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Differential branching fraction and angular analysis of the decay $ B_s^0 $ → ϕμ + μ −

R. AaijNikhef National Institute for Subatomic Physics, Amsterdam, The NetherlandsC. Abellán BetetaUniversitat de Barcelona, Barcelona, SpainB. AdevaUniversidad de Santiago de Compostela, Santiago de Compostela, SpainM. AdinolfiH.H. Wills Physics Laboratory, University of Bristol, Bristol, United KingdomC. AdroverCPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, FranceTony AffolderOliver Lodge Laboratory, University of Liverpool, Liverpool, United KingdomZ. AjaltouniClermont Université, Université Blaise Pascal, CNRS/IN2P3, LPC, Clermont-Ferrand, FranceJ. AlbrechtFakultät Physik, Technische Universität Dortmund, Dortmund, GermanyF. AlessioEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandM. AlexanderSchool of Physics and Astronomy, University of Glasgow, Glasgow, United KingdomS. AliNikhef National Institute for Subatomic Physics, Amsterdam, The NetherlandsG. AlkhazovPetersburg Nuclear Physics Institute (PNPI), Gatchina, RussiaP. Álvarez CartelleUniversidad de Santiago de Compostela, Santiago de Compostela, SpainA. A. AlvesSezione INFN di Roma La Sapienza, Roma, ItalyS. AmatoUniversidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, BrazilS. AmerioSezione INFN di Padova, Padova, ItalyY. AmhisLAL, Université Paris-Sud, CNRS/IN2P3, Orsay, FranceL. AnSezione INFN di Firenze, Firenze, ItalyJ. AndersonPhysik-Institut, Universität Zürich, Zürich, SwitzerlandR. AndreassenUniversity of Cincinnati, Cincinnati, OH, United StatesR. B. ApplebySchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomO. Aquines GutierrezMax-Planck-Institut für Kernphysik (MPIK), Heidelberg, GermanyF. ArchilliLaboratori Nazionali dell'INFN di Frascati, Frascati, ItalyA. ArtamonovInstitute for High Energy Physics (IHEP), Protvino, RussiaM. ArtusoSyracuse University, Syracuse, NY, United StatesE. AslanidesCPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, FranceG. AuriemmaSezione INFN di Roma La Sapienza, Roma, ItalyS. BachmannPhysikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, GermanyJ. J. BackDepartment of Physics, University of Warwick, Coventry, United KingdomC. BaessoPontif´ıcia Universidade Católica do Rio de Janeiro (PUC-Rio), Rio de Janeiro, Brazil, associated to2V. BalaguraInstitute of Theoretical and Experimental Physics (ITEP), Moscow, RussiaW. BaldiniSezione INFN di Ferrara, Ferrara, ItalyR. J. BarlowSchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomC. BarschelEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandS. BarsukLAL, Université Paris-Sud, CNRS/IN2P3, Orsay, FranceW. BarterCavendish Laboratory, University of Cambridge, Cambridge, United KingdomThomas BauerNikhef National Institute for Subatomic Physics, Amsterdam, The NetherlandsA. BayEcole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, SwitzerlandJ. BeddowSchool of Physics and Astronomy, University of Glasgow, Glasgow, United KingdomF. BedeschiSezione INFN di Pisa, Pisa, ItalyI. BediagaCentro Brasileiro de Pesquisas Físicas (CBPF), Rio de Janeiro, BrazilS. BelogurovInstitute of Theoretical and Experimental Physics (ITEP), Moscow, RussiaK. BelousInstitute for High Energy Physics (IHEP), Protvino, RussiaI. BelyaevInstitute of Theoretical and Experimental Physics (ITEP), Moscow, RussiaE. Ben-HaimLPNHE, Université Pierre et Marie Curie, Université Paris Diderot, CNRS/IN2P3, Paris, FranceG. BencivenniLaboratori Nazionali dell'INFN di Frascati, Frascati, ItalyS. BensonSchool of Physics and Astronomy, University of Edinburgh, Edinburgh, United KingdomJ. BentonH.H. Wills Physics Laboratory, University of Bristol, Bristol, United KingdomA. BerezhnoyInstitute of Nuclear Physics, Moscow State University (SINP MSU), Moscow, RussiaR. BernetPhysik-Institut, Universität Zürich, Zürich, SwitzerlandM.