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

dc.contributor.author
Comerma Montells, Albert
dc.contributor.author
Garcia Moreno, Paula
dc.contributor.author
Garrido Beltrán, Lluís
dc.contributor.author
Gioventù, Alessandra
dc.contributor.author
Gironella Gironell, Pere
dc.contributor.author
Gomez Fernandez, Sergio
dc.contributor.author
Graugés Pous, Eugeni
dc.contributor.author
Lobo Salvia, Aniol
dc.contributor.author
López Huertas, Albert
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Manera Escalero, Rafel
dc.contributor.author
Marin Benito, Carla
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Mauricio Ferre, Joan
dc.contributor.author
Calefice, Lukas
dc.contributor.author
Vazquez Gomez, Ricardo
dc.contributor.author
LHCb Collaboration
dc.date.issued
2025-07-04T15:15:26Z
dc.date.issued
2025-07-04T15:15:26Z
dc.date.issued
2024
dc.date.issued
2025-07-04T15:15:26Z
dc.identifier
1126-6708
dc.identifier
https://hdl.handle.net/2445/222020
dc.identifier
756555
dc.description.abstract
A 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
39 p.
dc.format
application/pdf
dc.language
eng
dc.publisher
Springer Verlag
dc.relation
Reproducció del document publicat a: https://doi.org/10.1007/JHEP08(2024)093
dc.relation
Journal of High Energy Physics, 2024, vol. 2024, num.93
dc.relation
https://doi.org/10.1007/JHEP08(2024)093
dc.rights
cc-by (c) Aaij, R. et al., 2024
dc.rights
http://creativecommons.org/licenses/by/4.0/
dc.rights
info:eu-repo/semantics/openAccess
dc.source
Articles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject
Física de partícules
dc.subject
Hadrons
dc.subject
Particle physics
dc.subject
Hadrons
dc.title
Amplitude analysis of the radiative decay B0 s → K+K−γ 
dc.type
info:eu-repo/semantics/article
dc.type
info:eu-repo/semantics/publishedVersion


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