Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/138437
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dc.contributor.authorGarra Ticó, Jordi-
dc.contributor.authorGraugés Pous, Eugeni-
dc.contributor.authorBABAR Collaboration-
dc.date.accessioned2019-07-26T10:46:24Z-
dc.date.available2019-07-26T10:46:24Z-
dc.date.issued2009-11-18-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/2445/138437-
dc.description.abstractWe present evidence of D 0 − ¯¯¯ D 0 mixing using a time-dependent amplitude analysis of the decay D 0 → K + π − π 0 in a data sample of 384     fb − 1 collected with the BABAR detector at the PEP-II e + e − collider at the Stanford Linear Accelerator Center. Assuming C P conservation, we measure the mixing parameters x ′ K π π 0 = [ 2.61 + 0.57 − 0.68 ( stat ) ± 0.39 ( syst ) ] % , y ′ K π π 0 = [ − 0.06 + 0.55 − 0.64 ( stat ) ± 0.34 ( syst ) ] % . This result is inconsistent with the no-mixing hypothesis with a significance of 3.2 standard deviations. We find no evidence of C P violation in mixing.-
dc.format.extent8 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.103.211801-
dc.relation.ispartofPhysical Review Letters, 2009, vol. 103, num. 21, p. 211801-
dc.relation.urihttps://doi.org/10.1103/PhysRevLett.103.211801-
dc.rights(c) American Physical Society, 2009-
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.titleMeasurement of D0−¯¯¯D0 Mixing from a Time-Dependent Amplitude Analysis of D0→K+π−π0 Decays-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec577730-
dc.date.updated2019-07-26T10:46:24Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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