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Measurement of the p(p)over-bar -> t(t)over-bar + X production cross section at root s=1.96 TeV in the fully hadronic decay channel

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Measurement of the p 

p ! t 

t  X production cross section at

p



s

 1:96 TeV

in the fully hadronic decay channel

V. M. Abazov,35B. Abbott,75M. Abolins,65B. S. Acharya,28M. Adams,51T. Adams,49E. Aguilo,5S. H. Ahn,30 M. Ahsan,59G. D. Alexeev,35G. Alkhazov,39A. Alton,64,*G. Alverson,63G. A. Alves,2M. Anastasoaie,34L. S. Ancu,34

T. Andeen,53S. Anderson,45B. Andrieu,16M. S. Anzelc,53Y. Arnoud,13M. Arov,52A. Askew,49B. A˚ sman,40 A. C. S. Assis Jesus,3O. Atramentov,49C. Autermann,20C. Avila,7C. Ay,23F. Badaud,12A. Baden,61L. Bagby,52 B. Baldin,50D. V. Bandurin,59P. Banerjee,28S. Banerjee,28E. Barberis,63P. Bargassa,80P. Baringer,58C. Barnes,43

J. Barreto,2J. F. Bartlett,50U. Bassler,16D. Bauer,43S. Beale,5A. Bean,58M. Begalli,3M. Begel,71

C. Belanger-Champagne,40L. Bellantoni,50A. Bellavance,67J. A. Benitez,65S. B. Beri,26G. Bernardi,16R. Bernhard,22 L. Berntzon,14I. Bertram,42M. Besanc¸on,17R. Beuselinck,43V. A. Bezzubov,38P. C. Bhat,50V. Bhatnagar,26M. Binder,24 C. Biscarat,19I. Blackler,43G. Blazey,52F. Blekman,43S. Blessing,49D. Bloch,18K. Bloom,67A. Boehnlein,50D. Boline,62 T. A. Bolton,59G. Borissov,42K. Bos,33T. Bose,77A. Brandt,78R. Brock,65G. Brooijmans,70A. Bross,50D. Brown,78

N. J. Buchanan,49D. Buchholz,53M. Buehler,81V. Buescher,22S. Burdin,50S. Burke,45T. H. Burnett,82E. Busato,16 C. P. Buszello,43J. M. Butler,62P. Calfayan,24S. Calvet,14J. Cammin,71S. Caron,33W. Carvalho,3B. C. K. Casey,77 N. M. Cason,55H. Castilla-Valdez,32S. Chakrabarti,17D. Chakraborty,52K. M. Chan,71A. Chandra,48F. Charles,18

E. Cheu,45F. Chevallier,13D. K. Cho,62S. Choi,31B. Choudhary,27L. Christofek,77D. Claes,67B. Cle´ment,18 C. Cle´ment,40Y. Coadou,5M. Cooke,80W. E. Cooper,50M. Corcoran,80F. Couderc,17M.-C. Cousinou,14B. Cox,44 S. Cre´pe´-Renaudin,13D. Cutts,77M. C´ wiok,29H. da Motta,2A. Das,62M. Das,60B. Davies,42G. Davies,43K. De,78

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Y. Gershtein,49D. Gillberg,5G. Ginther,71N. Gollub,40B. Go´mez,7A. Goussiou,55P. D. Grannis,72H. Greenlee,50 Z. D. Greenwood,60E. M. Gregores,4G. Grenier,19Ph. Gris,12J.-F. Grivaz,15A. Grohsjean,24S. Gru¨nendahl,50 M. W. Gru¨newald,29F. Guo,72J. Guo,72G. Gutierrez,50P. Gutierrez,75A. Haas,70N. J. Hadley,61P. Haefner,24 S. Hagopian,49J. Haley,68I. Hall,75R. E. Hall,47L. Han,6K. Hanagaki,50P. Hansson,40K. Harder,44A. Harel,71

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V. Hynek,8I. Iashvili,69R. Illingworth,50A. S. Ito,50S. Jabeen,62M. Jaffre´,15S. Jain,75K. Jakobs,22C. Jarvis,61 A. Jenkins,43R. Jesik,43K. Johns,45C. Johnson,70M. Johnson,50A. Jonckheere,50P. Jonsson,43A. Juste,50D. Ka¨fer,20 S. Kahn,73E. Kajfasz,14A. M. Kalinin,35J. M. Kalk,60J. R. Kalk,65S. Kappler,20D. Karmanov,37J. Kasper,62P. Kasper,50

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T. Kuhl,23A. Kumar,69S. Kunori,61A. Kupco,10T. Kurcˇa,19J. Kvita,8D. Lam,55S. Lammers,70G. Landsberg,77 J. Lazoflores,49A.-C. Le Bihan,18P. Lebrun,19W. M. Lee,50A. Leflat,37F. Lehner,41V. Lesne,12J. Leveque,45P. Lewis,43 J. Li,78L. Li,48Q. Z. Li,50S. M. Lietti,4J. G. R. Lima,52D. Lincoln,50J. Linnemann,65V. V. Lipaev,38R. Lipton,50Z. Liu,5

