07-Chowder-A1-PDAllEvents-ReReco-100pb/RECO
115     %& 25 M & event weights & - \\
116     \begin{tabular}{|c|c|c|c|c|} \hline
117     Sample & cross section [pb] & Events & Dataset name \\ \hline
118     $WZ$ & 1.12 & 59K & /WZ/CMSSW$\_1\_6\_7$-CSA07-1195663763\\ \hline
119     $Z b\bar{b}$ & 830*0.173 (NLO) & 1.9M & /comphep-bbll/CMSSW$\_1\_6\_7$-CSA07-1198677426\\ \hline
120     Chowder & Event Weight & $\sim$ 21M & /CSA07AllEvents/\\ & & & CMSSW$\_1\_6\_7$-CSA07-Chowder-A1-PDAllEvents-ReReco
121     -100pb\\ \hline
122 beaucero 1.12 $ZZ$ inclusif & 16.1 (NLO) & $\sim$ 140k & /ZZ$\_$incl/CMSSW$\_1\_6\_7$-CSA07-1194964234/RECO\\ \hline
123     $Z\gamma \rightarrow e^+e^-\gamma$ & 1.08 (NLO) & $\sim$125k &/Zeegamma/CMSSW$\_1\_6\_7$-CSA07-1198935518/RECO \\ \hline
124     $Z\gamma \rightarrow \mu^+\mu^-\gamma$ & 1.08 (NLO) & $\sim$ 93k & /Zmumugamma/CMSSW$\_1\_6\_7$-CSA07-1194806860/RECO\\ \hline
125 vuko 1.2 \end{tabular}
126 beaucero 1.7 \label{tab:MC}
127 vuko 1.2 \caption{Monte Carlo samples used in this analysis}
128     \end{table}
129    
130 vuko 1.1
131    
132