Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/3357
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dc.contributor.authorBhardwaj, V.-
dc.date.accessioned2020-12-24T07:08:15Z-
dc.date.available2020-12-24T07:08:15Z-
dc.date.issued2020-
dc.identifier.citationPhysical Review Letters 124(12).en_US
dc.identifier.otherhttps://doi.org/10.1103/PhysRevLett.124.122001-
dc.identifier.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.124.122001-
dc.identifier.urihttp://hdl.handle.net/123456789/3357-
dc.descriptionOnly IISERM authors are available in the record.-
dc.description.abstractWe report the first observation of the radiative decay of the Υ ( 1 S ) into a charmonium state. The significance of the observed signal of Υ ( 1 S ) → γ χ c 1 is 6.3 standard deviations including systematics. The branching fraction is calculated to be B [ Υ ( 1 S ) → γ χ c 1 ] = [ 4.7 + 2.4 − 1.8 ( stat ) + 0.4 − 0.5 ( sys ) × 10 − 5 ] . We also searched for Υ ( 1 S ) radiative decays into χ c 0 , 2 and η c ( 1 S , 2 S ) , 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 Υ ( 2 S ) mass using Υ ( 1 S ) tagging by the Υ ( 2 S ) → Υ ( 1 S ) π + π − transitions.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectAtomic physicsen_US
dc.subjectTaxonomyen_US
dc.subjectBelle detectorsen_US
dc.titleObservation of the Radiative Decays of Υ ( 1 S ) to χ c 1en_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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