L. Lobo,43A. Lobodenko,39M. Lokajicek,10A. Lounis,18P. Love,42H. J. Lubatti,82M. Lynker,55A. L. Lyon,50 A. K. A. Maciel,2R. J. Madaras,46P. Ma¨ttig,25C. Magass,20A. Magerkurth,64N. Makovec,15P. K. Mal,55 H. B. Malbouisson,3S. Malik,67V. L. Malyshev,35H. S. Mao,50Y. Maravin,59R. McCarthy,72A. Melnitchouk,66 A. Mendes,14L. Mendoza,7P. G. Mercadante,4M. Merkin,37K. W. Merritt,50A. Meyer,20J. Meyer,21M. Michaut,17 H. Miettinen,80T. Millet,19J. Mitrevski,70J. Molina,3R. K. Mommsen,44N. K. Mondal,28J. Monk,44R. W. Moore,5 T. Moulik,58G. S. Muanza,19M. Mulders,50M. Mulhearn,70O. Mundal,22L. Mundim,3E. Nagy,14M. Naimuddin,27 M. Narain,62N. A. Naumann,34H. A. Neal,64J. P. Negret,7P. Neustroev,39C. Noeding,22A. Nomerotski,50S. F. Novaes,4

T. Nunnemann,24V. O’Dell,50D. C. O’Neil,5G. Obrant,39C. Ochando,15V. Oguri,3N. Oliveira,3D. Onoprienko,59 N. Oshima,50J. Osta,55R. Otec,9G. J. Otero y Garzo´n,51M. Owen,44P. Padley,80M. Pangilinan,62N. Parashar,56

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S.-J. Park,71S. K. Park,30J. Parsons,70R. Partridge,77N. Parua,72A. Patwa,73G. Pawloski,80P. M. Perea,48K. Peters,44 Y. Peters,25P. Pe´troff,15M. Petteni,43R. Piegaia,1J. Piper,65M.-A. Pleier,21P. L. M. Podesta-Lerma,32V. M. Podstavkov,50 Y. Pogorelov,55M.-E. Pol,2A. Pomposˇ,75B. G. Pope,65A. V. Popov,38C. Potter,5W. L. Prado da Silva,3H. B. Prosper,49 S. Protopopescu,73J. Qian,64A. Quadt,21B. Quinn,66M. S. Rangel,2K. J. Rani,28K. Ranjan,27P. N. Ratoff,42P. Renkel,79

S. Reucroft,63M. Rijssenbeek,72I. Ripp-Baudot,18F. Rizatdinova,76S. Robinson,43R. F. Rodrigues,3C. Royon,17 P. Rubinov,50R. Ruchti,55G. Sajot,13A. Sa´nchez-Herna´ndez,32M. P. Sanders,16A. Santoro,3G. Savage,50L. Sawyer,60

T. Scanlon,43D. Schaile,24R. D. Schamberger,72Y. Scheglov,39H. Schellman,53P. Schieferdecker,24C. Schmitt,25 C. Schwanenberger,44A. Schwartzman,68R. Schwienhorst,65J. Sekaric,49S. Sengupta,49H. Severini,75E. Shabalina,51

M. Shamim,59V. Shary,17A. A. Shchukin,38R. K. Shivpuri,27D. Shpakov,50V. Siccardi,18R. A. Sidwell,59V. Simak,9 V. Sirotenko,50P. Skubic,75P. Slattery,71R. P. Smith,50G. R. Snow,67J. Snow,74S. Snyder,73S. So¨ldner-Rembold,44

X. Song,52L. Sonnenschein,16A. Sopczak,42M. Sosebee,78K. Soustruznik,8M. Souza,2B. Spurlock,78J. Stark,13 J. Steele,60V. Stolin,36A. Stone,51D. A. Stoyanova,38J. Strandberg,64S. Strandberg,40M. A. Strang,69M. Strauss,75

R. Stro¨hmer,24D. Strom,53M. Strovink,46L. Stutte,50S. Sumowidagdo,49P. Svoisky,55A. Sznajder,3M. Talby,14 P. Tamburello,45W. Taylor,5P. Telford,44J. Temple,45B. Tiller,24M. Titov,22V. V. Tokmenin,35M. Tomoto,50T. Toole,61 I. Torchiani,22T. Trefzger,23S. Trincaz-Duvoid,16D. Tsybychev,72B. Tuchming,17C. Tully,68P. M. Tuts,70R. Unalan,65

L. Uvarov,39S. Uvarov,39S. Uzunyan,52B. Vachon,5P. J. van den Berg,33B. van Eijk,35R. Van Kooten,54 W. M. van Leeuwen,33N. Varelas,51E. W. Varnes,45A. Vartapetian,78I. A. Vasilyev,38M. Vaupel,25P. Verdier,19

L. S. Vertogradov,35M. Verzocchi,50F. Villeneuve-Seguier,43P. Vint,43J.-R. Vlimant,16E. Von Toerne,59 M. Voutilainen,67,†M. Vreeswijk,33H. D. Wahl,49L. Wang,61M. H. L. S. Wang,50J. Warchol,55G. Watts,82M. Wayne,55

G. Weber,23M. Weber,50H. Weerts,65N. Wermes,21M. Wetstein,61A. White,78D. Wicke,25G. W. Wilson,58 S. J. Wimpenny,48M. Wobisch,50J. Womersley,50D. R. Wood,63T. R. Wyatt,44Y. Xie,77S. Yacoob,53R. Yamada,50

M. Yan,61T. Yasuda,50Y. A. Yatsunenko,35K. Yip,73H. D. Yoo,77S. W. Youn,53C. Yu,13J. Yu,78A. Yurkewicz,72 A. Zatserklyaniy,52C. Zeitnitz,25D. Zhang,50T. Zhao,82B. Zhou,64J. Zhu,72M. Zielinski,71D. Zieminska,54

A. Zieminski,54V. Zutshi,52and E. G. Zverev37

(D0 Collaboration)

1Universidad de Buenos Aires, Buenos Aires, Argentina 2LAFEX, Centro Brasileiro de Pesquisas Fı´sicas, Rio de Janeiro, Brazil

