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Committed: Mon Dec 13 03:09:17 2010 UTC (14 years, 4 months ago) by dbarge
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updated responses & resolutions in limits section, lines 429-425

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# Content
1 \section{Limit on new physics}
2 \label{sec:limit}
3
4 %{\bf \color{red} The numbers in this Section need to be double checked.}
5
6 As discussed in Section~\ref{sec:results}, we see one event
7 in the signal region, defined as SumJetPt$>$300 GeV and
8 \met/$\sqrt{\rm SumJetPt}>8.5$ GeV$^{\frac{1}{2}}$.
9
10 The background prediction from the SM Monte Carlo is 1.3 events.
11 %, where the uncertainty comes from
12 %the jet energy scale (30\%, see Section~\ref{sec:systematics}),
13 %the luminosity (10\%), and the lepton/trigger
14 %efficiency (10\%)\footnote{Other uncertainties associated with
15 %the modeling of $t\bar{t}$ in MadGraph have not been evaluated.
16 %The uncertainty on $pp \to \sigma(t\bar{t})$ is also not included.}.
17 The data driven background predictions from the ABCD method
18 and the $P_T(\ell\ell)$ method are $1.3 \pm 0.8({\rm stat}) \pm 0.3({\rm syst})$
19 and $2.1 \pm 2.1({\rm stat}) \pm 0.6({\rm syst})$, respectively.
20
21 These three predictions are in good agreement with each other
22 and with the observation of one event in the signal region.
23 We calculate a Bayesian 95\% CL upper limit\cite{ref:bayes.f}
24 on the number of non SM events in the signal region to be 4.1.
25 We have also calculated this limit using a profile likelihood method
26 as implemented in the cl95cms software, and we also find 4.1.
27 These limits were calculated using a background prediction of $N_{BG} = 1.4 \pm 0.8$
28 events, the error-weighted average of the ABCD and $P_T(\ell\ell)$ background
29 predictions. The upper limit is not very sensitive to the choice of
30 $N_{BG}$ and its uncertainty.
31
32 To get a feeling for the sensitivity of this search to some
33 popular SUSY models, we remind the reader of the number of expected
34 LM0 and LM1 events from Table~\ref{tab:sigcont}: $8.6 \pm 1.6$
35 events and $3.6 \pm 0.5$ events respectively, where the uncertainties
36 are from energy scale (Section~\ref{sec:systematics}), luminosity,
37 and lepton efficiency.
38
39 We also performed a scan of the mSUGRA parameter space. We set $\tan\beta=10$,
40 sign of $\mu = +$, $A_{0}=0$~GeV, and scan the $m_{0}$ and $m_{1/2}$ parameters
41 in steps of 10~GeV. For each scan point, we exclude the point if the expected
42 yield in the signal region exceeds 4.7, which is the 95\% CL upper limit
43 based on an expected background of $N_{BG}=1.4 \pm 0.8$ and a 20\% acceptance
44 uncertainty. The results are shown in Fig.~\ref{fig:msugra}.
45
46 \begin{figure}[tbh]
47 \begin{center}
48 \includegraphics[width=0.6\linewidth]{msugra.png}
49 \caption{\label{fig:msugra}\protect Exclusion curve in the mSUGRA parameter space,
50 assuming $\tan\beta=10$, sign of $\mu = +$ and $A_{0}=0$~GeVs.}
51 \end{center}
52 \end{figure}
53
54
55 Conveying additional useful information about the results of
56 a generic ``signature-based'' search such as the one described
57 in this note is a difficult issue. The next paragraph represent
58 our attempt at doing so.
59
60 Other models of new physics in the dilepton final state
61 can be confronted in an approximate way by simple
62 generator-level studies that
63 compare the expected number of events in 34.0~pb$^{-1}$
64 with our upper limit of 4.1 events. The key ingredients
65 of such studies are the kinematical cuts described
66 in this note, the lepton efficiencies, and the detector
67 responses for SumJetPt and \met/$\sqrt{\rm SumJetPt}$.
