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Contents lists available atSciVerse ScienceDirect

Physics Letters B

www.elsevier.com/locate/physletb

Search for heavy, top-like quark pair production in the dilepton final state in pp collisions at √

s = 7 TeV

.CMS Collaboration

CERN, Switzerland

a r t i c l e i n f o a b s t r a c t

Article history:

Received 24 March 2012

Received in revised form 24 July 2012 Accepted 24 July 2012

Available online 27 July 2012 Editor: M. Doser

Keywords:

CMS Physics Dilepton Top-like Tprime Fourth generation

The results of a search for pair production of a heavy, top-like quark, t, in the decay mode t¯t bW+bW¯ b+νb¯ν¯ are presented. The search is performed with a data sample corresponding to an integrated luminosity of 5.0 fb1 in pp collisions at a center-of-mass energy of 7 TeV, collected by the CMS experiment at the LHC. The observed number of events agrees with the expectation from standard model processes, and no evidence of t¯t production is found. Upper limits on the production cross section as a function of tmass are presented, and tmasses below 557 GeV/c2are excluded at the 95% confidence level.

©2012 CERN. Published by Elsevier B.V.

1. Introduction

Since the discovery of the top quark at the Tevatron [1,2], there have been many searches for a possible new generation of fermions. Those searches have found no evidence of new fermions beyond the standard model (SM). However, based on present knowledge, there is no compelling reason for the number of fermion generations to be limited to three[3]. Additional gener- ations of fermions may have a significant effect on neutrino, flavor, and Higgs physics. A fourth generation of quarks, t and b, may result in enough intrinsic matter and anti-matter asymmetry to explain the baryon asymmetry of the universe[4]. Therefore, there is continued theoretical and experimental interest in the search for a fourth generation fermion[3].

Previous direct searches restrict the masses of quarks in the fourth generation, Mt and Mb, to be greater than 404 and 372 GeV/c2, respectively, at the 95% confidence level[5,6], and the measurement of the Z lineshape at the Large Electron–Positron col- lider excludes a fourth generation of light neutrinos[7–10]. At the Large Hadron Collider (LHC), the quantum chromodynamics (QCD) production cross section of t¯t is expected to be two orders of magnitude larger than at the Tevatron for Mt=500 GeV/c2 [11].

This increase provides an opportunity to explore the possibility of

© CERN for the benefit of the CMS Collaboration.

 E-mail address:[email protected].

new physics with an additional generation of fermions at higher masses.

We present a search for pair production of a heavy top-like quark in the final state t¯tbW+bW¯ b+νb¯ν¯, where a branching fraction of 100% to bW is assumed and the charged lep- ton is either an electron or a muon. This search is motivated if Mt<Mb+MW, which is favored by precision electroweak con- straints[12,13]. The presence of two leptons (dileptons) in the final state helps to suppress SM backgrounds, providing a clean environ- ment to search for physics beyond the SM. The data sample corre- sponds to an integrated luminosity of 5.0 fb1 in pp collisions at a center-of-mass energy of 7 TeV, collected by the Compact Muon Solenoid (CMS) experiment at the LHC during 2011.

2. CMS detector

The central feature of the CMS apparatus is a superconduct- ing solenoid, 13 m in length and 6 m in diameter, which pro- vides an axial magnetic field of 3.8 T. Within the field volume are several particle detection systems. Charged particle trajectories are measured by silicon pixel and silicon strip trackers, covering 0 φ <2π in azimuth and |η| <2.5 in pseudorapidity, where

η= −ln[tan(θ/2)] and θ is the polar angle of the trajectory of the particle with respect to the counterclockwise proton beam di- rection. A lead tungstate crystal electromagnetic calorimeter and a brass/scintillator hadron calorimeter surround the tracking vol- ume, providing energy measurements of electrons and hadronic 0370-2693©2012 CERN. Published by Elsevier B.V.

http://dx.doi.org/10.1016/j.physletb.2012.07.059

Open access under CC BY-NC-ND license.

Open access under CC BY-NC-ND license.

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jets. Muons are identified and measured in gas-ionization detectors embedded in the steel flux return yoke of the solenoid. The CMS detector is nearly hermetic, allowing momentum balance measure- ments in the plane transverse to the beam direction. A two-tier trigger system selects pp collision events of interest for use in physics analyses. A more detailed description of the CMS detec- tor can be found elsewhere[14].

