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Combined Tevatron upper limit on <em>gg -&gt; H -&gt; W<sup>+</sup>W<sup>−</sup></em> and constraints on the Higgs boson mass in fourth-generation fermion models

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Article

Reference

Combined Tevatron upper limit on gg -> H -> W

+

W

and constraints on the Higgs boson mass in fourth-generation fermion

models

D0 Collaboration

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

Abstract

We combine results from searches by the CDF and D0 collaborations for a standard model Higgs boson (H) in the process gg→H→W+W− in pp collisions at the Fermilab Tevatron Collider at s√=1.96  TeV. With 4.8  fb−1 of integrated luminosity analyzed at CDF and 5.4  fb−1 at D0, the 95% confidence level upper limit on σ(gg→H)×B(H→W+W−) is 1.75 pb at mH=120   GeV, 0.38 pb at mH=165  GeV, and 0.83 pb at mH=200  GeV. Assuming the presence of a fourth sequential generation of fermions with large masses, we exclude at the 95% confidence level a standard-model-like Higgs boson with a mass between 131 and 204 GeV.

D0 Collaboration, CLARK, Allan Geoffrey (Collab.), et al . Combined Tevatron upper limit on gg -> H -> W

+

W

and constraints on the Higgs boson mass in fourth-generation fermion models.

Physical Review. D , 2010, vol. 82, p. 12p.

DOI : 10.1103/PhysRevD.82.011102

Available at:

http://archive-ouverte.unige.ch/unige:38696

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

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Combined Tevatron upper limit on gg ! H ! W

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W

and constraints on the Higgs boson mass in fourth-generation fermion models

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F. Scuri,40a,aA. Sedov,86,aS. Seidel,106,aY. Seiya,39,aJ. Sekaric,88,bA. Semenov,48,aH. Severini,116,b L. Sexton-Kennedy,77,aF. Sforza,40b,40a,aA. Sfyrla,82,aE. Shabalina,27,bS. Z. Shalhout,100,aV. Shary,21,b

A. A. Shchukin,51,bT. Shears,61,aP. F. Shepard,120,aM. Shimojima,40,xS. Shiraishi,78,aR. K. Shivpuri,34,bM. Shochet,78,a Y. Shon,129,aI. Shreyber,49,aV. Simak,12,bA. Simonenko,48,aP. Sinervo,6,aV. Sirotenko,77,bA. Sisakyan,48,aP. Skubic,116,b

P. Slattery,110,bA. J. Slaughter,77,aJ. Slaunwhite,114,aK. Sliwa,97,aD. Smirnov,85,bJ. R. Smith,68,aF. D. Snider,77,a R. Snihur,6,aG. R. Snow,103,bJ. Snow,115,bS. Snyder,112,bA. Soha,77,aS. So¨ldner-Rembold,64,bS. Somalwar,104,a

L. Sonnenschein,24,bA. Sopczak,60,bV. Sorin,54,aM. Sosebee,122,bK. Soustruznik,11,bB. Spurlock,122,b P. Squillacioti,40c,40a,aM. Stanitzki,73,aJ. Stark,17,bR. St. Denis,59,aB. Stelzer,6,aO. Stelzer-Chilton,6,aD. Stentz,81,a V. Stolin,49,bD. A. Stoyanova,51,bM. A. Strang,107,bE. Strauss,111,bM. Strauss,116,bR. Stro¨hmer,30,bJ. Strologas,106,a D. Strom,79,bG. L. Strycker,99,aL. Stutte,77,bJ. S. Suh,42,aA. Sukhanov,74,aI. Suslov,48,aP. Svoisky,47,bA. Taffard,82,i

M. Takahashi,64,bR. Takashima,38,aY. Takeuchi,40,aR. Tanaka,38,aA. Tanasijczuk,1,bJ. Tang,78,aW. Taylor,7,b M. Tecchio,99,aP. K. Teng,9,aJ. Thom,77,aJ. Thome,119,aG. A. Thompson,82,aE. Thomson,118,aB. Tiller,30,bP. Tipton,73,a

