Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/138427
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dc.contributor.authorGarra Ticó, Jordi-
dc.contributor.authorGraugés Pous, Eugeni-
dc.contributor.authorBABAR Collaboration-
dc.date.accessioned2019-07-26T13:14:39Z-
dc.date.available2019-07-26T13:14:39Z-
dc.date.issued2008-01-15-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/2445/138427-
dc.description.abstractWe present measurements of the semileptonic decays B − → D 0 τ − ¯ ν τ , B − → D * 0 τ − ¯ ν τ , ¯¯¯ B 0 → D + τ − ¯ ν τ , and ¯¯¯ B 0 → D * + τ − ¯ ν τ , which are potentially sensitive to non-standard model amplitudes. The data sample comprises 232 × 10 6 Υ ( 4 S ) → B ¯¯¯ B decays collected with the BABAR detector. From a combined fit to B − and ¯¯¯ B 0 channels, we obtain the branching fractions B ( B → D τ − ¯ ν τ ) = ( 0.86 ± 0.24 ± 0.11 ± 0.06 ) % and B ( B → D ∗ τ − ¯ ν τ ) = ( 1.62 ± 0.31 ± 0.10 ± 0.05 ) % (normalized for the ¯¯¯ B 0 ), where the uncertainties are statistical, systematic, and normalization-mode-related.-
dc.format.extent7 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoeng-
dc.publisherAmerican Physical Society-
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1103/PhysRevLett.100.021801-
dc.relation.ispartofPhysical Review Letters, 2008, vol. 100, num. 2, p. 021801-
dc.relation.urihttps://doi.org/10.1103/PhysRevLett.100.021801-
dc.rights(c) American Physical Society, 2008-
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)-
dc.subject.classificationFísica de partícules-
dc.subject.classificationExperiments-
dc.subject.otherParticle physics-
dc.subject.otherExperiments-
dc.titleObservation of the Semileptonic Decays B→D∗τ−¯ντ and Evidence for B→Dτ−¯ντ-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec577709-
dc.date.updated2019-07-26T13:14:39Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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