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S.Corcoran, M.Maravin, Y.Martin, B.Bagby, L.McCarthy, R.Grivaz, J. -F.Kehoe, R.Melnitchouk, A.Obrant, G.Cutts, D.Gruendahl, S.Ochando, C.Onoprienko, D.Oshima, N.Osta, J.Otec, R.Garzon, G. J. Otero Y.Banerjee, P.Kermiche, S.Owen, M.Padley, P.Pangilinan, M.Grunewald, M. W.Cwiok, M.Parashar, N.Park, S. -J.Park, S. K.Parsons, J.Partridge, R.Atramentov, O.Parua, N.Patwa, A.Barberis, E.Pawloski, G.Guo, J.Penning, B.da Motta, H.Perfilov, M.Peters, K.Peters, Y.Khalatyan, N.Petroff, P.Petteni, M.Piegaia, R.Piper, J.Pleier, M. -A.Guo, F.Barfuss, A. -F.Podesta-Lerma, P. L. M.Alverson, G.Podstavkov, V. M.Khanov, A.Pogorelov, Y.2013-09-302014-05-202013-09-302014-05-202009-02-06Physical Review Letters. College Pk: Amer Physical Soc, v. 102, n. 5, p. 7, 2009.0031-9007http://hdl.handle.net/11449/24450In a data sample of approximately 1.3 fb(-1) collected with the D0 detector between 2002 and 2006, the orbitally excited charm state D-s1(+/-)(2536) has been observed with a measured mass of 2535.7 +/- 0.6(stat) +/- 0.5(syst) MeV/c(2) via the decay mode B-s(0) -> D-s1(-)(2536)mu(+)nu X-mu. A first measurement is made of the branching ratio product Br((b) over bar -> D-s1(-)(2536)mu(+)nu X-mu) x Br(D-s1(-) -> D*K--(S)0). Assuming that D-s1(-)(2536) production in semileptonic decay is entirely from B-s(0), an extraction of the semileptonic branching ratio Br(B-s(0) -> D-s1(-)(2536)mu(+)nu X-mu) is made.7engArtigo10.1103/PhysRevLett.102.051801WOS:000263166400015Acesso restritoWOS000263166400015.pdf