3Universidade do Estado do Rio de Janeiro, Rio de Janeiro, Brazil 4Instituto de Fı´sica Teo´rica, Universidade Estadual Paulista, Sa˜o Paulo, Brazil

5University of Alberta, Edmonton, Alberta, Canada,

Simon Fraser University, Burnaby, British Columbia, Canada, York University, Toronto, Ontario, Canada,

and McGill University, Montreal, Quebec, Canada

6University of Science and Technology of China, Hefei, People’s Republic of China 7Universidad de los Andes, Bogota´, Colombia

8Center for Particle Physics, Charles University, Prague, Czech Republic 9Czech Technical University, Prague, Czech Republic

10Center for Particle Physics, Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic 11Universidad San Francisco de Quito, Quito, Ecuador

12Laboratoire de Physique Corpusculaire, IN2P3-CNRS, Universite´ Blaise Pascal, Clermont-Ferrand, France 13Laboratoire de Physique Subatomique et de Cosmologie, IN2P3-CNRS, Universite de Grenoble 1, Grenoble, France

14CPPM, IN2P3-CNRS, Universite´ de la Me´diterrane´e, Marseille, France

15Laboratoire de l’Acce´le´rateur Line´aire, IN2P3-CNRS et Universite´ Paris-Sud, Orsay, France 16LPNHE, IN2P3-CNRS, Universite´s Paris VI and VII, Paris, France

17DAPNIA/Service de Physique des Particules, CEA, Saclay, France 18IPHC, IN2P3-CNRS, Universite´ Louis Pasteur, Strasbourg, France,

and Universite´ de Haute Alsace, Mulhouse, France

19Institut de Physique Nucle´aire de Lyon, IN2P3-CNRS, Universite´ Claude Bernard, Villeurbanne, France 20III. Physikalisches Institut A, RWTH Aachen, Aachen, Germany

21Physikalisches Institut, Universita¨t Bonn, Bonn, Germany 22Physikalisches Institut, Universita¨t Freiburg, Freiburg, Germany

23Institut fu¨r Physik, Universita¨t Mainz, Mainz, Germany 24Ludwig-Maximilians-Universita¨t Mu¨nchen, Mu¨nchen, Germany 25Fachbereich Physik, University of Wuppertal, Wuppertal, Germany

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26Panjab University, Chandigarh, India 27Delhi University, Delhi, India

28Tata Institute of Fundamental Research, Mumbai, India 29University College Dublin, Dublin, Ireland 30Korea Detector Laboratory, Korea University, Seoul, Korea

31SungKyunKwan University, Suwon, Korea 32CINVESTAV, Mexico City, Mexico

33FOM-Institute NIKHEF, Amsterdam, The Netherlands

and University of Amsterdam/NIKHEF, Amsterdam, The Netherlands

34Radboud University Nijmegen/NIKHEF, Nijmegen, The Netherlands 35Joint Institute for Nuclear Research, Dubna, Russia 36Institute for Theoretical and Experimental Physics, Moscow, Russia

37Moscow State University, Moscow, Russia 38Institute for High Energy Physics, Protvino, Russia 39Petersburg Nuclear Physics Institute, St. Petersburg, Russia

40Lund University, Lund, Sweden, Royal Institute of Technology and Stockholm University, Stockholm, Sweden

and Uppsala University, Uppsala, Sweden

41Physik Institut der Universita¨t Zu¨rich, Zu¨rich, Switzerland 42Lancaster University, Lancaster, United Kingdom

43Imperial College, London, United Kingdom 44University of Manchester, Manchester, United Kingdom

45University of Arizona, Tucson, Arizona 85721, USA

46Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

and University of California, Berkeley, California 94720, USA

47California State University, Fresno, California 93740, USA 48University of California, Riverside, California 92521, USA 49Florida State University, Tallahassee, Florida 32306, USA 50Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA

51University of Illinois at Chicago, Chicago, Illinois 60607, USA 52Northern Illinois University, DeKalb, Illinois 60115, USA

53Northwestern University, Evanston, Illinois 60208, USA 54Indiana University, Bloomington, Indiana 47405, USA 55University of Notre Dame, Notre Dame, Indiana 46556, USA

56Purdue University Calumet, Hammond, Indiana 46323, USA 57Iowa State University, Ames, Iowa 50011, USA 58University of Kansas, Lawrence, Kansas 66045, USA 59Kansas State University, Manhattan, Kansas 66506, USA 60Louisiana Tech University, Ruston, Louisiana 71272, USA 61University of Maryland, College Park, Maryland 20742, USA

62Boston University, Boston, Massachusetts 02215, USA 63Northeastern University, Boston, Massachusetts 02115, USA

64University of Michigan, Ann Arbor, Michigan 48109, USA 65Michigan State University, East Lansing, Michigan 48824, USA

66University of Mississippi, University, Mississippi 38677, USA 67University of Nebraska, Lincoln, Nebraska 68588, USA 68Princeton University, Princeton, New Jersey 08544, USA 69State University of New York, Buffalo, New York 14260, USA

70Columbia University, New York, New York 10027, USA 71University of Rochester, Rochester, New York 14627, USA 72State University of New York, Stony Brook, New York 11794, USA

73Brookhaven National Laboratory, Upton, New York 11973, USA 74Langston University, Langston, Oklahoma 73050, USA 75University of Oklahoma, Norman, Oklahoma 73019, USA 76Oklahoma State University, Stillwater, Oklahoma 74078, USA

