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dc.contributor.authorCMS Collaboration
dc.date.accessioned2022-07-12T20:35:08Z
dc.date.available2022-07-12T20:35:08Z
dc.date.issued2022-05-31
dc.identifier.citationTumasyan, A., Adam, W., Andrejkovic, J.W. et al. Observation of B0 → ψ(2S)K0Sπ+π− and B0s → ψ(2S)K0S decays. Eur. Phys. J. C 82, 499 (2022). https://doi.org/10.1140/epjc/s10052-022-10315-yen_US
dc.identifier.urihttp://hdl.handle.net/1808/32841
dc.description.abstractUsing a data sample of 𝑠√=13TeV proton-proton collisions collected by the CMS experiment at the LHC in 2017 and 2018 with an integrated luminosity of 103fb−1, the B0s→ψ(2S)K0S and B0→ψ(2S)K0Sπ+π− decays are observed with significances exceeding 5 standard deviations. The resulting branching fraction ratios, measured for the first time, correspond to ℬ(B0s→ψ(2S)𝐾0S)/ℬ(B0→ψ(2S)𝐾0S)=(3.33±0.69(stat)±0.11(syst)±0.34(𝑓s/𝑓d))×10−2 and ℬ(B0→ψ(2S)K0Sπ+π−)/ℬ(B0→ψ(2S)K0S)=0.480±0.013(stat)±0.032(syst), where the last uncertainty in the first ratio is related to the uncertainty in the ratio of production cross sections of B0s and B0 mesons, 𝑓s/𝑓d.en_US
dc.publisherSpringerOpenen_US
dc.rights© CERN for the benefit of the CMS collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleObservation of B0 → ψ(2S)K0 Sπ + π− and B0 s → ψ(2S)K0 S decaysen_US
dc.typeArticleen_US
kusw.kuauthorAbreu, A.
kusw.kuauthorAnguiano, J.
kusw.kuauthorBaldenegro Barrera, C.
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorFlowers, Z.
kusw.kuauthorIsidori, T.
kusw.kuauthorKhalil, S.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
kusw.kuauthorKropivnitskaya, A.
kusw.kuauthorLazarovits, M.
kusw.kuauthorLe Mahieu, C.
kusw.kuauthorLindsey, C.
kusw.kuauthorMarquez, J.
kusw.kuauthorMinafra, N.
kusw.kuauthorMurray, M.
kusw.kuauthorNickel, M.
kusw.kuauthorRogan, C.
kusw.kuauthorRoyon, C.
kusw.kuauthorSalvatico, R.
kusw.kuauthorSanders, S.
kusw.kuauthorSchmitz, E.
kusw.kuauthorSmith, C.
kusw.kuauthorWang, Q.
kusw.kuauthorWarner, Z.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-022-10315-yen_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC35666690en_US
dc.rights.accessrightsopenAccessen_US


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© CERN for the benefit of the CMS collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.
Except where otherwise noted, this item's license is described as: © CERN for the benefit of the CMS collaboration 2022. This article is licensed under a Creative Commons Attribution 4.0 International License.