• Aucun résultat trouvé

Cross-Section-Constrained Top-Quark Mass Measurement from Dilepton Events at the Tevatron

N/A
N/A
Protected

Academic year: 2022

Partager "Cross-Section-Constrained Top-Quark Mass Measurement from Dilepton Events at the Tevatron"

Copied!
8
0
0

Texte intégral

(1)

Article

Reference

Cross-Section-Constrained Top-Quark Mass Measurement from Dilepton Events at the Tevatron

CDF Collaboration

CLARK, Allan Geoffrey (Collab.), et al.

Abstract

We report the first top-quark mass measurement that uses a cross-section constraint to improve the mass determination. This measurement is made with a dilepton tt event candidate sample collected with the Collider Detector II at Fermilab. From a data sample corresponding to an integrated luminosity of 1.2  fb−1, we measure a top-quark mass of 170.7+4.2−3.9(stat)±2.6(syst)±2.4(theory)  GeV/c2. The measurement without the cross-section constraint is 169.7+5.2−4.9(stat)±3.1(syst)  GeV/c2.

CDF Collaboration, CLARK, Allan Geoffrey (Collab.), et al . Cross-Section-Constrained Top-Quark Mass Measurement from Dilepton Events at the Tevatron. Physical Review Letters , 2008, vol. 100, no. 06, p. 062005

DOI : 10.1103/PhysRevLett.100.062005

Available at:

http://archive-ouverte.unige.ch/unige:38492

Disclaimer: layout of this document may differ from the published version.

1 / 1

(2)

Cross-Section-Constrained Top-Quark Mass Measurement from Dilepton Events at the Tevatron

T. Aaltonen,23J. Adelman,13T. Akimoto,54M. G. Albrow,17B. A´ lvarez Gonza´lez,11S. Amerio,42D. Amidei,34 A. Anastassov,51A. Annovi,19J. Antos,14M. Aoki,24G. Apollinari,17A. Apresyan,47T. Arisawa,56A. Artikov,15 W. Ashmanskas,17A. Attal,3A. Aurisano,52F. Azfar,41P. Azzi-Bacchetta,42P. Azzurri,45N. Bacchetta,42W. Badgett,17

A. Barbaro-Galtieri,28V. E. Barnes,47B. A. Barnett,25S. Baroiant,7V. Bartsch,30G. Bauer,32P.-H. Beauchemin,33 F. Bedeschi,45P. Bednar,14S. Behari,25G. Bellettini,45J. Bellinger,58A. Belloni,22D. Benjamin,16A. Beretvas,17 J. Beringer,28T. Berry,29A. Bhatti,49M. Binkley,17D. Bisello,42I. Bizjak,30R. E. Blair,2C. Blocker,6B. Blumenfeld,25 A. Bocci,16A. Bodek,48V. Boisvert,48G. Bolla,47A. Bolshov,32D. Bortoletto,47J. Boudreau,46A. Boveia,10B. Brau,10 A. Bridgeman,24L. Brigliadori,5C. Bromberg,35E. Brubaker,13J. Budagov,15H. S. Budd,48S. Budd,24K. Burkett,17

G. Busetto,42P. Bussey,21A. Buzatu,33K. L. Byrum,2S. Cabrera,16,rM. Campanelli,35M. Campbell,34F. Canelli,17 A. Canepa,44D. Carlsmith,58R. Carosi,45S. Carrillo,18,lS. Carron,33B. Casal,11M. Casarsa,17A. Castro,5P. Catastini,45

D. Cauz,53M. Cavalli-Sforza,3A. Cerri,28L. Cerrito,30,pS. H. Chang,27Y. C. Chen,1M. Chertok,7G. Chiarelli,45 G. Chlachidze,17F. Chlebana,17K. Cho,27D. Chokheli,15J. P. Chou,22G. Choudalakis,32S. H. Chuang,51K. Chung,12 W. H. Chung,58Y. S. Chung,48C. I. Ciobanu,24M. A. Ciocci,45A. Clark,20D. Clark,6G. Compostella,42M. E. Convery,17 J. Conway,7B. Cooper,30K. Copic,34M. Cordelli,19G. Cortiana,42F. Crescioli,45C. Cuenca Almenar,7,rJ. Cuevas,11,o

R. Culbertson,17J. C. Cully,34D. Dagenhart,17M. Datta,17T. Davies,21P. de Barbaro,48S. DeCecco,50A. Deisher,28 G. De Lentdecker,48,dG. De Lorenzo,3M. Dell’Orso,45L. Demortier,49J. Deng,16M. Deninno,5D. De Pedis,50 P. F. Derwent,17G. P. Di Giovanni,43C. Dionisi,50B. Di Ruzza,53J. R. Dittmann,4M. D’Onofrio,3S. Donati,45P. Dong,8

J. Donini,42T. Dorigo,42S. Dube,51J. Efron,38R. Erbacher,7D. Errede,24S. Errede,24R. Eusebi,17H. C. Fang,28 S. Farrington,29W. T. Fedorko,13R. G. Feild,59M. Feindt,26J. P. Fernandez,31C. Ferrazza,45R. Field,18G. Flanagan,47