77Brown University, Providence, Rhode Island 02912, USA 78University of Texas, Arlington, Texas 76019, USA 79Southern Methodist University, Dallas, Texas 75275, USA

Visitor from Helsinki Institute of Physics, Helsinki, Finland. *Visitor from Augustana College, Sioux Falls, SD, USA

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80Rice University, Houston, Texas 77005, USA 81University of Virginia, Charlottesville, Virginia 22901, USA

82University of Washington, Seattle, Washington 98195, USA (Received 18 December 2006; published 19 October 2007)

A measurement of the top quark pair production cross section in proton antiproton collisions at an interaction energy ofps 1:96 TeV is presented. This analysis uses 405  25 pb1 of data collected with the D0 detector at the Fermilab Tevatron Collider. Fully hadronic tt decays with final states of six or more jets are separated from the multijet background using secondary vertex tagging and a neural network. The tt cross section is measured as tt 4:52:01:9stat1:41:1syst  0:3lumi pb for a top quark mass of mt 175 GeV=c2.

DOI:10.1103/PhysRevD.76.072007 PACS numbers: 13.85.Lg, 13.85.Ni, 14.65.Ha

The standard model (SM) predicts that the top quark decays primarily into a W boson and a b quark. The measurement presented here tests the prediction of the SM in proton antiproton collisions at an interaction energy ofps 1:96 TeV. The measurement is performed in the dominant decay mode of the tt system: when both W bosons decay to quarks, the so-called fully hadronic decay channel. This topology occurs in 46% of tt events. The theoretical signature for fully hadronic tt events is six or more jets originating from the hadronization of the six quarks. Of the six jets, two originate from b quark decays. Fully hadronic tt events are difficult to identify at hadron colliders because the background rate is many orders of magnitude larger than that of the tt signal.

We report a measurement of the production cross section of top quark pairs, tt, that exploits the long lifetime of the

bhadrons in identifying b jets, using data collected with D0 in the fully hadronic channel. To increase the sensitivity for tt events, we used a neural network to distinguish the signal from the overwhelming background of multijet pro-duction through quantum chromodynamic processes (QCD).

The D0 detector [1] has a central tracking system con-sisting of a silicon micro strip tracker (SMT) and a central fiber tracker (CFT), both located within a 2 T supercon-ducting solenoidal magnet, with designs optimized for tracking and vertexing at pseudorapidities jj < 3 and jj < 2:5, respectively. Rapidity y and pseudorapidity  are defined as functions of the polar angle  and parameter

 as y;  1

2ln1   cos=1   cos and

  y; 1, where  is the ratio of the particle’s

momentum to its energy. The liquid-argon and uranium calorimeter has a central section (CC) covering pseudor-apidities jj up to 1:1 and two end calorimeters (EC) that extend coverage to jj 4:2, with all three housed in separate cryostats. Each calorimeter cryostat contains a multilayer electromagnetic calorimeter, a finely segmented hadronic calorimeter and a third hadronic calorimeter that is more coarsely segmented, providing both segmentation in depth and in projective towers of size 0:1 0:1 in - space, where  is the azimuthal angle in radians. An outer muon system, covering jj < 2, consists of a layer of

tracking detectors and scintillation trigger counters in front of 1.8 T iron toroids, followed by two similar layers after the toroids. The luminosity is measured using plastic scin-tillator arrays placed in front of the EC cryostats.

The data set was collected between 2002 and 2004 and corresponds to an integrated luminosity L  405  25 pb1 [2]. To isolate events with six jets, we used a dedicated multijet trigger. The requirements on the trigger, particularly on jet and trigger tower energy thresholds, were tightened during the collection of the data set to manage the increasing instantaneous luminosities deliv-ered by the Fermilab Tevatron Collider. The change in trigger requirements had little effect on the efficiency for signal, while removing an increasing number of back-ground events [3]. The trigger was tuned for the fully hadronic tt channel and was optimized to remain as effi-cient as possible while using limited bandwidth. The col-lection rate after all trigger levels was fixed to a few Hz, which was completely dominated by QCD multijet events as the hadronic tt event production rate is expected to be a few events per day. We required three or four trigger towers above a transverse energy threshold of 5 GeV at the first trigger level, three reconstructed jets with transverse en-ergies (ET) above 8 GeV at the second trigger level, com-bined with a requirement on the sum of the transverse momenta (pT) of the jets, and four or five reconstructed jets at transverse energy thresholds between 10 and 30 GeV at the highest trigger level [1].

We simulated tt production usingALPGEN 1.3to generate the parton-level processes andPYTHIA 6.2to model hadro-nization [4,5]. We used a top quark mass of mt 175 GeV=c2. The decay of hadrons carrying bottom

quarks was modeled using EVTGEN [6]. The simulated tt events were processed with the full GEANT-based D0 de-tector simulation, after which the Monte Carlo (MC) events were passed through the same reconstruction pro-gram as was used for data. The differences between the MC model and the data were very small and were corrected using factors derived from detailed comparisons between the MC model and the data for well understood SM pro-cesses such as the jets in Z boson and QCD dijet production.

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In the offline analysis, jets were defined with an iterative cone algorithm [7]. Before the jet algorithm was applied, calorimeter noise was suppressed by removing isolated cells whose measured energy was lower than 4 standard deviations above cell pedestal. In the case that a cell above this threshold was found to be adjacent to one with an energy less than 4 standard deviations above pedestal, the latter was retained if its signal exceeded 2.5 standard deviations above pedestal. Cells that were reconstructed with negative energies were always removed.