3. Event samples, reconstruction, and preselection

The data used for this measurement were collected using one of the ee, eμ, or μμ high-pT double-lepton triggers. Muon can- didates are reconstructed using two algorithms that require con- sistent signals in the tracker and muon systems: one matches the extrapolated trajectories from the silicon tracker to signals in the muon system (tracker-based muons), and the second performs a global fit requiring consistent patterns in the tracker and the muon system (globally fitted muons)[15]. Electron candidates are recon- structed starting from a cluster of energy deposits in the electro- magnetic calorimeter. The cluster is then matched to signals in the silicon tracker. A selection using electron identification vari- ables based on shower shape and track-cluster matching is applied to the reconstructed candidates [16]. Electron candidates within

R

( η)2+ ( φ)2<0.1 from a muon are rejected to remove candidates due to muon bremsstrahlung and final-state radiation.

Both electrons and muons are required to be isolated from other activity in the event. This is achieved by imposing a maximum allowed value of 0.15 on the ratio of the scalar sum of track trans- verse momenta and calorimeter transverse energy deposits within a cone of R<0.3 around the lepton candidate direction at the origin (the transverse momentum of the candidate is excluded), to the transverse momentum of the candidate.

Event preselection is applied to reject events other than those from t¯t or t¯t in the dilepton final state. Events are required to have two opposite-sign, isolated leptons (e+e, e±μ, orμ+μ).

Both leptons must have transverse momentum pT>20 GeV/c, and the electrons (muons) must have|η| <2.5 (2.4). The reconstructed lepton trajectories must be consistent with a common interaction vertex. In the rare case (<0.1%) of events with more than two such leptons, the two leptons with the highest pT are selected.

Events with an e+e orμ+μpair with invariant mass between 76 and 106 GeV/c2 or below 12 GeV/c2 are removed to suppress Drell–Yan (DY) events (Z/γ→ +) as well as low mass dilepton resonances. The jets and the missing transverse energy EmissT are reconstructed with a particle-flow technique[17]. The anti-kTclus- tering algorithm[18]with a distance parameter of 0.5 is used for jet clustering. At least two jets with pT>30 GeV/c and|η| <2.5, separated by R>0.4 from leptons passing the analysis selection, are required in each event. Exactly two of these jets are required to be consistent with coming from the decay of heavy flavor hadrons and be identified as b jets by the TCHEM b-tagging algorithm[19], which relies on tracks with large impact parameters. The EmissT in the event is required to exceed 50 GeV, consistent with the pres- ence of two undetected neutrinos with large pT.

Signal and background events are generated using the Mad- Graph 4.4.12 [20] and pythia 6.4.22 [21] event generators. The samples of t¯t, W+jets, DY with M>50 GeV/c2, diboson (WW, WZ, and ZZ only: the contribution from Wγ is assumed to be negligible), and single top quark events are generated using Mad- Graph. The DY event samples with M<50 GeV/c2are generated using pythia. The samples of t¯t events are generated using Mad- Graph, but decayed using pythia. The tWb decay is modeled assuming a V–A structure of the interaction. Events are then sim- ulated using a Geant4-based model[22]of the CMS detector, and finally reconstructed and analyzed with the same software used to

process collision data. The cross section for t¯t production is taken from a recent CMS measurement[23], while next-to-leading order (NLO) cross sections are used for the remaining SM background samples. The t¯tcross sections are calculated to approximate next- to-NLO (NNLO) using hathor[24].

With the steadily increasing LHC instantaneous luminosity, the mean number of interactions in a single bunch crossing also in- creased over the course of data taking, reaching about 15 at the end of the 2011 running period. In the following, the yields of simulated events are weighted such that the distribution of re- constructed vertices observed in data is reproduced. The average efficiency for events containing two leptons satisfying the analysis selection to pass at least one of the double-lepton triggers is mea- sured to be approximately 100%, 95%, and 90% for the ee, eμ, and

μμ triggers, respectively, and corresponding weights are applied to the simulated event yields. In addition, b-tagging scale factors are applied to simulated events for each jet, to account for the dif- ference between b-tagging efficiencies in data and simulation[19].

The observed and simulated yields after the above event pre- selection are listed in Table 1, in which the categories t¯t→ + and DY→ +correspond to dileptonic t¯t and DY decays, includ- ing τ leptons only when they also decay leptonically. All other tt¯ decay modes are included in the category tt¯other. The yields are dominated by top-pair production in the dilepton final state, and agreement is observed between data and simulation. The ex- pected yields from t¯tare also shown for different values of Mt. 4. Signal region

After preselection, the sample is dominated by SM tt events.¯ Since a tquark is expected to have a much larger mass than that of the top quark, variables that are correlated with the decaying quark mass can help distinguish t¯t events from t¯t events. The mass of the system defined by the lepton and b jet (Mb) from the quark decay is chosen for this purpose. In the decay of a given top quark, Mb is less than

Mt2MW2, where Mt and MW are the masses of the top quark and W boson. In contrast, most t de- cays have Mb larger than that value. At the reconstruction level, however, there are two ways to combine the two leptons and two b jets in each event, giving four possible values of Mb. The min- imum value of the four masses (Mminb ) is found to be a good variable for distinguishing t¯t events from tt events. A compari-¯ son between t¯tevents and t¯t events for this variable is shown in Fig. 1.

