Document Type
Article
Publication Date
11-17-2014
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.
Recommended Citation
Aartsen, M. G., Markus Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann et al. "Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube." Physical Review D 90, no. 10 (2014): 102002. http://doi.org/10.1103/PhysRevD.90.102002
Publication Title
Physical Review D - Particles, Fields, Gravitation and Cosmology
DOI
10.1103/PhysRevD.90.102002
Comments
© Physical Review D - Particles, Fields, Gravitation and Cosmology. Original version available at: http://doi.org/10.1103/PhysRevD.90.102002