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Revision: 1.16
Committed: Tue Jul 15 09:37:08 2008 UTC (16 years, 9 months ago) by ymaravin
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Added Zg to the list of intrumental backgrounds

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# Content
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 are generated with the leading order (LO) event generators
6 {\sl PYTHIA}~\cite{Sjostrand:2003wg}, {\sl ALPGEN} and {\sl COMPHEP}.
7 To accommodate the next-to-leading (NLO) effects, constant $k$-factors are applied
8 except for the signal where a $p_T$-dependence has been taken into account
9 and some of the backgrounds, $e.g.$ $t\bar{t}$, $W+jets$, and $Z+jets$ samples,
10 officially produced with NLO effects taken into account.
11
12 The $p_T$-dependent $k$-factor for the signal is estimated using
13 the NLO cross section calculator {\sl MCFM}~\cite{Campbell:2005}.
14 We estimate the PDF uncertainty on the cross-section using
15 {\sl MC@NLO 3.1}~\cite{Frixione:2002ik} NLO event generator
16 together with CTEQ6M PDF set.
17
18 \subsection{Signal definition}
19 The goal of this analysis is to study the associative production of the on-shell
20 $\W$ and $\Z$ bosons that decay into three leptons and a neutrino. In the
21 following we refer to a lepton to as either a muon or an electron, unless
22 specified otherwise.
23
24 Using {\sl MCFM} we estimate the total NLO $\WZ$ cross-section to be
25 \begin{equation}
26 \sigma_{NLO} ( pp \rightarrow W^+\Z; \sqrt{s}=14~{\rm TeV}) = 30.5~{\rm pb},
27 \end{equation}
28 \begin{equation}
29 \sigma_{NLO} ( pp \rightarrow W^-\Z; \sqrt{s}=14~{\rm TeV}) = 19.1~{\rm pb}.
30 \end{equation}
31
32 The LO and NLO distributions of the \Z boson transverse momentum are
33 shown in Fig.~\ref{fig:LOvsNLO} with the case of $W^+$ on the left and $W^-$
34 on the right side. The NLO/LO ratio, $k$-factor, is also presented on the figure,
35 and it is increasing with $p_T(\Z)$. We take into account the $p_T$ dependence
36 by re-weighting the LO Monte Carlo simulation as a function of the $p_T(\Z)$.
37 %
38 %
39 %The $p_T$ dependence of the $k$-factor
40 %becomes important when a proper NLO description of the $\Z$ boson transverse
41 %momentum must be obtained, $e.g$ to measure the strength of the $WWZ$ coupling.
42 %As the focus of this analysis is to prepare for the cross-section measurement,
43 %we take a $p_{T}$-averaged value of the $k$-factor, equal to 1.84.
44
45 \begin{figure}[!bt]
46 \begin{center}
47 \scalebox{0.8}{\includegraphics{figs/LOvsNLOZPtWminuns.eps}\includegraphics{figs/LOvsNLOZPtWplus.eps}}
48 \caption{$p_T(Z)$ distribution for LO (solid black histogram) and NLO (dashed black histogram)
49 in $W^-\Z$ events (left) and $W^+\Z$ events (right). The ratio NLO/LO is also given as a red
50 solid line.
51 }
52 \label{fig:LOvsNLO}
53 \end{center}
54 \end{figure}
55
56 %# for bbll:
57 %#CS NLO ((Z/gamma*->l+l-)bb) = 830pb = 345 pb * 2.4, where:
58 %#- 345 pb is LO CS calculated with precision of ~0.15%
59 %#- 2.4 is MCMF calculated k-factor with precision ~30% (!)
60 %# 830x0.173 (== XS x eff.) = 143.59pb
61
62
63 \subsection{Signal and background Monte Carlo samples}
64
65 The signal Monte Carlo sample is produced using {\sl PYTHIA}
66 generator. The decay for the \W lepton is forced to $e\nu_e$,
67 $\mu\nu_{\mu}$ or $\tau\nu_{\tau}$ final state, while the \Z decays
68 into electrons or muons only.
69
70 The background to the \WZ final state can be divided in physics and
71 instrumental. The only physics background is from $Z^0Z^0$ production
72 where one of the leptons is either mis-reconstructed or lost.
73
74 The instrumental backgrounds are all due to mis-identified electron candidates
75 from either jets or photons. These backgrounds include production of $\W$ and $\Z$ bosons
76 with jets and $t\bar{t}$ processes and $Z^0\gamma$ process. The background from $W\gamma$
77 production, where the $\gamma$ converts and produces a dielectron system is neglected
78 due to a requirement on the $\ell^+\ell^-$ invariant mass to be consistent with the nominal \Z boson mass.
79
80 All non-negligible instrumental backgrounds are summarized below.
81 \begin{itemize}
82 \item $\Z + jets$: this background is one of the dominant to the \WZ final state. Although
83 the misidentification rate for a jet to be misidentified as a lepton is quite small, the
84 $\Z+jets$ cross-section is 35 times larger than the signal one. We use the {\sl ALPGEN}
85 generated official samples of $\Z+jet$ production Monte Carlo samples for different
86 values of the jet transverse momentum.