The signal region is defined by adding the requirement for the minimum mass of lepton and jet pairs to be Mminb >170 GeV/c2. This additional selection reduces the expected number of t¯t events by four orders of magnitude compared with the preselection pre- diction given in Table 1. The simulated yields of t¯t events are typically reduced by 50%; they are given for different values of Mt

inTable 2.

5. Background estimation

One of the main sources of background events in the signal region is the misidentification of b jets and leptons. A misidenti- fied lepton is defined as a lepton candidate not originating from a prompt decay, such as a lepton from a semileptonic b or c quark decay, a muon from a pion or kaon decay, an unidentified photon conversion, or a pion misidentified as an electron. Misidentified b jets are referred to as “mistags”, and occur when a non-b jet satisfies the b-tagging requirements.

The background events in the signal region can be divided into the following categories:

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Table 1

The observed and simulated yields after the preselection described in the text. The uncertainties on the yields of the simulated samples are statistical only, while for the simulated total background yields the systematic uncertainties from the sources described in Section6are also given. For W+jets, where the simulated yields are zero, upper limits are given based on the weighted yield, had one of the simulated events passed the preselection.

Sample ee μμ eμ all

t¯t,Mt=400 GeV/c2 10.6±0.9 13.9±1.0 29.4±1.5 53.9±2.0

t¯t,Mt=500 GeV/c2 3.0±0.2 3.3±0.2 6.7±0.44 12.9±0.5

t¯t,Mt=600 GeV/c2 0.9±0.1 1.0±0.1 2.2±0.1 4.1±0.2

t¯t→ + 488±11 615±12 1472±19 2575±25

t¯tother 7.2±1.3 0.5±0.3 10.5±1.6 18.2±2.1

W+jets <1.9 <1.9 <1.9 <1.9

DY→ + 2.9±1.5 1.6±1.0 0.6±0.5 5.1±1.8

Diboson 0.5±0.1 1.1±0.2 1.9±0.2 3.6±0.3

Single top quark 15.6±1.0 19.5±1.1 46.9±1.7 82.0±2.2

Total background 514±54 637±67 1532±162 2683±284

Data 510 615 1487 2612

Table 2

The expected yields of t¯tevents in the signal region for different values of Mt. Uncertainties are statistical only.

t¯tsample ee μμ eμ all

Mt=400 GeV/c2 3.5±0.5 5.5±0.6 11.2±0.9 20.1±1.2

Mt=500 GeV/c2 1.4±0.2 1.9±0.2 3.3±0.2 6.7±0.4

Mt=600 GeV/c2 0.6±0.1 0.6±0.1 1.3±0.1 2.5±0.1

Category I: events with mistagged b jet(s) and two real lep- tons;

Category II: events with misidentified lepton(s) and two real b jets;

Category III: events with two real b jets and two real leptons;

Category IV: events with mistagged b jet(s) and misidentified lepton(s).

For each category, an estimate of the combined yield of ee, eμ, andμμevents is made.

To predict the number of events with mistagged b jet(s) (Cate- gory I), control regions in data are used where events pass all se- lection requirements except the number of b-tagged jets. The num- ber of background events with one mistag, N1mistag, is estimated from events with one b tag. Each event is weighted based on the mistag rate ri for each untagged jet in the event, where ri gives the pT- andη-dependent probability (with a mean of 0.02) for a non-b jet to be b-tagged [19]. Where there are no untagged jets passing the Mminb selection, the event weight is zero, and for each untagged jet i passing the selection the event weight is increased by ri/(1ri). The subtraction of riin the denominator is necessary to account for non-b jets that were mistagged, and are thus miss- ing from the sample of untagged jets. A similar calculation is made using events with no b tags to estimate the number of events with two mistags, N2mistags. This time a weight of ri/(1ri)×rj/(1rj) is used for each pair of untagged jets passing selection, where ri and rjare the mistag rates for the two untagged jets. The final pre- diction is obtained as Nmistags=N1mistagN2mistags, which takes into account that N2mistags is counted twice in N1mistag. The per- formance of the method is checked using simulated events, and an under-prediction of up to 50% is observed. We therefore assign a large systematic uncertainty, 100%, to this prediction. In data, the predicted number of events with mistags in the signal region is Nmistags=0.7±0.3±0.7, where the uncertainties are statistical and systematic, respectively. The Category I yield in the simulation, taken as a cross-check using the samples mentioned in Section3, is 1.0±0.3, and is consistent with the prediction based on data.

