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International Journal of Modern Physics D 18 (2009) 1655-1659
Joint Searches Between Gravitational-Wave Interferometers and High-Energy Neutrino Telescopes:. Science Reach and Analysis Strategies
V. Van Elewyck1, S. Ando, Y. Aso, B. Baret1, M. Barsuglia1, I. Bartos, E. Chassande-Mottin1, I. Di Palma, J. Dwyer, C. Finley, K. Kei, A. Kouchner1, S. Marka, Z. Marka, J. Rollins, C. D. Ott, T. Pradier2, A. Searle

Many of the astrophysical sources and violent phenomena observed in our Universe are potential emitters of gravitational waves (GWs) and high-energy neutrinos (HENs). A network of GW detectors such as LIGO and Virgo can determine the direction/time of GW bursts while the IceCube and ANTARES neutrino telescopes can also provide accurate directional information for HEN events. Requiring the consistency between both, totally independent, detection channels shall enable new searches for cosmic events arriving from potential common sources, of which many extra-galactic objects.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
2 :  IPHC - Institut Pluridisciplinaire Hubert Curien
APC - Cosmologie et Gravitation
Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie

Physique/Astrophysique/Phénomènes cosmiques de haute energie
Multi-messenger astronomy – neutrinos – gravitational waves
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