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Search for third generation vector leptoquarks in <em>pp</em> collisions at s√=1.96  TeV

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Reference

Search for third generation vector leptoquarks in pp collisions at s√=1.96  TeV

CDF Collaboration

CAMPANELLI, Mario (Collab.), et al.

Abstract

We search for a third generation vector leptoquark (VLQ3) that decays to a b quark and tau lepton usingthe CDF II detector and 320 pb-1 of integrated luminosity from the Fermilab Tevatron. Observing anumber of events in agreement with standard model expectations, we obtain, assuming Yang-Mills (minimal) couplings, the most stringent upper limit on the VLQ3 pair production cross section of 344 fb(493 fb) and lower limit on the VLQ3 mass of 317 GeV/c2 (251 GeV/c2) at 95% C.L.

CDF Collaboration, CAMPANELLI, Mario (Collab.), et al . Search for third generation vector leptoquarks in pp collisions at s√=1.96  TeV. Physical Review. D , 2008, vol. 77, no. 09, p.

091105

DOI : 10.1103/PhysRevD.77.091105

Available at:

http://archive-ouverte.unige.ch/unige:38497

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

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Search for third generation vector leptoquarks in p p collisions at ffiffiffi p s

¼ 1:96 TeV

T. Aaltonen,23A. Abulencia,24J. Adelman,13T. Affolder,10T. Akimoto,55M. G. Albrow,17S. Amerio,43D. Amidei,35 A. Anastassov,52K. Anikeev,17A. Annovi,19J. Antos,14M. Aoki,55G. Apollinari,17T. Arisawa,57A. Artikov,15 W. Ashmanskas,17A. Attal,3A. Aurisano,53F. Azfar,42P. Azzi-Bacchetta,43P. Azzurri,46N. Bacchetta,43W. Badgett,17

A. Barbaro-Galtieri,29V. E. Barnes,48B. A. Barnett,25S. Baroiant,7V. Bartsch,31G. Bauer,33P.-H. Beauchemin,34 F. Bedeschi,46S. Behari,25G. Bellettini,46J. Bellinger,59A. Belloni,33D. Benjamin,16A. Beretvas,17J. Beringer,29 T. Berry,30A. Bhatti,50M. Binkley,17D. Bisello,43I. Bizjak,31R. E. Blair,2C. Blocker,6B. Blumenfeld,25A. Bocci,16

A. Bodek,49V. Boisvert,49G. Bolla,48A. Bolshov,33D. Bortoletto,48J. Boudreau,47A. Boveia,10B. Brau,10 L. Brigliadori,5C. Bromberg,36E. Brubaker,13J. Budagov,15H. S. Budd,49S. Budd,24K. Burkett,17G. Busetto,43 P. Bussey,21A. Buzatu,34K. L. Byrum,2S. Cabrera,16,qM. Campanelli,20M. Campbell,35F. Canelli,17A. Canepa,45 S. Carrillo,18,iD. Carlsmith,59R. Carosi,46S. Carron,34B. Casal,11M. Casarsa,54A. Castro,5P. Catastini,46D. Cauz,54 M. Cavalli-Sforza,3A. Cerri,29L. Cerrito,31,mS. H. Chang,28Y. C. Chen,1M. Chertok,7G. Chiarelli,46G. Chlachidze,17

F. Chlebana,17I. Cho,28K. Cho,28D. Chokheli,15J. P. Chou,22G. Choudalakis,33S. H. Chuang,52K. Chung,12 W. H. Chung,59Y. S. Chung,49M. Cilijak,46C. I. Ciobanu,24M. A. Ciocci,46A. Clark,20D. Clark,6M. Coca,16 G. Compostella,43M. E. Convery,50J. Conway,7B. Cooper,31K. Copic,35M. Cordelli,19G. Cortiana,43F. Crescioli,46 C. Cuenca Almenar,7,qJ. Cuevas,11,lR. Culbertson,17J. C. Cully,35S. DaRonco,43M. Datta,17S. D’Auria,21T. Davies,21

D. Dagenhart,17P. de Barbaro,49S. De Cecco,51A. Deisher,29G. De Lentdecker,49,cG. De Lorenzo,3M. Dell’Orso,46 F. Delli Paoli,43L. Demortier,50J. Deng,16M. Deninno,5D. De Pedis,51P. F. Derwent,17G. P. Di Giovanni,44C. Dionisi,51