-O. BettlerCavendish Laboratory, University of Cambridge, Cambridge, United KingdomM. van BeuzekomNikhef National Institute for Subatomic Physics, Amsterdam, The NetherlandsA. BieńPhysikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, GermanyS. BifaniUniversity of Birmingham, Birmingham, United KingdomT. BirdSchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomA. BizzetiSezione INFN di Firenze, Firenze, ItalyP. M. BjørnstadSchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomT. BlakeEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandF. BlancEcole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, SwitzerlandJ. BlouwPhysikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, GermanyS. BluskSyracuse University, Syracuse, NY, United StatesV. BocciSezione INFN di Roma La Sapienza, Roma, ItalyA. BondarPetersburg Nuclear Physics Institute (PNPI), Gatchina, RussiaN. BondarPetersburg Nuclear Physics Institute (PNPI), Gatchina, RussiaW. BoniventoSezione INFN di Cagliari, Cagliari, ItalyS. BorghiSchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomA. BorgiaSyracuse University, Syracuse, NY, United StatesT. J. V. BowcockOliver Lodge Laboratory, University of Liverpool, Liverpool, United KingdomE. BowenPhysik-Institut, Universität Zürich, Zürich, SwitzerlandC. BozziSezione INFN di Ferrara, Ferrara, ItalyT. BrambachFakultät Physik, Technische Universität Dortmund, Dortmund, GermanyJ. F. J. van den BrandNikhef National Institute for Subatomic Physics and VU University Amsterdam, Amsterdam, The NetherlandsJ. BressieuxEcole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, SwitzerlandD. BrettSchool of Physics and Astronomy, University of Manchester, Manchester, United KingdomM. BritschMax-Planck-Institut für Kernphysik (MPIK), Heidelberg, GermanyT. BrittonSyracuse University, Syracuse, NY, United StatesN. H. BrookH.H. Wills Physics Laboratory, University of Bristol, Bristol, United KingdomH. BrownOliver Lodge Laboratory, University of Liverpool, Liverpool, United KingdomI. BurduceaHoria Hulubei National Institute of Physics and Nuclear Engineering, Bucharest-Magurele, RomaniaA. BurschePhysik-Institut, Universität Zürich, Zürich, SwitzerlandG. BusettoSezione INFN di Padova, Padova, ItalyJ. BuytaertEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandS. CadedduSezione INFN di Cagliari, Cagliari, ItalyO. CallotLAL, Université Paris-Sud, CNRS/IN2P3, Orsay, FranceM. CalviSezione INFN di Milano Bicocca, Milano, ItalyM. Calvo GomezUniversitat de Barcelona, Barcelona, SpainA. CamboniUniversitat de Barcelona, Barcelona, SpainP. CampanaLaboratori Nazionali dell'INFN di Frascati, Frascati, ItalyD. H. Cámpora PérezEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandA. CarboneSezione INFN di Bologna, Bologna, ItalyG. CarboniSezione INFN di Roma Tor Vergata, Roma, ItalyR. CardinaleSezione INFN di Genova, Genova, ItalyA. CardiniSezione INFN di Cagliari, Cagliari, ItalyH. Carranza-MejiaSchool of Physics and Astronomy, University of Edinburgh, Edinburgh, United KingdomL. CarsonImperial College London, London, United KingdomK. Carvalho AkibaUniversidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, BrazilG. CasseOliver Lodge Laboratory, University of Liverpool, Liverpool, United KingdomL. Castillo GarcíaEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandM. CattaneoEuropean Organization for Nuclear Research (CERN), Geneva, SwitzerlandCh. CauetFakultät Physik, Technische Universität Dortmund, Dortmund, Germany
2013en
ABI

Аннотация

A bstract The determination of the differential branching fraction and the first angular analysis of the decay $ B_s^0 $ → ϕμ + μ − are presented using data, corresponding to an integrated luminosity of 1.0 fb −1 , collected by the LHCb experiment at $ \sqrt{s}=7 $ TeV. The differential branching fraction is determined in bins of q 2 , the invariant dimuon mass squared. Integration over the full q 2 range yields a total branching fraction of $ \mathcal{B}\left( {B_s^0\to \phi {\mu^{+}}{\mu^{-}}} \right)=\left( {7.07_{-0.59}^{+0.64}\pm 0.71\pm 0.71} \right) $ × 10 −7 , where the first uncertainty is statistical, the second systematic, and the third originates from the branching fraction of the normalisation channel. An angular analysis is performed to determine the angular observables F L , S 3 , A 6 , and A 9 . The observables are consistent with Standard Model expectations.

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