The background from events with misidentified leptons (Cate- gory II) is predicted based on the number of events in data with a candidate lepton that can pass only loosened selection criteria[25].

Table 3

Summary of the predicted background yields and the measured yield in data. Statistical and systematic uncer- tainties are combined.

Sample Yield

Category I (from data) 0.7±0.8 Category II (from data) 0.0+00..40 Category III (simulated) 1.0±0.7

Total prediction 1.8±1.1

Data 1

Using a measurement of the fraction of such “loose” leptons that go on to pass the selection requirements, the number of misidenti- fied leptons in the event sample can be estimated. However, there are no observed data events where one or more of the lepton candidates passes only the loosened selection criteria, resulting in a prediction of 0.0+00..40 events where the upper uncertainty cor- responds to the prediction of the method, had there been one such event. The Category II event yield is also zero in the simu- lation.

The simulation is used to predict the number of events with no misidentified b jets or leptons (Category III), using the back- ground event samples of Section 3. Selecting only events where both b jets and leptons are well matched to the corresponding par- ticles at the generator level, the resulting prediction is 1.0±0.7 where the uncertainty is statistical. The systematic uncertainty is small in comparison (Section6), so the total uncertainty is also 0.7.

The contribution of events from Category IV is found to be negligible and is covered by both the Category I and Category II predictions. Since the Category II prediction is zero, there is no possibility of double-counting.

6. Systematic uncertainties

The systematic uncertainty on the overall selection efficiency is dominated by the uncertainty on the b-tagging efficiency. This uncertainty is 15% for b jets with pT>240 GeV/c, and 4% for b jets with pT240 GeV/c[19]. Other uncertainties include those on trigger efficiency (2%), lepton selection (2%), and jet and EmissT

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Table 5

The approximate NNLO theoretical cross section of t¯t production assuming standard QCD couplings[24], and the expected and observed 95% CL upper limits on the production cross section of t¯t, for different tmasses.

Mt(GeV/c2) 350 400 450 500 550 600

Theoretical cross section (pb) 3.20 1.41 0.62 0.33 0.17 0.09

Expected limit (pb) 0.53 0.29 0.24 0.21 0.18 0.16

Observed limit (pb) 0.47 0.26 0.22 0.18 0.16 0.14

Fig. 1. Comparison between the data and the simulated background for Mminb . The signal region is defined by Mminb >170 GeV/c2. The Category I simulated back- ground yield in the signal region is scaled so that it matches the yield estimated from control regions in data, as given inTable 3. Outside the signal region the sim- ulated background yields are taken without rescaling. One event is observed in the signal region. The expected distribution for a t¯tsignal with Mt=450 GeV/c2is also shown.

Table 4

Overall selection efficiency in simulated events for dif- ferent tmasses. The branching fraction of 6.5% for the dilepton decay mode of t¯tis included. The uncertain- ties are calculated using the systematic uncertainty of 19% from Section6.

t¯tsample Eff×Acc×Br (%) Mt=350 GeV/c2 0.16±0.03 Mt=400 GeV/c2 0.29±0.06 Mt=450 GeV/c2 0.35±0.07 Mt=500 GeV/c2 0.41±0.08 Mt=550 GeV/c2 0.48±0.09 Mt=600 GeV/c2 0.54±0.10

energy scale (8%)[26]. These four sources combine to yield a 19%

relative uncertainty on the overall selection efficiency for signal events. There is a further 2.2% uncertainty on the luminosity mea- surement[27].

The systematic uncertainty on the background estimate is dom- inated by the uncertainty on the estimate of events with mistagged b jets from data (100%), and by the lack of selected events in the loose-lepton control region. The systematic uncertainties on these sources of background are included in the summary of background predictions given inTable 3.

7. Results and summary

The number of expected events from background processes is 1.8±1.1, and one event is observed in the eμchannel. There is thus no evidence for an excess of events above SM expectations.

Fig. 2. The 95% CL upper limits on the production cross section of tt¯ as a func- tion of t mass. The observed (expected) 95% CL lower bound on Mt is 557 (547)GeV/c2.

A summary of the observed and predicted yields is presented in Table 3.

The simulated distribution of Mminb from background processes is compared with the data in Fig. 1, where the expected distribu- tion for a t¯tsignal with Mt=450 GeV/c2 is also shown.

Finally, 95% confidence level (CL) upper limits on the produc- tion cross section of t¯tas a function of tmass are set, using the CLs method[28,29], where nuisance parameters are varied in the ensemble tests using log-normal distributions.

The limit calculation is based on the information provided by the observed event count combined with the values and the un- certainties of the luminosity measurement, the background predic- tion, and the fraction of t¯t events expected to be selected. This fraction (the overall selection efficiency) is taken as the product of efficiency, acceptance, and the branching fraction for simulated signal events, and is given in Table 4for different values of Mt. The calculated limits are shown inTable 5andFig. 2.

