1 |
vimartin |
1.3 |
%\clearpage
|
2 |
benhoob |
1.1 |
|
3 |
vimartin |
1.12 |
[MAJOR REWORKING OF TEXT: \\
|
4 |
|
|
ADD GENERAL INTRODUCTION - INCLUDING WHY USING CR HERE \\
|
5 |
|
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CONSISTENT VARIABLE NAMES \\
|
6 |
|
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ALSO FOR EACH CR CATEGORY, DESCRIBE PURPOSE, DEFINE SELECTION CLEARLY, EXPLAIN
|
7 |
|
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SFS AND CLOSURE TEST, CONCLUSIONS]
|
8 |
|
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|
9 |
benhoob |
1.1 |
|
10 |
vimartin |
1.3 |
The dominant background to the signal sample comes from \ttll\
|
11 |
vimartin |
1.4 |
events. Due to the presence of a second neutrino, \ttll\ events do
|
12 |
|
|
not have a kinematic edge at $\mt \sim \mW$. These events satisfy the
|
13 |
|
|
selection criteria due to real \met\ and do not depend on detector
|
14 |
|
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resolution or \met\ mis-measurement effects. As a result, the
|
15 |
|
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\ttll\ background is expected to be well modeled in the MC. The
|
16 |
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prediction for this background is thus derived from MC and normalized
|
17 |
vimartin |
1.12 |
to the data in the \mt\ peak region.
|
18 |
|
|
|
19 |
|
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%the modeling of the isolated track veto efficiency, which is
|
20 |
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% applied to explicitly reject leptons from \W\ and $\W\To\tau$ decays
|
21 |
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% and single prong $\tau$ decays.
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22 |
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|
23 |
fkw |
1.8 |
The systematic uncertainty associated with the MC prediction then has two components.
|
24 |
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One that is
|
25 |
|
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derived by comparing various generators, and a second from the uncertainties on
|
26 |
vimartin |
1.12 |
the various correction factors used.
|
27 |
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%The \ttll\ sample is checked for differences between data and MC in the isolation for events with a
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28 |
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%second lepton. This correction is derived using $\Z+4$ jet events and
|
29 |
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%applied to the \ttll\ sample.
|
30 |
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These are described in section XXX.
|
31 |
vimartin |
1.4 |
|
32 |
vimartin |
1.11 |
\subsubsection{Normalization of the Top Prediction}
|
33 |
fkw |
1.9 |
\label{sec:topnorm}
|
34 |
|
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|
35 |
|
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In this section we discuss the factor $ {N_{peak}^{data} \over N_{peak}^{MC}} $ in Equation XX.
|
36 |
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The same factor is applied to both the single and dilepton estimates.
|
37 |
vimartin |
1.4 |
|
38 |
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The overall normalization of the \ttbar\ sample is determined by
|
39 |
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scaling to the \mt\ peak control region, following a procedure similar
|
40 |
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to that described in Section.~\ref{sec:bkg_singlelep}. This control
|
41 |
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region is dominated by \ttbar\, albeit in its single lepton decay
|
42 |
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mode. The basic idea is that after adjusting the modeling of
|
43 |
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additional jets from radiation in the \ttll\ sample and correcting
|
44 |
|
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the leptonic branching fractions in the \ttbar\ sample, the MC
|
45 |
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prediction for the \ttlj\ and \ttll\ samples is subject to the same
|
46 |
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sources of uncertainty: the \ttbar\ cross section, the luminosity, the
|
47 |
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selection efficiencies, etc$\dots$ The exception is the veto on events
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containing an isolated track, since this last requirement has a different
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49 |
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impact on the \ttlj\ and \ttll\ samples. The impact of this
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requirement is addressed separately in Section.~\ref{sec:trkveto}.
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52 |
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The \mt-peak scale factor is thus determined after applying the full
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analysis selection with the exception of the isolated track veto.