R. Forrest,7S. Forrester,7M. Franklin,22J. C. Freeman,28I. Furic,18M. Gallinaro,49J. Galyardt,12F. Garberson,10 J. E. Garcia,45A. F. Garfinkel,47H. Gerberich,24D. Gerdes,34S. Giagu,50V. Giakoumopolou,45,aP. Giannetti,45 K. Gibson,46J. L. Gimmell,48C. M. Ginsburg,17N. Giokaris,15,aM. Giordani,53P. Giromini,19M. Giunta,45V. Glagolev,15

D. Glenzinski,17M. Gold,36N. Goldschmidt,18A. Golossanov,17G. Gomez,11G. Gomez-Ceballos,32M. Goncharov,52 O. Gonza´lez,31I. Gorelov,36A. T. Goshaw,16K. Goulianos,49A. Gresele,42S. Grinstein,22C. Grosso-Pilcher,13 R. C. Group,17U. Grundler,24J. Guimaraes da Costa,22Z. Gunay-Unalan,35C. Haber,28K. Hahn,32S. R. Hahn,17 E. Halkiadakis,51A. Hamilton,20B.-Y. Han,48J. Y. Han,48R. Handler,58F. Happacher,19K. Hara,54D. Hare,51M. Hare,55 S. Harper,41R. F. Harr,57R. M. Harris,17M. Hartz,46K. Hatakeyama,49J. Hauser,8C. Hays,41M. Heck,26A. Heijboer,44 B. Heinemann,28J. Heinrich,44C. Henderson,32M. Herndon,58J. Heuser,26S. Hewamanage,4D. Hidas,16C. S. Hill,10,c D. Hirschbuehl,26A. Hocker,17S. Hou,1M. Houlden,29S.-C. Hsu,9B. T. Huffman,41R. E. Hughes,38U. Husemann,59

J. Huston,35J. Incandela,10G. Introzzi,45M. Iori,50A. Ivanov,7B. Iyutin,32E. James,17B. Jayatilaka,16D. Jeans,50 E. J. Jeon,27S. Jindariani,18W. Johnson,7M. Jones,47K. K. Joo,27S. Y. Jun,12J. E. Jung,27T. R. Junk,24T. Kamon,52

D. Kar,18P. E. Karchin,57Y. Kato,40R. Kephart,17U. Kerzel,26V. Khotilovich,52B. Kilminster,38D. H. Kim,27 H. S. Kim,27J. E. Kim,27M. J. Kim,17S. B. Kim,27S. H. Kim,54Y. K. Kim,13N. Kimura,54L. Kirsch,6S. Klimenko,18

M. Klute,32B. Knuteson,32B. R. Ko,16S. A. Koay,10K. Kondo,56D. J. Kong,27J. Konigsberg,18A. Korytov,18 A. V. Kotwal,16J. Kraus,24M. Kreps,26J. Kroll,44N. Krumnack,4M. Kruse,16V. Krutelyov,10T. Kubo,54S. E. Kuhlmann,2

T. Kuhr,26N. P. Kulkarni,57Y. Kusakabe,56S. Kwang,13A. T. Laasanen,47S. Lai,33S. Lami,45S. Lammel,17 M. Lancaster,30R. L. Lander,7K. Lannon,38A. Lath,51G. Latino,45I. Lazzizzera,42T. LeCompte,2J. Lee,48J. Lee,27

Y. J. Lee,27S. W. Lee,52,qR. Lefe`vre,20N. Leonardo,32S. Leone,45S. Levy,13J. D. Lewis,17C. Lin,59C. S. Lin,28 J. Linacre,41M. Lindgren,17E. Lipeles,9A. Lister,7D. O. Litvintsev,17T. Liu,17N. S. Lockyer,44A. Loginov,59M. Loreti,42

L. Lovas,14R.-S. Lu,1D. Lucchesi,42J. Lueck,26C. Luci,50P. Lujan,28P. Lukens,17G. Lungu,18L. Lyons,41J. Lys,28 R. Lysak,14E. Lytken,47P. Mack,26D. MacQueen,33R. Madrak,17K. Maeshima,17K. Makhoul,32T. Maki,23 P. Maksimovic,25S. Malde,41S. Malik,30G. Manca,29A. Manousakis,15,aF. Margaroli,47C. Marino,26C. P. Marino,24

A. Martin,59M. Martin,25V. Martin,21,jM. Martı´nez,3R. Martı´nez-Balları´n,31T. Maruyama,54P. Mastrandrea,50 T. Masubuchi,54M. E. Mattson,57P. Mazzanti,5K. S. McFarland,48P. McIntyre,52R. McNulty,29,iA. Mehta,29 P. Mehtala,23S. Menzemer,11,kA. Menzione,45P. Merkel,47C. Mesropian,49A. Messina,35T. Miao,17N. Miladinovic,6

