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  Gravitational Waves From Neutron-star R-modes

Owen, B. J. (2000). Gravitational Waves From Neutron-star R-modes. In Proceedings, 34th Rencontres de Moriond gravitational waves and experimental gravity (pp. 131-138 ). The Gioi world Publishers.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0000-62B5-5 Version Permalink: http://hdl.handle.net/21.11116/0000-0000-62B6-4
Genre: Conference Paper

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 Creators:
Owen, Benjamin J.1, Author              
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1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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 Abstract: It is now known that the r-modes of neutron stars are subject to a gravitational radiation­ driven instability in astrophysically realistic conditions. This instability will cause some rapidly rotating newborn neutron stars to spin down in the first year after their birth, emit­ting gravitational wave signals which may be detectable by the "enhanced" LIGO and VIRGO interferometers out to the Virgo cluster of galaxies-a distance at which several events per year may occur. The r-mode instability may also cause older accreting neutron · stars in low mass x-ray binaries to emit gravitational waves detectable within our own galaxy.

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 Dates: 2000
 Publication Status: Published in print
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Title: 34th Rencontres de Moriond gravitational waves and experimental gravity
Place of Event: Les Arcs, France
Start-/End Date: 1999-01-23 - 1999-01-30

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Title: Proceedings, 34th Rencontres de Moriond gravitational waves and experimental gravity
Source Genre: Proceedings
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Publ. Info: The Gioi world Publishers
Pages: - Volume / Issue: - Sequence Number: - Start / End Page: 131 - 138 Identifier: -