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K.Shochet, M.Shon, Y.Hara, K.Shreyber, I.Simak, V.Simonenko, A.Gorelov, I.Sinervo, P.Houben, P.Bisello, D.Yun, J. C.Carosi, R.Yu, G. B.Couderc, F.Yu, I.Sirotenko, V.Sisakyan, A.Skubic, P.Slattery, P.Yang, Y. C.Goshaw, A. T.Slaughter, A. J.Slaunwhite, J.Sliwa, K.Gadfort, T.Smirnov, D.Harder, K.Smith, J. R.Dudko, L. V.Snider, F. D.Williams, H. H.Cousinou, M. -C.Carrasco-Lizarraga, M. A.Cwiok, M.Bizjak, I.Snihur, R.Snow, G. R.Snow, J.Hare, D.Gallinaro, M.Snyder, S.Hou, S.Soha, A.Soeldner-Rembold, S.Arisawa, T.Somalwar, S.Goulianos, K.Sonnenschein, L.Antos, J.Sopczak, A.Yamaoka, J.Carrera, E.Bagby, L.Sorin, V.Cavalli-Sforza, M.Blair, R. E.Sosebee, M.Soustruznik, K.Spurlock, B.Goussiou, A.Duggan, D.Squillacioti, P.Zhu, J.Houlden, M.Stanitzki, M.Stark, J.Cox, C. A.St. Denis, R.Galyardt, J.Stelzer, B.Carrillo, S.Stelzer-Chilton, O.Grannis, P. D.Stentz, D.Vazquez, F.Hare, M.Blazey, G.Wolfe, H.Stolin, V.Stoyanova, D. A.Strang, M. A.Strauss, E.Garberson, F.Cox, D. J.Strauss, M.Hsu, S. -C.Zhao, T.Harel, A.Stroehmer, R.Strologas, J.Carron, S.Strom, D.Duperrin, A.Strycker, G. L.Stutte, L.Blessing, S.Wakisaka, T.Garcia, J. E.Suh, J. S.Wagner, R. L.Attal, A.Sukhanov, A.Crescioli, F.Suslov, I.Svoisky, P.Taffard, A.Takahashi, M.2013-09-302014-05-202013-09-302014-05-202010-07-15Physical Review D. College Pk: Amer Physical Soc, v. 82, n. 1, p. 17, 2010.1550-7998http://hdl.handle.net/11449/24389We 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 p (p) over bar collisions at the Fermilab Tevatron Collider at root 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 sigma(gg -> H) x B(H -> W+W-) is 1.75 pb at m(H) = 120 GeV, 0.38 pb at m(H) = 165 GeV, and 0.83 pb at m(H) = 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.17engArtigo10.1103/PhysRevD.82.011102WOS:000279941600001Acesso restritoWOS000279941600001.pdf