M. Titov,21,bS. Tkaczyk,77,aD. Toback,123,aS. Tokar,53,aV. V. Tokmenin,48,bK. Tollefson,101,aT. Tomura,40,a D. Tonelli,77,aS. Torre,37,aD. Torretta,77,aP. Totaro,42b,42a,aM. Trovato,40d,40a,aS.-Y. Tsai,9,aD. Tsybychev,111,b P. Ttito-Guzma´n,55,aB. Tuchming,21,bY. Tu,118,aC. Tully,105,bN. Turini,40c,40a,aP. M. Tuts,108,bF. Ukegawa,40,a R. Unalan,101,bS. Uozumi,42,aL. Uvarov,52,bS. Uvarov,52,bS. Uzunyan,80,bR. Van Kooten,83,bW. M. van Leeuwen,46,e N. van Remortel,15,aN. Varelas,79,bA. Varganov,99,aE. W. Varnes,66,bI. A. Vasilyev,51,bE. Vataga,40d,40a,aF. Va´zquez,74,q

G. Velev,77,aC. Vellidis,32,aP. Verdier,23,bL. S. Vertogradov,48,bM. Verzocchi,77,bM. Vesterinen,64,bM. Vidal,55,a I. Vila,56,aD. Vilanova,21,bR. Vilar,56,aP. Vint,62,bM. Vogel,106,aP. Vokac,12,bI. Volobouev,67,bbG. Volpi,40b,40a,a P. Wagner,118,aR. G. Wagner,76,aR. L. Wagner,77,aW. Wagner,28,ffJ. Wagner-Kuhr,28,aH. D. Wahl,75,bT. Wakisaka,39,a

R. Wallny,70,aM. H. L. S. Wang,110,bS. M. Wang,9,aA. Warburton,6,aJ. Warchol,85,bD. Waters,63,aG. Watts,128,b M. Wayne,85,bG. Weber,29,ooM. Weber,77,bM. Weinberger,123,aJ. Weinelt,28,aW. C. Wester III,77,aM. Wetstein,92,b A. White,122,bB. Whitehouse,97,aD. Whiteson,118,iD. Wicke,29,bA. B. Wicklund,76,aE. Wicklund,77,aS. Wilbur,78,a

G. Williams,6,aH. H. Williams,118,aM. R. J. Williams,60,bG. W. Wilson,88,bP. Wilson,77,aS. J. Wimpenny,71,b B. L. Winer,114,aP. Wittich,77,kM. Wobisch,90,bS. Wolbers,77,aC. Wolfe,78,aH. Wolfe,114,aD. R. Wood,94,bT. Wright,99,a

X. Wu,58,aF. Wu¨rthwein,69,aT. R. Wyatt,64,bY. Xie,77,bC. Xu,99,bS. Yacoob,81,bA. Yagil,69,aR. Yamada,77,b K. Yamamoto,39,aJ. Yamaoka,113,aU. K. Yang,78,vW.-C. Yang,64,bY. C. Yang,42,aW. M. Yao,67,aT. Yasuda,77,b Y. A. Yatsunenko,48,bZ. Ye,77,bG. P. Yeh,77,aK. Yi,77,rH. Yin,8,bK. Yip,112,bJ. Yoh,77,aH. D. Yoo,121,bK. Yorita,41,a T. Yoshida,39,oS. W. Youn,77,bG. B. Yu,113,aI. Yu,42,aJ. Yu,122,bS. S. Yu,77,aJ. C. Yun,77,aA. Zanetti,42a,aS. Zelitch,127,b

Y. Zeng,113,aX. Zhang,82,aT. Zhao,128,bY. Zheng,70,gB. Zhou,99,bJ. Zhu,111,bM. Zielinski,110,bD. Zieminska,83,b L. Zivkovic,108,band S. Zucchelli37a,hh

(aCDF Collaboration) (bD0 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

COMBINED TEVATRON UPPER LIMIT ON. . . PHYSICAL REVIEW D82,011102(R) (2010)

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4Universidade Federal do ABC, Santo Andre´, Brazil

5Instituto de Fı´sica Teo´rica, Universidade Estadual Paulista, Sa˜o Paulo, Brazil

6Institute of Particle Physics, McGill University, Montre´al, Que´bec, Canada;

Simon Fraser University, Burnaby, British Columbia, Canada;

University of Toronto, Toronto, Ontario, Canada;

and TRIUMF, Vancouver, British Columbia, Canada

7Simon Fraser University, Burnaby, British Columbia, Canada;

and York University, Toronto, Ontario, Canada

8University of Science and Technology of China, Hefei, People’s Republic of China