The elements for cone jet reconstruction consisted of projective towers of calorimeter cells. First, seeds were defined using a preclustering algorithm, using calorimeter towers above an energy threshold of 0.5 GeV. The cone jet reconstruction, an iterative clustering process where the jet axis was required to match the axis of a projective cone, was then run using all preclusters above 1.0 GeV as seeds. As jets from tt production are relatively narrow due to relatively high jet pT, the jets were defined using a cone with radius Rcone 0:5, where R py2 2.

The resulting jets (proto-jets) took into account all energy deposits contained in the jet cone. If two proto-jets were within 1 < R=Rcone< 2, an additional midpoint

cluster-ing was applied, where the combination of the two proto-jets was used as a seed for a possible additional proto-jet. At this stage, the proto-jets that share transverse momen-tum were examined with a splitting and merging algorithm, after which each calorimeter tower was assigned to one proto-jet at most. The proto-jets were merged if the shared

pTexceeded 50% of the pT of the proto-jet with the lowest transverse momentum and the towers were added to the most energetic proto-jet while the other candidate was rejected. If the proto-jets shared less than half of their

pT, the shared towers were individually assigned to the proto-jet which was closest in R space. The collection of stable proto-jets remaining was then referred to as the

reconstructed jets in the event. The minimal pT of a reconstructed jet was required to be 8 GeV=c before any energy corrections were applied.

We removed jets caused by electromagnetic particles and jets resulting from noise in hadronic sections of the calorimeter by requiring that the fraction of the jet energy deposited in the calorimeter was between 0.05 and 0.95 and the fraction of energy in the coarse hadronic calorimeter was less than 0.4. Jets formed from clusters of calorimeter cells known to be affected by noise were also rejected. The remaining noise contribution was removed by requiring that the jet also satisfied the first level trigger requirements. To correct the calorimeter jet energies back to the level of particle jets, a jet energy scale (JES) correction CJESwas

applied. The same procedure has to be applied to Monte Carlo jets to ensure an identical calorimeter re-sponse in data and simulation. The particle level or true jet energy Etruewas obtained from the measured jet energy

Em and the detector pseudorapidity, measured from the

center of the detector (det), using the relation

Etrue E m E 0det;L Rdet; EmSdet; Em  CJESEm;  det;L Em: (1) In data and MC the total correction was applied to the measured energy Em as a multiplicative factor CJES.

E0det;L was the offset energy created by electronics

noise and noise signal caused by the uranium in the calo-rimeter, pile-up energy from previous collisions, and the additional energy from the underlying physics event. The dependence on the luminosity L was caused by the fact that the number of additional interactions was dependent on the instantaneous luminosity, while the dependence on y was caused by variations in the calorimeter occupancy as a function of the jet rapidity.Rdet; Em parameterized the

energy response of the calorimeter, while Sdet; Em

rep-resents the fraction of the true particle jet energy that was deposited inside the jet cone. This out-of-cone showering correction depended on the energy of the jet and its loca-tion in the calorimeter.

The JES was measured directly in photon  jet events, which are quark dominated (like tt). The method was identical for data and simulation and used transverse mo-mentum balancing between the jet and the photon. As the energy scale of the photon was directly and precisely measured (the electromagnetic calorimeter response was derived from measurements of resonances in the ee

spectrum like the Z boson), the true jet energy could be derived from the difference between the photon and jet transverse momentum. E0,R, and S were fit as a function

of jet rapidity and measured energy, which lead to uncer-tainties coming from the fit (statistical) and the method (systematic). The total correction CJESwas approximately

1.4 for data jets in the energy range expected for jets associated with top quark events. The corrections for data and Monte Carlo simulation are in good agreement and the used systematic uncertainty cover for any possible differ-ence in scale. The systematic uncertainties on CJESwere of

the order of a few percent and depended on the jet energy and rapidity.

The jet energy resolution was measured in photon  jet data for low jet energies and dijet data for higher jet energy values. Fits to the transverse energy asymmetry pT1 

pT2=pT1  pT2 between the transverse momenta of the back-to-back jets and/or photon [pT1 and pT2] were then used to obtain the jet energy resolution as a function of jet rapidity and transverse energy. The uncer-tainties on the jet energy resolution were dominated by limited statistics in the samples used.

In this analysis, we considered a data set consisting of events with four or more reconstructed jets, in which the scalar sum of the uncorrected transverse momenta Huncorr

T of all the jets in the event was greater than 90 GeV=c. The final analysis sample was a subset of this sample, where at

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least six jets with corrected transverse momentum greater than 15 GeV=c and jyj < 2:5 were required. Events with isolated high transverse momentum electron or muon can-didates were vetoed to ensure that the all-hadronic and leptonic tt samples were disjoint [8,9]. In addition, we rejected events where two distinct p p interactions with separate primary vertices were observed and the jets in the event were not assigned to only one of the two primary vertices. The primary vertex requirement did not affect minimum bias interactions or tt events. Table I lists the efficiencies after the first set of selection cuts, commonly referred to as preselection, which includes the require-ments on the primary vertex, the number of reconstructed jets and the presence of isolated leptons, and the efficiency after preselection and after preselection and the trigger. Besides selecting all-hadronic tt events, the analysis was also expected to accept a small contribution from the semi-leptonic (lepton  jets) tt decay channel. The combined efficiency included the fully hadronic and semileptonic

W-boson branching fractions of 0:4619  0:0048 and 0:4349  0:0027 respectively [10].

