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2   \label{sec:gen}
3   \subsection{Monte Carlo generators}
4   The signal and background samples for the full detector simulation
5 < were generated with the leading order event generator PYTHIA~\cite{Sjostrand:2003wg}. To
6 < accomodate NLO effect constant k-factors were applied.
7 < Additionally the cross section calculator MCFM~\cite{Campbell:2005} was used to determine
8 < the next-to-leading order differential cross section for the WZ
9 < production process.  To estimate the PDF uncertainty for the signal
10 < process at NLO the NLO event generator MC@NLO 3.1~\cite{Frixione:2002ik} together with PDF set
11 < CTEQ6M was used.
12 <
13 < \subsection{Signal Definition}
14 <
15 < This analysis is studying the final state of on-shell $W$ and $Z$
16 < boson, both of them decaying leptonically. The fully final leptonic
17 < final state $l^+ l^- l^\pm \nu$ also receives a contribution from the
18 < $W\gamma *$ process, where the $\gamma *$ stands for a virtual photon
19 < through the $WW\gamma$ vertex. In this analysis, only events with $l^+
20 < l^-$ invariant mass consistent with $Z$ mass will be considered.
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:
# Line 26 | Line 60 | l^-$ invariant mass consistent with $Z$
60   %# 830x0.173 (== XS x eff.) = 143.59pb
61  
62  
63 < \begin{table}[tbh]
30 < \begin{tabular}{llllll} \hline
31 < Sample  & Generator   &  Sample name      & Events & $\sigma \cdot \epsilon \cdot k$ & k-factor \\ \hline
32 < WZ      & Pythia      & /WZ/CMSSW\_1\_6\_7-CSA07-1195663763/RECO   & 58897  &   0.585 pb    & 1.92 \\
33 < $Zb\bar{b}$   & COMPHEP &  /comphep-bbll/CMSSW\_1\_6\_7-CSA07-1198677426/RECO & 143.59 pb   & 2.4  \\
34 < ``Chowder'' & ALPGEN &  /CSA07AllEvents/CMSSW\_1\_6\_7-CSA07-Chowder-A1-PDAllEvents-ReReco-100pb/RECO     & 25 M & event weights & - \\
35 < \hline
36 < \end{tabular}
63 > \subsection{Signal and background Monte Carlo samples}
64  
65 < \caption{Monte Carlo samples used in this analysis}
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  
41 \subsection{Signal and Background Monte Carlo samples}
42
151  
152  
153  

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