9Institute of Physics, Academia Sinica, Taipei, Taiwan, Republic of China

10Universidad de los Andes, Bogota´, Colombia

11Charles University, Faculty of Mathematics and Physics, Center for Particle Physics, Prague, Czech Republic

12Czech Technical University in Prague, Prague, Czech Republic

13Center for Particle Physics, Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic

14Universidad San Francisco de Quito, Quito, Ecuador

15Division of High Energy Physics, Department of Physics, University of Helsinki and Helsinki Institute of Physics, FIN-00014, Helsinki, Finland

16LPC, Universite´ Blaise Pascal, CNRS/IN2P3, Clermont, France

17LPSC, Universite´ Joseph Fourier Grenoble 1, France,

and CNRS/IN2P3, Institut National Polytechnique de Grenoble, Grenoble, France

18CPPM, Aix-Marseille Universite´, CNRS/IN2P3, Marseille, France

19LAL, Universite´ Paris-Sud, CNRS/IN2P3, Orsay, France

20LPNHE, Universite´ Paris VI and Universite´ Paris VII, CNRS/IN2P3, Paris, France

21CEA, Irfu, SPP, Saclay, France

22IPHC, Universite´ de Strasbourg, CNRS/IN2P3, Strasbourg, France

23IPNL, Universite´ Lyon 1, CNRS/IN2P3, Villeurbanne, France, and Universite´ de Lyon, Lyon, France

24III. Physikalisches Institut A, RWTH Aachen University, Aachen, Germany

25Physikalisches Institut, Universita¨t Bonn, Bonn, Germany

26Physikalisches Institut, Universita¨t Freiburg, Freiburg, Germany

27II. Physikalisches Institut, Georg-August-Universita¨t Go¨ttingen, Go¨ttingen, Germany

28Institut fu¨r Experimentelle Kernphysik, Karlsruhe Institute of Technology, Karlsruhe, Germany

29Institut fu¨r Physik, Universita¨t Mainz, Mainz, Germany

30Ludwig-Maximilians-Universita¨t Mu¨nchen, Mu¨nchen, Germany

31Fachbereich Physik, Bergische Univerita¨t Wuppertal, Wuppertal, Germany

32University of Athens, 157 71 Athens, Greece

33Panjab University, Chandigarh, India

34Delhi University, Delhi, India

35Tata Institute of Fundamental Research, Mumbai, India

36University College Dublin, Dublin, Ireland

37aIstituto Nazionale di Fisica Nucleare Bologna, I-40127 Bologna, Italy

37bUniversity of Bologna, I-40127 Bologna, Italy

37Laboratori Nazionali di Frascati, Istituto Nazionale di Fisica Nucleare, I-00044 Frascati, Italy

39aIstituto Nazionale di Fisica Nucleare, Sezione di Padova-Trento, I-35131 Padova, Italy

39bUniversity of Padova, I-35131 Padova, Italy

40aIstituto Nazionale di Fisica Nucleare, Pisa, I-56127 Pisa, Italy

40bUniversity of Pisa, I-56127 Pisa, Italy

40cUniversity of Siena, I-56127 Pisa, Italy

40dScuola Normale Superiore, I-56127 Pisa, Italy

41aIstituto Nazionale di Fisica Nucleare, Sezione di Roma 1, I-00185 Roma, Italy

41bSapienza Universita` di Roma, I-00185 Roma, Italy

42aIstituto Nazionale di Fisica Nucleare Trieste/Udine, I-34100 Trieste, I-33100 Udine, Italy

42bUniversity of Trieste/Udine, I-33100 Udine, Italy

38Okayama University, Okayama 700-8530, Japan

39Osaka City University, Osaka 588, Japan

40University of Tsukuba, Tsukuba, Ibaraki 305, Japan

41Waseda University, Tokyo 169, Japan

42Center for High Energy Physics: Kyungpook National University, Daegu, Korea;

Seoul National University, Seoul, Korea;

Sungkyunkwan University, Suwon, Korea;

Korea Institute of Science and Technology Information, Daejeon, Korea;

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Chonnam National University, Gwangju, Korea;

Chonbuk National University, Jeonju, Korea

43Korea Detector Laboratory, Korea University, Seoul, Korea

44SungKyunKwan University, Suwon, Korea

45CINVESTAV, Mexico City, Mexico

46FOM-Institute NIKHEF and University of Amsterdam/NIKHEF, Amsterdam, The Netherlands

