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dc.contributor.authorKolcu, Onur Buğraen_US
dc.contributor.otherBESIII Collaboration
dc.date.accessioned2019-07-01T08:37:49Z
dc.date.available2019-07-01T08:37:49Z
dc.date.issued2017en_US
dc.identifier.citationAblikim, M., Achasov, M. N., Ahmed, S., Albrecht, M., Alekseev, M., Amoroso, A., . . . Collaboration, B. (2017). Branching fraction measurement of J=Psi -> KSKL and search for J=Psi -> KSKS. Physical Review D, 96(11), 7. doi:10.1103/PhysRevD.96.112001en_US
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttps://hdl.handle.net/20.500.12294/1525
dc.descriptionKolcu, Onur Buğra (Arel Author)en_US
dc.description.abstractUsing a sample of 1.31 x 10(9) J/Psi events collected with the BESIII detector at the BEPCII collider, we study the decays of J/Psi -> KSKL and KSKS. The branching fraction of J/Psi -> KSKL is determined to be B(J/Psi -> KSKL) = (1.93 +/- 0.01 (stat) +/- 0.05 (syst)) x 10(-4), which significantly improves on previous measurements. No clear signal is observed for the J/Psi -> KSKS process, and the upper limit at the 95% confidence level for its branching fraction is determined to be B(J/Psi -> KSKS) < 1.4 x 10(-8), which improves on the previous searches by 2 orders in magnitude and reaches the order of the Einstein-Podolsky-Rosen expectation.en_US
dc.language.isoengen_US
dc.publisherAmer Physical Soc.en_US
dc.relation.ispartofPhysical Review D.en_US
dc.identifier.doi10.1103/PhysRevD.96.112001en_US
dc.identifier.doi10.1103/PhysRevD.96.112001
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.titleBranching fraction measurement of J=Psi -> KSKL and search for J=Psi -> KSKSen_US
dc.typearticleen_US
dc.departmentMeslek Yüksekokulu, Optisyenlik Programıen_US
dc.authoridhttps://orcid.org/0000-0002-9177-1286en_US
dc.identifier.volume96en_US
dc.identifier.issue11en_US
dc.identifier.startpage1en_US
dc.identifier.endpage7en_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.institutionauthorKolcu, Onur Buğraen_US
dc.coverage.doi10.1103/PhysRevD.96.112001
dc.coverage.doi10.1103/PhysRevD.96.112001


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