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Searches for the Higgs boson decaying to W⁺ W⁻ -> l⁺nu l⁻nubar with the CDF II detector

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arxiv 1306.0023 v1 pith:5WZWYHKG submitted 2013-05-31 hep-ex

Searches for the Higgs boson decaying to W⁺ W⁻ -> l⁺nu l⁻nubar with the CDF II detector

CDF Collaboration: T. Aaltonen , S. Amerio , D. Amidei , A. Anastassov , A. Annovi , J. Antos , G. Apollinari , J.A. Appel
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T. Arisawa A. Artikov J. Asaadi W. Ashmanskas B. Auerbach A. Aurisano F. Azfar W. Badgett T. Bae A. Barbaro-Galtieri V.E. Barnes B.A. Barnett P. Barria P. Bartos M. Bauce F. Bedeschi S. Behari G. Bellettini J. Bellinger D. Benjamin A. Beretvas G. Bertoli A. Bhatti K.R. Bland B. Blumenfeld A. Bocci A. Bodek D. Bortoletto J. Boudreau A. Boveia L. Brigliadori C. Bromberg E. Brucken J. Budagov H.S. Budd K. Burkett G. Busetto P. Bussey P. Butti A. Buzatu A. Calamba S. Camarda M. Campanelli F. Canelli A. Canepa B. Carls D. Carlsmith R. Carosi S. Carrillo B. Casal M. Casarsa A. Castro P. Catastini D. Cauz V. Cavaliere M. Cavalli-Sforza A. Cerri L. Cerrito Y.C. Chen M. Chertok G. Chiarelli G. Chlachidze K. Cho D. Chokheli M.A. Ciocci A. Clark C. Clarke M.E. Convery J. Conway M. Corbo M. Cordelli C.A. Cox D.J. Cox M. Cremonesi D. Cruz J. Cuevas R. Culbertson N. d'Ascenzo M. Datta P. De Barbaro L. Demortier M. Deninno M. d'Errico F. Devoto A. Di Canto B. Di Ruzza J.R. Dittmann M. D'Onofrio S. Donati M. Dorigo A. Driutti K. Ebina R. Edgar A. Elagin R. Erbacher S. Errede B. Esham R. Eusebi S. Farrington J.P. Fernandez Ramos R. Field G. Flanagan R. Forrest M. Franklin J.C. Freeman H. Frisch Y. Funakoshi A.F. Garfinkel P. Garosi H. Gerberich E. Gerchtein S. Giagu V. Giakoumopoulou K. Gibson C.M. Ginsburg N. Giokaris P. Giromini G. Giurgiu V. Glagolev D. Glenzinski M. Gold D. Goldin A. Golossanov G. Gomez G. Gomez-Ceballos M. Goncharov O. Gonzalez Lopez I. Gorelov A.T. Goshaw K. Goulianos E. Gramellini S. Grinstein C. Grosso-Pilcher R.C. Group J. Guimaraes da Costa S.R. Hahn J.Y. Han F. Happacher K. Hara M. Hare R.F. Harr T. Harrington-Taber K. Hatakeyama C. Hays J. Heinrich M. Herndon D. Hidas A. Hocker Z. Hong W. Hopkins S. Hou S.-C. Hsu R.E. Hughes U. Husemann M. Hussein J. Huston G. Introzzi M. Iori A. Ivanov E. James D. Jang B. Jayatilaka E.J. Jeon S. Jindariani M. Jones K.K. Joo S.Y. Jun T.R. Junk M. Kambeitz T. Kamon P.E. Karchin A. Kasmi Y. Kato W. Ketchum J. Keung B. Kilminster D.H. Kim H.S. Kim J.E. Kim M.J. Kim S.B. Kim S.H. Kim Y.J. Kim Y.K. Kim N. Kimura M. Kirby K. Knoepfel K. Kondo D.J. Kong J. Konigsberg A.V. Kotwal M. Kreps J. Kroll M. Kruse T. Kuhr M. Kurata A.T. Laasanen S. Lammel M. Lancaster K. Lannon G. Latino H.S. Lee J.S. Lee S. Leo S. Leone J.D. Lewis A. Limosani E. Lipeles A. Lister H. Liu Q. Liu T. Liu S. Lockwitz A. Loginov A. Luca D. Lucchesi J. Lueck P. Lujan P. Lukens G. Lungu J. Lys R. Lysak R. Madrak P. Maestro S. Malik G. Manca A. Manousakis-Katsikakis F. Margaroli P. Marino M. Martinez K. Matera M.E. Mattson A. Mazzacane P. Mazzanti R. McNulty A. Mehta P. Mehtala C. Mesropian T. Miao D. Mietlicki A. Mitra H. Miyake S. Moed N. Moggi C.S. Moon