47Radboud University Nijmegen/NIKHEF, Nijmegen, The Netherlands

48Joint Institute for Nuclear Research, Dubna, Russia

49Institute for Theoretical and Experimental Physics, Moscow, Russia

50Moscow State University, Moscow, Russia

51Institute for High Energy Physics, Protvino, Russia

52Petersburg Nuclear Physics Institute, St. Petersburg, Russia

53Comenius University, 842 48 Bratislava, Slovakia;

Institute of Experimental Physics, 040 01 Kosice, Slovakia

54Institut de Fisica d’Altes Energies, Universitat Autonoma de Barcelona, E-08193, Bellaterra (Barcelona), Spain

55Centro de Investigaciones Energeticas Medioambientales y Tecnologicas, E-28040 Madrid, Spain

56Instituto de Fisica de Cantabria, CSIC-University of Cantabria, 39005 Santander, Spain

57Stockholm University, Stockholm, Sweden, and Uppsala University, Uppsala, Sweden

58University of Geneva, CH-1211 Geneva 4, Switzerland

59Glasgow University, Glasgow G12 8QQ, United Kingdom

60Lancaster University, Lancaster LA1 4YB, United Kingdom

61University of Liverpool, Liverpool L69 7ZE, United Kingdom

62Imperial College London, London SW7 2AZ, United Kingdom

63University College London, London WC1E 6BT, United Kingdom

64The University of Manchester, Manchester M13 9PL, United Kingdom

65University of Oxford, Oxford OX1 3RH, United Kingdom

66University of Arizona, Tucson, Arizona 85721, USA

67Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA

68University of California Davis, Davis, California 95616, USA

69University of California San Diego, La Jolla, California 92093, USA

70University of California Los Angeles, Los Angeles, California 90024, USA

71University of California Riverside, Riverside, California 92521, USA

72University of California Santa Barbara, Santa Barbara, California 93106, USA

73Yale University, New Haven, Connecticut 06520, USA

74University of Florida, Gainesville, Florida 32611, USA

75Florida State University, Tallahassee, Florida 32306, USA

76Argonne National Laboratory, Argonne, Illinois 60439, USA

77Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA

78Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637, USA

79University of Illinois at Chicago, Chicago, Illinois 60607, USA

80Northern Illinois University, DeKalb, Illinois 60115, USA

81Northwestern University, Evanston, Illinois 60208, USA

82University of Illinois, Urbana, Illinois 61801, USA

83Indiana University, Bloomington, Indiana 47405, USA

84Purdue University Calumet, Hammond, Indiana 46323, USA

85University of Notre Dame, Notre Dame, Indiana 46556, USA

86Purdue University, West Lafayette, Indiana 47907, USA

87Iowa State University, Ames, Iowa 50011, USA

88University of Kansas, Lawrence, Kansas 66045, USA

89Kansas State University, Manhattan, Kansas 66506, USA

90Louisiana Tech University, Ruston, Louisiana 71272, USA

91The Johns Hopkins University, Baltimore, Maryland 21218, USA

92University of Maryland, College Park, Maryland 20742, USA

93Boston University, Boston, Massachusetts 02215, USA

94Northeastern University, Boston, Massachusetts 02115, USA

95Harvard University, Cambridge, Massachusetts 02138, USA

96Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

97Tufts University, Medford, Massachusetts 02155, USA

98Brandeis University, Waltham, Massachusetts 02254, USA

99University of Michigan, Ann Arbor, Michigan 48109, USA

100Wayne State University, Detroit, Michigan 48201, USA

COMBINED TEVATRON UPPER LIMIT ON. . . PHYSICAL REVIEW D82,011102(R) (2010)

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101Michigan State University, East Lansing, Michigan 48824, USA

102University of Mississippi, University, Mississippi 38677, USA

103University of Nebraska, Lincoln, Nebraska 68588, USA

104Rutgers University, Piscataway, New Jersey 08855, USA

105Princeton University, Princeton, New Jersey 08544, USA

106University of New Mexico, Albuquerque, New Mexico 87131, USA

107State University of New York, Buffalo, New York 14260, USA

108Columbia University, New York, New York 10027, USA

109The Rockefeller University, New York, New York 10021, USA

110University of Rochester, Rochester, New York 14627, USA

111State University of New York, Stony Brook, New York 11794, USA

112Brookhaven National Laboratory, Upton, New York 11973, USA

113Duke University, Durham, North Carolina 27708, USA

114The Ohio State University, Columbus, Ohio 43210, USA

115Langston University, Langston, Oklahoma 73050, USA

116University of Oklahoma, Norman, Oklahoma 73019, USA

117Oklahoma State University, Stillwater, Oklahoma 74078, USA

118University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA

119Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA

120University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA

121Brown University, Providence, Rhode Island 02912, USA

122University of Texas, Arlington, Texas 76019, USA

aDeceased.

