1 |
claudioc |
1.1 |
\section{Introduction}
|
2 |
|
|
\label{sec:intro}
|
3 |
|
|
|
4 |
|
|
|
5 |
|
|
In this Letter we describe a search for physics beyond the Standard Model (BSM)
|
6 |
|
|
in a \lumi\ sample of proton-proton collisions collected by the Compact Muon
|
7 |
|
|
Solenoid (CMS) detector at the Large Hadron Collider (LHC), at a center-of-mass
|
8 |
|
|
energy of $\sqrt{s}=7$~TeV. We search for events with $Z \to \ell \ell$ ($\ell =
|
9 |
|
|
e$ or $\mu$),
|
10 |
|
|
accompanied by significant
|
11 |
|
|
hadronic energy and missing transverse energy (\met). This search is motivated by
|
12 |
|
|
three general considerations:
|
13 |
|
|
astrophysical evidence for dark matter suggests that we concentrate on
|
14 |
|
|
events with high \met, production of $Z$ bosons with high \met is
|
15 |
|
|
a rare process in the SM,
|
16 |
|
|
and high cross section BSM physics signals are likely to be produced
|
17 |
|
|
strongly, producing significant hadronic activity in conjunction with the $Z$-boson.
|
18 |
|
|
A specific BSM scenario which results in this signature is provided by
|
19 |
|
|
Supersymmetric (SUSY) models in which new, heavy particles are pair-produced and subsequently
|
20 |
|
|
undergo cascade decays, producing hadronic jets and, in some cases,
|
21 |
|
|
$Z$-bosons~\cite{Martin:fk}. These
|
22 |
|
|
cascade decays terminate in the production of a weakly-interacting massive particle (WIMP),
|
23 |
|
|
which escapes detection and results in large \met.
|
24 |
|
|
|
25 |
|
|
Our strategy is as follows. We select clean samples of $Z \to ee$ and
|
26 |
|
|
$Z \to \mu \mu$ with two or more hadronic jets. We compare the \met distribution
|
27 |
|
|
in these events with Standard Model (SM) expectations obtained using data-driven
|
28 |
|
|
methods to minimize the dependence on Monte Carlo simulation. Having found
|
29 |
|
|
no evidence for events with anomalously high \met, we proceed
|
30 |
|
|
to set limits on the cross-section for the
|
31 |
|
|
production of $Z$-bosons with jets and \met $> 60$ and
|
32 |
|
|
$> 120$ GeV. Finally, we provide information to enable others
|
33 |
|
|
to use our results for model testing.
|
34 |
|
|
|