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Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data.
Abbasi, R; Ackermann, M; Adams, J; Aguilar, J A; Ahlers, M; Ahrens, M; Alispach, C; Alves, A A; Amin, N M; An, R; Andeen, K; Anderson, T; Anton, G; Argüelles, C; Ashida, Y; Axani, S; Bai, X; Balagopal V, A; Barbano, A; Barwick, S W; Bastian, B; Basu, V; Baur, S; Bay, R; Beatty, J J; Becker, K-H; Becker Tjus, J; Bellenghi, C; BenZvi, S; Berley, D; Bernardini, E; Besson, D Z; Binder, G; Bindig, D; Blaufuss, E; Blot, S; Boddenberg, M; Bontempo, F; Borowka, J; Böser, S; Botner, O; Böttcher, J; Bourbeau, E; Bradascio, F; Braun, J; Bron, S; Brostean-Kaiser, J; Browne, S; Burgman, A; Burley, R T.
Afiliación
  • Abbasi R; Department of Physics, Loyola University Chicago, Chicago, Illinois 60660, USA.
  • Ackermann M; DESY, D-15738 Zeuthen, Germany.
  • Adams J; Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch, New Zealand.
  • Aguilar JA; Science Faculty CP230, Université Libre de Bruxelles, B-1050 Brussels, Belgium.
  • Ahlers M; Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark.
  • Ahrens M; Oskar Klein Centre and Department of Physics, Stockholm University, SE-10691 Stockholm, Sweden.
  • Alispach C; Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland.
  • Alves AA; Karlsruhe Institute of Technology, Institute for Astroparticle Physics, D-76021 Karlsruhe, Germany.
  • Amin NM; Bartol Research Institute and Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA.
  • An R; Department of Physics and Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, Massachusetts 02138, USA.
  • Andeen K; Department of Physics, Marquette University, Milwaukee, Wisconsin, 53201, USA.
  • Anderson T; Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA.
  • Anton G; Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen, Germany.
  • Argüelles C; Department of Physics and Laboratory for Particle Physics and Cosmology, Harvard University, Cambridge, Massachusetts 02138, USA.
  • Ashida Y; Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • Axani S; Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.
  • Bai X; Physics Department, South Dakota School of Mines and Technology, Rapid City, South Dakota 57701, USA.
  • Balagopal V A; Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • Barbano A; Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland.
  • Barwick SW; Department of Physics and Astronomy, University of California, Irvine, California 92697, USA.
  • Bastian B; DESY, D-15738 Zeuthen, Germany.
  • Basu V; Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • Baur S; Science Faculty CP230, Université Libre de Bruxelles, B-1050 Brussels, Belgium.
  • Bay R; Department of Physics, University of California, Berkeley, California 94720, USA.
  • Beatty JJ; Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA.
  • Becker KH; Department of Physics and Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, Ohio 43210, USA.
  • Becker Tjus J; Department of Physics, University of Wuppertal, D-42119 Wuppertal, Germany.
  • Bellenghi C; Fakultät für Physik and Astronomie, Ruhr-Universität Bochum, D-44780 Bochum, Germany.
  • BenZvi S; Physik-department, Technische Universität München, D-85748 Garching, Germany.
  • Berley D; Department of Physics and Astronomy, University of Rochester, Rochester, New York 14627, USA.
  • Bernardini E; Department of Physics, University of Maryland, College Park, Maryland 20742, USA.
  • Besson DZ; DESY, D-15738 Zeuthen, Germany.
  • Binder G; Department of Physics and Astronomy, University of Kansas, Lawrence, Kansas 66045, USA.
  • Bindig D; Department of Physics, University of California, Berkeley, California 94720, USA.
  • Blaufuss E; Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.
  • Blot S; Department of Physics, University of Wuppertal, D-42119 Wuppertal, Germany.
  • Boddenberg M; Department of Physics, University of Maryland, College Park, Maryland 20742, USA.
  • Bontempo F; DESY, D-15738 Zeuthen, Germany.
  • Borowka J; III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany.
  • Böser S; Karlsruhe Institute of Technology, Institute for Astroparticle Physics, D-76021 Karlsruhe, Germany.
  • Botner O; III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany.
  • Böttcher J; Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz, Germany.
  • Bourbeau E; Department of Physics and Astronomy, Uppsala University, Box 516, S-75120 Uppsala, Sweden.
  • Bradascio F; III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen, Germany.
  • Braun J; Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark.
  • Bron S; DESY, D-15738 Zeuthen, Germany.
  • Brostean-Kaiser J; Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • Browne S; Département de physique nucléaire et corpusculaire, Université de Genève, CH-1211 Genève, Switzerland.
  • Burgman A; DESY, D-15738 Zeuthen, Germany.
  • Burley RT; Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, D-76021 Karlsruhe, Germany.
Phys Rev Lett ; 128(5): 051101, 2022 Feb 04.
Article en En | MEDLINE | ID: mdl-35179913
We present an all-sky 90% confidence level upper limit on the cosmic flux of relativistic magnetic monopoles using 2886 days of IceCube data. The analysis was optimized for monopole speeds between 0.750c and 0.995c, without any explicit restriction on the monopole mass. We constrain the flux of relativistic cosmic magnetic monopoles to a level below 2.0×10^{-19} cm^{-2} s^{-1} sr^{-1} over the majority of the targeted speed range. This result constitutes the most strict upper limit to date for magnetic monopoles with ß≳0.8 and up to ß∼0.995 and fills the gap between existing limits on the cosmic flux of nonrelativistic and ultrarelativistic magnetic monopoles.
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Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Estados Unidos Pais de publicación: Estados Unidos
Texto completo
Añadir a Mi BVS
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XML
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Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Estados Unidos Pais de publicación: Estados Unidos