bNow at Temple University, Philadelphia, PA 19122, USA.

cDeceased.

dVisitor to CDF from University of Massachusetts Amherst, Amherst, MA 01003, USA.

eVisitor to CDF from Universiteit Antwerpen, B-2610 Antwerp, Belgium.

fVisitor to CDF from University of Bristol, Bristol BS8 1TL, United Kingdom.

gVisitor to CDF from Chinese Academy of Sciences, Beijing 100864, China.

hVisitor to CDF from Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari, 09042 Monserrato (Cagliari), Italy.

iVisitor to CDF from University of California Irvine, Irvine, CA 92697, USA.

jVisitor to CDF from University of California Santa Cruz, Santa Cruz, CA 95064, USA.

kVisitor to CDF from Cornell University, Ithaca, NY 14853, USA.

lVisitor to CDF from University of Cyprus, Nicosia CY-1678, Cyprus.

mVisitor to CDF from University College Dublin, Dublin 4, Ireland.

nVisitor to CDF from University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom.

oVisitor to CDF from University of Fukui, Fukui City, Fukui Prefecture, Japan 910-0017.

pVisitor to CDF from Kinki University, Higashi-Osaka City, Japan 577-8502.

qVisitor to CDF from Universidad Iberoamericana, Mexico D.F., Mexico.

rVisitor to CDF from University of Iowa, Iowa City, IA 52242, USA.

sVisitor to CDF from Iowa State University, Ames, IA 50011, USA.

tVisitor to CDF from Kansas State University, Manhattan, KS 66506, USA.

mmVisitor to D0 from Centro de Investigacion en Computacion—IPN, Mexico City, Mexico.

llVisitor to D0 from ICREA/IFAE, Barcelona, Spain.

kkVisitor to D0 from SLAC, Menlo Park, CA, 94025, USA.

jjVisitor to D0 from The University of Liverpool, Liverpool, United Kingdom.

iiVisitor to D0 from Augustana College, Sioux Falls, SD, 61201, USA.

hhOn leave from J. Stefan Institute, Ljubljana, Slovenia.

ggVisitor to CDF from Yarmouk University, Irbid 211-63, Jordan.

ffVisitor to CDF from Bergische Universita¨t Wuppertal, 42097 Wuppertal, Germany.

eeVisitor to CDF from University of Virginia, Charlottesville, VA 22906, USA.

ddVisitor to CDF from Universidad Tecnica Federico Santa Maria, 110v Valparaiso, Chile.

ccVisitor to CDF from IFIC (CSIC-Universitat de Valencia), 56071 Valencia, Spain.

bbVisitor to CDF from Texas Tech University, Lubbock, TX 79609, USA.

aaVisitor to CDF from University de Oviedo, E-33007 Oviedo, Spain.

zVisitor to CDF from Obninsk State University, Obninsk, Russia.

yVisitor to CDF from University of Notre Dame, Notre Dame, IN 46556, USA.

xVisitor to CDF from Nagasaki Institute of Applied Science, Nagasaki, Japan.

wVisitor to CDF from Muons, Inc., Batavia, IL 60510, USA.

vVisitor to CDF from University of Manchester, Manchester M13 9PL, United Kingdom.

uVisitor to CDF from Queen Mary, University of London, London, E1 4NS, United Kingdom.

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123Texas A&M University, College Station, Texas 77843, USA

124Southern Methodist University, Dallas, Texas 75275, USA

125Rice University, Houston, Texas 77005, USA

126Baylor University, Waco, Texas 76798, USA

127University of Virginia, Charlottesville, Virginia 22901, USA

128University of Washington, Seattle, Washington 98195, USA

129University of Wisconsin, Madison, Wisconsin 53706, USA (Received 18 May 2010; published 15 July 2010)

We combine results from searches by the CDF and D0 collaborations for a standard model Higgs boson (H) in the process gg!H!WþW in pp collisions at the Fermilab Tevatron Collider at ffiffiffi

ps

¼ 1:96 TeV. With 4:8 fb1 of integrated luminosity analyzed at CDF and 5:4 fb1 at D0, the 95%

confidence level upper limit onðgg!HÞ BðH!WþWÞis 1.75 pb atmH¼120 GeV, 0.38 pb at mH¼165 GeV, and 0.83 pb at mH¼200 GeV. Assuming the presence of a fourth sequential generation of fermions with large masses, we exclude at the 95% confidence level a standard-model- like Higgs boson with a mass between 131 and 204 GeV.