J. Miles,32R. Miller,35C. Mills,22M. Milnik,26A. Mitra,1G. Mitselmakher,18H. Miyake,54S. Moed,22N. Moggi,5 C. S. Moon,27R. Moore,17M. Morello,45P. Movilla Fernandez,28J. Mu¨lmensta¨dt,28A. Mukherjee,17Th. Muller,26

R. Mumford,25P. Murat,17M. Mussini,5J. Nachtman,17Y. Nagai,54A. Nagano,54J. Naganoma,56K. Nakamura,54

(3)

I. Nakano, A. Napier, V. Necula, C. Neu, M. S. Neubauer, J. Nielsen, L. Nodulman, M. Norman, O. Norniella,24E. Nurse,30S. H. Oh,16Y. D. Oh,27I. Oksuzian,18T. Okusawa,40R. Oldeman,29R. Orava,23K. Osterberg,23 S. Pagan Griso,42C. Pagliarone,45E. Palencia,17V. Papadimitriou,17A. Papaikonomou,26A. A. Paramonov,13B. Parks,38

S. Pashapour,33J. Patrick,17G. Pauletta,53M. Paulini,12C. Paus,32D. E. Pellett,7A. Penzo,53T. J. Phillips,16 G. Piacentino,45J. Piedra,43L. Pinera,18K. Pitts,24C. Plager,8L. Pondrom,58X. Portell,3O. Poukhov,15N. Pounder,41

F. Prakoshyn,15A. Pronko,17J. Proudfoot,2F. Ptohos,17,hG. Punzi,45J. Pursley,58J. Rademacker,41,cA. Rahaman,46 V. Ramakrishnan,58N. Ranjan,47I. Redondo,31B. Reisert,17V. Rekovic,36P. Renton,41M. Rescigno,50S. Richter,26 F. Rimondi,5L. Ristori,45A. Robson,21T. Rodrigo,11E. Rogers,24S. Rolli,55R. Roser,17M. Rossi,53R. Rossin,10P. Roy,33 A. Ruiz,11J. Russ,12V. Rusu,17H. Saarikko,23A. Safonov,52W. K. Sakumoto,48G. Salamanna,50O. Salto´,3L. Santi,53 S. Sarkar,50L. Sartori,45K. Sato,17A. Savoy-Navarro,43T. Scheidle,26P. Schlabach,17E. E. Schmidt,17M. A. Schmidt,13

M. P. Schmidt,59M. Schmitt,37T. Schwarz,7L. Scodellaro,11A. L. Scott,10A. Scribano,45F. Scuri,45A. Sedov,47 S. Seidel,36Y. Seiya,40A. Semenov,15L. Sexton-Kennedy,17A. Sfyria,20S. Z. Shalhout,57M. D. Shapiro,28T. Shears,29

P. F. Shepard,46D. Sherman,22M. Shimojima,54,nM. Shochet,13Y. Shon,58I. Shreyber,20A. Sidoti,45P. Sinervo,33 A. Sisakyan,15A. J. Slaughter,17J. Slaunwhite,38K. Sliwa,55J. R. Smith,7F. D. Snider,17R. Snihur,33M. Soderberg,34

A. Soha,7S. Somalwar,51V. Sorin,35J. Spalding,17F. Spinella,45T. Spreitzer,33P. Squillacioti,45M. Stanitzki,59 R. St. Denis,21B. Stelzer,8O. Stelzer-Chilton,41D. Stentz,37J. Strologas,36D. Stuart,10J. S. Suh,27A. Sukhanov,18 H. Sun,55I. Suslov,15T. Suzuki,54A. Taffard,24,eR. Takashima,39Y. Takeuchi,54R. Tanaka,39M. Tecchio,34P. K. Teng,1 K. Terashi,49J. Thom,17,gA. S. Thompson,21G. A. Thompson,24E. Thomson,44P. Tipton,59V. Tiwari,12S. Tkaczyk,17 D. Toback,52S. Tokar,14K. Tollefson,35T. Tomura,54D. Tonelli,17S. Torre,19D. Torretta,17S. Tourneur,43W. Trischuk,33

Y. Tu,44N. Turini,45F. Ukegawa,54S. Uozumi,54S. Vallecorsa,20N. van Remortel,23A. Varganov,34E. Vataga,36 F. Va´zquez,18,lG. Velev,17C. Vellidis,45,aV. Veszpremi,47M. Vidal,31R. Vidal,17I. Vila,11R. Vilar,11T. Vine,30 M. Vogel,36I. Volobouev,28,qG. Volpi,45F. Wu¨rthwein,9P. Wagner,44R. G. Wagner,2R. L. Wagner,17J. Wagner-Kuhr,26 W. Wagner,26T. Wakisaka,40R. Wallny,8S. M. Wang,1A. Warburton,33D. Waters,30M. Weinberger,52W. C. Wester III,17

B. Whitehouse,55D. Whiteson,44,eA. B. Wicklund,2E. Wicklund,17G. Williams,33H. H. Williams,44P. Wilson,17 B. L. Winer,38P. Wittich,17,gS. Wolbers,17C. Wolfe,13T. Wright,34X. Wu,20S. M. Wynne,29A. Yagil,9K. Yamamoto,40 J. Yamaoka,51T. Yamashita,39C. Yang,59U. K. Yang,13,mY. C. Yang,27W. M. Yao,28G. P. Yeh,17J. Yoh,17K. Yorita,13

