Show simple item record

dc.contributor.authorAaij, R.
dc.contributor.authorAbdelmotteleb, A. S. W.
dc.contributor.authorAbellan Beteta, C.
dc.contributor.authorAbudinén, F.
dc.contributor.authorAckernley, T.
dc.contributor.authorAdefisoye, A. A.
dc.contributor.authorAdeva, B.
dc.contributor.authorAdinolfi, M.
dc.contributor.authorAdlarson, P.
dc.contributor.authorAgapopoulou, C.
dc.contributor.authorAidala, C. A.
dc.contributor.authorAjaltouni, Z.
dc.contributor.authorAkar, S.
dc.contributor.authorAkiba, K.
dc.contributor.authorAlbicocco, P.
dc.contributor.authorAlbrecht, J.
dc.date.accessioned2024-08-26T18:32:58Z
dc.date.available2024-08-26T18:32:58Z
dc.date.issued2024-08-13
dc.identifier.urihttps://hdl.handle.net/1721.1/156394
dc.description.abstractA search for radiative decay of 𝐵0𝑠 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/c2 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 {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 fit fractions along with constructive interference leads to the relative branching ratio measurement (𝐵0𝑠→𝑓′2𝛾)(𝐵0𝑠→𝜙𝛾)=19.4+0.9−0.8(stat.)+1.4−0.5(syst.)±0.5()%, where the last uncertainty is due to the ratio of measured branching fractions to the K+K− final state. This result represents the first observation of the radiative 𝐵0𝑠→𝑓′2(1525)𝛾 decay, which is the second radiative transition observed in the 𝐵0𝑠 sector.en_US
dc.publisherSpringer Berlin Heidelbergen_US
dc.relation.isversionofhttps://doi.org/10.1007/JHEP08(2024)093en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer Berlin Heidelbergen_US
dc.titleAmplitude analysis of the radiative decay B0s → K+K−γen_US
dc.typeArticleen_US
dc.identifier.citationJournal of High Energy Physics. 2024 Aug 13;2024(8):93en_US
dc.relation.journalJournal of High Energy Physicsen_US
dc.identifier.mitlicensePUBLISHER_CC
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2024-08-25T03:18:45Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.embargo.termsN
dspace.date.submission2024-08-25T03:18:45Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record