Gravitational waves from accreting neutron stars
Abstract
Description
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}.
10 pages, no figure, to appear in the Proceedings of the International Conference on Gravitational Waves: Sources and Detectors, Cascina (Pisa), Italy --- March 19-23, 1996, eds. I. Ciufolini, F. Fidecaro (World Scientific, in press)
10 pages, no figure, to appear in the Proceedings of the International Conference on Gravitational Waves: Sources and Detectors, Cascina (Pisa), Italy --- March 19-23, 1996, eds. I. Ciufolini, F. Fidecaro (World Scientific, in press)