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dc.contributor.authorAaltonen, Timo Antero
dc.contributor.authorCasal Laraña, Bruno
dc.contributor.authorCuevas Maestro, Francisco Javier
dc.contributor.authorGómez Gramuglio, Gervasio 
dc.contributor.authorPalencia Cortezón, José Enrique
dc.contributor.authorRuiz Jimeno, Alberto 
dc.contributor.authorScodellaro, Luca 
dc.contributor.authorVilar Cortabitarte, Rocío 
dc.contributor.authorVizán García, Jesús Manuel 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2018-06-13T08:59:21Z
dc.date.available2018-06-13T08:59:21Z
dc.date.issued2014-07
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.otherFPA2014-55295-C3-1-R
dc.identifier.otherFPA 2011-28694-C02-01
dc.identifier.urihttp://hdl.handle.net/10902/13863
dc.description.abstractUsing the full CDF Run II data sample, we report evidence for a new resonance, which we refer to as B(5970), found simultaneously in the B0p+ and B+p- mass distributions with a significance of 4.4 standard deviations. We further report the first study of resonances consistent with orbitally excited B+ mesons and an updated measurement of the properties of orbitally excited B0 and B0s mesons. We measure the masses and widths of all states, as well as the relative production rates of the B1, B*2, and B(5970) states and the branching fraction of the B*0s2 state to either B*+K- and B+K-. Furthermore, we measure the production rates of the orbitally excited B0,+ states relative to the B0,+ ground state. The masses of the new B(5970) resonances are 5978±5(stat)±12(syst)??MeV/c2 for the neutral state and 5961±5(stat)±12(syst)??MeV/c2 for the charged state, assuming that the resonance decays into Bp final states. The properties of the orbitally excited and the new B(5970)0,+ states are compatible with isospin symmetry.es_ES
dc.description.sponsorshipWe 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 the National Science Foundation; the Italian Istituto Nazionale di Fisica Nucleare; the Ministry of Education,Culture, Sports, Science and Technology of Japan; theNatural Sciences and Engineering Research Council of Canada; the National Science Council of the Republic ofChina; the Swiss National Science Foundation; the A.P.Sloan Foundation; the Bundesministerium für Bildung und Forschung, Germany; the Korean World Class University Program, the National Research Foundation of Korea; the Science and Technology Facilities Council and the RoyalSociety, UK; the Russian Foundation for Basic Research;t he Ministerio de Ciencia e Innovación, and Programa Consolider-Ingenio 2010, Spain; the Slovak R&D Agency; the Academy of Finland; the Australian Research Council(ARC); and the EU community Marie Curie Fellowship contract 302103.es_ES
dc.format.extent14 p.es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rights© 2014 American Physical Society*
dc.sourcePhys. Rev. D, Vol. 90, Num. 1, Pag. 012013 (2014)es_ES
dc.titleStudy of orbitally excited B mesons and evidence for a new Bp resonancees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1103/PhysRevD.90.012013es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1103/PhysRevD.90.012013
dc.type.versionpublishedVersiones_ES


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