T. Yoshida,40G. B. Yu,48I. Yu,27S. S. Yu,17J. C. Yun,17L. Zanello,50A. Zanetti,53I. Zaw,22X. Zhang,24 Y. Zheng,8,band S. Zucchelli5

(CDF Collaboration)

1Institute of Physics, Academia Sinica, Taipei, Taiwan 11529, Republic of China

2Argonne National Laboratory, Argonne, Illinois 60439, USA

3Institut de Fisica d’Altes Energies, Universitat Autonoma de Barcelona, E-08193, Bellaterra (Barcelona), Spain

4Baylor University, Waco, Texas 76798, USA

5Istituto Nazionale di Fisica Nucleare, University of Bologna, I-40127 Bologna, Italy

6Brandeis University, Waltham, Massachusetts 02254, USA

7University of California, Davis, Davis, California 95616, USA

8University of California, Los Angeles, Los Angeles, California 90024, USA

9University of California, San Diego, La Jolla, California 92093, USA

10University of California, Santa Barbara, Santa Barbara, California 93106, USA

11Instituto de Fisica de Cantabria, CSIC-University of Cantabria, 39005 Santander, Spain

12Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA

13Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA

14Comenius University, 842 48 Bratislava, Slovakia; Institute of Experimental Physics, 040 01 Kosice, Slovakia

15Joint Institute for Nuclear Research, RU-141980 Dubna, Russia

16Duke University, Durham, North Carolina 27708

17Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA

18University of Florida, Gainesville, Florida 32611, USA

19Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, I-00044 Frascati, Italy

20University of Geneva, CH-1211 Geneva 4, Switzerland

21Glasgow University, Glasgow G12 8QQ, United Kingdom

22Harvard University, Cambridge, Massachusetts 02138, USA

23Division of High Energy Physics, Department of Physics, University of Helsinki and Helsinki Institute of Physics, FIN-00014, Helsinki, Finland

062005-2

(4)

24University of Illinois, Urbana, Illinois 61801, USA

25The Johns Hopkins University, Baltimore, Maryland 21218, USA

26Institut fu¨r Experimentelle Kernphysik, Universita¨t Karlsruhe, 76128 Karlsruhe, Germany

27Center for High Energy Physics: Kyungpook National University, Daegu 702-701, Korea;

Seoul National University, Seoul 151-742, Korea;

Sungkyunkwan University, Suwon 440-746, Korea;

Korea Institute of Science and Technology Information, Daejeon, 305-806, Korea;

Chonnam National University, Gwangju, 500-757, Korea

28Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

29University of Liverpool, Liverpool L69 7ZE, United Kingdom

30University College London, London WC1E 6BT, United Kingdom

31Centro de Investigaciones Energeticas Medioambientales y Tecnologicas, E-28040 Madrid, Spain

32Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

33Institute of Particle Physics: McGill University, Montre´al, Canada H3A 2T8;

and University of Toronto, Toronto, Canada M5S 1A7

34University of Michigan, Ann Arbor, Michigan 48109, USA

35Michigan State University, East Lansing, Michigan 48824, USA

36University of New Mexico, Albuquerque, New Mexico 87131, USA

37Northwestern University, Evanston, Illinois 60208, USA

38The Ohio State University, Columbus, Ohio 43210, USA

39Okayama University, Okayama 700-8530, Japan

40Osaka City University, Osaka 588, Japan

41University of Oxford, Oxford OX1 3RH, United Kingdom

42University of Padova, Istituto Nazionale di Fisica Nucleare, Sezione di Padova-Trento, I-35131 Padova, Italy

43LPNHE, Universite Pierre et Marie Curie/IN2P3-CNRS, UMR7585, Paris, F-75252 France

44University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

45Istituto Nazionale di Fisica Nucleare Pisa, Universities of Pisa, Siena and Scuola Normale Superiore, I-56127 Pisa, Italy

46University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA

47Purdue University, West Lafayette, Indiana 47907, USA

48University of Rochester, Rochester, New York 14627, USA

49The Rockefeller University, New York, New York 10021, USA

50Istituto Nazionale di Fisica Nucleare, Sezione di Roma 1, University of Rome ‘‘La Sapienza’’, I-00185 Roma, Italy

51Rutgers University, Piscataway, New Jersey 08855, USA

52Texas A&M University, College Station, Texas 77843, USA

53Istituto Nazionale di Fisica Nucleare, University of Trieste/Udine, Italy

54University of Tsukuba, Tsukuba, Ibaraki 305, Japan

55Tufts University, Medford, Massachusetts 02155, USA

56Waseda University, Tokyo 169, Japan

57Wayne State University, Detroit, Michigan 48201, USA

58University of Wisconsin, Madison, Wisconsin 53706, USA

59Yale University, New Haven, Connecticut 06520, USA (Received 22 October 2007; published 15 February 2008)

We report the first top-quark mass measurement that uses a cross-section constraint to improve the mass determination. This measurement is made with a dileptonttevent candidate sample collected with the Collider Detector II at Fermilab. From a data sample corresponding to an integrated luminosity of 1:2 fb1, we measure a top-quark mass of170:74:23:9stat 2:6syst 2:4theoryGeV=c2. The mea- surement without the cross-section constraint is169:75:24:9stat 3:1systGeV=c2.

