Gravitational waves from accreting neutron stars
| dc.creator | Bonazzola, S. | |
| dc.creator | Gourgoulhon, E. | |
| dc.date | 1996-06-20 | |
| dc.date.accessioned | 2026-07-25T20:09:59Z | |
| dc.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}. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9606123 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9606123 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/69361 | |
| dc.subject | Astrophysics | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gravitational waves from accreting neutron stars | |
| dc.type | text |