We used a secondary vertex tagging algorithm (SVT) to identify b-quark jets. The algorithm was the same as that used in previously published D0 tt production cross section measurements [8,9]. Secondary vertex candidates were reconstructed from two or more tracks in the jet, removing vertices consistent with those having originated from long-lived light hadrons, for example K0

S and . Two configu-rations of the secondary vertex algorithm were used; these were labeled ‘‘loose’’ and ‘‘tight,’’ respectively. If a recon-structed secondary vertex in the jet had a transverse decay length Lxy significance Lxy=Lxy > 57, the jet was

tagged as a loose (tight) b-quark jet. The loose SVT was chosen to efficiently identify b-quark jets, while the tight SVT was configured to accept only very few light-quark jets while sacrificing a small reduction in the efficiency for

b-quark jets. Events with two or more loosely tagged jets were called double-tag events. The sample that did not contain two loosely tagged jets was inspected for events with one tight tag. Events thus isolated were labeled single-tag events. The fully exclusive samples of single-single-tag and double-tag events were treated separately because of their different signal-to-background ratios. The use of the tight SVT selection for single tagged events optimized the

re-jection of mistags; the main background in the single-tag analysis. When two tags were required, the background sample started to be dominated by direct b bproduction. The choice to use the loose SVT optimized the double-tag analysis for signal efficiency instead of background rejection.

Compared to light-quark QCD multijet events, tt events on average have more jets of higher energy and with less boost in the beam direction, resulting in events with many central jets that all have similar and relatively high ener-gies. Moreover, the fully hadronic decay makes it possible to reconstruct the W boson and t quark four-momenta. To distinguish between signal and background, we used the following event characteristics [11]:

(i) HT: The scalar sum of the corrected transverse mo-menta of the jets (Fig.1).

(ii) E56

T: The square root of the product of the transverse momenta of the fifth and sixth leading jet (Fig.2). (iii) A: The aplanarity as calculated from the

normal-ized momentum tensor (Fig.3) [8,9,11]. (iv) h2i: The p

T-weighted mean square of the y of the jets in an event (Fig.4), see also Ref. [11]. (v) M: The mass-2 variable, which was defined as

M  MW1 MW 2=2 MW MW2 MW 2=2 MW mt1 mt22=2

mt, where the parameters MW, MW,

and mtwere the invariant mass and mass resolution from the jet four-momenta calculated as observed in all-hadronic tt MC, respectively, 79, 11, and 21 GeV=c2 after all corrections and resolutions were included [12]. MWi and mti were calculated for every possible permutation of the jets in the event. We did not distinguish between tagged and untagged jets. The combination of jets that yielded the lowest value ofM is used (Fig.5).

(vi) M34

min: The second-smallest dijet mass in the event.

First, all possible dijet masses were considered and the jets that yield the smallest mass were rejected.

M34

minwas the smallest dijet mass as found from the

remaining jets (Fig.6).

The top quark production cross section was calculated from the output of NN, an artificial neural network trained to force its output near 1 for tt events and near 1 for QCD multijet events, using the multilayer perceptron in theROOT

analysis program [13]. The six parameters illustrated in TABLE I. Efficiency for selection criteria applied before b-jet identification. Efficiencies

listed include the efficiency for all previous selection criteria. The trigger efficiency is quoted for events that have passed the preselection. The uncertainties are due to Monte Carlo statistics. Listed are the selection efficiencies as determined for tt in the hadronic decay channel, the lepton  jets decay channel, and the efficiency for all different decay channels corrected for W boson branching fractions.

Cut tt !hadrons tt ! ‘ jets Any tt

Preselection 0:2706  0:0016 0:0311  0:0008 0:1385  0:0011

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Figs.1–6were used as input for the neural net. The input parameters were shown to be correlated in dedicated stud-ies used to select appropriate input for NN, where many different quantities were considered. The correlation be-tween the six quantities was observed to be smaller than

j0:20j, while the most powerful quantity for the discrimi-nation between signal and background was observed to be

HT. The very large background-to-signal ratio in the un-tagged data allowed us to use unun-tagged data as background input for the training of NN, while tt MC was used for the

0 20 40 60 80 100 events 0 1000 2000 0 00 20 40 60 80 100 200 400 600 800

ET56 [GeV] ET56 [GeV]

events

(a: 1 SVT tag ) (b: 2 SVT tag ) -1

D Run II 405 pb D Run II 405 pb-1

FIG. 2 (color online). The E56

T distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the

background (solid line), and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

0 0.1 0.2 0.3 0.4 0.5 events 0 500 1000 Aplanarity 0 0.1 0.2 0.3 0.4 0.5 0 100 200 300 400 Aplanarity 0 events

(a: 1 SVT tag ) (b: ≥2 SVT tag )

-1

D Run II 405 pb D Run II 405 pb-1

FIG. 3 (color online). TheA distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the background (solid line) and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

0 200 400 600 800 1000 events 500 1000 1500 -1 D Run II 405 pb (a: 1 SVT tag ) [GeV] T H 0 200 400 600 800 1000 0 200 400 600 [GeV] T H 0 events -1 D Run II 405 pb ) (b: 2 SVT tag )

FIG. 1 (color online). The HT distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the

background (solid line), and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

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signal. Figure 7shows the NN discriminant for tt signal and multijet background. Although the distributions for single- and double-tag events were different due to in-creased heavy flavor content in the double-tag sample,

both samples showed a clear discrimination between signal and background.