DOI:10.1103/PhysRevLett.100.062005 PACS numbers: 14.65.Ha, 12.15.Ff, 13.85.Ni, 13.85.Qk

The top-quark mass Mt is a fundamental parameter in the standard model (SM). Together with the W-boson mass,Mtplaces constraints on the SM Higgs boson mass [1]. At hadron colliders, the top quarks are mainly pair produced via the strong interaction. Nearly every top quark decays into aW boson and abquark, and in the dilepton channel both W bosons decay to a charged lepton and a neutrino. The ttdilepton events have a small branching ratio, but they have a higher purity than single-lepton or all-hadronic final states. Because the two neutrinos in the

final state are not detected, the dilepton channel top mass fit is underconstrained. However, measuring the mass in this channel is important because it provides an indepen- dent measurement ofMtthat can be compared to measure- ments in other decay channels, allowing a consistency check of the tthypothesis. Previous measurements of Mt in the dilepton channel are described in [2–4].

The SM predicts thettcross section as a function of the top mass [5,6]. Therefore, the top mass can be determined from the observed event yield alone. By combining the

(5)

theoreticalttMtdependence with the top mass determi- nation from the event kinematics, we can use the cross- section information to improve the mass measurement, as reported in this Letter.

In this novel measurement, the constraint provided by the mass dependent theoreticalttcross section is combined with a ‘‘template method’’ in which a top-quark massmrtis reconstructed for each event and in which the distribu- tion ofmrtis compared with template distributions derived from simulation. We include the cross-section constraint while properly taking into account the top mass depen- dence of the acceptance and all the correlated systematic uncertainties.

The template method adopted here is an enhanced ver- sion of the ‘‘full kinematic analysis’’ described in [2]. The enhanced version treats b-tagged and nontagged events separately. This separation improves the expected statisti- cal uncertainty by 20%; this represents a significant im- provement over the previous analysis, which handled b-tagged and nontagged events as a single sample.

Introducing the cross-section constraint improves the ex- pected statistical uncertainty further by 20%. In this Letter, the measurement without the cross-section constraint will be referred to as the ‘‘traditional’’ measurement.

This measurement uses data collected by the CDF II detector corresponding to an integrated luminosity of 1:2 fb1. The CDF II detector [7] is a multipurpose particle detector at the pp Tevatron Collider. Charged particle trajectories are measured with a silicon detector and a drift chamber, which are immersed in a 1.4 T uniform magnetic field parallel to the beam directions. Electron, photon, and hadron energies are measured with electromagnetic and hadronic calorimeters. Muons are detected with drift chambers and scintillation counter hodoscopes located out- side the calorimeters. CDF employs cylindrical coordi- nates where is the polar angle with respect to the proton beam. Transverse energy and momentum are de- fined as ET Esin and pT psin, where E is the energy andpis the momentum.

The data for this analysis were collected using an in- clusive lepton trigger that required an electron or a muon withpT>18 GeV=c[8]. After the offline reconstruction, the dilepton events were selected using the selection de- scribed in [9]; the main selection criteria are two oppo- sitely charged leptons with pT>20 GeV=c [8], missing transverse energy [2] due to the undetected neutrinos (ET >25 GeV), and at least two jets withET >15 GeV.

The expected and observed numbers of events are summa- rized in TableI. After the event selection, the sample was divided into two subsamples with significantly different signal-to-background ratios. Theb-tagged sample includes 32 events in which at least one of the jets is identified as a b-quark candidate through the presence of a displaced vertex [10]. This subsample has an expected signal-to- background ratio of11:1. The nontagged sample comprises

45 events in which none of the jets is identified as ab-quark candidate. In this subsample the expected signal-to- background ratio is1:1.

Because the two neutrinos are not detected, the recon- struction of the top-quark mass from dilepton events is underconstrained. Top mass reconstruction can be accom- plished by considering a kinematic variable that is not observable on an event-by-event basis, but that has a predictable distribution independent of the top mass value.

In this analysis the distribution of ptzt, the longitudinal momentum of the ttsystem, was adopted as the variable.

Monte Carlo simulations, generated withPYTHIA[11] and the CDF II detector simulation [12], indicate that the distribution of ptzt is nearly independent of the top mass, and is described by a Gaussian distribution with a mean of zero and width of 195 GeV=c. The validity of the Monte Carlo simulation was tested with data from the leptonjets decay channel where ptzt can be explicitly reconstructed.

For each event, a top massmrt is reconstructed from the event kinematics as follows. The jet energies are corrected to correspond to the energies of the primarybquarks. After these jet energy corrections, the two Cartesian components of transverse missing momentum are taken as the sum of the neutrino transverse momentum components. Along with assumptions on the masses of the final state particles and additional constraints onMW80:4 GeV=c2,Mt Mt, andptzptzptzt, a top mass can be calculated [2].

