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Search for gamma (1S,2S) -˃ Z(c)(+)Z(c)((')-) and e(+)e(-) -˃ Z(c)(+)Z(c)((')-) at root s=10.52, 10.58, and 10.867 Gev

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dc.contributor.authorJia, S.-
dc.contributor.authorShen, C. P.-
dc.contributor.authorYuan, C. Z.-
dc.contributor.authorAdachi, I.-
dc.contributor.authorAihara, H.-
dc.contributor.authorAl Said, S.-
dc.contributor.authorAsner, D. M.-
dc.contributor.authorCheon, B. G.-
dc.contributor.authorKim, S. H.-
dc.contributor.authorLee, I. S.-
dc.date.accessioned2022-07-11T17:14:47Z-
dc.date.available2022-07-11T17:14:47Z-
dc.date.created2021-05-14-
dc.date.issued2018-06-
dc.identifier.issn2470-0010-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/149826-
dc.description.abstractThe first search for double charged charmoniumlike state production in gamma (IS) and gamma (2S) decays and in e(+) e(-) annihilation at root s = 10.52, 10.58, and 10.867 GcV is conducted using data collected with the Belle detector at the KEKB asymmetric energy electron-positron collider. No significant signals are observed in any of the studied modes, and the 90% credibility level upper limits on their product branching fractions in gamma(1S) and gamma(2S) decays [B(gamma(1S, 2S) -˃ Z(c)(+)Z(c)((')-)) x B(Z(c)(+) -˃ pi(+) + c (c) over bar ) (c (c) over bar = J / psi, chi(c1) (1P), psi(2S))] and the product of Born cross section and branching fraction for e(+)e(-) -˃ Z(c)(+)Z(c)((')-)) (sigma(e(+)e(-) -˃ Z(c)(+)Z(c)((')-)) x B(Z(c)(+) -˃ pi(+) + c (c) over bar )) at root s = 10.52, 10.58, and 10.867 GeV are determined. Here, Z(c) refers to the Z(c) (3900) and Z(c) (4200) observed in the pi J/psi final state, the Z(c1)(4050) and Z(c2)(4250) in the pi chi(c1)(1P) final state, and the Z(c)(4050) and Z(c)(4430) in the pi psi(2S) final state.-
dc.language영어-
dc.language.isoen-
dc.publisherAMER PHYSICAL SOC-
dc.titleSearch for gamma (1S,2S) -˃ Z(c)(+)Z(c)((')-) and e(+)e(-) -˃ Z(c)(+)Z(c)((')-) at root s=10.52, 10.58, and 10.867 Gev-
dc.title.alternativeSearch for ϒ(1S,2S)→Zc+Zc(′)− and e+e−→Zc+Zc(′)− at s=10.52 , 10.58, and 10.867 GeV-
dc.typeArticle-
dc.contributor.affiliatedAuthorCheon, B. G.-
dc.identifier.doi10.1103/PhysRevD.97.112004-
dc.identifier.scopusid2-s2.0-85050300383-
dc.identifier.wosid000435334600001-
dc.identifier.bibliographicCitationPHYSICAL REVIEW D, v.97, no.11, pp.1 - 16-
dc.relation.isPartOfPHYSICAL REVIEW D-
dc.citation.titlePHYSICAL REVIEW D-
dc.citation.volume97-
dc.citation.number11-
dc.citation.startPage1-
dc.citation.endPage16-
dc.type.rimsART-
dc.type.docType정기학술지(Article(Perspective Article포함))-
dc.description.journalClass1-
dc.description.isOpenAccessY-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
dc.subject.keywordPlusPHOTON ANNIHILATION-
dc.subject.keywordPlusIDENTIFICATION-
dc.identifier.urlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.97.112004-
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