The overwhelming background also made it possible to use the entire (tagged and untagged) sample to estimate the

0 1 2 3 4 events 0 500 1000 > 2 η < 0 1 2 3 4 0 200 400 > 2 η < events

(a: 1 SVT tag ) (b: 2 SVT tag ) -1

D Run II 405 pb D Run II 405 pb-1

FIG. 4 (color online). The h2i distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the background (solid line), and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

0 10 20 30 40 50 events 0 1000 2000 0 2 M 0 10 20 30 40 50 0 200 400 600 800 M events

(a: 1 SVT tag ) (b: 2 SVT tag ) -1

D Run II 405 pb D Run II 405 pb-1

FIG. 5 (color online). The M distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the background (solid line), and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

0 20 40 60 80 100 events 0 200 400 600 800 0 3,4 min M 0 20 40 60 80 100 0 100 200 300 [GeV] 3,4 min M [GeV] 0 0 events

(a: 1 SVT tag ) (b: 2 SVT tag ) -1

D Run II 405 pb D Run II 405 pb-1

FIG. 6 (color online). The M34

min distribution for single-tag events (a) and double-tag events (b). Shown are the data (points), the background (solid line), and the expected tt distribution (filled histogram) multiplied by 140 (60) for the single (double)-tag analysis.

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background. For the loose and tight SVT, we derived a tag rate function (TRF — the probability for any individual jet to have a secondary vertex tag) from the data with Ntags 1. The TRF was parameterized in terms of the pT, , and y of the jet and the coordinate along the beam axis (z) of the primary vertex of the event, zPV, in four different HT bins. To predict the number of tagged jets in the event, it was necessary to correct for a possible correlation between tagged jets. In the single-tag analysis the correlation factor was negligible, unlike in the double-tag analysis, where the presence of b b jets events in the sample enhanced the correlation correction. We corrected for correlations caused by b bbackground by applying a correlation factor

Cij, that was parameterized as a function of the cone distance between the tagged jets, R. Figure8shows the number of double-tagged events versus R as observed in data, and the distribution as modeled by the TRF with and without including Cij. We considered significantly differ-ent functional forms for the parameterization of Cij and found that the choice of parameterization had little effect on the shape of the modeled background distribution.

The probabilities pi were used to assign a weight, the probability that the event could have a given number of tags, to every tagged and untagged event in the sample. To ensure the TRF prediction was accurate in the region of phase space outside the ‘‘background’’ peak of the neural network, we used the region 0:7 < NN < 0:5 to deter-mine a normalization. In this region of phase space, the tt content was negligible. A possible dependence on tt

con-tent was studied by the addition and/or subtraction of simulated tt events, as was the variation of the interval used for the normalization. Outside the background peak, the TRF predictions were corrected by SF1  1:000 

0:009 for the single-tag analysis and SF2  0:969 

0:014 for the double-tag analysis. The errors on the

nor-NN

-1

-0.5

0

0.5

1

events

-3 10 -2 10 -1 10 signal MC, single-tag signal MC, double-tag background, single-tag background, double-tag -1

D Run II 405 pb

FIG. 7 (color online). The output discriminant of an artificial neural network (NN) with six input nodes. All distributions are normalized to area. NN is optimized to distinguish between fully hadronic tt Monte Carlo events (signal) and the background from multijet production (background) as predicted by the tag rate functions.

R(tagged jets)

0

1

2

3

4

5

double-tagged events

0 200 400 double-tagged data TRF prediction, no correlations TRF prediction, incl. correlations TRF prediction, incl. correlations

-1

D Run II 405 pb

FIG. 8 (color online). The performance of the TRF prediction on double-tag events (points), without including the correlation factor Cij(dashed histogram), and including Cijfor two different

functional parameterizations (solid histograms).

NN

0.6

0.8

1

events

0 200 400 =1 tags data, N background (6.5 pb) t expected t expected s+b -1

D Run II 405 pb

FIG. 9 (color online). The distribution of the NN output vari-able for single-tag events. Shown are the data (points), back-ground (hashed band), signal (filled histogram), and signal  background (dashed histogram). The vertical line rep-resents the used cut of NN > 0:81.

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malization were taken into account as a systematic uncer-tainty on the number of background events.

Both the single-tag and the double-tag analysis were expected to be dominated by background, even at large values of NN. Figures9and10show the distribution for data (points), the Monte Carlo simulation prediction for

tt 6:5 pb (filled histogram), the background prediction (line histogram), and the signal  background distribution (dashed histogram) [9,14].

The cross section was calculated from the number of tt and background candidates above a cut value of the NN discriminant. The cut value was chosen to maximize the expected statistical significance s=ps  b, where s and b were the number of expected signal and background events. The signal and background distributions were esti-mated using the TRF prediction and tt Monte Carlo events [15]. For both analyses, the expected statistical signifi-cance was about 2 standard deviations. The optimal cut for the single (double)-tag analysis was NN 0:810:78 shown by a vertical line in Figs.9and10. TableIIgives the observed numbers of events (Ni

obs), the background

pre-diction (Ni

bg), and the efficiency for signal ("tt) that can be used to calculate the tt production cross section via

tt Nobsi  Ni bg "i ttL1  "iTRF ; (2)

where i was ‘‘ 1’’ for the single-tag analysis and ‘‘ 2’’ for the double-tag analysis. The number of background events is predicted using the TRF method. It was likely that at values of NN close to unity a certain fraction of the sample used to predict the background actually consists of

tagged or untagged tt events, resulting in an increased background prediction. The expected tt contamination of the background sample was corrected by a factor "i

TRF. In

the higher value bins of NN, the contribution from un-tagged tt events was significant. "i

TRF was estimated by

applying the TRF on tt MC and comparing the predicted tagging probability for signal to what was expected from background. The size of the Monte Carlo sample domi-nates the uncertainty on "i

TRF.

TableIIlists the systematic uncertainties on the estimate of the number of background events, the selection effi-ciency and the background contamination. The first was uncorrelated between the two analyses, while the latter two were correlated as they were derived from the same Monte Carlo samples.