A wide range of possibleptztvalues is incorporated by calculating the top mass 10 000 times. For each iteration, ptzt is randomly drawn from its expected distribution.

Similarly, the jet energies and ET are smeared according to their resolutions. For each iteration, if a solution is not found using the fixed values of MW and Mt, solutions within MW 80:43:0 GeV=c2 and MtMt 2:0 GeV=c2 are accepted.

For a given event, we obtain two distributions of pos- sible top-quark masses, each corresponding to a different lepton-jet pairing. The pairing which has the higher frac- tion of solutions is selected. This choice is correct for 70%

event selection criteria. Statistical and systematic uncertainties have been combined.

Expected background

Diboson 5:80:9

Z=!ll,le,, 10:92:3

Misidentified leptons 8:83:9

Total 25:65:5

Expected signal ttM t170 GeV=c2 62:14:3

Total expected 87:78:9

Data 77

062005-4

(6)

of simulated tt events. Events with fewer than 100 solu- tions are rejected. According to Monte Carlo studies, 91%

of signal and 78% of background events pass this mass reconstruction requirement. The most probable value of a spline fit to the distribution selected is taken as a per-event top massmrt.

Templates of reconstructed top mass distributions were created from various ttand background samples. Signal templates were generated from tt Monte Carlo samples with generated top masses ranging from 150 to 200 GeV=c2, separately forb-tagged and nontagged signal events. Diboson andZ!lltemplates were generated from Monte Carlo simulation. A template for misidentified lep- tons was created using data. The background templates were combined according to the expected contribution of each background source. It was observed from simulation that using the same common background template for b-tagged and nontagged samples provides as good a per- formance as using separate templates. The common back- ground template was therefore used for both subsamples.

The templates were parametrized to form continuous probability density functions [2].

In the traditional measurement, the top mass is extracted by comparing the reconstructed mass distributions from data to the signal and background template parametriza- tions using an unbinned likelihood fit. The likelihood in- cludes free parameters for the number of signal eventsns and background eventsnb in each subsample, and for the top massMt. The total likelihood takes the form

L Lb-taggedMt; nbs; nbbLnon-taggedMt; nnons ; nnonb ; (1) where each of the subsample likelihoods is as the like- lihood function described in [2]. The top-quark mass hy- pothesis which minimizeslnLis taken.

To test the method, we performed Monte Carlo experi- ments of signal and background events. The numbers of signal and background events in each experiment were varied according to Poisson distributions using the ex- pected mean numbers of events. According to the Monte Carlo experiments, the method is unbiased and returns appropriate uncertainties.

In 1:2 fb1 of data, 31 b-tagged and 39 nontagged events pass the event selection criteria and have solu- tions formrt. Applying the traditional method to the two subsamples [see Eq. (1)], we measure Mt 169:75:24:9statGeV=c2. The reconstructed top mass distri- bution from data is shown in Fig.1.

The top mass measurement can be improved by taking into account the top mass dependence of thettproduction cross section. The expected number of signal events can be expressed as

nsMt ttMtaMtLprm; (2) where ttMtis the theoretical ttcross section,aMtis

the acceptance ofttevents,Lis the integrated luminosity, andprm is the probability of obtaining a solution formrt.

The principal dependence on the top-quark mass in Eq. (2) arises fromtt. We use a NLO calculation oftt

evaluated at three different top masses [5]; we parametrize the mass dependence of tt on the top mass using the functional form described in [6]:

ttMt 6:70e175Mt=32:29pb: (3) The acceptanceaMtwas studied usingttMonte Carlo simulation, separately for b-tagged and nontagged samples. The Monte Carlo acceptances were corrected for trigger efficiencies and for scale factors arising from differences between data and simulation. The combined Monte Carlo acceptance corrections are between 74% and 95%, depending on the lepton flavor and pseudorapidity.

The dependence of the acceptance on the top mass is linear, increasing about 30% in the top mass range of 150 to 200 GeV=c2. The integrated luminosity, L, is 1118 67 pb1 for theb-tagged sample and118971 pb1 for the nontagged sample. The signal mass reconstruction probability, prm, was measured to be 911:1% for both b-tagged and nontagged samples, and was found to be independent of the top mass.

The cross-section-constrained top mass measurement uses information from the reconstructed top mass dis- tribution as well as the observed number of events. The per-event mass reconstruction method and the tem- plate parametrizations are the same as in the tradi- tional measurement. The information from the number of events is added to the likelihood function by replac- ing ns in Eq. (1) with nsMt from Eq. (2); thus L Lb-taggedMt; nbbLnon-taggedMt; nnonb . The number of back- ground eventsnband the top massMtare free fit parame- ters as in the likelihood function of the traditional

2 ) Reconstructed Mass ( GeV/c

100 150 200 250 300 350

)2 Events / (10.5 GeV/c

0 5 10

70 data events signal+bckg bckg

FIG. 1 (color online). Reconstructed top mass distribution from data together with the signal and background parametriza- tions.

