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

M. G. Aartsen, N. A. Lockerbie, K. V. Tokmakov, LIGO Scientific Collaboration, Virgo Collaboration

Research output: Contribution to journalArticle

24 Citations (Scopus)

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 10−2  M⊙c2 at ∼150  Hz with ∼60  ms duration, and high-energy neutrino emission of 1051  erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10−2  Mpc−3 yr−1. We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.
LanguageEnglish
Article number102002
Number of pages22
JournalPhysical Review D
Volume90
Issue number10
DOIs
Publication statusPublished - 17 Nov 2014

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LIGO (observatory)
gravitational waves
neutrinos
energy
detectors
gamma ray bursts
observatories
strings
gamma rays

Keywords

  • gravitational waves
  • high energy neutrinos
  • LIGO scientific collaboration

Cite this

Aartsen, M. G. ; LIGO Scientific Collaboration ; Virgo Collaboration. / Multimessenger search for sources of gravitational waves and high-energy neutrinos : initial results for LIGO-Virgo and IceCube. In: Physical Review D. 2014 ; Vol. 90, No. 10.
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Multimessenger search for sources of gravitational waves and high-energy neutrinos : initial results for LIGO-Virgo and IceCube. / Aartsen, M. G.; LIGO Scientific Collaboration; Virgo Collaboration.

In: Physical Review D, Vol. 90, No. 10, 102002, 17.11.2014.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Multimessenger search for sources of gravitational waves and high-energy neutrinos

T2 - Physical Review D

AU - Aartsen, M. G.

AU - Lockerbie, N. A.

AU - Tokmakov, K. V.

AU - LIGO Scientific Collaboration

AU - Virgo Collaboration

N1 - Please consult the manuscript for full attribution details.

PY - 2014/11/17

Y1 - 2014/11/17

N2 - 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 10−2  M⊙c2 at ∼150  Hz with ∼60  ms duration, and high-energy neutrino emission of 1051  erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10−2  Mpc−3 yr−1. We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.

AB - 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 10−2  M⊙c2 at ∼150  Hz with ∼60  ms duration, and high-energy neutrino emission of 1051  erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6×10−2  Mpc−3 yr−1. We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.

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KW - high energy neutrinos

KW - LIGO scientific collaboration

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