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Searches for relativistic magnetic monopoles in IceCube

  • Icecube Collaboration
  • University of Adelaide
  • Technical University of Munich
  • German Electron Synchrotron
  • University of Canterbury
  • Université libre de Bruxelles
  • University of Wisconsin-Madison
  • Stockholm University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Pennsylvania State University
  • Johannes Gutenberg University Mainz
  • RWTH Aachen University
  • South Dakota School of Mines & Technology
  • University of California at Irvine
  • University of California at Berkeley
  • Ohio State University
  • Ruhr University Bochum
  • University of Wuppertal
  • New York University Abu Dhabi
  • University of Maryland
  • University of Kansas
  • Lawrence Berkeley National Laboratory
  • Uppsala University
  • TU Dortmund University
  • Sungkyunkwan University
  • Vrije Universiteit Brussel
  • University of Alberta
  • Georgia Institute of Technology
  • University of Geneva
  • Ghent University
  • University of Toronto
  • Michigan State University
  • University of Delaware
  • Humboldt University of Berlin
  • Southern University and A&M College
  • Chiba University
  • University of Copenhagen
  • University of Bonn
  • The University of Tokyo
  • Clark Atlanta University
  • Yale University
  • Stony Brook University
  • Universite de Mons
  • Drexel University
  • University of Wisconsin-River Falls
  • Department of Physics and Astronomy
  • University of Alaska Anchorage
  • University of Oxford
  • NASA Goddard Space Flight Center

Research output: Contribution to journalArticlepeer-review

52 Scopus citations

Abstract

Various extensions of the Standard Model motivate the existence of stable magnetic monopoles that could have been created during an early high-energy epoch of the Universe. These primordial magnetic monopoles would be gradually accelerated by cosmic magnetic fields and could reach high velocities that make them visible in Cherenkov detectors such as IceCube. Equivalently to electrically charged particles, magnetic monopoles produce direct and indirect Cherenkov light while traversing through matter at relativistic velocities. This paper describes searches for relativistic ((Formula presented.)) and mildly relativistic ((Formula presented.)) monopoles, each using one year of data taken in 2008/2009 and 2011/2012, respectively. No monopole candidate was detected. For a velocity above (Formula presented.) the monopole flux is constrained down to a level of (Formula presented.). This is an improvement of almost two orders of magnitude over previous limits.

Original languageEnglish
Article number133
JournalEuropean Physical Journal C
Volume76
Issue number3
DOIs
StatePublished - 1 Mar 2016
Externally publishedYes

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