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Search for charmonium and charmoniumlike states in Y(1S) radiative decays

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dc.contributor.authorShen, C. P.-
dc.contributor.authorWang, X. L.-
dc.contributor.authorYuan, C. Z.-
dc.contributor.authorWang, P.-
dc.contributor.authorAdachi, I.-
dc.contributor.authorAihara, H.-
dc.contributor.authorAushev, T.-
dc.contributor.authorBakich, A. M.-
dc.contributor.authorBalagura, V.-
dc.contributor.authorBelous, K.-
dc.contributor.authorBhardwaj, V.-
dc.contributor.authorBischofberger, M.-
dc.contributor.authorBracko, M.-
dc.contributor.authorBrowder, T. E.-
dc.contributor.authorChang, M. -C.-
dc.contributor.authorChen, K. -F.-
dc.contributor.authorChen, P.-
dc.contributor.authorCheon, B. G.-
dc.contributor.authorChoi, Y.-
dc.contributor.authorDalseno, J.-
dc.contributor.authorDanilov, M.-
dc.contributor.authorDolezal, Z.-
dc.contributor.authorEidelman, S.-
dc.contributor.authorGabyshev, N.-
dc.contributor.authorHa, H.-
dc.contributor.authorHaba, J.-
dc.contributor.authorHayasaka, K.-
dc.contributor.authorHayashii, H.-
dc.contributor.authorHorii, Y.-
dc.contributor.authorHoshi, Y.-
dc.contributor.authorHou, W. -S.-
dc.contributor.authorHyun, H. J.-
dc.contributor.authorInami, K.-
dc.contributor.authorItoh, R.-
dc.contributor.authorIwabuchi, M.-
dc.contributor.authorIwasaki, Y.-
dc.contributor.authorJulius, T.-
dc.contributor.authorKang, J. H.-
dc.contributor.authorKawai, H.-
dc.contributor.authorKawasaki, T.-
dc.contributor.authorKichimi, H.-
dc.contributor.authorKiesling, C.-
dc.contributor.authorKim, H. J.-
dc.contributor.authorKim, M. J.-
dc.contributor.authorKim, Y. J.-
dc.contributor.authorKo, B. R.-
dc.contributor.authorKrizan, P.-
dc.contributor.authorKuhr, T.-
dc.contributor.authorKuzmin, A.-
dc.contributor.authorLange, J. S.-
dc.contributor.authorLee, M. J.-
dc.contributor.authorLee, S. -H.-
dc.contributor.authorLeitner, R.-
dc.contributor.authorLi, J.-
dc.contributor.authorLiu, C.-
dc.contributor.authorLouvot, R.-
dc.contributor.authorMcOnie, S.-
dc.contributor.authorMiyabayashi, K.-
dc.contributor.authorMiyata, H.-
dc.contributor.authorMiyazaki, Y.-
dc.contributor.authorMohanty, G. B.-
dc.contributor.authorMussa, R.-
dc.contributor.authorNakano, E.-
dc.contributor.authorNakao, M.-
dc.contributor.authorNatkaniec, Z.-
dc.contributor.authorNishida, S.-
dc.contributor.authorOhshima, T.-
dc.contributor.authorOkuno, S.-
dc.contributor.authorOlsen, S. L.-
dc.contributor.authorPakhlova, G.-
dc.contributor.authorPark, C. W.-
dc.contributor.authorPark, H.-
dc.contributor.authorPestotnik, R.-
dc.contributor.authorPetric, M.-
dc.contributor.authorPiilonen, L. E.-
dc.contributor.authorRoehrken, M.-
dc.contributor.authorRyu, S.-
dc.contributor.authorSakai, Y.-
dc.contributor.authorSchneider, O.-
dc.contributor.authorSchwanda, C.-
dc.contributor.authorSenyo, K.-
dc.contributor.authorSevior, M. E.-
dc.contributor.authorShang, L.-
dc.contributor.authorShapkin, M.-
dc.contributor.authorShiu, J. -G.-
dc.contributor.authorShwartz, B.-
dc.contributor.authorSmerkol, P.-
dc.contributor.authorSolovieva, E.-
dc.contributor.authorStanic, S.-
dc.contributor.authorStaric, M.-
dc.contributor.authorTeramoto, Y.-
dc.contributor.authorUglov, T.-
dc.contributor.authorUnno, Y.-
dc.contributor.authorUno, S.-
dc.contributor.authorVarner, G.-
dc.contributor.authorVervink, K.-
dc.contributor.authorWang, C. H.-
dc.contributor.authorWang, M. -Z.-
dc.contributor.authorWedd, R.-
dc.contributor.authorWon, E.-
dc.contributor.authorYamashita, Y.-
dc.contributor.authorYamauchi, M.-
dc.contributor.authorZhang, C. C.-
dc.contributor.authorZhang, Z. P.-
dc.contributor.authorZhou, P.-
dc.contributor.authorZhulanov, V.-
dc.contributor.authorZivko, T.-
dc.contributor.authorZupanc, A.-
dc.contributor.authorZyukova, O.-
dc.date.accessioned2021-09-08T00:10:52Z-
dc.date.available2021-09-08T00:10:52Z-
dc.date.created2021-06-14-
dc.date.issued2010-09-22-
dc.identifier.issn1550-7998-
dc.identifier.urihttps://scholar.korea.ac.kr/handle/2021.sw.korea/115663-
dc.description.abstractUsing a sample of 102 X 10(6) Y(1S) events collected with the Belle detector, we report on the first search for charge-parity-even charmonium and charmoniumlike states in Y(1S) radiative decays. No significant chi(cJ) or eta(c) signal is observed and 90% C. L. limits on B(Y(1S) -> gamma chi(c0)) < 6.5 X 10(-4), B(Y(1S) -> gamma chi(c1)) < 2.3 X 10(-5), B(Y(1S) -> gamma chi(c2)) < 7.6 X 10(-6), and B(Y(1S) -> gamma eta(c)) < 5.7 X 10(-5) are obtained. The product branching fraction limits B(Y(1S) -> gamma X(3872))B(X(3872) -> pi(+) pi(-) J/psi) < 1.6 X 10(-6), B(Y(1S) -> gamma X(3872))B(X(3872) -> pi+ pi(-) pi(0) J/psi) < 2.8 X 10(-6), B(Y(1S) -> gamma X(3915)) B(X(3915) -> omega J/psi) < 3.0 X 10(-6), and B(Y(1S) -> gamma Y(4140))B(Y(4140) -> phi J/psi) < 2.2 X 10(-6) are obtained at the 90% C.L. Furthermore, no evidence is found for excited charmonium states below 4.8 GeV/c(2).-
dc.languageEnglish-
dc.language.isoen-
dc.publisherAMER PHYSICAL SOC-
dc.titleSearch for charmonium and charmoniumlike states in Y(1S) radiative decays-
dc.typeArticle-
dc.contributor.affiliatedAuthorWon, E.-
dc.identifier.doi10.1103/PhysRevD.82.051504-
dc.identifier.scopusid2-s2.0-78651112953-
dc.identifier.wosid000282046500001-
dc.identifier.bibliographicCitationPHYSICAL REVIEW D, v.82, no.5-
dc.relation.isPartOfPHYSICAL REVIEW D-
dc.citation.titlePHYSICAL REVIEW D-
dc.citation.volume82-
dc.citation.number5-
dc.type.rimsART-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaAstronomy & Astrophysics-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryAstronomy & Astrophysics-
dc.relation.journalWebOfScienceCategoryPhysics, Particles & Fields-
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