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Observation of the Radiative Decays of ϒ⁡(1⁢) to ⁢1

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dc.contributor.authorKatrenko, P.-
dc.contributor.authorAdachi, I-
dc.contributor.authorAihara, H.-
dc.contributor.authorAl Said, S.-
dc.contributor.authorAsner, D. M.-
dc.contributor.authorAushev, T.-
dc.contributor.authorBadhrees, I-
dc.contributor.authorBahinipati, S.-
dc.contributor.authorBehera, P.-
dc.contributor.authorBeleno, C.-
dc.contributor.authorBennett, J.-
dc.contributor.authorBhardwaj, V-
dc.contributor.authorBhuyan, B.-
dc.contributor.authorBiswal, J.-
dc.contributor.authorBobrov, A.-
dc.contributor.authorBonvicini, G.-
dc.contributor.authorBracko, M.-
dc.contributor.authorCampajola, M.-
dc.contributor.authorCao, L.-
dc.contributor.authorCervenkov, D.-
dc.contributor.authorChekelian, V-
dc.contributor.authorChen, A.-
dc.contributor.authorCheon, B. G.-
dc.contributor.authorChilikin, K.-
dc.contributor.authorCho, H. E.-
dc.contributor.authorCho, K.-
dc.contributor.authorChoi, S. K.-
dc.contributor.authorChoi, Y.-
dc.contributor.authorChoudhury, S.-
dc.contributor.authorCinabro, D.-
dc.contributor.authorCunliffe, S.-
dc.contributor.authorDi Capua, F.-
dc.contributor.authorDi Carlo, S.-
dc.contributor.authorDolezal, Z.-
dc.contributor.authorDong, T., V-
dc.contributor.authorEidelman, S.-
dc.contributor.authorEpifanov, D.-
dc.contributor.authorFast, J. E.-
dc.contributor.authorFulsom, B. G.-
dc.contributor.authorGarg, R.-
dc.contributor.authorGaur, V-
dc.contributor.authorGabyshev, N.-
dc.contributor.authorGarmash, A.-
dc.contributor.authorGiri, A.-
dc.contributor.authorGoldenzweig, P.-
dc.contributor.authorGolob, B.-
dc.contributor.authorGrzymkowska, O.-
dc.contributor.authorHartbrich, O.-
dc.contributor.authorHayasaka, K.-
dc.contributor.authorHayashii, H.-
dc.contributor.authorHou, W. S.-
dc.contributor.authorIijima, T.-
dc.contributor.authorInami, K.-
dc.contributor.authorIshikawa, A.-
dc.contributor.authorItoh, R.-
dc.contributor.authorIwasaki, M.-
dc.contributor.authorIwasaki, Y.-
dc.contributor.authorJacobs, W. W.-
dc.contributor.authorJeon, H. B.-
dc.contributor.authorJia, S.-
dc.contributor.authorJin, Y.-
dc.contributor.authorJoffe, D.-
dc.contributor.authorJoo, K. K.-
dc.contributor.authorKaryan, G.-
dc.contributor.authorKichimi, H.-
dc.contributor.authorKim, D. Y.-
dc.contributor.authorKim, K. T.-
dc.contributor.authorKim, S. H.-
dc.contributor.authorKinoshita, K.-
dc.contributor.authorKodys, P.-
dc.contributor.authorKorpar, S.-
dc.contributor.authorKrizan, P.-
dc.contributor.authorKroeger, R.-
dc.contributor.authorKuhr, T.-
dc.contributor.authorLee, I. S.-
dc.contributor.authorLee, S. C.-
dc.contributor.authorLewis, P.-
dc.contributor.authorLi, Y. B.-
dc.contributor.authorLi Gioi, L.-
dc.contributor.authorLibby, J.-
dc.contributor.authorLieret, K.-
dc.contributor.authorMacQueen, C.-
dc.contributor.authorMasuda, M.-
dc.contributor.authorMatsuda, T.-
dc.contributor.authorMatvienko, D.-
dc.contributor.authorMerola, M.-
dc.contributor.authorMiyabayashi, K.-
dc.contributor.authorMiyata, H.-
dc.contributor.authorMizuk, R.-
dc.contributor.authorMohanty, G. B.-
dc.contributor.authorMoon, T. J.-
dc.contributor.authorMori, T.-
dc.contributor.authorMussa, R.-
dc.contributor.authorNakano, E.-
dc.contributor.authorNakano, T.-
dc.contributor.authorNakao, M.-
dc.contributor.authorNayak, M.-
dc.contributor.authorNisar, N. K.-
dc.contributor.authorNishida, S.-
dc.contributor.authorNishimura, K.-
dc.contributor.authorOno, H.-
dc.contributor.authorOnuki, Y.-
dc.contributor.authorOskin, P.-
dc.contributor.authorPakhlov, P.-
dc.contributor.authorPakhlova, G.-
dc.contributor.authorPang, T.-
dc.contributor.authorPardi, S.-
dc.contributor.authorPark, C. W.-
dc.contributor.authorPark, H.-