68 {LOOKING AT THE 38X MC PLOTS BY EYE, THE FOLLOWING QUANTITIES LOOK ABOUT RIGHT.}
69 The muon identification efficiency is $\approx 95\%$;
70 the electron identification efficiency varies from $\approx$ 63\% at
71 $P_T = 10$ GeV to 91\% for $P_T > 30$ GeV. The isolation
72 efficiency in top events varies from $\approx 83\%$ (muons)
73 and $\approx 89\%$ (electrons) at $P_T=10$ GeV to
74 $\approx 95\%$ for $P_T>60$ GeV. {\bf \color{red} The}
75 {\bf \color{red} following numbers were derived from Fall 10 samples. }
76 The average detector
77 responses for SumJetPt and $\met/\sqrt{\rm SumJetPt}$ are
78 $1.00 \pm 0.05$ and $0.96 \pm 0.05$ respectively, where
79 the uncertainties are from the jet energy scale uncertainty.
80 The experimental resolutions on these quantities are 11\% and
81 16\% respectively.
82
83 To justify the statements in the previous paragraph
84 about the detector responses, we plot
85 in Figure~\ref{fig:response} the average response for
86 SumJetPt and \met/$\sqrt{\rm SumJetPt}$ in MC, as well as the
87 efficiency for the cuts on these quantities used in defining the
88 signal region.
89 % (SumJetPt $>$ 300 GeV and \met/$\sqrt{\rm SumJetPt} > 8.5$
90 % Gev$^{\frac{1}{2}}$).
91 {\bf \color{red} The following numbers were derived from Fall10 samples }
92 We find that the average SumJetPt response
93 in the Monte Carlo is very close to one, with an RMS of order 11\% while
94 the response of \met/$\sqrt{\rm SumJetPt}$ is approximately 0.96 with an
95 RMS of 16\%.
96
97 %Using this information as well as the kinematical
98 %cuts described in Section~\ref{sec:eventSel} and the lepton efficiencies
99 %of Figures~\ref{fig:effttbar}, one should be able to confront
100 %any existing or future model via a relatively simple generator
101 %level study by comparing the expected number of events in 35 pb$^{-1}$
102 %with our upper limit of 4.1 events.
103
104 \begin{figure}[tbh]
105 \begin{center}
106 \includegraphics[width=\linewidth]{selectionEffDec10.png}
107 \caption{\label{fig:response} Left plots: the efficiencies
108 as a function of the true quantities for the SumJetPt (top) and
109 tcMET/$\sqrt{\rm SumJetPt}$ (bottom) requirements for the signal
110 region as a function of their true values. The value of the
111 cuts is indicated by the vertical line.
112 Right plots: The average response and its RMS for the SumJetPt
113 (top) and tcMET/$\sqrt{\rm SumJetPt}$ (bottom) measurements.
114 The response is defined as the ratio of the reconstructed quantity
115 to the true quantity in MC. These plots are done using the LM0
116 Monte Carlo, but they are not expected to depend strongly on
117 the underlying physics.
118 {\bf \color{red} These plots were made with Fall10 samples. } }
119 \end{center}
120 \end{figure}
121
122
123
124 %%% Nominal
125 % -----------------------------------------
126 % observed events 1
127 % relative error on acceptance 0.000
128 % expected background 1.400
129 % absolute error on background 0.770
130 % desired confidence level 0.95
131 % integration upper limit 30.00
132 % integration step size 0.0100
133 % -----------------------------------------
134 % Are the above correct? y
135 % 1 16.685 0.29375E-06
136 %
137 % limit: less than 4.112 signal events
138
139
140
141 %%% Add 20% acceptance uncertainty based on LM0
142 % -----------------------------------------
143 % observed events 1
144 % relative error on acceptance 0.200
145 % expected background 1.400
146 % absolute error on background 0.770
147 % desired confidence level 0.95
148 % integration upper limit 30.00
149 % integration step size 0.0100
150 % -----------------------------------------
151 % Are the above correct? y
152 % 1 29.995 0.50457E-06
153 %
154 % limit: less than 4.689 signal events