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Specifically, the pre-veto sample is defined by the following requirements
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55 |
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\begin{itemize}
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\item At least 1 selected electron (muon) with \pt $>$ 30 GeV and $|\eta|<2.5$ ($|\eta|<2.1$)
|
57 |
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\item At least 4 selected jets, of which at least 1 is b-tagged
|
58 |
vimartin |
1.12 |
\item \met\ $>$ 100 GeV or corresponding SR requirement
|
59 |
vimartin |
1.4 |
\end{itemize}
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60 |
vimartin |
1.3 |
|
61 |
fkw |
1.9 |
%As in the case of the single lepton + jets sample,
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62 |
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Scaling the overall
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vimartin |
1.4 |
normalization to the \mt\ peak largely reduces the dependence on the
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\ttbar\ cross section and cancels systematic uncertainties associated
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65 |
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with effects such as the luminosity, selection efficiencies,
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66 |
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etc$\dots$ However, the \mt\ peak control sample is contaminated
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67 |
benhoob |
1.7 |
by non-\ttbar\ processes, particularly \wjets\ that contributes at
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68 |
vimartin |
1.4 |
the $5-10\%$ level, even after requiring a b-tagged jet. The \wjets+HF
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69 |
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process is a particular concern given the large theoretical
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70 |
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uncertainties associated with their production.
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71 |
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Therefore a systematic uncertainty is derived to account for
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72 |
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the uncertainty in this background component. The normalization of
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73 |
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the \wjets\ sample is scaled up and down by $50\%$ and the full
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74 |
vimartin |
1.11 |
background estimate recomputed.
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vimartin |
1.4 |
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76 |
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In conclusion, the pre-veto sample is used to define an overall data
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77 |
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over MC scale factor ($SF^{\rm{all}}$) in the \mt\ peak control region, that is
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78 |
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applied to all background predictions and is simply defined as
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79 |
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\begin{itemize}
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80 |
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\item $N_{\rm{peak}}^{\rm{all}}$ = data yield in the peak region $60<\mt<100$ GeV
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81 |
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\item $M_{\rm{peak}}^{\rm{all}}$ = MC yield in the peak region $60<\mt<100$ GeV
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82 |
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\item $SF^{\rm{all}} = N_{\rm{peak}}^{\rm{all}} / M_{\rm{peak}}^{\rm{all}}$
|
83 |
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\end{itemize}
|
84 |
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For all subsequent steps, the scale factor $SF^{\rm{all}}$ is applied to all MC contributions.
|
85 |
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|
86 |
vimartin |
1.11 |
\subsubsection{The Isolated Track Veto}
|
87 |
vimartin |
1.4 |
\label{sec:trkveto}
|
88 |
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|
89 |
fkw |
1.9 |
In this section we discuss the factors
|
90 |
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${(1- \epsilon_{fake})^{data} \over (1 - \epsilon_{fake})^{MC}} $
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91 |
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and
|
92 |
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${(1- \epsilon_{iso\ trk})^{data} \over (1 - \epsilon_{iso\ trk})^{MC}} $
|
93 |
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in Equation XXX.
|
94 |
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|
95 |
vimartin |
1.4 |
The \ttll\ background is further suppressed after the $4$-jet
|
96 |
fkw |
1.9 |
requirement by removing events with any isolated track with
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97 |
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$\pt>10~\GeV$.
|
98 |
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%
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99 |
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As isolation definition we use
|
100 |
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relative track isolation $\sum \pt/\pt(trk)$ in a cone of size $R=0.3<0.1$.
|
101 |
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%
|
102 |
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This isolated track veto rejects events with an
|
103 |
vimartin |
1.4 |
\E\ or a \M, as well as single-prong $\tau$-decays.
|
104 |
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This veto is very effective at reducing the dilepton background. In
|
105 |
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particular, according to the \ttll\ MC, the veto removes about
|
106 |
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three-quarters of events with an \E\ or \M\ from the \W\ decay and
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107 |
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almost half the leptonic and single prong $\tau$
|
108 |
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decays. The veto has no impact on multi-prong $\tau$s, though this is
|
109 |
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a smaller component overall. Since the \ttll\ background includes
|
110 |
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different types of processes, it is useful to first characterize the
|
111 |
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composition of this background.
