Study of γ γ → γ ψ ( 2 S ) at Belle

dc.contributor.authorBhardwaj, Vishal
dc.contributor.authorPatra, Sourav
dc.date.accessioned2023-08-23T12:07:11Z
dc.date.available2023-08-23T12:07:11Z
dc.date.issued2022
dc.descriptionOnly IISER Mohali authors are available in the record.en_US
dc.description.abstractUsing 980     fb − 1 of data at and around the Υ ( n S ) ( n = 1 , 2, 3, 4, 5) resonances collected with the Belle detector at the KEKB asymmetric-energy e + e − collider, the two-photon process γ γ → γ ψ ( 2 S ) is studied from the threshold to 4.2 GeV for the first time. Two structures are seen in the invariant mass distribution of γ ψ ( 2 S ) : one at M R 1 = 3922.4 ± 6.5 ± 2.0     MeV / c 2 with a width of Γ R 1 = 22 ± 17 ± 4     MeV , and another at M R 2 = 4014.3 ± 4.0 ± 1.5     MeV / c 2 with a width of Γ R 2 = 4 ± 11 ± 6     MeV ; the signals are parametrized with the incoherent sum of two Breit-Wigner functions. The first structure is consistent with the X ( 3915 ) or the χ c 2 ( 3930 ) , and the local statistical significance is determined to be 3.1 σ with the systematic uncertainties included. The second matches none of the known charmonium or charmoniumlike states, and its global significance is determined to be 2.8 σ including the look-elsewhere effect. The production rates are Γ γ γ B ( R 1 → γ ψ ( 2 S ) ) = 9.8 ± 3.6 ± 1.3     eV assuming ( J P C , | λ | ) = ( 0 + + , 0 ) or 2.0 ± 0.7 ± 0.2     eV with ( 2 + + , 2 ) for the first structure and Γ γ γ B ( R 2 → γ ψ ( 2 S ) ) = 6.2 ± 2.2 ± 0.8     eV with ( 0 + + , 0 ) or 1.2 ± 0.4 ± 0.2     eV with ( 2 + + , 2 ) for the second. Here, the first errors are statistical and the second systematic, and λ is the helicity.en_US
dc.identifier.citationPhysical Review D, 105(11), 112011(1-11).en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.105.112011
dc.identifier.urihttp://hdl.handle.net/123456789/5093
dc.language.isoen_USen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectγ γ → γ ψen_US
dc.subject( 2 S ) at Belleen_US
dc.titleStudy of γ γ → γ ψ ( 2 S ) at Belleen_US
dc.typeArticleen_US

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