Amplitude analysis of the radiative decay B0 s → K+K−γ 

dc.contributor.authorComerma Montells, Albert
dc.contributor.authorGarcia Moreno, Paula
dc.contributor.authorGarrido Beltrán, Lluís
dc.contributor.authorGioventù, Alessandra
dc.contributor.authorGironella Gironell, Pere
dc.contributor.authorGomez Fernandez, Sergio
dc.contributor.authorGraugés Pous, Eugeni
dc.contributor.authorLobo Salvia, Aniol
dc.contributor.authorLópez Huertas, Albert
dc.contributor.authorManera Escalero, Rafel
dc.contributor.authorMarin Benito, Carla
dc.contributor.authorMauricio Ferre, Joan
dc.contributor.authorCalefice, Lukas
dc.contributor.authorVazquez Gomez, Ricardo
dc.contributor.authorLHCb Collaboration
dc.date.accessioned2025-07-04T15:15:26Z
dc.date.available2025-07-04T15:15:26Z
dc.date.issued2024
dc.date.updated2025-07-04T15:15:26Z
dc.description.abstractA search for radiative decay of B0 s mesons to orbitally excited K+K− states is performed using proton proton collisions recorded by the LHCb experiment, corresponding to an integrated luminosity of 9 fb−1 . The dikaon spectrum in the mass range mKK < 2400 MeV/c 2 is dominated by the ϕ(1020) resonance that accounts for almost 70% of the decay rate. Considering the possible contributions of f2(1270), f ′ 2 (1525) and f2(2010) meson states, the overall tensor contribution to the amplitude is measured to be F{f2} = 16.8 ± 0.5 (stat.) ± 0.7 (syst.)%, mostly dominated by the f ′ 2 (1525) state. Several statistically equivalent solutions are obtained for the detailed resonant structure depending on whether the smaller amplitudes interfere destructively or constructively with the dominant amplitude. The preferred solution that corresponds to the lowest values of the ft fractions along with constructive interference leads to the relative branching ratio measurement B(B0 s → f ′ 2γ) B(B0 s → ϕγ) = 19.4 +0.9 −0.8 (stat.) +1.4 −0.5 (syst.) ± 0.5 (B)%, where the last uncertainty is due to the ratio of measured branching fractions to the K+K− fnal state. This result represents the frst observation of the radiative B0 s → f ′ 2 (1525)γ decay, which is the second radiative transition observed in the B0 s sector. 
dc.format.extent39 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec756555
dc.identifier.issn1126-6708
dc.identifier.urihttps://hdl.handle.net/2445/222020
dc.language.isoeng
dc.publisherSpringer Verlag
dc.relation.isformatofReproducció del document publicat a: https://doi.org/10.1007/JHEP08(2024)093
dc.relation.ispartofJournal of High Energy Physics, 2024, vol. 2024, num.93
dc.relation.urihttps://doi.org/10.1007/JHEP08(2024)093
dc.rightscc-by (c) Aaij, R. et al., 2024
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationFísica de partícules
dc.subject.classificationHadrons
dc.subject.otherParticle physics
dc.subject.otherHadrons
dc.titleAmplitude analysis of the radiative decay B0 s → K+K−γ 
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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