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1   \section{Limits on New Physics}
2   \label{sec:limit}
3  
4 < %As discussed in Section~\ref{sec:results}, we see one event
5 < %in the signal region.
6 < %The background prediction from the SM MC is
7 < %1.3 events.
8 < %The data driven background predictions from the ABCD method
9 < %and the $\pt(\ell\ell)$ method are $1.3 \pm 0.8({\rm stat}) \pm 0.3({\rm syst})$ and
10 < %$2.1 \pm 2.1({\rm stat}) \pm 0.6({\rm syst})$ events, respectively.
4 > We first set an upper limit on the signal yield extracted by the fit to the dilepton mass
5 > distribution, assuming the LM1 shape. The 95\% confidence level (CL) upper limit (UL)
6 > is extracted using a profile likelihood technique, giving an UL of X events. The expected
7 > LM1 yield is X $\pm$ X events; hence LM1 is excluded by these results.
8 >
9 > We proceed to set upper limits on the non-SM contributions to the high \MET\ and high \Ht\ signal regions.
10 > For both regions, we find reasonable agreement between the observed yields and the predictions from MC and from the 2
11 > data-driven methods. We choose here to extract the upper limits using the MC prediction for the
12 > background estimate. The 95\% CL upper limit is extracted using a Bayesian technique~\cite{ref:cl95cms},
13 > using a log-normal model of nuissance parameter integration. The results are summarized in
14 > Table~\ref{tab:results}. Based on these results, we exclude LM1.
15  
16 < %These three predictions are in good agreement with each other
13 < %and with the observation of one event in the signal region.
14 < %We calculate a Bayesian 95\% CL upper limit~\cite{ref:cl95cms}
15 < %on the number of non SM events in the signal region to be 4.1,
16 < %using a background prediction of $N_\textrm{BG}=1.4 \pm 0.8$
17 < %events and a Gaussian model of nuissance parameter integration.  
18 < %The upper limit is not very sensitive to $N_\textrm{BG}$ and its uncertainty.
19 <
20 <
21 < The three background predictions for the high-\pt\ lepton trigger search
22 < discussed in Section~\ref{sec:results} are in good agreement with each other and
23 < with the observation of one event in the signal region.
24 < A Bayesian 95\%~confidence level (CL) upper limit~\cite{ref:cl95cms}  on the number of
25 < non-SM events in the signal region is determined to be 4.0,
26 < using a background prediction of $N_\textrm{BG} = 1.4 \pm 0.8$
27 < events and a log-normal model of nuisance parameter integration.
28 < The upper limit is not very sensitive to $N_\textrm{BG}$ and its uncertainty.
29 < This generic upper limit is not corrected for the possibility
30 < of signal contamination in the control regions. This is justified because
31 < the two independent background estimation methods based on data agree
32 < and are also consistent with the SM MC prediction.
33 < Moreover,  no evidence for non-SM contributions in
34 < the control regions is observed (Table~\ref{tab:datayield} and Figure~\ref{fig:victory}).
35 < This bound rules out the benchmark SUSY scenario LM0, for which the
36 < number of expected signal events is $8.6 \pm 1.6$, while the LM1 scenario predicts
37 < $3.6 \pm 0.5$ events.
38 < The uncertainties in the LM0 and LM1 event yields arise from energy scale, luminosity,
39 < and lepton efficiency, as discussed in Section~\ref{sec:systematics}.
40 <
41 < For the same-flavour search using hadronic activity triggers discussed in Section~\ref{sec:HT},
42 < no same-flavour events are observed and the corresponding Bayesian 95\% CL upper limit on the
43 < non-SM yield is 3.0 events.
44 < This bound rules out the benchmark SUSY scenarios LM0 and LM1, for which the
45 < numbers of expected signal events are $7.3 \pm 1.6$ and $3.6 \pm 0.7$, respectively.