B. Di Ruzza,54J. R. Dittmann,4M. D’Onofrio,3C. Do¨rr,26S. Donati,46P. Dong,8J. Donini,43T. Dorigo,43S. Dube,52 J. Efron,39R. Erbacher,7D. Errede,24S. Errede,24R. Eusebi,17H. C. Fang,29S. Farrington,30I. Fedorko,46W. T. Fedorko,13

R. G. Feild,60M. Feindt,26J. P. Fernandez,32R. Field,18G. Flanagan,48R. Forrest,7S. Forrester,7M. Franklin,22 J. C. Freeman,29I. Furic,13M. Gallinaro,50J. Galyardt,12J. E. Garcia,46F. Garberson,10A. F. Garfinkel,48C. Gay,60 H. Gerberich,24D. Gerdes,35S. Giagu,51P. Giannetti,46K. Gibson,47J. L. Gimmell,49C. Ginsburg,17N. Giokaris,15,a M. Giordani,54P. Giromini,19M. Giunta,46G. Giurgiu,25V. Glagolev,15D. Glenzinski,17M. Gold,37N. Goldschmidt,18

J. Goldstein,42,bA. Golossanov,17G. Gomez,11G. Gomez-Ceballos,33M. Goncharov,53O. Gonza´lez,32I. Gorelov,37 A. T. Goshaw,16K. Goulianos,50A. Gresele,43S. Grinstein,22C. Grosso-Pilcher,13R. C. Group,17U. Grundler,24 J. Guimaraes da Costa,22Z. Gunay-Unalan,36C. Haber,29K. Hahn,33S. R. Hahn,17E. Halkiadakis,52A. Hamilton,20

B.-Y. Han,49J. Y. Han,49R. Handler,59F. Happacher,19K. Hara,55D. Hare,52M. Hare,56S. Harper,42R. F. Harr,58 R. M. Harris,17M. Hartz,47K. Hatakeyama,50J. Hauser,8C. Hays,42M. Heck,26A. Heijboer,45B. Heinemann,29 J. Heinrich,45C. Henderson,33M. Herndon,59J. Heuser,26D. Hidas,16C. S. Hill,10,bD. Hirschbuehl,26A. Hocker,17

A. Holloway,22S. Hou,1M. Houlden,30S.-C. Hsu,9B. T. Huffman,42R. E. Hughes,39U. Husemann,60J. Huston,36 J. Incandela,10G. Introzzi,46M. Iori,51A. Ivanov,7B. Iyutin,33E. James,17D. Jang,52B. Jayatilaka,16D. Jeans,51 E. J. Jeon,28S. Jindariani,18W. Johnson,7M. Jones,48K. K. Joo,28S. Y. Jun,12J. E. Jung,28T. R. Junk,24T. Kamon,53

P. E. Karchin,58Y. Kato,41Y. Kemp,26R. Kephart,17U. Kerzel,26V. Khotilovich,53B. Kilminster,39D. H. Kim,28 H. S. Kim,28J. E. Kim,28M. J. Kim,17S. B. Kim,28S. H. Kim,55Y. K. Kim,13N. Kimura,55L. Kirsch,6S. Klimenko,18

M. Klute,33B. Knuteson,33B. R. Ko,16K. Kondo,57D. J. Kong,28J. Konigsberg,18A. Korytov,18A. V. Kotwal,16 A. C. Kraan,45J. Kraus,24M. Kreps,26J. Kroll,45N. Krumnack,4M. Kruse,16V. Krutelyov,10T. Kubo,55S. E. Kuhlmann,2

T. Kuhr,26N. P. Kulkarni,58Y. Kusakabe,57S. Kwang,13A. T. Laasanen,48S. Lai,34S. Lami,46S. Lammel,17 M. Lancaster,31R. L. Lander,7K. Lannon,39A. Lath,52G. Latino,46I. Lazzizzera,43T. LeCompte,2J. Lee,49J. Lee,28

Y. J. Lee,28S. W. Lee,53,oR. Lefe`vre,20N. Leonardo,33S. Leone,46S. Levy,13J. D. Lewis,17C. Lin,60C. S. Lin,17 M. Lindgren,17E. Lipeles,9A. Lister,7D. O. Litvintsev,17T. Liu,17N. S. Lockyer,45A. Loginov,60M. Loreti,43R.-S. Lu,1