|
112 |
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|
113 |
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\subsubsection{Top Dilepton Sample Composition}
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114 |
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|
115 |
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The \ttll\ background may be categorized based on the type of
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116 |
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second lepton, as shown in Table.~\ref{tab:ttdlcomposition}. The main
|
117 |
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component is from electrons and muons from a \W\ decay or through an
|
118 |
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intermediate $\tau$ decay. The second largest component arises from
|
119 |
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single-prong hadronic $\tau$ decays, followed by multi-prong
|
120 |
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$\tau$s. Finally an additional contribution arises from leptons
|
121 |
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falling in the forward region, outside the Tracker acceptance
|
122 |
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$|\eta|>2.5$ (refered to as `lost').
|
123 |
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|
124 |
|
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\begin{table}[!ht]
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125 |
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|
\begin{center}
|
126 |
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\begin{tabular}{l|c|c}
|
127 |
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\hline
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128 |
|
|
Sample & Yield & Fraction [\%]\\
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129 |
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|
\hline
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130 |
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\hline
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131 |
|
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$t\bar{t} \rightarrow l^{+}l^{-} (\mathrm{lost})$ & 7 $\pm$ 1 & 6\\
|
132 |
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$t\bar{t} \rightarrow l^{+}l^{-} (e/\mu)$ & 30 $\pm$ 3 & 26\\
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133 |
|
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$t\bar{t} \rightarrow l^{+}l^{-} (\tau_{\mathrm{lep}})$ & 21 $\pm$ 2 & 18\\
|
134 |
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$t\bar{t} \rightarrow l^{+}l^{-} (\tau_{\mathrm{had}}\rightarrow \mathrm{1-prong})$ & 39 $\pm$ 3 & 34\\
|
135 |
|
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$t\bar{t} \rightarrow l^{+}l^{-} (\tau_{\mathrm{had}}\rightarrow \mathrm{3-prong})$ & 19 $\pm$ 2 & 16\\
|
136 |
|
|
\hline
|
137 |
|
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total $t\bar{t} \rightarrow l^{+}l^{-} $ & 117 $\pm$ 5 & 100\\
|
138 |
|
|
\hline
|
139 |
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|
\end{tabular}
|
140 |
|
|
\caption{Dilepton events satisfying the full selection criteria
|
141 |
benhoob |
1.7 |
and \met\ $>$ 100 GeV, \mt\ $>$ 150 GeV, separated by decay modes.
|
142 |
vimartin |
1.12 |
Recall that \ttll\ accounts for $\approx80$\% of the total
|
143 |
|
|
background.{\bf Fix me: Is this before or after the isolated track
|
144 |
|
|
veto? This is after the isolated track veto, numbers derived at 7
|
145 |
|
|
TeV, to be udpdated to 8 TeV}
|
146 |
benhoob |
1.7 |
\label{tab:ttdlcomposition}}
|
147 |
vimartin |
1.4 |
\end{center}
|
148 |
|
|
\end{table}
|
149 |
|
|
|
150 |
|
|
The isolated track veto does not apply to the components where the
|
151 |
|
|
second lepton falls outside the acceptance or where it decays to a
|
152 |
|
|
hadronic tau that is not explicitly rejected. For the cases where the
|
153 |
|
|
second lepton includes an electron or muon or a charged $\pi/K$, it is
|
154 |
|
|
possible to further distinguish cases when the relevant particle
|
155 |
|
|
targeted by the veto is below the \pt\ threshold. Matching the
|
156 |
|
|
truth-level particle to reconstructed tracks shows that in \ttll\ MC
|
157 |
|
|
\begin{itemize}
|
158 |
|
|
\item for $t\bar{t} \rightarrow l^{+}l^{-} (e/\mu)$, about a third of
|
159 |
|
|
the sample falls below the \pt\ threshold of the track veto, and the remaining
|
160 |
|
|
two thirds fail the isolation
|
161 |
|
|
\item for $t\bar{t} \rightarrow l^{+}l^{-} (\tau_{\mathrm{lep}})$,
|
162 |
|
|
about $80\%$ are soft $\pt<10~\GeV$ and about $20\%$ are
|
163 |
|
|
non-isolated
|
164 |
|
|
\item for $t\bar{t} \rightarrow l^{+}l^{-}
|
165 |
|
|
(\tau_{\mathrm{had}}\rightarrow \mathrm{1-prong})$,
|
166 |
|
|
about $70\%$ are soft, as expected from a $\tau$ decay product and the
|
167 |
|
|
rest fail the isolation criteria.