87 \item $t\bar{t}$: each of the top quarks decay into a $\W b$ pair producing at least two
88 leptons and two $b$-quark jets. Although this process does not have a genuine $\Z$
89 candidate and can be suppressed be a $\Z$ candidate invariant mass requirement,
90 the probability for a $b$-quark jet to decay semi-leptonically and be misidentified
91 as a lepton is higher than that from a light-quark jets. The cross-section of the $t\bar{t}$
92 production is also exceed by about 15 times the cross-section of the \WZ production.
93 Thus, this background is also one of the most dominant. We use the official $t\bar{t}$
94 samples produced with {\sl ALPGEN} generator to estimate this background.
95 \item $\Z + b\bar{b}$: this process is produced by the {\sl COMPHEP}
96 generator and have a genuine $\Z$ candidate in the final state. One of the $b$-quark
97 jets are misidentified as the third lepton from the $\W$ boson.
98 \item $\W+jets$: in this process, the \W boson produces a genuine lepton,
99 while the other two leptons are misidentified jets. As the misidentification
100 probability is low, this channel does not contribute significantly to the \WZ
101 final state. The additional \Z candidate invariant mass requirement suppresses
102 this background further. We use the officially produced sample of $\W+jets$ processes
103 for different number of jets in the final state generated by the {\sl ALPGEN}
104 generator.
105 \item $Z^0\gamma$: this process is calculated with {\sl PYTHIA}.
106 \end{itemize}
107
108 All the samples we use in this study are a part of the CSA07 production and
109 are generated using $\mathrm{CMSSW}\_1\_4_\_6$ using the full {\sl GEANT}
110 simulation of the CMS detector. The digitization and reconstruction are
111 done using a newer $\mathrm{CMSSW}\_1\_6_\_7$ release with a
112 misalignment/miscalibration of the detector scenario expected
113 to be achieved after collection of $\sim$ 100~pb$^{-1}$ of data.
114 All {\sl ALPGEN} samples are mixed together in further referred to as to a
115 ``Chowder soup''.
116
117 The summary of all datasets used for signal and background is given in
118 Table~\ref{tab:MC}. We use the RECO production level to access to
119 low-level detector information, such as reconstructed hits. This lets
120 us to use full granularity of the CMS sub-detectors to use isolation
121 discriminants.
122
123 Analysis of the samples is done using CMSSW$\_1\_6\_7$ CMS software
124 release. The information is stored in ROOT trees using a code in
125 CVS:/UserCode/Vuko/WZAnalysis, which is based on Physics Tools candidates.
126
127 \begin{table}[!tb]
128 %\begin{tabular}{llllll} \hline
129 %Sample & Generator & Sample name & Events & $\sigma \cdot \epsilon
130 %\cdot k$ & k-factor \\ \hline WZ & Pythia &
131 %/WZ/CMSSW\_1\_6\_7-CSA07-1195663763/RECO & 58897 & 0.585 pb & 1.92 \\
132 %$Zb\bar{b}$ & COMPHEP &
133 %/comphep-bbll/CMSSW\_1\_6\_7-CSA07-1198677426/RECO & 143.59 pb & 2.4
134 %\\ ``Chowder'' & ALPGEN &
135 %/CSA07AllEvents/CMSSW\_1\_6\_7-CSA07-Chowder-A1-PDAllEvents-ReReco-100pb/RECO
136 %& 25 M & event weights & - \\
137 \begin{tabular}{|c|c|c|c|c|} \hline
138 Sample & cross section, pb & Events & Dataset name \\ \hline
139 $\WZ$ & 1.12 & 59K & /WZ/CMSSW$\_1\_6\_7$-CSA07-1195663763\\ \hline
140 $\Z b\bar{b}$ & 830*0.173 (NLO) & 1.9M & /comphep-bbll/CMSSW$\_1\_6\_7$-CSA07-1198677426\\ \hline
141 Chowder & Event Weight & $\sim$ 21M & /CSA07AllEvents/\\ & & & CMSSW$\_1\_6\_7$-CSA07-Chowder-A1-PDAllEvents-ReReco
142 -100pb\\ \hline
143 $\Z\Z$ inclusive & 16.1 (NLO) & $\sim$ 140k & /ZZ$\_$incl/CMSSW$\_1\_6\_7$-CSA07-1194964234/RECO\\ \hline
144 $\Z\gamma \rightarrow e^+e^-\gamma$ & 1.08 (NLO) & $\sim$125k &/Zeegamma/CMSSW$\_1\_6\_7$-CSA07-1198935518/RECO \\ \hline
145 $\Z\gamma \rightarrow \mu^+\mu^-\gamma$ & 1.08 (NLO) & $\sim$ 93k & /Zmumugamma/CMSSW$\_1\_6\_7$-CSA07-1194806860/RECO\\ \hline
146 \end{tabular}
147 \label{tab:MC}
148 \caption{Monte Carlo samples used in this analysis using 100 pb$^{-1}$ scenario}
149 \end{table}
150
151
152
153