D. Lucchesi,43P. Lujan,29P. Lukens,17G. Lungu,18L. Lyons,42J. Lys,29R. Lysak,14E. Lytken,48P. Mack,26 D. MacQueen,34R. Madrak,17K. Maeshima,17K. Makhoul,33T. Maki,23P. Maksimovic,25S. Malde,42S. Malik,31 G. Manca,30A. Manousakis,15,aF. Margaroli,5R. Marginean,17C. Marino,26C. P. Marino,24A. Martin,60M. Martin,25 V. Martin,21,gM. Martı´nez,3R. Martı´nez-Balları´n,32T. Maruyama,55P. Mastrandrea,51T. Masubuchi,55H. Matsunaga,55 M. E. Mattson,58R. Mazini,34P. Mazzanti,5K. S. McFarland,49P. McIntyre,53R. McNulty,30,fA. Mehta,30P. Mehtala,23 S. Menzemer,11,hA. Menzione,46P. Merkel,48C. Mesropian,50A. Messina,36T. Miao,17N. Miladinovic,6J. Miles,33 R. Miller,36C. Mills,10M. Milnik,26A. Mitra,1G. Mitselmakher,18A. Miyamoto,27S. Moed,20N. Moggi,5B. Mohr,8

C. S. Moon,28R. Moore,17M. Morello,46P. Movilla Fernandez,29J. Mu¨lmensta¨dt,29A. Mukherjee,17Th. Muller,26 R. Mumford,25P. Murat,17M. Mussini,5J. Nachtman,17A. Nagano,55J. Naganoma,57K. Nakamura,55I. Nakano,40 A. Napier,56V. Necula,16C. Neu,45M. S. Neubauer,9J. Nielsen,29,nL. Nodulman,2O. Norniella,3E. Nurse,31S. H. Oh,16

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Y. D. Oh,28I. Oksuzian,18T. Okusawa,41R. Oldeman,30R. Orava,23K. Osterberg,23C. Pagliarone,46E. Palencia,11 V. Papadimitriou,17A. Papaikonomou,26A. A. Paramonov,13B. Parks,39S. Pashapour,34J. Patrick,17G. Pauletta,54 M. Paulini,12C. Paus,33D. E. Pellett,7A. Penzo,54T. J. Phillips,16G. Piacentino,46J. Piedra,44L. Pinera,18K. Pitts,24

C. Plager,8L. Pondrom,59X. Portell,3O. Poukhov,15N. Pounder,42F. Prakoshyn,15A. Pronko,17J. Proudfoot,2 F. Ptohos,19,eG. Punzi,46J. Pursley,25J. Rademacker,42,bA. Rahaman,47V. Ramakrishnan,59N. Ranjan,48I. Redondo,32 B. Reisert,17V. Rekovic,37P. Renton,42M. Rescigno,51S. Richter,26F. Rimondi,5L. Ristori,46A. Robson,21T. Rodrigo,11 E. Rogers,24S. Rolli,56R. Roser,17M. Rossi,54R. Rossin,10P. Roy,34A. Ruiz,11J. Russ,12V. Rusu,13H. Saarikko,23 A. Safonov,53W. K. Sakumoto,49G. Salamanna,51O. Salto´,3L. Santi,54S. Sarkar,51L. Sartori,46K. Sato,17P. Savard,34

A. Savoy-Navarro,44T. Scheidle,26P. Schlabach,17E. E. Schmidt,17M. P. Schmidt,60M. Schmitt,38T. Schwarz,7 L. Scodellaro,11A. L. Scott,10A. Scribano,46F. Scuri,46A. Sedov,48S. Seidel,37Y. Seiya,41A. Semenov,15 L. Sexton-Kennedy,17A. Sfyrla,20S. Z. Shalhout,58M. D. Shapiro,29T. Shears,30P. F. Shepard,47D. Sherman,22 M. Shimojima,55,kM. Shochet,13Y. Shon,59I. Shreyber,20A. Sidoti,46P. Sinervo,34A. Sisakyan,15A. J. Slaughter,17 J. Slaunwhite,39K. Sliwa,56J. R. Smith,7F. D. Snider,17R. Snihur,34M. Soderberg,35A. Soha,7S. Somalwar,52V. Sorin,36

J. Spalding,17F. Spinella,46T. Spreitzer,34P. Squillacioti,46M. Stanitzki,60A. Staveris-Polykalas,46R. St. Denis,21 B. Stelzer,8O. Stelzer-Chilton,42D. Stentz,38J. Strologas,37D. Stuart,10J. S. Suh,28A. Sukhanov,18H. Sun,56I. Suslov,15