DOI:10.1103/PhysRevD.82.011102 PACS numbers: 13.85.Rm, 14.80.Bn, 14.70.Fm, 14.65.Jk

Exploring the mechanism for breaking the SUð2Þ Uð1Þ electroweak gauge symmetry is a priority in high energy physics. Not only are this symmetry and its break- ing [1] necessary components for the consistency of the successful standard model (SM) [2], but measurable prop- erties of the breaking mechanism are also very sensitive to possible phenomena that have not yet been observed at collider experiments. Measuring these properties, or set- ting limits on them, can constrain broad classes of exten- sions to the SM.

A natural extension to the SM that can be tested with Higgs boson search results at the Fermilab Tevatron Collider is the presence of a fourth generation of fermions with masses much larger than those of the three known generations [3]. While fits to precision electroweak data favor a low-mass Higgs boson in the SM, the addition of a fourth generation of fermions to the SM modifies the fit parameters such that a heavy Higgs boson is consistent for up to mH 300 GeV at the 68% confidence level (CL) [4]. Measurements of theZboson decay width [5] exclude models in which the fourth neutrino mass eigenstate has a mass less than 45 GeV. If the neutrino masses are very large, however, a fourth generation of fermions is not yet excluded.

One consequence of the extra fermions is that theggH coupling is enhanced by a factor of roughly three relative to the SM coupling [4,6,7]. Since the lowest-orderggHcou- pling arises from a quark loop. The top quark contribution is the largest due to its large coupling with the Higgs boson.

In the limitmq4mH, wheremq4is the fourth-generation quark mass, the Higgs boson coupling cancels the mass dependence for each of the three propagators in the loop, and the contribution to theggHcoupling becomes asymp- totically independent of the masses of the two fourth- generation quarks. Each additional fourth-generation quark then contributes as much as the top quark, and the ggHcoupling is thus enhanced by a factorKe of approxi- mately three.

The production cross section will be enhanced by a factor of Ke2. For mH near the low end of our search range, mH 110 GeV, the gg!H production cross section is enhanced by roughly a factor of 9 relative to the SM prediction. This factor drops to approximately 7.5 near the upper end of the search range, mH 300 GeV, assuming asymptotically large masses for the fourth-generation quarks. The reason for this drop is that the denominator of the enhancement factor, the SM cross section, has a larger contribution from the SM top quark as mH nears 2mt. The partial decay width for H!gg is enhanced by the same factor as the production cross section. However, because the decay H!gg is loop mediated, the H!WþW decay continues to dominate for Higgs boson masses mH>

135 GeV.

We consider two scenarios for the masses of the fourth- generation fermions. In the first scenario, the ‘‘low-mass’’

scenario, we set the mass of the fourth-generation neutrino to m4¼80 GeV, and the mass of the fourth-generation charged lepton to m‘4¼100 GeV in order to evade ex- perimental constraints [8] and to have the maximum im- pact on the Higgs boson decay branching ratios. In the second scenario, the ‘‘high-mass’’ scenario, we setm4 ¼ m‘4 ¼1 TeV, so that the fourth-generation leptons do not affect the decay branching ratios of the Higgs boson. In both scenarios, we choose the masses of the quarks to be those of the second scenario in Ref. [7], that is, we set the mass of the fourth-generation down-type quark to be md4¼400 GeV and the mass of the fourth- generation up-type quark to be mu4¼md4þ50 GeVþ 10 logðmH=115 GeVÞGeV. The other mass spectrum of Ref. [7] chooses md4 ¼300 GeV, resulting in slightly larger predictions for ðgg!HÞ. We use the next-to- next-to-leading order (NNLO) production cross section calculation of Ref. [7], which builds on the NNLO SM calculations of Refs. [9–16], the results of which are also listed in Ref. [17].