In summary, assuming a branching fraction of 100% for t bW, the expected and observed 95% CL lower bounds on the t mass are 547 and 557 GeV/c2, respectively, from the analysis of a data sample of pp collisions at

s=7 TeV, corresponding to an integrated luminosity of 5.0 fb1.

Acknowledgements

We congratulate our colleagues in the CERN accelerator depart- ments for the excellent performance of the LHC machine. We thank the technical and administrative staff at CERN and other CMS institutes, and acknowledge support from: FMSR (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP (Brazil);

MES (Bulgaria); CERN; CAS, MoST, and NSFC (China); COLCIENCIAS (Colombia); MSES (Croatia); RPF (Cyprus); MoER, SF0690030s09 and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland);

CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany);

GSRT (Greece); OTKA and NKTH (Hungary); DAE and DST (India);

IPM (Iran); SFI (Ireland); INFN (Italy); NRF and WCU (Korea); LAS (Lithuania); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico);

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MSI (New Zealand); PAEC (Pakistan); MSHE and NSC (Poland);

FCT (Portugal); JINR (Armenia, Belarus, Georgia, Ukraine, Uzbek- istan); MON, RosAtom, RAS and RFBR (Russia); MSTD (Serbia);

MICINN and CPAN (Spain); Swiss Funding Agencies (Switzerland);

NSC (Taipei); TUBITAK and TAEK (Turkey); STFC (United Kingdom);

DOE and NSF (USA).

Open access

This article is published Open Access at sciencedirect.com. It is distributed under the terms of the Creative Commons Attribu- tion License 3.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original authors and source are credited.

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Yerevan Physics Institute, Yerevan, Armenia

W. Adam, T. Bergauer, M. Dragicevic, J. Erö, C. Fabjan, M. Friedl, R. Frühwirth, V.M. Ghete, J. Hammer1, N. Hörmann, J. Hrubec, M. Jeitler, W. Kiesenhofer, M. Krammer, D. Liko, I. Mikulec, M. Pernicka, B. Rahbaran, C. Rohringer, H. Rohringer, R. Schöfbeck, J. Strauss, A. Taurok, F. Teischinger, P. Wagner, W. Waltenberger, G. Walzel, E. Widl, C.-E. Wulz

Institut für Hochenergiephysik der OeAW, Wien, Austria

V. Mossolov, N. Shumeiko, J. Suarez Gonzalez

National Centre for Particle and High Energy Physics, Minsk, Belarus

S. Bansal, K. Cerny, T. Cornelis, E.A. De Wolf, X. Janssen, S. Luyckx, T. Maes, L. Mucibello, S. Ochesanu, B. Roland, R. Rougny, M. Selvaggi, H. Van Haevermaet, P. Van Mechelen, N. Van Remortel,

A. Van Spilbeeck

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Universiteit Antwerpen, Antwerpen, Belgium

F. Blekman, S. Blyweert, J. D’Hondt, R. Gonzalez Suarez, A. Kalogeropoulos, M. Maes, A. Olbrechts, W. Van Doninck, P. Van Mulders, G.P. Van Onsem, I. Villella

Vrije Universiteit Brussel, Brussel, Belgium

O. Charaf, B. Clerbaux, G. De Lentdecker, V. Dero, A.P.R. Gay, T. Hreus, A. Léonard, P.E. Marage, T. Reis, L. Thomas, C. Vander Velde, P. Vanlaer

Université Libre de Bruxelles, Bruxelles, Belgium

V. Adler, K. Beernaert, A. Cimmino, S. Costantini, G. Garcia, M. Grunewald, B. Klein, J. Lellouch,

A. Marinov, J. Mccartin, A.A. Ocampo Rios, D. Ryckbosch, N. Strobbe, F. Thyssen, M. Tytgat, L. Vanelderen, P. Verwilligen, S. Walsh, E. Yazgan, N. Zaganidis

Ghent University, Ghent, Belgium

S. Basegmez, G. Bruno, L. Ceard, C. Delaere, T. du Pree, D. Favart, L. Forthomme, A. Giammanco2, J. Hollar, V. Lemaitre, J. Liao, O. Militaru, C. Nuttens, D. Pagano, A. Pin, K. Piotrzkowski,

N. Schul

Université Catholique de Louvain, Louvain-la-Neuve, Belgium

N. Beliy, T. Caebergs, E. Daubie, G.H. Hammad

Université de Mons, Mons, Belgium

G.A. Alves, M. Correa Martins Jr., D. De Jesus Damiao, T. Martins, M.E. Pol, M.H.G. Souza

Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Brazil

W.L. Aldá Júnior, W. Carvalho, A. Custódio, E.M. Da Costa, C. De Oliveira Martins, S. Fonseca De Souza, D. Matos Figueiredo, L. Mundim, H. Nogima, V. Oguri, W.L. Prado Da Silva, A. Santoro,

S.M. Silva Do Amaral, L. Soares Jorge, A. Sznajder

Universidade do Estado do Rio de Janeiro, Rio de Janeiro, Brazil

T.S. Anjos3, C.A. Bernardes3, F.A. Dias4, T.R. Fernandez Perez Tomei, E.M. Gregores3, C. Lagana, F. Marinho, P.G. Mercadante3, S.F. Novaes, Sandra S. Padula

Instituto de Fisica Teorica, Universidade Estadual Paulista, Sao Paulo, Brazil

V. Genchev1, P. Iaydjiev1, S. Piperov, M. Rodozov, S. Stoykova, G. Sultanov, V. Tcholakov, R. Trayanov, M. Vutova

Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria

A. Dimitrov, R. Hadjiiska, V. Kozhuharov, L. Litov, B. Pavlov, P. Petkov

University of Sofia, Sofia, Bulgaria

J.G. Bian, G.M. Chen, H.S. Chen, C.H. Jiang, D. Liang, S. Liang, X. Meng, J. Tao, J. Wang, J. Wang, X. Wang, Z. Wang, H. Xiao, M. Xu, J. Zang, Z. Zhang

Institute of High Energy Physics, Beijing, China

C. Asawatangtrakuldee, Y. Ban, S. Guo, Y. Guo, W. Li, S. Liu, Y. Mao, S.J. Qian, H. Teng, S. Wang, B. Zhu, W. Zou

State Key Lab. of Nucl. Phys. and Tech., Peking University, Beijing, China

C. Avila, B. Gomez Moreno, A.F. Osorio Oliveros, J.C. Sanabria

(7)

Universidad de Los Andes, Bogota, Colombia

N. Godinovic, D. Lelas, R. Plestina5, D. Polic, I. Puljak1

Technical University of Split, Split, Croatia

Z. Antunovic, M. Dzelalija, M. Kovac

University of Split, Split, Croatia

V. Brigljevic, S. Duric, K. Kadija, J. Luetic, S. Morovic

Institute Rudjer Boskovic, Zagreb, Croatia

A. Attikis, M. Galanti, G. Mavromanolakis, J. Mousa, C. Nicolaou, F. Ptochos, P.A. Razis

University of Cyprus, Nicosia, Cyprus

M. Finger, M. Finger Jr.

Charles University, Prague, Czech Republic

Y. Assran6, S. Elgammal, A. Ellithi Kamel7, S. Khalil8, M.A. Mahmoud9, A. Radi8,10

Academy of Scientific Research and Technology of the Arab Republic of Egypt, Egyptian Network of High Energy Physics, Cairo, Egypt

M. Kadastik, M. Müntel, M. Raidal, L. Rebane, A. Tiko

National Institute of Chemical Physics and Biophysics, Tallinn, Estonia

V. Azzolini, P. Eerola, G. Fedi, M. Voutilainen

Department of Physics, University of Helsinki, Helsinki, Finland

J. Härkönen, A. Heikkinen, V. Karimäki, R. Kinnunen, M.J. Kortelainen, T. Lampén, K. Lassila-Perini, S. Lehti, T. Lindén, P. Luukka, T. Mäenpää, T. Peltola, E. Tuominen, J. Tuominiemi, E. Tuovinen, D. Ungaro, L. Wendland

Helsinki Institute of Physics, Helsinki, Finland

K. Banzuzi, A. Korpela, T. Tuuva

Lappeenranta University of Technology, Lappeenranta, Finland

M. Besancon, S. Choudhury, M. Dejardin, D. Denegri, B. Fabbro, J.L. Faure, F. Ferri, S. Ganjour,

A. Givernaud, P. Gras, G. Hamel de Monchenault, P. Jarry, E. Locci, J. Malcles, L. Millischer, A. Nayak, J. Rander, A. Rosowsky, I. Shreyber, M. Titov

DSM/IRFU, CEA/Saclay, Gif-sur-Yvette, France

S. Baffioni, F. Beaudette, L. Benhabib, L. Bianchini, M. Bluj11, C. Broutin, P. Busson, C. Charlot, N. Daci, T. Dahms, L. Dobrzynski, R. Granier de Cassagnac, M. Haguenauer, P. Miné, C. Mironov, C. Ochando, P. Paganini, D. Sabes, R. Salerno, Y. Sirois, C. Veelken, A. Zabi