T. Suzuki,55A. Taffard,24,pR. Takashima,40Y. Takeuchi,55R. Tanaka,40M. Tecchio,35P. K. Teng,1K. Terashi,50 J. Thom,17,dA. S. Thompson,21E. Thomson,45P. Tipton,60V. Tiwari,12S. Tkaczyk,17D. Toback,53S. Tokar,14 K. Tollefson,36T. Tomura,55D. Tonelli,46S. Torre,19D. Torretta,17S. Tourneur,44W. Trischuk,34S. Tsuno,40Y. Tu,45 N. Turini,46F. Ukegawa,55S. Uozumi,55S. Vallecorsa,20N. van Remortel,23A. Varganov,35E. Vataga,37F. Vazquez,18,i

G. Velev,17C. Vellidis,46,aG. Veramendi,24V. Veszpremi,48M. Vidal,32R. Vidal,17I. Vila,11R. Vilar,11T. Vine,31 M. Vogel,37I. Vollrath,34I. Volobouev,29,oG. Volpi,46F. Wu¨rthwein,9P. Wagner,53R. G. Wagner,2R. L. Wagner,17 J. Wagner,26W. Wagner,26R. Wallny,8S. M. Wang,1A. Warburton,34D. Waters,31M. Weinberger,53W. C. Wester III,17

B. Whitehouse,56D. Whiteson,45,pA. B. Wicklund,2E. Wicklund,17G. Williams,34H. H. Williams,45P. Wilson,17 B. L. Winer,39P. Wittich,17,dS. Wolbers,17C. Wolfe,13T. Wright,35X. Wu,20S. M. Wynne,30A. Yagil,9

K. Yamamoto,41J. Yamaoka,52T. Yamashita,40C. Yang,60U. K. Yang,13,jY. C. Yang,28W. M. Yao,29G. P. Yeh,17J. Yoh,17 K. Yorita,13T. Yoshida,41G. B. Yu,49I. Yu,28S. S. Yu,17J. C. Yun,17L. Zanello,51A. Zanetti,54I. Zaw,22X. Zhang,24

J. Zhou,52and 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, USA

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

24University of Illinois, Urbana, Illinois 61801, USA

T. AALTONENet al. PHYSICAL REVIEW D77,091105(R) (2008)

091105-2

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

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

27High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305, Japan

28Center for High Energy Physics: Kyungpook National University, Taegu 702-701, Korea;

Seoul National University, Seoul 151-742, Korea;

SungKyunKwan University, Suwon 440-746, Korea

29Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

30University of Liverpool, Liverpool L69 7ZE, United Kingdom

31University College London, London WC1E 6BT, United Kingdom

32Centro de Investigaciones Energeticas Medioambientales y Tecnologicas, E-28040 Madrid, Spain

33Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

34Institute of Particle Physics: McGill University, Montre´al, Canada H3A 2T8;

and University of Toronto, Toronto, Canada M5S 1A7

35University of Michigan, Ann Arbor, Michigan 48109, USA

36Michigan State University, East Lansing, Michigan 48824, USA

37University of New Mexico, Albuquerque, New Mexico 87131, USA

38Northwestern University, Evanston, Illinois 60208, USA

39The Ohio State University, Columbus, Ohio 43210, USA

40Okayama University, Okayama 700-8530, Japan

41Osaka City University, Osaka 588, Japan

42University of Oxford, Oxford OX1 3RH, United Kingdom

43University of Padova, Istituto Nazionale di Fisica Nucleare, Sezione di Padova-Trento, I-35131 Padova, Italy

44LPNHE, Universite Pierre et Marie Curie/ IN2P3-CNRS, UMR7585, Paris, F-75252 France

45University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

46Istituto Nazionale di Fisica Nucleare Pisa, Universities of Pisa, Siena and Scuola Normale Superiore, I-56127 Pisa, Italy

47University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA

48Purdue University, West Lafayette, Indiana 47907, USA

49University of Rochester, Rochester, New York 14627, USA

50The Rockefeller University, New York, New York 10021, USA

51Istituto Nazionale di Fisica Nucleare, Sezione di Roma 1, University of Rome ‘‘La Sapienza,’’ I-00185 Roma, Italy

52Rutgers University, Piscataway, New Jersey 08855, USA

53Texas A&M University, College Station, Texas 77843, USA

54Istituto Nazionale di Fisica Nucleare, University of Trieste/Udine, Italy

55University of Tsukuba, Tsukuba, Ibaraki 305, Japan

56Tufts University, Medford, Massachusetts 02155, USA

57Waseda University, Tokyo 169, Japan

58Wayne State University, Detroit, Michigan 48201, USA

59University of Wisconsin, Madison, Wisconsin 53706

60Yale University, New Haven, Connecticut 06520, USA (Received 15 June 2007; published 30 May 2008)

