Coalescing binaries and Doppler experiments
| dc.creator | Vecchio, A. | |
| dc.creator | Bertotti, B. | |
| dc.creator | Iess, L. | |
| dc.date | 1997-08-16 | |
| dc.date.accessioned | 2026-07-07T03:31:43Z | |
| dc.date.available | 2026-07-07T03:31:43Z | |
| dc.description | We discuss the sensitivity of the CASSINI experiments to gravitational waves emitted by the in-spiral of compact binaries. We show that the maximum distance reachable by the instrument is $\sim 100$ Mpc. In particular, CASSINI can detect massive black hole binaries with chirp mass $\simgt 10^6 \Ms$ in the Virgo Cluster with signal-to-noise ratio between 5 and 30 and possible compact objects of mass $\simgt 30 \Ms$ orbiting the massive black hole that our Galactic Centre is likely to harbour. | |
| dc.description | 5 pages, LaTeX, one postscript figure included. Talk given at the "Second Amaldi Conference on Gravitational Waves" (CERN, 1-4 July 1997). To be published in the Proceedings (World Scientific, Singapore), eds. E. Coccia et al | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9708033 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9708033 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35964 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Coalescing binaries and Doppler experiments | |
| dc.type | text |