Laboratoire Leprince-Ringuet, Ecole Polytechnique, IN2P3-CNRS, Palaiseau, France

J.-L. Agram12, J. Andrea, D. Bloch, D. Bodin, J.-M. Brom, M. Cardaci, E.C. Chabert, C. Collard, E. Conte12, F. Drouhin12, C. Ferro, J.-C. Fontaine12, D. Gelé, U. Goerlach, P. Juillot, M. Karim12, A.-C. Le Bihan, P. Van Hove

Institut Pluridisciplinaire Hubert Curien, Université de Strasbourg, Université de Haute Alsace Mulhouse, CNRS/IN2P3, Strasbourg, France

F. Fassi, D. Mercier

Centre de Calcul de l’Institut National de Physique Nucleaire et de Physique des Particules (IN2P3), Villeurbanne, France

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S. Beauceron, N. Beaupere, O. Bondu, G. Boudoul, H. Brun, J. Chasserat, R. Chierici1, D. Contardo, P. Depasse, H. El Mamouni, J. Fay, S. Gascon, M. Gouzevitch, B. Ille, T. Kurca, M. Lethuillier, L. Mirabito, S. Perries, V. Sordini, S. Tosi, Y. Tschudi, P. Verdier, S. Viret

Université de Lyon, Université Claude Bernard Lyon 1, CNRS-IN2P3, Institut de Physique Nucléaire de Lyon, Villeurbanne, France

L. Rurua

E. Andronikashvili Institute of Physics, Academy of Science, Tbilisi, Georgia

G. Anagnostou, S. Beranek, M. Edelhoff, L. Feld, N. Heracleous, O. Hindrichs, R. Jussen, K. Klein, J. Merz, A. Ostapchuk, A. Perieanu, F. Raupach, J. Sammet, S. Schael, D. Sprenger, H. Weber, B. Wittmer,

V. Zhukov13

RWTH Aachen University, I. Physikalisches Institut, Aachen, Germany

M. Ata, J. Caudron, E. Dietz-Laursonn, D. Duchardt, M. Erdmann, A. Güth, T. Hebbeker, C. Heidemann, K. Hoepfner, T. Klimkovich, D. Klingebiel, P. Kreuzer, D. Lanske, J. Lingemann, C. Magass,

M. Merschmeyer, A. Meyer, M. Olschewski, P. Papacz, H. Pieta, H. Reithler, S.A. Schmitz, L. Sonnenschein, J. Steggemann, D. Teyssier, M. Weber

RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany

M. Bontenackels, V. Cherepanov, M. Davids, G. Flügge, H. Geenen, M. Geisler, W. Haj Ahmad, F. Hoehle, B. Kargoll, T. Kress, Y. Kuessel, A. Linn, A. Nowack, L. Perchalla, O. Pooth, J. Rennefeld, P. Sauerland, A. Stahl

RWTH Aachen University, III. Physikalisches Institut B, Aachen, Germany

M. Aldaya Martin, J. Behr, W. Behrenhoff, U. Behrens, M. Bergholz14, A. Bethani, K. Borras, A. Burgmeier, A. Cakir, L. Calligaris, A. Campbell, E. Castro, F. Costanza, D. Dammann, G. Eckerlin, D. Eckstein,

D. Fischer, G. Flucke, A. Geiser, I. Glushkov, S. Habib, J. Hauk, H. Jung1, M. Kasemann, P. Katsas, C. Kleinwort, H. Kluge, A. Knutsson, M. Krämer, D. Krücker, E. Kuznetsova, W. Lange, W. Lohmann14, B. Lutz, R. Mankel, I. Marfin, M. Marienfeld, I.-A. Melzer-Pellmann, A.B. Meyer, J. Mnich, A. Mussgiller, S. Naumann-Emme, J. Olzem, H. Perrey, A. Petrukhin, D. Pitzl, A. Raspereza, P.M. Ribeiro Cipriano,

C. Riedl, M. Rosin, J. Salfeld-Nebgen, R. Schmidt14, T. Schoerner-Sadenius, N. Sen, A. Spiridonov, M. Stein, R. Walsh, C. Wissing

Deutsches Elektronen-Synchrotron, Hamburg, Germany

C. Autermann, V. Blobel, S. Bobrovskyi, J. Draeger, H. Enderle, J. Erfle, U. Gebbert, M. Görner, T. Hermanns, R.S. Höing, K. Kaschube, G. Kaussen, H. Kirschenmann, R. Klanner, J. Lange, B. Mura, F. Nowak, N. Pietsch, D. Rathjens, C. Sander, H. Schettler, P. Schleper, E. Schlieckau, A. Schmidt, M. Schröder, T. Schum, M. Seidel, H. Stadie, G. Steinbrück, J. Thomsen

