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Use of event-level neutrino telescope data in global fits for theories of new physics

  • The IceCube Collaboration
  • McGill University
  • Stockholm University
  • University of Wisconsin-Madison
  • Ghent University
  • German Electron Synchrotron
  • University of Canterbury
  • University of Geneva
  • Humboldt University of Berlin
  • University of Delaware
  • South Dakota School of Mines & Technology
  • University of California at Irvine
  • Johannes Gutenberg University Mainz
  • University of California at Berkeley
  • Lawrence Berkeley National Laboratory
  • Ohio State University
  • Université libre de Bruxelles
  • Ruhr University Bochum
  • University of Wuppertal
  • Pennsylvania State University
  • University of Maryland
  • University of Kansas
  • RWTH Aachen University
  • Vrije Universiteit Brussel
  • University of Bonn
  • Uppsala University
  • Swiss Federal Institute of Technology Lausanne
  • Georgia Institute of Technology
  • TU Dortmund University
  • Southern University and A&M College
  • University of Alberta
  • Technical University of Munich
  • University of Adelaide
  • Los Alamos National Laboratory
  • Chiba University
  • Clark Atlanta University
  • Stony Brook University
  • Universite de Mons
  • Department of Physics and Astronomy
  • University of Wisconsin-River Falls
  • National Institute for Nuclear Physics
  • University of Alaska Anchorage
  • University of Oxford
  • University of the West Indies
  • NASA Goddard Space Flight Center

Research output: Contribution to journalArticlepeer-review

41 Scopus citations

Abstract

We present a fast likelihood method for including event-level neutrino telescope data in parameter explorations of theories for new physics, and announce its public release as part of DarkSUSY 5.0.6. Our construction includes both angular and spectral information about neutrino events, as well as their total number. We also present a corresponding measure for simple model exclusion, which can be used for single models without reference to the rest of a parameter space. We perform a number of supersymmetric parameter scans with IceCube data to illustrate the utility of the method: example global fits and a signal recovery in the constrained minimal supersymmetric standard model (CMSSM), and a model exclusion exercise in a 7-parameter phenomenological version of the MSSM. The final IceCube detector configuration will probe almost the entire focus-point region of the CMSSM, as well as a number of MSSM-7 models that will not otherwise be accessible to e.g. direct detection. Our method accurately recovers the mock signal, and provides tight constraints on model parameters and derived quantities. We show that the inclusion of spectral information significantly improves the accuracy of the recovery, providing motivation for its use in future IceCube analyses.

Original languageEnglish
Article number057
JournalJournal of Cosmology and Astroparticle Physics
Volume2012
Issue number11
DOIs
StatePublished - 1 Nov 2012
Externally publishedYes

Keywords

  • Cosmology of theories beyond the SM
  • Dark matter experiments
  • Dark matter theory
  • Neutrino astronomy

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