Gravitational waves from accreting neutron stars

Details Gravitational waves from accreting neutron stars Gravitational waves from accreting neutron stars

1996-06-20

arxiv.org/abs/astro-ph/9606123v1

Astronomy and Astrophysics

Astrophysics

10 pages, no figure, to appear in the Proceedings of the International Conference on Gravitational Waves: Sources and Detector

Scientific paper

We show that accreting neutron stars in binary systems or in
Landau-Thorne-Zytkow objects are good candidates for continuous gravitational
wave emission. Their gravitational radiation is strong enough to be detected by
the next generation of detectors having a typical noise of 10^{-23} Hz^{-1/2}.

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