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Revision: 1.5
Committed: Fri Jun 20 13:43:34 2008 UTC (16 years, 10 months ago) by beaucero
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Branch: MAIN
Changes since 1.4: +33 -2 lines
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Steph Modif

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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 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. CMS
21 detector have a very good energy resolution for electrons and muons,
22 the mass windows will be $\pm 10$ GeV around 91 GeV.
23
24 Using MCFM to estimate the total NLO cross section, we found:
25 \begin{equation}
26 \sigma_{NLO} ( pp \rightarrow W^+Z^0; \sqrt{s}=14TeV) = 30.5 pb
27 \end{equation}
28 \begin{equation}
29 \sigma_{NLO} ( pp \rightarrow W^-Z^0; \sqrt{s}=14TeV) = 19.1 pb
30 \end{equation}
31
32 The LO and NLO distribution of \Z transverse momentum are shown of
33 figure~\ref{fig:LOvsNLO} for the case of $W^+$ on the left and $W^-$
34 on the right side. The ratio NLO/LO is also presented on the figure
35 and it is increasing as $P_T(Z)$ increased. In the following analysis
36 we consider a constant $k-factor$ of 1.84 as we concentrate on the
37 first data taking. On the other side, if in the future one wants to
38 use such distribution to study the effect of possible anomalous triple
39 gauge couplings, it will be necessary to take the $p_T$ dependance of
40 this $k-factor$ into account.
41
42 \begin{figure}[!bt]
43 \begin{center}
44 \scalebox{0.8}{\includegraphics{figs/LOvsNLOZPtWminuns.eps}\includegraphics{figs/LOvsNLOZPtWplus.eps}}
45 \caption{$P_T(Z)$ in $W^-Z$ events on the left and $W^+Z$ events on the right
46 distribution for LO and NLO calculation. The ratio NLO/LO is also given.
47 }
48 \label{fig:LOvsNLO}
49 \end{center}
50 \end{figure}
51
52 %# for bbll:
53 %#CS NLO ((Z/gamma*->l+l-)bb) = 830pb = 345 pb * 2.4, where:
54 %#- 345 pb is LO CS calculated with precision of ~0.15%
55 %#- 2.4 is MCMF calculated k-factor with precision ~30% (!)
56 %# 830x0.173 (== XS x eff.) = 143.59pb
57
58
59 \subsection{Signal and Background Monte Carlo samples}
60
61 \begin{table}[tbh]
62 \begin{tabular}{llllll} \hline
63 Sample & Generator & Sample name & Events & $\sigma \cdot \epsilon \cdot k$ & k-factor \\ \hline
64 WZ & Pythia & /WZ/CMSSW\_1\_6\_7-CSA07-1195663763/RECO & 58897 & 0.585 pb & 1.92 \\
65 $Zb\bar{b}$ & COMPHEP & /comphep-bbll/CMSSW\_1\_6\_7-CSA07-1198677426/RECO & 143.59 pb & 2.4 \\
66 ``Chowder'' & ALPGEN & /CSA07AllEvents/CMSSW\_1\_6\_7-CSA07-Chowder-A1-PDAllEvents-ReReco-100pb/RECO & 25 M & event weights & - \\
67 \hline
68 \end{tabular}
69
70 \caption{Monte Carlo samples used in this analysis}
71 \end{table}
72
73
74
75