46 <
47 < %As an example of the sensitivity of this search, we
48 < %remind the reader that the number of expected signal events in the benchmark
49 < %SUSY scenarios LM0 and LM1 are $8.6 \pm 1.6$ and $3.6 \pm 0.5$, respectively,
50 < %where the uncertainties are from energy scale, luminosity, and lepton efficiency.
51 <
52 <
53 < %Following text on CMSSM scan taken from RA1 paper
54 < We also quote the result more generally in the context of the CMSSM.
55 < The Bayesian 95\% CL limit  in the  $(m_0,m_{1/2})$ plane,  for $\tan\beta=3$,
56 < $A_0 = 0$ and $\mu > 0$ is shown in Figure~\ref{fig:msugra}.
57 < The high-\pt\ lepton and hadronic trigger searches have similar sensitivity to the CMSSM;
58 < here we choose to show results based on the high-\pt\ lepton trigger search. The
59 < SUSY particle  spectrum is calculated using  SoftSUSY~\cite{Allanach:2002uq}, and the
60 < signal  events  are  generated  at  leading  order  (LO)  with  \PYTHIA6.4.22.
61 < NLO  cross sections,  obtained  with the
62 < program  Prospino~\cite{Beenakker:1997kx},  are used  to  calculate  the observed
63 < exclusion  contour.  
64 < At each point in the  $(m_0,m_{1/2})$ plane, the acceptance uncertainty is calculated by
65 < summing in quadrature the uncertainties from jet and \MET\ energy scale using the
66 < procedure discussed in Section~\ref{sec:systematics}, the uncertainty in the
67 < NLO cross section due to the choice of factorization and renormalization scale,
68 < and the uncertainty from the parton distribution function (PDF) for CTEQ6.6~\cite{Nadolsky:2008fk},
69 < estimated from  the  envelope  provided  by  the  CTEQ6.6  error sets.
70 < The luminosity uncertainty and dilepton
71 < selection efficiency uncertainty are also included, giving a total relative acceptance uncertainty which varies
72 < in the range 0.2--0.3.
73 < %We consider a point excluded if the NLO yield exceeds the 95\% CL Bayesian upper limit
74 < %calculated with this acceptance uncertainty, using a log-normal model for the nuisance
75 < %parameter integration.
76 < A point is considered to be excluded if the NLO yield exceeds the 95\% CL
77 < Bayesian upper limit calculated with this acceptance uncertainty, using
78 < a log-normal model for the nuisance parameter integration.
79 < The limit curves do not include the effect of signal
80 < contamination in the control regions.  We have verified that this
81 < has a negligible impact on the excluded regions in Figure~\ref{fig:msugra}.
82 <
83 < \begin{figure}[tbh]
16 > \begin{table}[hbt]
17   \begin{center}
18 < \includegraphics[width=1\linewidth]{plots_final/RA6_ExclusionLimit_tanb3_LO.pdf}
19 < \caption{\label{fig:msugra}\protect
87 < %Text taken from RA1 paper
88 < The observed 95\% CL exclusion contour at NLO (solid red line) and LO (dashed blue line)
89 < in the CMSSM $(m_0,m_{1/2})$ plane for  $\tan\beta=3$, $A_0 = 0$ and $\mu > 0$.
90 < The area below the curve is excluded by this measurement. Exclusion limits obtained from
91 < previous experiments are presented as filled areas in the plot. Thin grey lines correspond to
92 < constant squark and gluino masses.
93 < %The plot also shows the two benchmark points LM0 and LM1 for comparison.
94 < %Exclusion curve in the CMSSM parameter space,
95 < %assuming $\tan\beta=3$, sign of $\mu = +$ and $A_{0}=0\GeVcc$.
18 > \caption{\label{tab:results}
19 > Summary of the observed and predicted yields in the 2 signal regions. MC errors are statistical only.