(7)

measurement. The uncertainty in the theoretical modeling ofttis not included in the likelihood; it is treated in the same way as other systematic uncertainties described below.

Simulated experiments are used to verify that the cross-section-constrained method is unbiased and re- turns appropriate uncertainties. We measure Mt 170:74:23:9statGeV=c2. The statistical uncertainty is con- sistent with expectations.

The sources of systematic uncertainties are summarized in TableII. The jet energy scale uncertainty is dominated by the uncertainty in jet energy corrections. This uncer- tainty was studied by shifting the jet energies by1, and half of the mass difference was taken as the systematic uncertainty. Since the jet energy corrections were deter- mined for light quark jets, we evaluated an additional systematic uncertainty from possible differences between bjets and light quark jets [13]. The total uncertainty from the jet energy scale is 1:82:9GeV=c2 for the cross-sec- tion-constrained (traditional) measurement. The cross-sec- tion-constrained measurement is less sensitive to the jet energy corrections because a change in the jet energy scale shifts the top mass determination from the event yield in the opposite direction to that from kinematic reconstruc- tion. The signal modeling uncertainty is0:90:8GeV=c2, and takes into account differences in parton showering between the PYTHIA [11] and HERWIG [14] Monte Carlo generators, uncertainties in initial and final state radiation modeling, and differences in parton distribution functions between MRST [15] and the full set of CTEQ6M [16]

eigenvectors. Possible imperfections in modeling theZ! ll and misidentified lepton backgrounds combine to give 0:30:3 GeV=c2 background modeling uncertainty. The contribution from uncertainties in background composition amounts to0:3GeV=c2. The uncertainty from template statistics is 0:40:5GeV=c2. A 1% uncertainty in the lepton pT introduces an uncertainty of 0:20:2GeV=c2. The cross-section-constrained measurement has an addi- tional uncertainty of1:6 GeV=c2 from the expected num- ber of events. This uncertainty includes 1:1 GeV=c2

uncertainty from the integrated luminosity, 0:5 GeV=c from the acceptance,0:9 GeV=c2 from the expected num- ber of background events (including relative background composition) and 0:5 GeV=c2 from the mass reconstruc- tion probability.

The uncertainty in the theoretical ttMt 175 GeV=c2 is 0:71–0:88 pb [5]. We propagated this uncertainty to the top mass by changing the number of signal events in the Monte Carlo experiments. The estimated uncertainty on the top mass is 2:4 GeV=c2. Simulation studies show that this cross-section-constrained top mass measurement is not very sensitive to the proba- bility shape of the theoretical tt uncertainty. Figure 2 shows the cross-section-constrained top mass measure- ment in the Mttt plane. The extracted top mass from the cross-section measurement [17] only is 178:310:18:0 exp4:05:8theoryGeV=c2, consistent within about 1 standard deviation with the result from the tradi- tional analysis.

In summary, we have introduced a new way to improve the template top mass measurement in the dilepton channel by using a theoretical cross-section constraint. With this measurement, we compare the reconstructed top mass distribution to templates and the observed number of events to expectation. In1:2 fb1 of data collected by the CDF II detector, we measure a top-quark mass of 170:74:23:9stat 2:6syst 2:4theory GeV=c2. This measurement is in good agreement with the top mass measurement made without a cross-section constraint, which gives169:75:24:9stat 3:1systGeV=c2, and with

2) (GeV/c Mt

150 155 160 165 170 175 180 185 190 195 200 (pb) ttσ

0 2 4 6 8 10 12 14 16

t σt theoretical

t σt measured

dep.

t σt , no measured Mt

dep.

t σt t, measured M

FIG. 2 (color online). The measured cross-section-constrained top mass is shown in the Mttt plane. The innermost error bars correspond to the statistical uncertainty, the middle ones the statisticalsystematic uncertainty, and the outermost error bars show the statisticalsystematictheory uncertainty. The hatched areas mark the traditional top mass measurement and the tt measurement in the dilepton channel with statistical systematic uncertainties.

TABLE II. Summary of systematic uncertainties for the tradi- tional (T) and cross-section-constrained (C) measurements.

Systematic Source Mt (GeV=c2)

T C

Jet energy scale 2.9 1.8

Signal modeling 0.8 0.9

Background modeling 0.3 0.3

Background composition 0.3 n.a

Template statistics 0.5 0.4

LeptonpT 0.2 0.2

Expected number of events n.a 1.6

Total 3.1 2.6

062005-6

(8)

top-quark mass measurements made in other decay chan- nels [18–20].

We thank the Fermilab staff and the technical staffs of the participating institutions for their vital contributions.