|
168 |
|
|
\end{itemize}
|
169 |
|
|
In summary, the combination of these fractions with the relative sample
|
170 |
|
|
composition listed in Table.~\ref{tab:ttdlcomposition} shows that only
|
171 |
benhoob |
1.7 |
about a third of the \ttll\ background sample is from 2nd leptons (e, $\mu$, or $\tau\to$1-prong)
|
172 |
|
|
which satisfy \pt\ $>$ 10 GeV but fail the track isolation criterion
|
173 |
vimartin |
1.4 |
veto\footnote{Explicitly, the fraction of events that give rise to a
|
174 |
|
|
sufficiently energetic lepton or single prong $\tau$ is: $70\%$ of \E-\M\ events
|
175 |
|
|
which are $26\%$ of the sample, $20\%$ of leptonic tau events which
|
176 |
|
|
are $18\%$ of the sample and $30\%$ of single prong $\tau$ events
|
177 |
|
|
which are $10\%$ of the sample.}. The performance of the isolation
|
178 |
vimartin |
1.12 |
used in the track veto requirement is the subject of section XXX.
|
179 |
vimartin |
1.4 |
|
180 |
|
|
It should also be noted that according to the MC, track reconstruction
|
181 |
|
|
inefficiencies affect a few percent ($\sim 1-2\%$) of the
|
182 |
|
|
leptonic and single prong $\tau$ events. The tracking efficiency in
|
183 |
|
|
this analysis is taken from MC, which is expected to provide good modeling of isolated
|
184 |
|
|
tracks with $\pt>10~\GeV$. The impact of
|
185 |
|
|
possible differences between data and MC is found to be negligible.
|
186 |
|
|
In particular, the case of single-prong taus is the most challenging to
|
187 |
|
|
model due to the effect of nuclear interactions in the tracker material.
|
188 |
|
|
Past studies of the tracking efficiency for pions~\cite{TRK10002}
|
189 |
|
|
provide a data/MC uncertainty in the tracking efficiency of $3.9\%$\footnote{
|
190 |
|
|
This tracking efficiency uncertainty estimate is conservative for this
|
191 |
|
|
analysis since it includes tracks of \pt\ down to $250$ MeV, where
|
192 |
|
|
material effects are larger and so are the corresponding
|
193 |
|
|
uncertainties.}. Propagating this uncertainty to the total background
|
194 |
|
|
estimate yields a total uncertainty of $< 0.5\%$. The reason is that
|
195 |
|
|
the tracking efficiency uncertainty only applies to single prong
|
196 |
|
|
$\tau$ decays with $\pt> 10~\GeV$, which are under $30\%$ of the
|
197 |
|
|
dilepton component, which in turn is $\sim 80\%$ of the total sample.
|
198 |
|
|
|
199 |
|
|
To conclude, the \ttll\ background arises from events where the second
|
200 |
|
|
lepton falls outside the acceptance (both in $\eta$ and $\pt$),
|
201 |
|
|
because the event contains a hadronic tau that is not explicitly rejected or
|
202 |
|
|
because the second lepton fails the isolation requirement.
|
203 |
|
|
Even though the \ttll\ sample is quite heterogenous and comprises
|
204 |
|
|
multiple types of second lepton events, there are two
|
205 |
|
|
main sources of uncertainty in this estimate:
|
206 |
|
|
\begin{itemize}
|
207 |
|
|
\item Acceptance effects, which are estimated by using alternative MC
|
208 |
fkw |
1.9 |
samples. Here acceptance refers to the combination of $\eta$ and \pt of the leptons.
