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MoEDAL Search in the CMS Beam Pipe for Magnetic Monopoles Produced via the Schwinger Effect.
Acharya, B; Alexandre, J; Behera, S C; Benes, P; Bergmann, B; Bertolucci, S; Bevan, A; Brancaccio, R; Branzas, H; Burian, P; Campbell, M; Cecchini, S; Cho, Y M; de Montigny, M; De Roeck, A; Ellis, J R; Fairbairn, M; Felea, D; Frank, M; Gould, O; Hays, J; Hirt, A M; Ho, D L-J; Hung, P Q; Janecek, J; Kalliokoski, M; Lacarrère, D H; Leroy, C; Levi, G; Margiotta, A; Maselek, R; Maulik, A; Mauri, N; Mavromatos, N E; Millward, L; Mitsou, V A; Musumeci, E; Ostrovskiy, I; Ouimet, P-P; Papavassiliou, J; Patrizii, L; Pavalas, G E; Pinfold, J L; Popa, L A; Popa, V; Pozzato, M; Pospisil, S; Rajantie, A; Ruiz de Austri, R; Sahnoun, Z.
Afiliação
  • Acharya B; Theoretical Particle Physics & Cosmology Group, Physics Department, King's College, London, United Kingdom.
  • Alexandre J; Theoretical Particle Physics & Cosmology Group, Physics Department, King's College, London, United Kingdom.
  • Behera SC; Department of Physics and Astronomy, <a href="https://ror.org/03xrrjk67">University of Alabama</a>, Tuscaloosa, Alabama, USA.
  • Benes P; IEAP, Czech Technical University, Prague, Czech Republic.
  • Bergmann B; IEAP, Czech Technical University, Prague, Czech Republic.
  • Bertolucci S; INFN, Section of Bologna, Bologna, Italy.
  • Bevan A; School of Physics and Astronomy, Queen Mary University, London, United Kingdom.
  • Brancaccio R; INFN, Section of Bologna &amp; Department of Physics &amp; Astronomy, University of Bologna, Bologna, Italy.
  • Branzas H; Institute of Space Science, Bucharest, Magurele, Romania.
  • Burian P; IEAP, Czech Technical University, Prague, Czech Republic.
  • Campbell M; Experimental Physics Department, <a href="https://ror.org/01ggx4157">CERN</a>, Geneva, Switzerland.
  • Cecchini S; INFN, Section of Bologna, Bologna, Italy.
  • Cho YM; Center for Quantum Spacetime, Sogang University, Seoul, Korea.
  • de Montigny M; Physics Department, University of Alberta, Edmonton, Alberta, Canada.
  • De Roeck A; Experimental Physics Department, <a href="https://ror.org/01ggx4157">CERN</a>, Geneva, Switzerland.
  • Ellis JR; Theoretical Particle Physics &amp; Cosmology Group, Physics Department, King's College, London, United Kingdom.
  • Fairbairn M; Theoretical Physics Department, <a href="https://ror.org/01ggx4157">CERN</a>, Geneva, Switzerland.
  • Felea D; Theoretical Particle Physics &amp; Cosmology Group, Physics Department, King's College, London, United Kingdom.
  • Frank M; Institute of Space Science, Bucharest, Magurele, Romania.
  • Gould O; Department of Physics, Concordia University, Montreal, Quebec, Canada.
  • Hays J; University of Nottingham, Nottingham, United Kingdom.
  • Hirt AM; School of Physics and Astronomy, Queen Mary University, London, United Kingdom.
  • Ho DL; Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland.
  • Hung PQ; Department of Physics, Imperial College, London, United Kingdom.
  • Janecek J; Department of Physics, University of Virginia, Charlottesville, Virginia, USA.
  • Kalliokoski M; IEAP, Czech Technical University, Prague, Czech Republic.
  • Lacarrère DH; Helsinki Institute of Physics, University of Helsinki, Helsinki, Finland.
  • Leroy C; Experimental Physics Department, <a href="https://ror.org/01ggx4157">CERN</a>, Geneva, Switzerland.
  • Levi G; Departement de Physique, Universite de Montreal, Quebec, Canada.
  • Margiotta A; INFN, Section of Bologna &amp; Department of Physics &amp; Astronomy, University of Bologna, Bologna, Italy.
  • Maselek R; INFN, Section of Bologna &amp; Department of Physics &amp; Astronomy, University of Bologna, Bologna, Italy.
  • Maulik A; Institute of Theoretical Physics, University of Warsaw, Warsaw, Poland.
  • Mauri N; INFN, Section of Bologna, Bologna, Italy.
  • Mavromatos NE; Physics Department, University of Alberta, Edmonton, Alberta, Canada.
  • Millward L; INFN, Section of Bologna &amp; Department of Physics &amp; Astronomy, University of Bologna, Bologna, Italy.
  • Mitsou VA; Theoretical Particle Physics &amp; Cosmology Group, Physics Department, King's College, London, United Kingdom.
  • Musumeci E; School of Physics and Astronomy, Queen Mary University, London, United Kingdom.
  • Ostrovskiy I; IFIC, Universitat de Valencia, CSIC, Valencia, Spain.
  • Ouimet PP; IFIC, Universitat de Valencia, CSIC, Valencia, Spain.
  • Papavassiliou J; Department of Physics and Astronomy, <a href="https://ror.org/03xrrjk67">University of Alabama</a>, Tuscaloosa, Alabama, USA.
  • Patrizii L; Physics Department, University of Regina, Regina, Saskatchewan, Canada.
  • Pavalas GE; IFIC, Universitat de Valencia, CSIC, Valencia, Spain.
  • Pinfold JL; INFN, Section of Bologna, Bologna, Italy.
  • Popa LA; Institute of Space Science, Bucharest, Magurele, Romania.
  • Popa V; Physics Department, University of Alberta, Edmonton, Alberta, Canada.
  • Pozzato M; Institute of Space Science, Bucharest, Magurele, Romania.
  • Pospisil S; Institute of Space Science, Bucharest, Magurele, Romania.
  • Rajantie A; INFN, Section of Bologna, Bologna, Italy.
  • Ruiz de Austri R; IEAP, Czech Technical University, Prague, Czech Republic.
  • Sahnoun Z; Department of Physics, Imperial College, London, United Kingdom.
Phys Rev Lett ; 133(7): 071803, 2024 Aug 16.
Article em En | MEDLINE | ID: mdl-39213579
ABSTRACT
We report on a search for magnetic monopoles (MMs) produced in ultraperipheral Pb-Pb collisions during Run 1 of the LHC. The beam pipe surrounding the interaction region of the CMS experiment was exposed to 184.07 µb^{-1} of Pb-Pb collisions at 2.76 TeV center-of-mass energy per collision in December 2011, before being removed in 2013. It was scanned by the MoEDAL experiment using a SQUID magnetometer to search for trapped MMs. No MM signal was observed. The two distinctive features of this search are the use of a trapping volume very close to the collision point and ultrahigh magnetic fields generated during the heavy-ion run that could produce MMs via the Schwinger effect. These two advantages allowed setting the first reliable, world-leading mass limits on MMs with high magnetic charge. In particular, the established limits are the strongest available in the range between 2 and 45 Dirac units, excluding MMs with masses of up to 80 GeV at a 95% confidence level.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Reino Unido

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Reino Unido