For the single-tag analysis, the systematic uncertainty on the selection efficiency was dominated by the uncertainty in the jet calibration and identification, which were esti-mated by varying the parameterizations used by 1 standard deviation. The uncertainty on the background prediction was dominated by the uncertainty on the TRF method and the uncertainty on "TRF was due to limited Monte Carlo

statistics. The uncertainty of the TRF prediction was com-prised from the uncertainties coming from the fits of the probability density functions at the jet level, the statistics of the background sample, and the uncertainty on the normalization and correlation factors SF and Cij. For the double-tag analysis, the contribution from the uncertainties due to calibration of the b quark jet identification efficiency was an additional systematic uncertainty on "tt. These uncertainties were derived by varying the parameteriza-tions used within their known uncertainties.

The single-tag analysis yielded a cross section of

tt 4:13:0

3:0stat1:30:9syst  0:3lumi pb: (3)

For the double-tag analysis the measured cross section was

tt 4:72:6

2:5stat1:71:4syst  0:3lumi pb: (4)

As the single-tag and double-tag analysis were measured on independent samples, the statistical uncertainties were

NN

0.6

0.8

1

events

0 100 200 300 2tags data, N background (6.5 pb) t expected t expected s+b -1 D Run II 405 pb

FIG. 10 (color online). The distribution of the NN output variable for double-tag events. Shown are the data (points), background (hashed band), signal (filled histogram), and signal  background (dashed histogram). The vertical line rep-resents the used cut of NN > 0:78.

TABLE II. Overview of observed events, background predic-tions, and efficiencies.

Symbol Value

Observed events Nobs1 495

Background events Nbg1 464:3  4:6syst

ttefficiency "1tt 0:02420:00490:0058syst

ttcontamination "1TRF 0:245  0:031syst

Observed events Nobs 2 439

Background events Nbg 2 400:27:36:2syst

ttefficiency " 2

tt 0:02540:00650:0070syst

ttcontamination " 2

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uncorrelated. The uncertainties on the selection efficiency were completely correlated. Taking all uncertainties into account, a combined cross section measurement of

tt 4:52:0

1:9stat1:41:1syst  0:3lumi pb (5)

was obtained, for a top quark mass of mt 175 GeV=c2. For a top quark mass of mt 165 GeV=c2, the cross section is tt165  6:22:82:7stat2:01:5

syst  0:4lumi pb, while for a top quark mass of mt 185 GeV=c2 the value shifted down to tt185  4:31:91:8stat1:4

1:0syst  0:3lumi pb.

In summary, we have measured the tt production cross section in p p collisions at ps 1:96 TeV in the fully hadronic decay channel. We used lifetime b-tagging and an artificial neural network to distinguish tt from

back-ground. Our measurement yields a value consistent with SM predictions and previous measurements.

We thank the staffs at Fermilab and collaborating insti-tutions and acknowledge support from the DOE and NSF (USA); CEA and CNRS/IN2P3 (France); FASI, Rosatom, and RFBR (Russia); CAPES, CNPq, FAPERJ, FAPESP, and FUNDUNESP (Brazil); DAE and DST (India); Colciencias (Colombia); CONACyT (Mexico); KRF and KOSEF (Korea); CONICET and UBACyT (Argentina); FOM (The Netherlands); PPARC (United Kingdom); MSMT (Czech Republic); CRC Program, CFI, NSERC and WestGrid Project (Canada); BMBF and DFG (Germany); SFI (Ireland); The Swedish Research Council (Sweden); Research Corporation; Alexander von Humboldt Foundation; and the Marie Curie Program.

[1] V. M. Abazov et al. (D0 Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 565, 463 (2006).

[2] T. Andeen et al., FERMILAB Report No. TM-2365-E, 2006.

[3] The efficiency for signal remained between 85% and 90% throughout the data collection period. Efficiencies were estimated on tt Monte Carlo both using a simulation of the trigger system and using parameterizations derived from data.

[4] M. L. Mangano et al., J. High Energy Phys. 07 (2003) 001.

[5] T. Sjo¨strand et al., Comput. Phys. Commun. 135, 238 (2001).

[6] D. Lange, Nucl. Instrum. Methods Phys. Res., Sect. A 462, 152 (2001).

[7] G. C. Blazey et al., in Proceedings of the Workshop: QCD

and Weak Boson Physics in Run II, edited by U. Baur,

R. K. Ellis, and D. Zeppenfeld (Fermilab, Batavia, IL, 2000).

[8] V. M. Abazov et al. (D0 Collaboration), Phys. Lett. B 626, 35 (2005).

[9] V. M. Abazov et al. (D0 Collaboration), Phys. Rev. D 74, 112004 (2006).

[10] W.-M. Yao et al., J. Phys. G 33, 1 (2006).

[11] B. Abbott et al. (D0 Collaboration), Phys. Rev. Lett. 83, 1908 (1999).

[12] The possibility that the wrong permutations of jets could be chosen was taken into account in the determination of the values of 79, 11, and 21 GeV=c2 for M

W, MW, and

mt.

[13] R. Brun and F. Rademakers, Nucl. Instrum. Methods Phys. Res., Sect. A 389, 81 (1997). See also http://root.cern.ch/. [14] N. Kidonakis and R. Vogt, Phys. Rev. D 68, 114014

(2003).

[15] The expected tt content used to optimize the NN cut was estimated using a hypothetical cross section of tt

6:5 pb. The chosen cuts are stable under variation of the

ttcross section assumed during the optimization.

Referências

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