|
209 |
vimartin |
1.4 |
\item Detector effects, mainly arising from understanding the
|
210 |
|
|
performance of the isolated track veto, which impacts only about a
|
211 |
|
|
third of the total \ttll\ sample.
|
212 |
|
|
\end{itemize}
|
213 |
vimartin |
1.3 |
|
214 |
|
|
|
215 |
vimartin |
1.11 |
\subsubsection{Summary of the \ttdl\ Background Estimation Procedure}
|
216 |
benhoob |
1.10 |
|
217 |
vimartin |
1.12 |
[ADD CORRECT VARIABLE NAMES TO MATCH EQUATIONS, SHOULD HELP MAKE IT
|
218 |
|
|
EASIER TO FOLLOW]
|
219 |
|
|
|
220 |
vimartin |
1.11 |
The SM background in the signal region, defined by requirements of
|
221 |
|
|
large \met\ and \mt, is estimated using MC. The MC is validated using
|
222 |
|
|
data control samples, which are used to derive data-to-MC scale
|
223 |
|
|
factors and corresponding uncertainties.
|
224 |
benhoob |
1.10 |
|
225 |
vimartin |
1.11 |
The procedure to estimate the background prediction may be summarized
|
226 |
|
|
as
|
227 |
benhoob |
1.10 |
\begin{itemize}
|
228 |
vimartin |
1.11 |
\item Apply the state-of-the-art corrections to the MC, reflecting the
|
229 |
|
|
best knowlege of the detector performance, in order to improve the agreement
|
230 |
|
|
with the data. This includes effects such as the modeling of the pileup, the jet energy scale,
|
231 |
|
|
\met\ corrections, etc$\dots$
|
232 |
|
|
\item Correct the leptonic branching fractions in the \ttbar\ MC
|
233 |
|
|
\item Use the dilepton sample with two selected leptons to reweight
|
234 |
|
|
the \njets\ distribution in \ttll\ MC, which is not necessarily
|
235 |
|
|
well-modeled due to the presence of additional jets from radiation.
|
236 |
|
|
\item Use the pre-veto sample (i.e. applying the full analysis selection
|
237 |
|
|
with the exception of the isolated track veto) to define a scale
|
238 |
|
|
factor in the \mt\ peak region. This scale factor corrects for
|
239 |
|
|
effects of integrated luminosity, \ttbar\ cross section, lepton
|
240 |
|
|
selection and trigger efficiencies.
|
241 |
|
|
\item In the signal sample, after applying the full selection
|
242 |
|
|
including the isolated track veto, derive a scale factor to
|
243 |
|
|
account for possible data vs. MC discrepancies in the isolated track
|
244 |
|
|
fake rate for backgrounds which have a single genuine lepton. This
|
245 |
|
|
scale factor is applied to the single lepton backgrounds only.
|
246 |
|
|
\end{itemize}
|
247 |
benhoob |
1.10 |
|
248 |
|
|
|
249 |
vimartin |
1.11 |
\clearpage
|
250 |
benhoob |
1.10 |
|
251 |
vimartin |
1.11 |
\subsection{Check of MC modelling of \ttdl}
|
252 |
benhoob |
1.10 |
|
253 |
|
|
|
254 |
vimartin |
1.11 |
[EXPLAIN THE CROSS CHECKS DONE TO VALIDATE THE MC MODELLING OF \ttdl]
|
255 |
benhoob |
1.10 |
|
256 |
vimartin |
1.11 |
\subsubsection{Validation of the ``Physics'' Modelling of the \ttdl\ MC}
|
257 |
benhoob |
1.10 |
|
258 |
vimartin |
1.11 |
[EXPLAIN ALL THE CR4 2-lepton \ttdl\ SAMPLE ]
|
259 |
benhoob |
1.10 |
|
260 |
vimartin |
1.11 |
\begin{table}[!h]
|
261 |
benhoob |
1.10 |
\begin{center}
|
262 |
vimartin |
1.11 |
\begin{tabular}{l||c|c|c|c}
|
263 |
benhoob |
1.10 |
\hline
|
264 |
vimartin |
1.11 |
Sample & CR4A & CR4B & CR4C & CR4D \\
|
265 |
benhoob |
1.10 |
\hline
|
266 |
|
|
\hline
|
267 |
vimartin |
1.11 |
Muon Data/MC-SF & $0.91 \pm 0.04$ & $0.94 \pm 0.07$ & $1.06 \pm 0.13$ & $1.03 \pm 0.22$ \\
|
268 |
benhoob |
1.10 |
\hline
|
269 |
|
|
\hline
|
270 |
vimartin |
1.11 |
Electron Data/MC-SF & $0.95 \pm 0.04$ & $1.00 \pm 0.08$ & $0.85 \pm 0.12$ & $0.83 \pm 0.19$ \\
|
271 |
benhoob |
1.10 |
\hline
|
272 |
vimartin |
1.11 |
\end{tabular}
|
273 |
|
|
\caption{ Data/MC scale factors for total yields, applied to compare
|
274 |
|
|
the shapes of the distributions.