University of Hamburg, Hamburg, Germany

C. Barth, J. Berger, T. Chwalek, W. De Boer, A. Dierlamm, M. Feindt, M. Guthoff1, C. Hackstein,

F. Hartmann, M. Heinrich, H. Held, K.H. Hoffmann, S. Honc, U. Husemann, I. Katkov13, J.R. Komaragiri, D. Martschei, S. Mueller, Th. Müller, M. Niegel, A. Nürnberg, O. Oberst, A. Oehler, J. Ott, T. Peiffer, G. Quast, K. Rabbertz, F. Ratnikov, N. Ratnikova, S. Röcker, C. Saout, A. Scheurer, F.-P. Schilling, M. Schmanau, G. Schott, H.J. Simonis, F.M. Stober, D. Troendle, R. Ulrich, J. Wagner-Kuhr, T. Weiler, M. Zeise, E.B. Ziebarth

Institut für Experimentelle Kernphysik, Karlsruhe, Germany

G. Daskalakis, T. Geralis, S. Kesisoglou, A. Kyriakis, D. Loukas, I. Manolakos, A. Markou, C. Markou, C. Mavrommatis, E. Ntomari

Institute of Nuclear Physics “Demokritos”, Aghia Paraskevi, Greece

(9)

L. Gouskos, T.J. Mertzimekis, A. Panagiotou, N. Saoulidou

University of Athens, Athens, Greece

I. Evangelou, C. Foudas1, P. Kokkas, N. Manthos, I. Papadopoulos, V. Patras

University of Ioánnina, Ioánnina, Greece

G. Bencze, C. Hajdu1, P. Hidas, D. Horvath15, K. Krajczar16, B. Radics, F. Sikler1, V. Veszpremi, G. Vesztergombi16

KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary

N. Beni, S. Czellar, J. Molnar, J. Palinkas, Z. Szillasi

Institute of Nuclear Research ATOMKI, Debrecen, Hungary

J. Karancsi, P. Raics, Z.L. Trocsanyi, B. Ujvari

University of Debrecen, Debrecen, Hungary

S.B. Beri, V. Bhatnagar, N. Dhingra, R. Gupta, M. Jindal, M. Kaur, J.M. Kohli, M.Z. Mehta, N. Nishu, L.K. Saini, A. Sharma, J. Singh, S.P. Singh

Panjab University, Chandigarh, India

S. Ahuja, A. Bhardwaj, B.C. Choudhary, A. Kumar, A. Kumar, S. Malhotra, M. Naimuddin, K. Ranjan, V. Sharma, R.K. Shivpuri

University of Delhi, Delhi, India

S. Banerjee, S. Bhattacharya, S. Dutta, B. Gomber, Sa. Jain, Sh. Jain, R. Khurana, S. Sarkar

Saha Institute of Nuclear Physics, Kolkata, India

A. Abdulsalam, R.K. Choudhury, D. Dutta, S. Kailas, V. Kumar, A.K. Mohanty1, L.M. Pant, P. Shukla

Bhabha Atomic Research Centre, Mumbai, India

T. Aziz, S. Ganguly, M. Guchait17, A. Gurtu18, M. Maity19, G. Majumder, K. Mazumdar, G.B. Mohanty, B. Parida, K. Sudhakar, N. Wickramage

Tata Institute of Fundamental Research – EHEP, Mumbai, India

S. Banerjee, S. Dugad

Tata Institute of Fundamental Research – HECR, Mumbai, India

H. Arfaei, H. Bakhshiansohi20, S.M. Etesami21, A. Fahim20, M. Hashemi, H. Hesari, A. Jafari20,

M. Khakzad, A. Mohammadi22, M. Mohammadi Najafabadi, S. Paktinat Mehdiabadi, B. Safarzadeh23, M. Zeinali21

Institute for Research in Fundamental Sciences (IPM), Tehran, Iran

M. Abbresciaa,b, L. Barbonea,b, C. Calabriaa,b,1, S.S. Chhibraa,b, A. Colaleoa, D. Creanzaa,c, N. De Filippisa,c,1, M. De Palmaa,b, L. Fiorea, G. Iasellia,c, L. Lusitoa,b, G. Maggia,c, M. Maggia, B. Marangellia,b, S. Mya,c, S. Nuzzoa,b, N. Pacificoa,b, A. Pompilia,b, G. Pugliesea,c, G. Selvaggia,b, L. Silvestrisa, G. Singha,b, G. Zitoa

aINFN Sezione di Bari, Bari, Italy bUniversità di Bari, Bari, Italy cPolitecnico di Bari, Bari, Italy

G. Abbiendia, A.C. Benvenutia, D. Bonacorsia,b, S. Braibant-Giacomellia,b, L. Brigliadoria,b,

P. Capiluppia,b, A. Castroa,b, F.R. Cavalloa, M. Cuffiania,b, G.M. Dallavallea, F. Fabbria, A. Fanfania,b,

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