dc.contributor.authorPark, S. H.-
dc.contributor.authorPaul, S.-
dc.contributor.authorPedlar, T. K.-
dc.contributor.authorPestotnik, R.-
dc.contributor.authorPiilonen, L. E.-
dc.contributor.authorPopov, V-
dc.contributor.authorPrencipe, E.-
dc.contributor.authorPrim, M. T.-
dc.contributor.authorRitter, M.-
dc.contributor.authorRostomyan, A.-
dc.contributor.authorRout, N.-
dc.contributor.authorRusso, G.-
dc.contributor.authorSahoo, D.-
dc.contributor.authorSakai, Y.-
dc.contributor.authorSandilya, S.-
dc.contributor.authorSanuki, T.-
dc.contributor.authorSavinov, V-
dc.contributor.authorSchneider, O.-
dc.contributor.authorSchnell, G.-
dc.contributor.authorSchueler, J.-
dc.contributor.authorSchwanda, C.-
dc.contributor.authorSeino, Y.-
dc.contributor.authorSenyo, K.-
dc.contributor.authorSevior, M. E.-
dc.contributor.authorShen, C. P.-
dc.contributor.authorShiu, J. G.-
dc.contributor.authorSolovieva, E.-
dc.contributor.authorStaric, M.-
dc.contributor.authorStottler, Z. S.-
dc.contributor.authorSumiyoshi, T.-
dc.contributor.authorSutcliffe, W.-
dc.contributor.authorTakizawa, M.-
dc.contributor.authorTamponi, U.-
dc.contributor.authorTanida, K.-
dc.contributor.authorTenchini, F.-
dc.contributor.authorTrabelsi, K.-
dc.contributor.authorUchida, M.-
dc.contributor.authorUehara, S.-
dc.contributor.authorUglov, T.-
dc.contributor.authorUnno, Y.-
dc.contributor.authorUno, S.-
dc.contributor.authorUrquijo, P.-
dc.contributor.authorUsov, Y.-
dc.contributor.authorVan Tonder, R.-
dc.contributor.authorVarner, G.-
dc.contributor.authorVossen, A.-
dc.contributor.authorWang, B.-
dc.contributor.authorWang, C. H.-
dc.contributor.authorWang, M. Z.-
dc.contributor.authorWang, P.-
dc.contributor.authorWang, X. L.-
dc.contributor.authorWon, E.-
dc.contributor.authorYang, S. B.-
dc.contributor.authorYe, H.-
dc.contributor.authorYelton, J.-
dc.contributor.authorYin, J. H.-
dc.contributor.authorYuan, C. Z.-
dc.contributor.authorYusa, Y.-
dc.contributor.authorZhang, Z. P.-
dc.contributor.authorZhilich, V-
dc.contributor.authorZhukova, V-
dc.date.accessioned2024-12-02T22:30:40Z-
dc.date.available2024-12-02T22:30:40Z-
dc.date.issued2020-03-
dc.identifier.issn0031-9007-
dc.identifier.issn1079-7114-
dc.identifier.urihttps://scholarworks.gnu.ac.kr/handle/sw.gnu/72410-
dc.description.abstractWe report the first observation of the radiative decay of the Upsilon(1S) into a charmonium state. The significance of the observed signal of Upsilon(1S) -> gamma chi(c1) is 6.3 standard deviations including systematics. The branching fraction is calculated to be B[Upsilon(1S) -> gamma chi(c1)] = [4.7(-1.8)(+2.4) (stat)(-0.5)(+0.4) (sys) x 10(-5)]. We also searched for Upsilon(1S) radiative decays into chi(c0.2) and eta(c)(1S, 2S), and set upper limits on their branching fractions. These results are obtained from a 24.9 fb(-1) data sample collected with the Belle detector at the KEKB asymmetric-energy e(+)e(-) collider at a center-of-mass energy equal to the Upsilon(2S) mass using Upsilon(1S) tagging by the Upsilon(2S) -> Upsilon(1S)pi(+)pi(-) transitions.-
dc.language영어-
dc.language.isoENG-
dc.publisherAmerican Physical Society-
dc.titleObservation of the Radiative Decays of ϒ⁡(1⁢) to ⁢1-
dc.title.alternativeObservation of the Radiative Decays of Υ(1<i>S</i>) to χ<sub><i>c</i>1</sub>-
dc.typeArticle-
dc.publisher.location미국-
dc.identifier.doi10.1103/PhysRevLett.124.122001-
dc.identifier.scopusid2-s2.0-85083545972-
dc.identifier.wosid000522195100004-
dc.identifier.bibliographicCitationPhysical Review Letters, v.124, no.12-
dc.citation.titlePhysical Review Letters-
dc.citation.volume124-
dc.citation.number12-
dc.type.docTypeArticle-
dc.description.isOpenAccessY-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryPhysics, Multidisciplinary-
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