|
275 |
|
|
The uncertainties are statistical only.
|
276 |
|
|
\label{tab:cr4mtsf}}
|
277 |
|
|
\end{center}
|
278 |
|
|
\end{table}
|
279 |
|
|
|
280 |
|
|
|
281 |
|
|
\begin{table}[!h]
|
282 |
|
|
\begin{center}
|
283 |
|
|
\begin{tabular}{l||c|c|c|c}
|
284 |
benhoob |
1.10 |
\hline
|
285 |
vimartin |
1.11 |
Sample & CR4A & CR4B & CR4C & CR4D \\
|
286 |
benhoob |
1.10 |
\hline
|
287 |
|
|
\hline
|
288 |
vimartin |
1.11 |
Muon MC & $199 \pm 7$ & $102 \pm 6$ & $29 \pm 3$ & $8 \pm 1$ \\
|
289 |
|
|
Muon Data & $187$ & $108$ & $34$ & $9$ \\
|
290 |
benhoob |
1.10 |
\hline
|
291 |
vimartin |
1.11 |
Muon Data/MC SF & $0.94 \pm 0.08$ & $1.06 \pm 0.12$ & $1.17 \pm 0.23$ & $1.09 \pm 0.40$ \\
|
292 |
benhoob |
1.10 |
\hline
|
293 |
|
|
\hline
|
294 |
vimartin |
1.11 |
Electron MC & $203 \pm 8$ & $97 \pm 5$ & $26 \pm 2$ & $8 \pm 1$ \\
|
295 |
|
|
Electron Data & $201$ & $102$ & $25$ & $5$ \\
|
296 |
benhoob |
1.10 |
\hline
|
297 |
vimartin |
1.11 |
Electron Data/MC SF & $0.99 \pm 0.08$ & $1.06 \pm 0.12$ & $0.97 \pm 0.21$ & $0.60 \pm 0.29$ \\
|
298 |
benhoob |
1.10 |
\hline
|
299 |
vimartin |
1.11 |
\end{tabular}
|
300 |
|
|
\caption{ Yields in \mt\ tail comparing the MC prediction (after
|
301 |
|
|
applying SFs) to data. The uncertainties are statistical only.
|
302 |
|
|
\label{tab:cr4yields}}
|
303 |
|
|
\end{center}
|
304 |
|
|
\end{table}
|
305 |
|
|
|
306 |
|
|
\begin{figure}[hbt]
|
307 |
|
|
\begin{center}
|
308 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/met_met50_leadmuo_nj4.pdf}%
|
309 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/met_met50_leadele_nj4.pdf}
|
310 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met100_leadmuo_nj4.pdf}%
|
311 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met100_leadele_nj4.pdf}
|
312 |
|
|
\caption{
|
313 |
|
|
Comparison of the \met\ (top) and \mt\ for $\met>100$ (bottom) distributions in data vs. MC for events
|
314 |
|
|
with a leading muon (left) and leading electron (right)
|
315 |
|
|
satisfying the requirements of CR4.
