Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/131735
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dc.contributor.authorGarra Ticó, Jordi-
dc.contributor.authorGraugés Pous, Eugeni-
dc.contributor.authorBABAR Collaboration-
dc.date.accessioned2019-04-08T09:33:22Z-
dc.date.available2019-04-08T09:33:22Z-
dc.date.issued2010-11-09-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2445/131735-
dc.description.abstractWe present a study of 649 ± 35 e + e − → c ¯ c events produced at √ s ≈ 10.6     GeV containing both a Λ + c baryon and a ¯¯¯ Λ − c antibaryon. The number observed is roughly 4 times that expected if the leading charmed hadron types are uncorrelated, confirming an observation by the CLEO Collaboration. We find a 2-jet topology in these events but very few additional baryons, demonstrating that the primary c and ¯ c are predominantly contained in a correlated baryon-antibaryon system. In addition to the charmed baryons we observe on average 2.6 ± 0.2 charged intermediate mesons, predominantly pions, carrying 65% of the remaining energy.-
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/PhysRevD.82.091102-
dc.relation.ispartofPhysical Review D, 2010, vol. 82, num. 9, p. 091102-
dc.relation.urihttps://doi.org/10.1103/PhysRevD.82.091102-
dc.rights(c) American Physical Society, 2010-
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.titleCorrelated leading baryon-antibaryon production in e+e−→c¯c→Λ+c¯¯¯Λ−cX-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.identifier.idgrec601951-
dc.date.updated2019-04-08T09:33:23Z-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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