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# Content
1
2 \section{Introduction}
3
4 In this note we describe a search for new physics in the 2011
5 opposite sign isolated dilepton sample ($ee$, $e\mu$, and $\mu\mu$).
6 The main sources of high \pt isolated dileptons at CMS are Drell Yan and \ttbar.
7 Here we concentrate on dileptons with invariant mass consistent
8 with $Z \to ee$ and $Z \to \mu\mu$. A separate search for new physics in the non-\Z
9 sample is described in~\cite{ref:GenericOS}.
10
11 We search for new physics in the final state of \Z plus two or more jets plus missing
12 transverse energy (MET). We reconstruct the \Z boson
13 in its decay to $e^+e^-$ or $\mu^+\mu^-$. Our search regions are defined as
14 MET $\ge$ \signalmetl~GeV (loose signal region) and MET $\ge$ \signalmett~GeV
15 (tight signal region), and two or more jets. We use data driven techniques to predict the
16 standard model background in these search regions.
17 Contributions from Drell-Yan production combined with detector mis-measurements that
18 produce fake MET are modeled via MET templates based on photon plus jets or QCD events.
19 Top pair production backgrounds, as well as other backgrounds for which the lepton
20 flavors are uncorrelated such as WW and DY$\rightarrow\tau\tau$, are
21 modeled via $e^\pm\mu^\mp$ subtraction.
22
23 As leptonically decaying \Z bosons are a signature that has very little background,
24 they provide a clean final state in which to search for new physics.
25 Because new physics is expected to be connected to the Standard Model Electroweak sector,
26 it is likely that new particles will couple to W and Z bosons.
27 For example, in mSUGRA, low $M_{1/2}$ can lead to a significant branching fraction
28 for $\chi_2^0 \rightarrow Z \chi_1^0$.
29 In addition, we are motivated by the existence of dark matter to search for new physics with MET.
30 Enhanced MET is a feature of many new physics scenarios, and R-parity conserving SUSY
31 again provides a popular example. The main challenge of this search is therefore to
32 understand the tail of the fake MET distribution in \Z plus jets events.
33
34 The basic idea of the MET template method~\cite{ref:templates1}\cite{ref:templates2} is
35 to measure the MET distribution in data in a control sample which has no true MET
36 and a similar topology to the signal events.
37 %Start the qcd vs photon discussion
38 Templates can be derived from either a QCD sample (as was done in the original implementation)
39 or a photon plus jets sample.
40 %In our case, we choose a photon sample with two or more jets as the control sample.
41 %Both the control sample and signal sample consist of a well measured object (either a
42 %photon or a leptonically decaying $Z$), which recoils against a system of hadronic jets.
43 In both cases, the instrumental MET is dominated by mismeasurements of the hadronic system,
44 and can be classified by the number of jets in the event and the scalar sum of their transverse
45 momenta.
46 The prediction is made such that the jet system in the control sample is similar to that of the
47 signal sample.
48 By using two independent control samples--QCD and photon plus jets--we are able to illustrate
49 the robustness of the MET templates method and to cross check the data driven background
50 prediction.
51
52 This note is organized as follows.
53 In sections \ref{sec:datasets} and \ref{sec:trigSel} we descibe
54 the datasets and triggers used, followed by the detailed object definitions (electrons, muons, photons,
55 jets, MET) and event selections in sections \ref{sec:evtsel} through \ref{sec:jetsel}.
56 We define a preselection and compare data vs. MC yields passing this preselection in
57 Section~\ref{sec:yields}.
58 We then define the signal regions and show the number of observed events and MC expected
59 yields in Section~\ref{sec:sigregion}.
60 Section~\ref{sec:templates} introduces the MET template method and discusses its derivation
61 in some detail and is followed by a demonstration in Section~\ref{sec:mc}
62 that the method works in Monte Carlo.
63 Section~\ref{sec:topbkg} introduces the top background estimate based on opposite flavor subtraction,
64 and contributions from other backgrounds are discussed in Section~\ref{sec:othBG}.
65 Section~\ref{sec:results} shows the results for applying these methods in data.
66 We analyze the systematic uncertainties in the background predictions and in signal acceptance
67 in Section~\ref{sec:systematics}.
68 We then proceed to calculate an upper limit on the non-SM contributions to our signal regions
69 in Section~\ref{sec:upperlimit}.
70 Efficiencies which can be used to test specific models of new physics are given
71 in Section \ref{sec:outreach}.
72 Finally, in Section~\ref{sec:models} we calculate upper limits on the quantity \sta\
73 assuming efficiencies and uncertainties from sample benchmark SUSY processes.
74