We search for a third generation vector leptoquark (VLQ3) that decays to abquark and tau lepton using the CDF II detector and320 pb1 of integrated luminosity from the Fermilab Tevatron. Observing a number of events in agreement with standard model expectations, we obtain, assuming Yang-Mills

oWith visitors from Texas Tech University, Lubbock, TX 79409, USA

nWith visitors from the University of California Santa Cruz, Santa Cruz, CA 95064, USA

mWith visitors from the University of London, Queen Mary College, London, E1 4NS, England,

lWith visitors from the University de Oviedo, E-33007 Oviedo, Spain,

kWith visitors from the Nagasaki Institute of Applied Science, Nagasaki, Japan,

hWith visitors from the University of Heidelberg, D-69120 Heidelberg, Germany,

pWith visitors from the University of California, Irvine, Irvine, CA 92697, USA

jWith visitors from the University of Manchester, Manchester M13 9PL, England,

gWith visitors from the University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom,

fWith visitors from the University College Dublin, Dublin 4, Ireland,

eWith visitors from the University of Cyprus, Nicosia CY-1678, Cyprus,

dWith visitors from Cornell University, Ithaca, NY 14853, USA

cWith visitors from the University Libre de Bruxelles, B-1050 Brussels, Belgium,

bWith visitors from the University of Bristol, Bristol BS8 1TL, United Kingdom,

iWith visitors from Universidad Iberoamericana, Mexico D.F., Mexico,

aWith visitors from the University of Athens, 15784 Athens, Greece,

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(minimal) couplings, the most stringent upper limit on theVLQ3pair production cross section of 344 fb (493 fb) and lower limit on theVLQ3mass of317 GeV=c2(251 GeV=c2) at 95% C.L.

DOI:10.1103/PhysRevD.77.091105 PACS numbers: 14.80.j, 13.85.Rm

Despite its extraordinary success, the standard model (SM) of elementary particles has structural deficiencies.

The parallels between the families of quarks and leptons suggest a possible link between these two sectors at higher mass scales. Leptoquarks, therefore, have been proposed as fractionally charged color-triplet bosons carrying both lep- ton and baryon quantum numbers. Leptoquarks appear in a wide range of models, including SU(5) grand unification [1], superstrings [2], SU(4) Pati-Salam [3], and composite- ness models [4].

The various leptoquark states are classified according to the quantum numbers of SM gauge group interactions [5].

At the Tevatron collider, these states would be predomi- nantly pair-produced through quark antiquark annihilation.

In general, larger cross sections, and thus better search sensitivities, are predicted for vector (spin 1) than for scalar leptoquarks [6].

We search for third generation vector leptoquark (VLQ3) pair production, and assume eachVLQ3 decays promptly to abquark and a tau lepton. As the trilinear and quartic couplings between vector leptoquarks and gluons can have model-dependent ‘‘anomalous’’ contributions, we examine two scenarios: one with Yang-Mills couplings, where vector leptoquarks are fundamental gauge bosons of an extended gauge group, and the other with minimal anomalous couplings [6,7]. PreviousVLQ3searches have been carried out in experiments at pp, eþe, and ep colliders [8–11]. Our new results substantially extend the reach beyond the previous limits.

The results reported in this paper are obtained from 320 pb1 of integrated luminosity collected between March 2002 and August 2004 by the CDF II detector [12], operating at the Tevatron pp collider. CDF II is a general-purpose particle detector and has a solenoidal charged particle spectrometer, consisting of 7–8 layers of silicon microstrip detectors and a cylindrical drift chamber immersed in a 1.4 T magnetic field, segmented sampling electromagnetic (EM) and hadronic calorimeters, and a set of charged particle detectors outside the calorimeters used to identify muon candidates. We use a cylindrical coordi- nate system with thezaxis along the beam axis, polar angle , azimuthal angle , and pseudorapidity ln tanð=2Þ. We define pT psin and ET Esin, wherepis the momentum measured by the tracking cham- bers andEis the energy measured by the calorimeters.

This search assumes a branching ratioBðVLQ3! bÞ ¼1, and considers a signature where the decay prod- ucts of theVLQ3pair,þbb, yield two jets from the b quarks, an electron or muon from a leptonically decaying tau, and a hadronically decaying tau (h). We do not

attempt to identify the jets as originating from bquarks, as this degrades the search sensitivity. A three-level trigger system selects events with lepton candidates and charged tracks [13]. These events are then classified asehorh based on the flavor of the leptonic tau decay.

