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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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sign leptons is particularly interesting since this final state is absent in the St<strong>and</strong>ard Mo<strong>de</strong>l.<br />

The dominant background is therefore given by fake leptons: for instance tt events in which<br />

one lepton is a real isolated lepton from the W <strong>and</strong> the other one comes from the heavy flavour<br />

<strong>de</strong>cay. The fake lepton contributions are estimated with several data-driven techniques, which<br />

are all based on the concept of the “tight-loose” method: the probability of a lepton passing a<br />

loose selection to pass also a tight selection is estimated in <strong>QCD</strong> multijet sample as a function of<br />

lepton pT <strong>and</strong> η; the contribution in the signal region is estimated by multiplying this efficiency<br />

to the yield in a preselected loose sample. Different variations of the method are used for the<br />

different analyses <strong>and</strong> for the different backgrounds. The number of observed events in data is<br />

in agreement with all the Monte Carlo <strong>and</strong> data-driven estimates in all the four regions. The<br />

exclusion region in a mSUGRA plane is given (fig. 1), as well as a parametrization of efficiencies<br />

<strong>and</strong> acceptances to make possible generator level studies of different mo<strong>de</strong>ls. As a cross check,<br />

the same analysis has been repeated at generator level using this parametrization: an agreement<br />

with the actual exclusion region better than the theoretical error is achieved 13 .<br />

7 Conclusions<br />

In this talk a review of the analyses performed by the CMS Collaboration with the first 35 pb −1 of<br />

data is presented. No evi<strong>de</strong>nce of Supersymmetry has been found, in any of the final states. The<br />

previous explored range of the mo<strong>de</strong>l parameters has been significantly exten<strong>de</strong>d. The results<br />

are presented in the mSUGRA scenario in or<strong>de</strong>r to compare them with the results by previous<br />

experiments, but other interpretations are given in terms of simplified mo<strong>de</strong>ls. In addition,<br />

in some of the analyses, a parametrization of efficiencies <strong>and</strong> acceptances is given, in or<strong>de</strong>r to<br />

make possible generator level studies on other mo<strong>de</strong>ls. The most important achievement is that<br />

a road-map for discoveries has been established: the physics objects are commissioned; many<br />

different analyses are performed on many final states; the analyses are often complementary<br />

among them; the backgrounds are estimated with data-driven techniques whenever possible:<br />

multiple techniques are used for the various analyses, <strong>and</strong> for every analysis, different techniques<br />

are used for the different backgrounds. The CMS collaboration set up a robust <strong>and</strong> complete<br />

suite of analyses aimed at discoveries in the <strong>2011</strong>-2012 run.<br />

References<br />

1. R. Adolphi et al. (CMS Collaboration), J. Inst. 3, S08004 (2008).<br />

2. L. R<strong>and</strong>all <strong>and</strong> D. Tucker-Smith, Phys. Rev. Lett. 101, 221803 (2008).<br />

3. V. Khachatryan et al. (CMS Collaboration), Phys. Lett. B 698, 196-218 (<strong>2011</strong>).<br />

4. CMS Collaboration, arXiv:1106.3272, CMS-SUS-10-011.<br />

5. CMS Collaboration, arXiv:1106.4503, CMS-SUS-10-005.<br />

6. CMS Collaboration, CMS-SUS-10-009.<br />

7. J. Alwall, P. Schuster, <strong>and</strong> N. Toro, Phys. Rev. D 79, 075020 (2009).<br />

8. CMS Collaboration, arXiv:1103.0953, CMS-SUS-10-002.<br />

9. CMS Collaboration, arXiv:1105.2758, CMS-EWK-10-008.<br />

10. CMS Collaboration, arXiv:1105.3152, CMS-SUS-11-002.<br />

11. V. Khachatryan et al. (CMS Collaboration), Phys. Lett. B 695, 424-443 (<strong>2011</strong>).<br />

12. CMS Collaboration, arXiv:1103.1348, CMS-SUS-10-007.<br />

13. CMS Collaboration, arXiv:1104.3168, CMS-SUS-10-004.

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