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dc.contributor.author천병구-
dc.date.accessioned2021-05-13T05:35:25Z-
dc.date.available2021-05-13T05:35:25Z-
dc.date.issued2020-03-
dc.identifier.citationPHYSICAL REVIEW LETTERS, v. 124, no. 12, article no. 122001en_US
dc.identifier.issn0031-9007-
dc.identifier.issn1079-7114-
dc.identifier.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.124.122001-
dc.identifier.urihttps://repository.hanyang.ac.kr/handle/20.500.11754/162028-
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.en_US
dc.description.sponsorshipWe thank the KEKB group for excellent operation of the accelerator; the KEK cryogenics group for efficient solenoid operations; and the KEK computer group, the NII, and PNNL/EMSL for valuable computing and SINET5 network support. We acknowledge support from MEXT, JSPS and Nagoya’s TLPRC (Japan); ARC (Australia); FWF (Austria); NSFC and CCEPP (China); MSMT (Czechia); CZF, DFG, EXC153, and VS (Germany); DST (India); INFN (Italy); MOE, MSIP, NRF, RSRI, FLRFAS project, GSDC of KISTI and KREONET/GLORIAD (Korea); MNiSW and NCN (Poland); RSF, Grant No. 18-12-00226 (Russia); ARRS (Slovenia); IKERBASQUE (Spain); SNSF (Switzerland); MOE and MOST (Taiwan); and DOE and NSF (USA).en_US
dc.language.isoenen_US
dc.publisherAMER PHYSICAL SOCen_US
dc.titleObservation of the Radiative Decays of Upsilon(1S) to chi(c1)en_US
dc.typeArticleen_US
dc.relation.no12-
dc.relation.volume124-
dc.identifier.doi10.1103/PhysRevLett.124.122001-
dc.relation.page122001-122001-
dc.relation.journalPHYSICAL REVIEW LETTERS-
dc.contributor.googleauthorKatrenko, P.-
dc.contributor.googleauthorAdachi, I.-
dc.contributor.googleauthorAihara, H.-
dc.contributor.googleauthorAl Said, S.-
dc.contributor.googleauthorAsner, D. M.-
dc.contributor.googleauthorAushev, T.-
dc.contributor.googleauthorBadhrees, I.-
dc.contributor.googleauthorBahinipati, S.-
dc.contributor.googleauthorBehera, P.-
dc.contributor.googleauthorCheon, B. G.-
dc.relation.code2020048853-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidbgcheon-


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