Selected events are required to contain at least one well- identified electron (muon) candidate that passes fully through the fiducial volume of the cylindrical drift cham- ber, with transverse energy (momentum) ET>10 GeV (pT >10 GeV=c). To reduce the background due to multi- jet quantum chromodynamics (QCD) events, an isolation requirement is imposed upon the electron or muon candi- date. Specifically, the sum of thepTof all additional tracks within a cone inspace ofR <0:4around the track direction of the candidate is required to be less than 2 GeV=c, whereR ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi

ðÞ2þ ðÞ2

p .

Hadronic tau candidates are formed by matching narrow clusters of calorimeter towers with tracks [14]. Tracks and 0candidates are included within the tau candidate if they are within an angle!max from the highest pT track asso- ciated with theh, where!maxdepends on the total cluster energy and ranges from 0.05 to 0.17 rad. Tau candidates with one or three tracks are considered. We reconstruct the 0candidates as single narrow clusters in a set of strip and wire chambers embedded in the EM calorimeter at the depth where the longitudinal development of EM showers is expected to be maximal. Thehcandidates are required to havejj<1:0andET>15 GeV. The region between the tau selection cone and a larger 0.52 rad cone serves as an isolation annulus that contains no tracks with pT>

1 GeV=cand in which the summedET of all0 mesons must be less than 0.6 GeV.

To ensure efficient event reconstruction, the electron or muon candidate (‘) direction must be separated from the hadronic tau candidate direction by Rðh; ‘Þ>0:7. Jet candidates, withET>15 GeV, are identified in the region jj<2:4and are required to be separated from the lepton and tau candidates byRð‘=h;jetÞ>0:8.

There are a number of SM processes which can mimic theVLQ3signal. The first category consists of background processes which contain a realehorhplus at least two jets. The primary processes are Z0=!plus at least two jets, andtt!WbWb, where oneWyields a hadronic tau viaW! , the otherW similarly yields an electron (muon) or leptonically decaying tau, and the twobquarks give jets.

The second category of backgrounds consists of those that include misidentified final state particles. These in- clude tt!WbWb, where a jet from a hadronicW decay can be misidentified as an electron (muon). The processes

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tt!WbWb, Z0=!eþe plus jets, and Z0= ! þ plus jets also contribute as backgrounds when an electron (muon) or jet is misidentified as the h. Events withW plus jets can pass the selection if one of at least three jets is misidentified as the h. Contributions from diboson channels (WW,WZ, andZZ) plus jets are negli- gible. The above contributions and their uncertainties are estimated usingPYTHIA[15] Monte Carlo simulation and

GEANT[16] CDF II detector simulation. Background from multijet QCD can contribute when jets from quarks are misidentified as an electron (muon) orh. Photon plus jets background enters when high-pT photons convert within the detector and at least one of the resulting electrons appears as a primary electron candidate, while a jet is misidentified as theh. Contributions from both of these sources are estimated directly from the data, using methods described elsewhere [14].

Further event selection reduces the backgrounds.

Backgrounds associated with misidentification are reduced by approximately one-half through a requirement of oppo- sitely charged electron (muon) andh candidates, where the charge of thehcandidate is defined as the sum of the charges of all constituent tracks. Events consistent with photon conversions and cosmic rays are removed. To re- duce contributions from Z boson production, events are rejected if 76< mð‘; XÞ<106 GeV=c2, whereX can be the tau candidate or a second electron candidate in theeh channel, or a second muon candidate in theh channel.

We require E6 T>10 GeV, where E6 T ¼ j6~ETj [17]. This requirement reduces backgrounds from Z0=!þ and multijet QCD processes and is nearly 100% efficient for the signal process. We defineHT as the scalar sum of electron (muon) candidateET, tau candidateET, eventE6 T, and the transverse energies of the two highest ET jet candidates. The requirements on HT are given below.

The final selection requirement is that the event must contain two or more jets.

To simulateVLQ3pair production and decay [18], we have added the production and decay processes to the

GRACE[19] matrix element event generator, which calcu- lates amplitudes, and to theGR@PPA[20] interface, which speeds up computations of the interactions of the primary

hadrons. In addition to providing the theoretical cross section, these programs yield events that are processed throughTAUOLA[21] to simulate tau decays,PYTHIA[15]

to simulate parton showering, fragmentation, and addi- tional particle decays, andGEANT[16] for the full CDF II detector simulation. For the first time, this framework includes helicity amplitudes for the full matrix element at tree level and propagation of helicity information from the leptoquarks to the tau decay products. We use the parton distribution functions (PDFs) CTEQ5L [22], which we evaluate at an energy scaleQ2 ¼mVLQ3. The absence of higher orders in our theoretical cross section calculation likely results in conservative limits.