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The CDF and D0 Collaborations have searched for the SM Higgs boson in the decayH!WþW using all SM production processes:gg!H,qq!WH,qq!ZH, and vector-boson fusion (VBF) [18–20]. The results of these searches for the SM Higgs boson cannot be used directly to constrain fourth-generation models, as theggHcoupling is enhanced but theWWHandZZHcouplings are not, and the signal acceptances and the backgrounds in the multiple analysis channels differ for the various production modes.

Therefore, these searches rely on the SM to predict the ratios of the production rates of thegg!H,WH,ZH, and VBF signals. Previous external analyses have used the Tevatron’s SM Higgs boson search results to constrain fourth-generation models, incorrectly arguing that the WH, ZH, and VBF production rates are not significant, thus obtaining only approximate results. Furthermore, the SM results [18–20] extend only up tomHof 200 GeV. This paper addresses both of these issues by placing limits on ðgg!HÞ BðH!WþWÞup tomH ¼300 GeV.

Previously, the CDF and D0 collaborations have pub- lished searches for the process gg!H!WþW, also neglecting the WH, ZH, and VBF signal contributions [21,22]. The D0 search includes a fourth-generation inter- pretation. Here we update these searches with those using 4:8 fb1 from CDF [18] and5:4 fb1 from D0 [19]. We present new limits on ðgg!HÞ BðH!WþWÞ in which thegg!Hproduction mechanism is considered as the unique signal source. These limits are compared to models for Higgs boson production in which the ggH coupling is enhanced by the presence of a single additional generation of fermions. In this comparison, the decay branching ratios of the Higgs boson are also modified to reflect changes due to the fourth generation relative to the SM prediction. While the decays of the heavy quarks and leptons may includeWbosons in the final state, we do not include these as additional sources of signal. The branch-

ing ratios for H!WþW are calculated using HDECAY

[23] modified to include fourth-generation fermions [4].

The modified Higgs branching ratio to WþW is multi- plied by the cross section [7] to predict the fourth- generation enhancedgg!H!WþW production rate.

The event selections are similar for the corresponding CDF and D0 analyses. Both collaborations select events with largeE6 Tand two oppositely charged, isolated leptons, targeting theH!WþWsignal in which bothW bosons decay leptonically. The D0 analysis classifies events in three channels defined by the number of charged leptons (eor ), eþe,e, and þ and no classification based upon jet multiplicity. The CDF analysis separates opposite-sign candidate events into five nonoverlapping channels. Events are classified by their jet multiplicity (0, 1, or2), and the 0 and 1 jet channels are further divided according to whether both leptons are in the central part of the detector or if either lepton is in the forward part of the detector. Two changes have been made in the D0 event selection from the analysis presented in Ref. [19]. For higher Higgs boson masses (mH >200 GeV), the dilepton azimuthal-opening angle distribution is no longer peaked at low values (ð‘; ‘Þ<1). Therefore, to enhance the signal acceptance for large mH, the requirement on the dilepton azimuthal-opening angle [ð‘; ‘Þ] has been re- moved for e candidate events and relaxed to ð‘; ‘Þ<2:5in the eþe andþ candidate events.

In addition, a requirement on the-opening angle between the leading muon and the missing transverse energy, ð; E6 TÞ>0:5, has been included to remove additional background in a signal-free region. The predicted contri- butions from the different background processes are com- pared with the numbers of events observed in data for the CDF and D0 analyses in TablesIandII, respectively.

The presence of neutrinos in the final state prevents event-by-event reconstruction of the Higgs boson mass

TABLE I. Expected and observed event yields in the 0-jet exclusive, 1-jet exclusive, and 2-jet inclusive samples at final selection for the CDF analysis summed across all lepton categories.

The systematic uncertainty is shown for all samples. The signal expectation is given for the low- mass fourth-generation scenario with an SM Higgs mass of 200 GeV with a predictedðgg! HÞ BRðH!WþWÞof 1.02 pb.

CDF Run II

RL¼4:8 fb1 0-jet 1-jet 2-jets

Z=!‘þ 12830 13342 5117

tt 1:990:31 48:47:6 14524

WW 44748 12113 25:65:8

WZ 19:72:7 20:02:7 5:300:73

ZZ 29:94:1 8:01:1 2:360:32

Wþjets 15437 5915 21:95:9

W 11219 16:23:6 2:720:67

Total Background 89379 40652 25433

gg!H(MH¼200 GeV) 35:25:0 20:25:1 8:55:1

Data 950 393 224

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