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dc.contributor.authorBabar Collaboration-
dc.contributor.authorLópez-March, Neus-
dc.contributor.authorMartínez-Vidal, Fernando-
dc.contributor.authorMilanés, Diego A.-
dc.contributor.authorOyanguren, Arantza-
dc.contributor.authorSánchez, P. D.-
dc.contributor.authorLees, J. P.-
dc.date.accessioned2010-11-16T13:44:26Z-
dc.date.available2010-11-16T13:44:26Z-
dc.date.issued2010-10-19-
dc.identifier.citationPhysical Review Letters 105 (17): 172001(2010)es_ES
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10261/29133-
dc.description.abstractWe present a search for f(J)(2220) production in radiative J/psi --> gamma f(J)(2220) decays using 460 fb(-1) of data collected with the BABAR detector at the SLAC PEP-II e(+)e(-) collider. The f(J)(2220) is searched for in the decays to K+K- and (KSKS0)-K-0. No evidence of this resonance is observed, and 90% confidence level upper limits on the product of the branching fractions for J/psi --> gamma f(J)(2220) and f(J)(2220) --> K+K-((KSKS0)-K-0) as a function of spin and helicity are set at the level of 10(-5), below the central values reported by the Mark III experiment.es_ES
dc.description.sponsorshipWe are grateful for the excellent luminosity and machine conditions provided by our PEP-II colleagues, and for the substantial dedicated effort from the computing organizations that support BABAR. The collaborating institutions wish to thank SLAC for its support and kind hospitality. This work is supported by DOE and NSF (USA), NSERC (Canada), CEA and CNRS-IN2P3 (France), BMBF and DFG (Germany), INFN (Italy), FOM (The Netherlands), NFR (Norway), MES (Russia), MICIIN (Spain), STFC (United Kingdom). Individuals have received support from the Marie Curie EIF (European Union), the A. P. Sloan Foundation (USA) and the Binational Science Foundation (USA-Israel).es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rightsopenAccesses_ES
dc.titleSearch for f (J) (2220) in Radiative J/psi Decayses_ES
dc.typeartículoes_ES
dc.identifier.doi10.1103/PhysRevLett.105.172001-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1103/PhysRevLett.105.172001es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.cerifentitytypePublications-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.languageiso639-1en-
item.openairetypeartículo-
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