We determine total selection efficiencies, including fac- tors for triggering, geometrical and kinematic acceptance, particle candidate identification and isolation, and back- ground suppression criteria. The total efficiencies, aver- aged between theehandhchannels, range from about 2.2% (1.4%) to about 6.1% (5.9%) for Yang-Mills (mini- mal) couplings over the mass range 160 GeV=c2 to 400 GeV=c2. The slightly higher acceptances for the Yang-Mills couplings scenario are due to the fact that the leptoquarks and decay products are more central in this case than they are for the minimal couplings case. For the example of mVLQ3¼320 GeV=c2 and Yang-Mills cou- plings, the efficiencies for the eh and h channels are ð6:00:1Þ%andð6:10:1Þ%, respectively.

We define two signal regions. In addition, three side- band control regions in the plane of the number of jets (Njets) versusHT are used to verify the expected composi- tion of the backgrounds and the distributions for kinematic quantities. The primary signal region (SRA) hasNjets 2 and HT>400 GeV, and is sensitive to the highest mass leptoquarks. The secondary signal region (SRB) has Njets2and250< HT <400 GeV, and adds sensitivity to lowerVLQ3masses (down to the previous mass limits).

The three control regions are called CR0J, CR1J, and CR2J, where 0J, 1J, or 2J specifies the number of jets (0, 1, or2). Regions CR0J and CR1J include theHT range HT>80 GeV, while region CR2J is restricted to 80<

HT<250 GeV. Table I shows the expected background contributions in the control and signal regions, as well as

TABLE I. Numbers of events observed in data and estimates for the total background, for the eh and h channels, in the control regions (CR0J, CR1J, CR2J) and signal regions (SRB, SRA). For the backgrounds, the statistical uncertainty is given first, followed by the systematic uncertainty.

eh h

Data Background Data Background

CR0J 129 122:12:111:3 129 147:12:612:3

CR1J 110 109:22:39:3 79 100:52:56:7

CR2J 36 33:41:44:8 26 30:61:63:8

SRB 5 3:30:30:5 3 2:20:30:3

SRA 0 0:30:10:1 0 0:20:10:1

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the number of events observed in all regions. The signal regions are examined only after ana priorioptimization of the HT ranges that maximizes signal sensitivity. Control region CR1J in theh channel contains the largest dif- ference between the expected and observed number of events, with a difference of 1.9 sigma. Figure 1 shows the HT distributions for the eh and h channels, and includes the control region CR2J and the two signal regions.

The dominant sources of systematic uncertainties on the signal efficiencies are the amount of initial state radiation (ISR) and final state radiation (FSR), the tau identification, and the isolation requirements. The ISR and FSR uncer- tainties, as evaluated by varying the amount of ISR and FSR in simulation, are each approximately 3.7% of the selection efficiency. The tau identification systematic un- certainty, as measured using methods described elsewhere [14], is 3.0% of the selection efficiency and is primarily due to uncertainties in the response of the hadronic calo- rimeter to charged tracks and uncertainties in the track reconstruction efficiency. Uncertainty in simulating the

effect of the lepton isolation requirement is evaluated by comparing the efficiency of this isolation requirement in data and simulation. This yields a 3.0% uncertainty on the selection efficiency. Additional sources of systematic un- certainty on the signal efficiency are the choices of the PDFs and the jet energy scale, as well as smaller contribu- tions from the acceptance criteria, the electron (muon) identification, and theE6 T simulation. The total systematic uncertainty on signal efficiency ranges from 10.5%

(10.4%) for the eh (h) channel, for a VLQ3 with mass mVLQ3 ¼160 GeV=c2, down to 7.0% (7.4%) for mVLQ3¼400 GeV=c2. The systematic uncertainties on the theoretical prediction of the VLQ3 pair production cross section arise from the choices of PDFs and energy scale Q2. These two contributions are combined in quadrature.

A likelihood function is constructed using a Poisson probability distribution of the expected rates of signal plus backgrounds and observed number of events in each channel and signal region. For eachVLQ3mass, the ex- pected signal rates are functions of theVLQ3pair produc- tion cross section. The expected signal rates also include factors for the branching ratios of leptonic and hadronic tau decays, luminosity, and full selection efficiencies.

Systematic uncertainties, including 6% due to the luminos- ity measurement (not included in TableI), are incorporated into the fit. We apply Gaussian probabilities for the un- certainties on the background estimates, and account for correlations among different sources of systematic uncer- tainties. To set cross section limits for each mass, we integrate the likelihood distribution over all parameters except the cross section, and then integrate as a function of cross section from zero up to the cross section where the integral reaches 0.95.

