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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

  • Icecube Collaboration
  • , LIGO Scientific Collaboration
  • , the Virgo Collaboration
  • University of Adelaide
  • German Electron Synchrotron
  • University of Canterbury
  • University of Geneva
  • University of Wisconsin-Madison
  • Stockholm University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Pennsylvania State University
  • RWTH Aachen University
  • South Dakota School of Mines & Technology
  • University of California at Irvine
  • Johannes Gutenberg University Mainz
  • Ohio State University
  • Ruhr University Bochum
  • University of Wuppertal
  • University of Maryland
  • Technical University of Munich
  • University of Kansas
  • University of California at Berkeley
  • Lawrence Berkeley National Laboratory
  • Uppsala University
  • Sungkyunkwan University
  • University of Bonn
  • Vrije Universiteit Brussel
  • Georgia Institute of Technology
  • University of Toronto
  • TU Dortmund University
  • Ghent University
  • Humboldt University of Berlin
  • University of Delaware
  • Southern University and A&M College
  • University of Alberta
  • Université libre de Bruxelles
  • Chiba University
  • Clark Atlanta University
  • Stony Brook University
  • Universite de Mons
  • University of Copenhagen
  • University of Wisconsin-River Falls
  • Massachusetts Institute of Technology
  • Department of Physics and Astronomy
  • University of Alaska Anchorage
  • University of Oxford
  • Southeastern Louisiana University
  • California Institute of Technology
  • Louisiana State University
  • University of Salerno
  • National Institute for Nuclear Physics
  • University of Florida
  • LIGO Livingston
  • Cardiff University
  • University of Sannio
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • National Institute for Subatomic Physics
  • Instituto Nacional de Pesquisas Espaciais
  • International Centre for Theoretical Sciences
  • Syracuse University
  • University of Wisconsin-Milwaukee
  • Leibniz University Hannover
  • University of Siena
  • Stanford University
  • University of Mississippi
  • California State University Fullerton
  • University of Birmingham
  • Montana State University
  • European Gravitational Observatory
  • LIGO Hanford
  • University of Glasgow
  • APC - AstroParticule et Cosmologie
  • Columbia University
  • University of Pisa
  • CAMK-PAN
  • University of Warsaw
  • University of Genoa
  • Lomonosov Moscow State University
  • Université Paris-Sud
  • NASA Goddard Space Flight Center
  • University of Western Australia
  • Radboud University Nijmegen
  • Université Côte d'Azur
  • Institute for Nuclear Research
  • Institut de Physique de Rennes
  • Université Savoie Mont Blanc
  • Washington State University Pullman
  • Inter-University Centre for Astronomy and Astrophysics India
  • Kyoto University
  • University of Urbino
  • University of Oregon
  • Laboratoire Kastler Brossel
  • Vrije Universiteit Amsterdam
  • University of Maryland, College Park
  • University of Massachusetts
  • Université de Lyon
  • University of the Balearic Islands
  • University of Naples Federico II
  • Tsinghua University
  • University of Michigan, Ann Arbor
  • National Tsing Hua University
  • Charles Sturt University
  • Caltech-CaRT
  • Pusan National University
  • Australian National University
  • Carleton College
  • University of Rome Tor Vergata
  • University of Rome La Sapienza
  • University of Brussels
  • Sonoma State University
  • George Washington University
  • University of Cambridge
  • University of Minnesota Twin Cities
  • University of Texas at Brownsville and Texas Southmost College
  • University of Sheffield
  • Wigner Research Centre for Physics
  • Argentinian Gravitational Wave Group
  • University of Trento
  • Northwestern University
  • Montclair State University
  • Eotvos Lorand University
  • University of Perugia
  • Rutherford Appleton Laboratory
  • Embry-Riddle Aeronautical University
  • Seoul National University
  • Perimeter Institute for Theoretical Physics
  • American University Washington DC
  • College of William and Mary
  • Raman Research Institute
  • Korea Institute of Science and Technology Information
  • University of Białystok
  • University of Southampton
  • CET Campus
  • Institute of Applied Physics of the Russian Academy of Sciences
  • Hanyang University
  • National Centre for Nuclear Research
  • Polish Academy of Sciences
  • Institute for Plasma Research
  • University of Melbourne
  • Monash University
  • University of Strathclyde
  • Louisiana Tech University
  • CNRS
  • University of Camerino
  • Indian Institute of Science Education and Research, Kolkata
  • National Institute for Mathematical Sciences
  • Hobart and William Smith Colleges
  • Raja Ramanna Centre for Advanced Technology
  • Tata Institute of Fundamental Research
  • University of the West of Scotland
  • Institute of Astronomy
  • Indian Institute of Technology Gandhinagar
  • Universidade Estadual Paulista Júlio de Mesquita Filho
  • Andrews University
  • Trinity University
  • University of Washington
  • Rochester Institute of Technology
  • Abilene Christian University

Research output: Contribution to journalArticlepeer-review

43 Scopus citations

Abstract

We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10-2M c2 at ∼150Hz with ∼60ms duration, and high-energy neutrino emission of 1051erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10-2Mpc-3yr-1. We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.

Original languageEnglish
Article number102002
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume90
Issue number10
DOIs
StatePublished - 17 Nov 2014
Externally publishedYes

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