Your browser doesn't support javascript.
loading
First Observation of Excited Ω_{b}
Aaij, R; Abellán Beteta, C; Ackernley, T; Adeva, B; Adinolfi, M; Afsharnia, H; Aidala, C A; Aiola, S; Ajaltouni, Z; Akar, S; Albicocco, P; Albrecht, J; Alessio, F; Alexander, M; Alfonso Albero, A; Alkhazov, G; Alvarez Cartelle, P; Alves, A A; Amato, S; Amhis, Y; An, L; Anderlini, L; Andreassi, G; Andreotti, M; Archilli, F; Arnau Romeu, J; Artamonov, A; Artuso, M; Arzymatov, K; Aslanides, E; Atzeni, M; Audurier, B; Bachmann, S; Back, J J; Baker, S; Balagura, V; Baldini, W; Baranov, A; Barlow, R J; Barsuk, S; Barter, W; Bartolini, M; Baryshnikov, F; Bassi, G; Batozskaya, V; Batsukh, B; Battig, A; Bay, A; Becker, M; Bedeschi, F.
Afiliação
  • Aaij R; Nikhef National Institute for Subatomic Physics, Amsterdam, Netherlands.
  • Abellán Beteta C; Physik-Institut, Universität Zürich, Zürich, Switzerland.
  • Ackernley T; Oliver Lodge Laboratory, University of Liverpool, Liverpool, United Kingdom.
  • Adeva B; Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain.
  • Adinolfi M; H.H. Wills Physics Laboratory, University of Bristol, Bristol, United Kingdom.
  • Afsharnia H; Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France.
  • Aidala CA; University of Michigan, Ann Arbor, USA (associated Syracuse University, Syracuse, New York, USA).
  • Aiola S; INFN Sezione di Milano, Milano, Italy.
  • Ajaltouni Z; Université Clermont Auvergne, CNRS/IN2P3, LPC, Clermont-Ferrand, France.
  • Akar S; Los Alamos National Laboratory (LANL), Los Alamos, New Mexico, USA.
  • Albicocco P; INFN Laboratori Nazionali di Frascati, Frascati, Italy.
  • Albrecht J; Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany.
  • Alessio F; European Organization for Nuclear Research (CERN), Geneva, Switzerland.
  • Alexander M; School of Physics and Astronomy, University of Glasgow, Glasgow, United Kingdom.
  • Alfonso Albero A; ICCUB, Universitat de Barcelona, Barcelona, Spain.
  • Alkhazov G; Petersburg Nuclear Physics Institute NRC Kurchatov Institute (PNPI NRC KI), Gatchina, Russia.
  • Alvarez Cartelle P; Imperial College London, London, United Kingdom.
  • Alves AA; Instituto Galego de Física de Altas Enerxías (IGFAE), Universidade de Santiago de Compostela, Santiago de Compostela, Spain.
  • Amato S; Universidade Federal do Rio de Janeiro (UFRJ), Rio de Janeiro, Brazil.
  • Amhis Y; LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay, France.
  • An L; INFN Sezione di Firenze, Firenze, Italy.
  • Anderlini L; INFN Sezione di Firenze, Firenze, Italy.
  • Andreassi G; Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland.
  • Andreotti M; INFN Sezione di Ferrara, Ferrara, Italy.
  • Archilli F; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany.
  • Arnau Romeu J; Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France.
  • Artamonov A; Institute for High Energy Physics NRC Kurchatov Institute (IHEP NRC KI), Protvino, Russia, Protvino, Russia.
  • Artuso M; Syracuse University, Syracuse, New York, USA.
  • Arzymatov K; Yandex School of Data Analysis, Moscow, Russia.
  • Aslanides E; Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France.
  • Atzeni M; Physik-Institut, Universität Zürich, Zürich, Switzerland.
  • Audurier B; INFN Sezione di Cagliari, Monserrato, Italy.
  • Bachmann S; Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany.
  • Back JJ; Department of Physics, University of Warwick, Coventry, United Kingdom.
  • Baker S; Imperial College London, London, United Kingdom.
  • Balagura V; LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay, France.
  • Baldini W; INFN Sezione di Ferrara, Ferrara, Italy.
  • Baranov A; European Organization for Nuclear Research (CERN), Geneva, Switzerland.
  • Barlow RJ; Yandex School of Data Analysis, Moscow, Russia.
  • Barsuk S; Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom.
  • Barter W; LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, Orsay, France.
  • Bartolini M; Imperial College London, London, United Kingdom.
  • Baryshnikov F; INFN Sezione di Genova, Genova, Italy.
  • Bassi G; European Organization for Nuclear Research (CERN), Geneva, Switzerland.
  • Batozskaya V; National University of Science and Technology "MISIS", Moscow, Russia (associated with Institute of Theoretical and Experimental Physics NRC Kurchatov Institute (ITEP NRC KI), Moscow, Russia, Moscow, Russia).
  • Batsukh B; INFN Sezione di Pisa, Pisa, Italy.
  • Battig A; National Center for Nuclear Research (NCBJ), Warsaw, Poland.
  • Bay A; Syracuse University, Syracuse, New York, USA.
  • Becker M; Fakultät Physik, Technische Universität Dortmund, Dortmund, Germany.
  • Bedeschi F; Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland.
Phys Rev Lett ; 124(8): 082002, 2020 Feb 28.
Article em En | MEDLINE | ID: mdl-32167334
ABSTRACT
We report four narrow peaks in the Ξ_{b}^{0}K^{-} mass spectrum obtained using pp collisions at center-of-mass energies of 7, 8, and 13 TeV, corresponding to a total integrated luminosity of 9 fb^{-1} recorded by the LHCb experiment. Referring to these states by their mass, the mass values are m[Ω_{b}(6316)^{-}]=6315.64±0.31±0.07±0.50 MeV, m[Ω_{b}(6330)^{-}]=6330.30±0.28±0.07±0.50 MeV, m[Ω_{b}(6340)^{-}]=6339.71±0.26±0.05±0.50 MeV, m[Ω_{b}(6350)^{-}]=6349.88±0.35±0.05±0.50 MeV, where the uncertainties are statistical, systematic, and the last is due to the knowledge of the Ξ_{b}^{0} mass. The natural widths of the three lower mass states are consistent with zero, and the 90% confidence-level upper limits are determined to be Γ[Ω_{b}(6316)^{-}]<2.8 MeV, Γ[Ω_{b}(6330)^{-}]<3.1 MeV and Γ[Ω_{b}(6340)^{-}]<1.5 MeV. The natural width of the Ω_{b}(6350)^{-} peak is 1.4_{-0.8}^{+1.0}±0.1 MeV, which is 2.5σ from zero and corresponds to an upper limit of 2.8 MeV. The peaks have local significances ranging from 3.6σ to 7.2σ. After accounting for the look-elsewhere effect, the significances of the Ω_{b}(6316)^{-} and Ω_{b}(6330)^{-} peaks are reduced to 2.1σ and 2.6σ, respectively, while the two higher mass peaks exceed 5σ. The observed peaks are consistent with expectations for excited Ω_{b}^{-} resonances.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article