|
316 |
|
|
\label{fig:cr4met}
|
317 |
|
|
}
|
318 |
|
|
\end{center}
|
319 |
|
|
\end{figure}
|
320 |
|
|
|
321 |
|
|
\begin{figure}[hbt]
|
322 |
|
|
\begin{center}
|
323 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met150_leadmuo_nj4.pdf}%
|
324 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met150_leadele_nj4.pdf}
|
325 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met200_leadmuo_nj4.pdf}%
|
326 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met200_leadele_nj4.pdf}
|
327 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met250_leadmuo_nj4.pdf}%
|
328 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR4plots/mt_met250_leadele_nj4.pdf}
|
329 |
|
|
\caption{
|
330 |
|
|
Comparison of the \mt\ distribution in data vs. MC for events
|
331 |
|
|
with a leading muon (left) and leading electron (right)
|
332 |
|
|
satisfying the requirements of CR4. The \met\ requirements used are
|
333 |
|
|
150 GeV (top), 200 GeV (middle) and 250 GeV (bottom).
|
334 |
|
|
\label{fig:cr4mtrest}
|
335 |
|
|
}
|
336 |
|
|
\end{center}
|
337 |
|
|
\end{figure}
|
338 |
|
|
|
339 |
|
|
|
340 |
|
|
\clearpage
|
341 |
|
|
|
342 |
vimartin |
1.12 |
\subsubsection{Validation of the lepton + isolated track Sample
|
343 |
|
|
Prediction [FIX NAME]}
|
344 |
vimartin |
1.11 |
|
345 |
|
|
[EXPLAIN ALL THE CHECKS FOR CR5: LEPTON + ISOLATED TRACK SAMPLE]
|
346 |
|
|
|
347 |
|
|
[ALSO NEED BETTER TITLE FOR THIS SECTION!]
|
348 |
|
|
|
349 |
|
|
\begin{table}[!h]
|
350 |
|
|
\begin{center}
|
351 |
|
|
\begin{tabular}{l||c|c|c|c}
|
352 |
benhoob |
1.10 |
\hline
|
353 |
vimartin |
1.11 |
Sample & CR5A & CR5B & CR5C & CR5D \\
|
354 |
benhoob |
1.10 |
\hline
|
355 |
|
|
\hline
|
356 |
vimartin |
1.11 |
Muon pre-veto \mt-SF & $0.98 \pm 0.02$ & $0.95 \pm 0.04$ & $0.99 \pm 0.08$ & $0.89 \pm 0.15$ \\
|
357 |
|
|
Muon post-veto \mt-SF & $1.28 \pm 0.07$ & $1.20 \pm 0.13$ & $1.22 \pm 0.24$ & $1.25 \pm 0.43$ \\
|
358 |
benhoob |
1.10 |
\hline
|
359 |
|
|
\hline
|
360 |
vimartin |
1.11 |
Electron pre-veto \mt-SF & $0.83 \pm 0.02$ & $0.75 \pm 0.04$ & $0.64 \pm 0.07$ & $0.63 \pm 0.12$ \\
|
361 |
|
|
Electron post-veto \mt-SF & $1.10 \pm 0.08$ & $1.02 \pm 0.11$ & $0.89 \pm 0.19$ & $1.27 \pm 0.41$ \\
|
362 |
benhoob |
1.10 |
\hline
|
363 |
vimartin |
1.11 |
\end{tabular}
|
364 |
|
|
\caption{ \mt\ peak Data/MC scale factors. The pre-veto SFs are applied to the
|
365 |
|
|
\ttdl\ sample, while the post-veto SFs are applied to the single
|
366 |
|
|
lepton samples. The raw MC is used for backgrounds from rare processes.
|
367 |
|
|
The uncertainties are statistical only.