R. Moore M.J. Morello S. Mrenna A. Mukherjee Th. Muller P. Murat M. Mussini J. Nachtman Y. Nagai J. Naganoma I. Nakano A. Napier J. Nett C. Neu M.S. Neubauer T. Nigmanov L. Nodulman S.Y. Noh O. Norniella L. Oakes S.H. Oh Y.D. Oh I. Oksuzian T. Okusawa R. Orava L. Ortolan S. Pagan Griso C. Pagliarone E. Palencia P. Palni V. Papadimitriou W. Parker G. Pauletta M. Paulini C. Paus T.J. Phillips G. Piacentino E. Pianori J. Pilot K. Pitts C. Plager L. Pondrom S. Poprocki K. Potamianos A. Pranko F. Prokoshin F. Ptohos G. Punzi J. Pursley N. Ranjan I. Redondo Fernandez P. Renton M. Rescigno F. Rimondi L. Ristori A. Robson T. Rodriguez S. Rolli M. Ronzani R. Roser J.L. Rosner F. Ruffini A. Ruiz J. Russ V. Rusu W.K. Sakumoto Y. Sakurai L. Santi K. Sato V. Saveliev A. Savoy-Navarro P. Schlabach E.E. Schmidt T. Schwarz L. Scodellaro F. Scuri S. Seidel Y. Seiya A. Semenov F. Sforza S.Z. Shalhout T. Shears P.F. Shepard M. Shimojima M. Shochet I. Shreyber-Tecker A. Simonenko P. Sinervo K. Sliwa J.R. Smith F.D. Snider H. Song V. Sorin M. Stancari R. St. Denis B. Stelzer O. Stelzer-Chilton D. Stentz J. Strologas Y. Sudo A. Sukhanov I. Suslov K. Takemasa Y. Takeuchi J. Tang M. Tecchio P.K. Teng J. Thom A.S. Thompson E. Thomson V. Thukral D. Toback S. Tokar K. Tollefson T. Tomura D. Tonelli S. Torre D. Torretta P. Totaro M. Trovato F. Ukegawa S. Uozumi F. Vazquez G. Velev C. Vellidis C. Vernieri M. Vidal R. Vilar J. Vizan M. Vogel G. Volpi F. Wurthwein P. Wagner R. Wallny S.M. Wang A. Warburton D. Waters W.C. Wester III D. Whiteson A.B. Wicklund S. Wilbur H.H. Williams J.S. Wilson P. Wilson B.L. Winer P. Wittich S. Wolbers H. Wolfe T. Wright X. Wu Z. Wu K. Yamamoto D. Yamato T. Yang U.K. Yang Y.C. Yang W.-M. Yao G.P. Yeh K. Yi J. Yoh K. Yorita T. Yoshida G.B. Yu I. Yu A.M. Zanetti Y. Zeng C. Zhou S. Zucchelli
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keywords bosonhiggsmodelproductionrangestandardexcludemass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present a search for a standard model Higgs boson decaying to two $W$ bosons that decay to leptons using the full data set collected with the CDF II detector in $\sqrt{s}=1.96$ TeV $p\bar{p}$ collisions at the Fermilab Tevatron, corresponding to an integrated luminosity of 9.7 fb${}^{-1}$. We obtain no evidence for production of a standard model Higgs boson with mass between 110 and 200 GeV/$c^2$, and place upper limits on the production cross section within this range. We exclude standard model Higgs boson production at the 95% confidence level in the mass range between 149 and 172 GeV/$c^2$, while expecting to exclude, in the absence of signal, the range between 155 and 175 GeV/$c^2$. We also interpret the search in terms of standard model Higgs boson production in the presence of a fourth generation of fermions and within the context of a fermiophobic Higgs boson model. For the specific case of a standard model-like Higgs boson in the presence of fourth-generation fermions, we exclude at the 95% confidence level Higgs boson production in the mass range between 124 and 200 GeV/$c^2$, while expecting to exclude, in the absence of signal, the range between 124 and 221 GeV/$c^2$.

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