Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/131427
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dc.contributor.authorGraugés Pous, Eugeni-
dc.contributor.authorBABAR Collaboration-
dc.date.accessioned2019-04-04T13:32:36Z-
dc.date.available2019-04-04T13:32:36Z-
dc.date.issued2006-12-22-
dc.identifier.issn1550-7998-
dc.identifier.urihttps://hdl.handle.net/2445/131427-
dc.description.abstractWe report the observation of e + e − → ϕ η near √ s = 10.58     GeV with 6.5 σ significance in the K + K − γ γ final state in a data sample of 224     fb − 1 collected by the BABAR experiment at the PEP-II e + e − storage rings. We measure the restricted radiation-corrected cross section to be σ ( e + e − → ϕ η ) = 2.1 ± 0.4 ( stat ) ± 0.1 ( syst )     fb within the range | cos  θ ∗ | < 0.8 , where θ ∗ is the center-of-mass polar angle of the ϕ meson. The ϕ meson is required to be in the invariant mass range of 1.008 < m ϕ < 1.035     GeV / c 2 . The radiation-corrected cross section in the full cos  θ ∗ range is extrapolated to be 2.9 ± 0.5 ( stat ) ± 0.1 ( syst )     fb .-
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/PhysRevD.74.111103-
dc.relation.ispartofPhysical Review D, 2006, vol. 74, num. 11, p. 111103(R)-
dc.relation.urihttps://doi.org/10.1103/PhysRevD.74.111103-
dc.rights(c) American Physical Society, 2006-
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 exclusive reaction e+e− → ϕη at √-s = 10.58 GeV-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec551673-
dc.date.updated2019-04-04T13:32:36Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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