dc.contributor.author | Aaltonen, Timo Antero | |
dc.contributor.author | Casal Laraña, Bruno | |
dc.contributor.author | Cuevas Maestro, Francisco Javier | |
dc.contributor.author | Gómez Gramuglio, Gervasio | |
dc.contributor.author | Palencia Cortezón, José Enrique | |
dc.contributor.author | Ruiz Jimeno, Alberto | |
dc.contributor.author | Scodellaro, Luca | |
dc.contributor.author | Vilar Cortabitarte, Rocío | |
dc.contributor.author | Vizán García, Jesús Manuel | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2018-06-13T08:59:21Z | |
dc.date.available | 2018-06-13T08:59:21Z | |
dc.date.issued | 2014-07 | |
dc.identifier.issn | 1550-7998 | |
dc.identifier.issn | 1550-2368 | |
dc.identifier.other | FPA2014-55295-C3-1-R | |
dc.identifier.other | FPA 2011-28694-C02-01 | |
dc.identifier.uri | http://hdl.handle.net/10902/13863 | |
dc.description.abstract | Using 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.sponsorship | We 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.extent | 14 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | American Physical Society | es_ES |
dc.rights | © 2014 American Physical Society | * |
dc.source | Phys. Rev. D, Vol. 90, Num. 1, Pag. 012013 (2014) | es_ES |
dc.title | Study of orbitally excited B mesons and evidence for a new Bp resonance | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1103/PhysRevD.90.012013 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1103/PhysRevD.90.012013 | |
dc.type.version | publishedVersion | es_ES |