|
368 |
|
|
\label{tab:cr5mtsf}}
|
369 |
|
|
\end{center}
|
370 |
|
|
\end{table}
|
371 |
|
|
|
372 |
|
|
|
373 |
|
|
\begin{table}[!h]
|
374 |
|
|
\begin{center}
|
375 |
|
|
\begin{tabular}{l||c|c|c|c}
|
376 |
benhoob |
1.10 |
\hline
|
377 |
vimartin |
1.11 |
Sample & CR5A & CR5B & CR5C & CR5D \\
|
378 |
benhoob |
1.10 |
\hline
|
379 |
|
|
\hline
|
380 |
vimartin |
1.11 |
Muon MC & $293 \pm 9$ & $161 \pm 7$ & $51 \pm 4$ & $16 \pm 2$ \\
|
381 |
|
|
Muon Data & $315$ & $165$ & $62$ & $13$ \\
|
382 |
benhoob |
1.10 |
\hline
|
383 |
vimartin |
1.11 |
Muon Data/MC SF & $1.07 \pm 0.07$ & $1.03 \pm 0.09$ & $1.21 \pm 0.18$ & $0.82 \pm 0.25$ \\
|
384 |
benhoob |
1.10 |
\hline
|
385 |
|
|
\hline
|
386 |
vimartin |
1.11 |
Electron MC & $253 \pm 8$ & $126 \pm 5$ & $37 \pm 3$ & $12 \pm 2$ \\
|
387 |
|
|
Electron Data & $286$ & $135$ & $39$ & $15$ \\
|
388 |
benhoob |
1.10 |
\hline
|
389 |
vimartin |
1.11 |
Electron Data/MC SF & $1.13 \pm 0.08$ & $1.07 \pm 0.10$ & $1.07 \pm 0.19$ & $1.21 \pm 0.35$ \\
|
390 |
benhoob |
1.10 |
\hline
|
391 |
|
|
\end{tabular}
|
392 |
vimartin |
1.11 |
\caption{ Yields in \mt\ tail comparing the MC prediction (after
|
393 |
|
|
applying SFs) to data. The uncertainties are statistical only.
|
394 |
|
|
\label{tab:cr5yields}}
|
395 |
benhoob |
1.10 |
\end{center}
|
396 |
|
|
\end{table}
|
397 |
|
|
|
398 |
vimartin |
1.11 |
\begin{figure}[hbt]
|
399 |
|
|
\begin{center}
|
400 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/met_met50_leadmuo_nj4.pdf}%
|
401 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/met_met50_leadele_nj4.pdf}
|
402 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met100_leadmuo_nj4.pdf}%
|
403 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met100_leadele_nj4.pdf}
|
404 |
|
|
\caption{
|
405 |
|
|
Comparison of the \met\ (top) and \mt\ for $\met>100$ (bottom) distributions in data vs. MC for events
|
406 |
|
|
with a leading muon (left) and leading electron (right)
|
407 |
|
|
satisfying the requirements of CR5.
|
408 |
|
|
\label{fig:cr5met}
|
409 |
|
|
}
|
410 |
|
|
\end{center}
|
411 |
|
|
\end{figure}
|
412 |
vimartin |
1.5 |
|
413 |
|
|
\begin{figure}[hbt]
|
414 |
|
|
\begin{center}
|
415 |
vimartin |
1.11 |
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met150_leadmuo_nj4.pdf}%
|
416 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met150_leadele_nj4.pdf}
|
417 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met200_leadmuo_nj4.pdf}%
|
418 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met200_leadele_nj4.pdf}
|
419 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met250_leadmuo_nj4.pdf}%
|
420 |
|
|
\includegraphics[width=0.5\linewidth]{plots/CR5plots/mt_met250_leadele_nj4.pdf}
|
421 |
|
|
\caption{
|
422 |
|
|
Comparison of the \mt\ distribution in data vs. MC for events
|
423 |
|
|
with a leading muon (left) and leading electron (right)
|
424 |
|
|
satisfying the requirements of CR5. The \met\ requirements used are
|
425 |
|
|
150 GeV (top), 200 GeV (middle) and 250 GeV (bottom).
|
426 |
|
|
\label{fig:cr5mtrest}
|
427 |
|
|
}
|
428 |
vimartin |
1.5 |
\end{center}
|
429 |
|
|
\end{figure}
|
430 |
|
|
|
431 |
|
|
|
432 |
|
|
|
433 |
|
|
|
434 |
vimartin |
1.2 |
|
435 |
|
|
|
436 |
benhoob |
1.1 |
|