Events / (25 GeV)

10-1

1

10 Data ( Ldt=322 pb-1)

2) /c GeV (m=320 VLQ3 VLQ3

µ µ

ee/

τ , Z τ

Z QCD

t t

jets W+

jets γ+

(a)

10-1

1 10

(GeV) HT

0 100 200 300 400 500 600 700 800 900 1000

Events / (25 GeV)

10-2

10-1

1 10 (b)

(GeV) HT

0 100 200 300 400 500 600 700 800 900 1000 10-2

10-1

1 10

FIG. 1 (color online). Distributions of HT for the (a) eh channel and (b) h channel, including one of the control regions used for validation (80< HT<250 GeV), and the regions used for the search (HT>250 GeV). The individual background contributions are shown, as is a hypothetical signal with mass mVLQ3¼320 GeV=c2, normalized to the data sam- ple size.

2) VLQ3 Mass (GeV/c

150 200 250 300 350 400

(pb)2 β⋅σ

10-2

10-1

1 10 102

Theoretical Predictions

Yang-Mills Couplings Minimal Couplings Theory Uncertainty

Observed 95% C.L. Limits

Minimal Couplings Yang-Mills Couplings

FIG. 2 (color online). The 95% C.L. upper limits on ðpp! VLQ3VLQ3Þ 2 versus mass (lines with symbols), where BðVLQ3!bÞ. The theoretical expectations are shown for the Yang-Mills (solid line) and minimal (dashed line) cou- plings scenarios for the case ¼1, with bands for uncertainties due to the choices of PDFs and Q2. The dot-dashed and dotted curves show the threshold effect when the VLQ3! tchannel is open.

T. AALTONENet al. PHYSICAL REVIEW D77,091105(R) (2008)

091105-6

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The results are shown in Fig.2, as a function ofVLQ3 mass, along with the leading order theoretical predictions.

For aVLQ3with Yang-Mills couplings, at 95% confidence level (C.L.), the upper limit on the cross section is <

344 fb, assumingB¼1, and the lower limit on the mass is mVLQ3>317 GeV=c2. With theoretical uncertainties in- cluded on the predicted cross section, the results are <

354 fb and mVLQ3>303 GeV=c2. If decay to t is al- lowed [23,24], the mass limit ismVLQ3>299 GeV=c2. For the minimal couplings model, the upper limit on the cross section is <493 fb and the lower limit on the mass is mVLQ3>251 GeV=c2. With theoretical uncertainties in- cluded on the predicted cross section, the results are <

555 fb and mVLQ3>235 GeV=c2. If decay to t is al- lowed, the mass limit ismVLQ3>238 GeV=c2. The mass limits are approximately80–90 GeV=c2 higher than those of previous comparable results [8,9].

Using 320 pb1 of luminosity at CDF II, we have searched forVLQ3pair production and subsequent decay to two tau leptons and two jets. We observe no excess of events beyond the expected SM processes and set the most stringent limits to date on the VLQ3 mass and pair pro-

duction cross section in the context of two coupling scenarios.

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 Foundation; the A. P. Sloan Foundation; the Bundes- ministerium fu¨r Bildung und Forschung, Germany; the Korean Science and Engineering Foundation and the Korean Research Foundation; the Science and Technology Facilities Council 14 (April 16, 2008) and the Royal Society, UK; the Institut National de Physique Nucleaire et Physique des Particules/CNRS; the Russian Foundation for Basic Research; the Comisı´on Interministerial de Ciencia y Tecnolog´a, Spain; the European Community’s Human Potential Programme;

the Slovak R Agency; and the Academy of Finland.

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[17] The missing transverse energy is defined by 6~ET¼ P

iEiTn^i, where i¼calorimeter tower number with jj<3:6 and n^i is a unit vector perpendicular to the beam axis and pointing at theith calorimeter tower.

[18] B. C. Allanachet al., arXiv:hep-ph/0602198.

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[23] In the case where decay to tis allowed, the parameter can be written as bbþ tÞ. The partial decay widths are b¼p42½2 ðm2þm2bÞ=mVLQ32 ðm2 m2bÞ2=mVLQ34þ6mmb=mVLQ32 and t¼p82

½2 ðm2þm2tÞ=mVLQ32 ðm2m2tÞ2=mVLQ34, whereis the coupling constant with fermions andpis the momentum of the relevant decay products in the center of mass frame.

[24] Note that we do not include the decay of leptoquarks to

tin the background accounting. This leads to slightly conservative limits in the case where decay to t is allowed.

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