This work was supported by the U.S. Department of Energy and National Science Foundation; the Italian Istituto Nazionale di Fisica Nucleare; the Ministry of Education, Culture, Sports, Science and Technology of Japan; the Natural Sciences and Engineering Research Council of Canada; the National Science Council of the Republic of China; the Swiss National Science Founda- tion; the A. P. Sloan Foundation; the Bundesministerium fu¨r Bildung und Forschung, Germany; the Korean Science and Engineering Foundation and the Korean Research Foundation; the Science and Technology Facilities Council and the Royal Society, U.K.; the Institut National de Physique Nucleaire et Physique des Particules/CNRS; the Russian Foundation for Basic Research; the Comisio´n Interministerial de Ciencia y Tecnologı´a, Spain; the European Community’s Human Potential Programme; the Slovak R&D Agency; and the Academy of Finland.

aVisitor from University of Athens, 15784 Athens, Greece.

bVisitor from Chinese Academy of Sciences, Beijing 100864, China.

cVisitor from University of Bristol, Bristol BS8 1TL, U.K.

dVisitor from University Libre de Bruxelles, B-1050 Brussels, Belgium.

eVisitor from University of California Irvine, Irvine, CA 92697, USA.

fVisitor from University of California Santa Cruz, Santa Cruz, CA 95064, USA.

gVisitor from Cornell University, Ithaca, NY 14853, USA.

hVisitor from University of Cyprus, Nicosia CY-1678, Cyprus.

iVisitor from University College Dublin, Dublin 4, Ireland.

jVisitor from University of Edinburgh, Edinburgh EH9 3JZ, U.K.

kVisitor from University of Heidelberg, D-69120 Heidelberg, Germany.

lVisitor from Universidad Iberoamericana, Mexico D.F., Mexico.

mVisitor from University of Manchester, Manchester M13 9PL, U.K.

nVisitor from Nagasaki Institute of Applied Science, Nagasaki, Japan.

oVisitor from University de Oviedo, E-33007 Oviedo, Spain.

pVisitor from Queen Mary, University of London, London, E1 4NS, U.K.

qVisitor from Texas Tech University, Lubbock, TX 79409, USA.

rVisitor from IFIC (CSIC-Universitat de Valencia), 46071 Valencia, Spain.

[1] LEP Collaborations, LEP Electroweak Working Group, SLD Electroweak, and Heavy Flavor Groups, CERN Report No. CERN-PH-EP/2006-042.

[2] A. Abulenciaet al.(CDF Collaboration), Phys. Rev. D73, 112006 (2006).

[3] A. Abulenciaet al.(CDF Collaboration), Phys. Rev. D75, 031105 (2007).

[4] V. M. Abazovet al.(D0 Collaboration), Phys. Lett. B655, 7 (2007).

[5] M. Cacciariet al., J. High Energy Phys. 04 (2004) 068.

[6] S. Cataniet al., Phys. Lett. B378, 329 (1996).

[7] D. Acosta et al.(CDF Collaboration), Phys. Rev. D71, 032001 (2005).

[8] For electrons, transverse energy is used.

[9] D. Acostaet al.(CDF Collaboration), Phys. Rev. Lett.93, 142001 (2004).

[10] T. Affolderet al.(CDF Collaboration), Phys. Rev. D64, 032002 (2001).

[11] T. Sjostrand et al., Comput. Phys. Commun. 135, 238 (2001).

[12] T. Affolderet al., Nucl. Instrum. Methods Phys. Res., Sect.

A447, 1 (2000).

[13] A. Abulenciaet al.(CDF Collaboration), Phys. Rev. D73, 032003 (2006).

[14] G. Corcellaet al., J. High Energy Phys. 01 (2001) 10.

[15] A. D. Martinet al., Phys. Lett. B356, 89 (1995).

[16] J. Pumplinet al., J. High Energy Phys. 07 (2002) 012.

[17] M. Datta for the (CDF and D0 Collaborations), Proceedings of Hadron Collider Physics Symposium 2007 (unpublished).

[18] T. Aaltonenet al.(CDF Collaboration), Phys. Rev. Lett.

99, 182002 (2007).

[19] T. Aaltonenet al.(CDF Collaboration), Phys. Rev. D76, 072009 (2007).

[20] V. M. Abazovet al.(D0 Collaboration), Phys. Rev. D74, 092005 (2006).

Références

Documents relatifs

First, a visible tt cross section σ tt vis , defined for a phase space corresponding to the experimentally accessible fidu- cial volume, as described in Sect. 6, is determined. For

35 ( a ) Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; ( b ) Department of Modern Physics, University of Science and Technology of China, Anhui; ( c

The new method is already being applied to data being collected by the CDF and DØ experiments at the new run of the Fermilab Tevatron and should provide even higher precision on

events for several input values for the top quark mass used in the simulation. The overlayed curves are predictions from the param- etrization of templates at 18 different top

The measured statistical uncertainty is consistent with the distribution of statistical uncertainties in Monte Carlo experiments where signal events with M t 165 GeV=c 2 are

The method described above is checked for any possible systematic biases by running large numbers of ‘‘pseudoex- periments,’’ where we create, using Monte Carlo simula- tion,

The distributions of reconstructed top quark masses obtained from the data are compared with simulated mass distributions (templates) for signal and background events, and

A systematic uncertainty is estimated for each jet energy correction by performing Monte Carlo experiments drawn from simulated signal and background events with 1 standard deviation