20   }
21 + \begin{tabular}{|l|c|c|c}
22 + \hline
23 +                                       &     high \met\ signal region             &  high \Ht\ signal region              \\
24 + \hline
25 + Observed yield                         &                          4               &                        3              \\
26 + \hline
27 + MC prediction                          &              2.6 $\pm$ 0.8               &            2.5 $\pm$ 0.8              \\
28 + ABCD' prediction                       &   1.2 $\pm$ 0.4 (stat) $\pm$ 0.5 (syst)  & 0.0 $\pm$ 0.6 (stat) $\pm$ 0.3 (syst) \\
29 + \ptll\ prediction                      &   5.4 $\pm$ 3.8 (stat) $\pm$ 2.2 (syst)  & 1.7 $\pm$ 1.7 (stat) $\pm$ 0.6 (syst) \\
30 + non-SM yield UL                        &                 5.2                      &               4.1                     \\
31 + LM1 yield                              &                17 $\pm$ 3.1              &             14 $\pm$ 3.1              \\
32 + LM3 yield                              &               4.3 $\pm$ 0.9              &            4.3 $\pm$ 1.0              \\
33 + \hline
34 + OF subtraction ($\Delta$)              &   1.3 $\pm$ 1.9 (stat) $\pm$ 0.1 (syst)  & 0.1 $\pm$ 1.5 (stat) $\pm$ 0.0 (syst) \\
35 + \hline
36 + \end{tabular}
37   \end{center}
38 < \end{figure}
99 <
100 < The excluded regions  for the CDF
101 < search for  jets + missing  energy final states~\cite{PhysRevLett.102.121801} were
102 < obtained for $\tan\beta=5$, while those from D0~\cite{Abazov2008449} were obtained for
103 < $\tan\beta=3$, each with  approximately  2~fb$^{-1}$ of  data and for $\mu < 0$.
104 < The  LEP-excluded
105 < regions  are based  on searches  for  sleptons and  charginos~\cite{LEPSUSY}.  
106 < %A comparison of the exclusion limit for tan b = 3 to that for tan b = 10
107 < %for fixed values of A0 =  0 and sign(m) > 0 indicates that
108 < %the exclusion  reach is only weakly  dependent on the value  of tan b;
109 < %the limit shifts  by less than 20\GeV  in m0 and by less  than 10\GeV in
110 < %m1/2.
111 < The D0 exclusion limit, valid for $\tan\beta=3$  and obtained from
112 < a  search  for  associated  production   of  charginos $\chi_{1}^{\pm}$ and
113 < neutralinos $\chi_2^0$ in  trilepton final states~\cite{Abazov200934}, is also
114 < included  in Figure~\ref{fig:msugra}. In  contrast to  the other  limits  presented in
115 < Figure~\ref{fig:msugra},  the results of our search and of the  trilepton search are  strongly dependent on
116 < the choice  of $\tan\beta$ and  they reach the  highest sensitivity  in the
117 < CMSSM for $\tan\beta$ values below 10.
118 <
119 < %We also performed a scan of the CMSSM parameter space. We set $\tan\beta=3$,
120 < %sign of $\mu = +$, $A_{0}=0\GeVcc$, and scan the $m_{0}$ and $m_{1/2}$ parameters
121 < %in steps of 10\GeVcc. At each point we calculate the acceptance uncertainty by
122 < %summing in quadrature the uncertainties from jet and \MET\ energy scale using the
123 < %procedure discussed in Section~\ref{sec:systematics} ($2-21$\%), the uncertainty in the
124 < %NLO cross-section assessed by varying the factorization and renormalization scale
125 < %by a factor of 2 ($12-15$\%), and the uncertainty from the parton density function (PDF)
126 < %assessed by () ($X-X$\%). We also include the luminosity uncertainty (11\%) and dilepton
127 < %selection efficiency uncertainty (5\%), giving a total acceptance uncertainty of $X-X$\%.
128 < %For each scan point, we calculate a 95\% CL upper limit using a Bayesian technique
129 < %using the observed signal yield (1 event), the acceptance uncertainty as calculated above, and
130 < %the predicted background yield and uncertainty $N_\textrm{BG}=1.4 \pm 0.8$. The point is considered
131 < %excluded if the NLO event yield exceeds this upper limit. The results are shown in Figure~\ref{fig:msugra}.
132 <
38 > \end{table}

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