van Elewyck, Veronique and Ando, S. and Aso, Y. and Baret, B. and Barsuglia, M. and Bartos, I. and Chassande-Mottin, E. and Di Palma, I. and Dwyer, J. and Finley, C. and Kei, K. and Kouchner, A. and Marka, S. and Marka, Z. and Rollins, J. and Ott, C. D. and Pradier, T. and Searle, A. (2009) Joint searches between gravitational-wave interferometers and high-energy neutrino telescopes: science reach and analyis strategies. International Journal of Modern Physics D, 18 (10). pp. 1655-1659. ISSN 0218-2718 . http://resolver.caltech.edu/CaltechAUTHORS:20091119-142513435
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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.
|Additional Information:||© 2009 World Scientific Publishing Co. V. Van Elewyck warmly thanks the organizers for the lively and friendly atmosphere created during the workshop. The authors acknowledge financial support from the EC 7th Framework Program (Marie Curie Reintegration Grant) and from the National Science Foundation under grants PHY-0107417/0757058/0457528/0757982.|
|Subject Keywords:||Multi-messenger astronomy; neutrinos; gravitational waves|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Jason Perez|
|Deposited On:||20 Nov 2009 22:09|
|Last Modified:||26 Dec 2012 11:34|
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