Gravitational waves from accreting neutron stars
S. Bonazzola, E. Gourgoulhon
Abstract
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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