Published October 2009
| public
Journal Article
Joint searches between gravitational-wave interferometers and high-energy neutrino telescopes: science reach and analyis strategies
Abstract
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.Additional details
- Eprint ID
- 16766
- Resolver ID
- CaltechAUTHORS:20091119-142513435
- EC 7th Framework Program (Marie Curie Reintegration Grant)
- NSF
- PHY-0107417
- NSF
- PHY-0757058
- NSF
- PHY-0457528
- NSF
- PHY-0757982
- Created
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2009-11-20Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Caltech groups
- TAPIR