Modelling Gravitational Waves from Inspiralling Compact Binaries
| dc.creator | Damour, T. | |
| dc.creator | Iyer, B. R. | |
| dc.creator | Sathyaprakash, B. S. | |
| dc.date | 1998-01-07 | |
| dc.date.accessioned | 2026-07-07T03:32:09Z | |
| dc.date.available | 2026-07-07T03:32:09Z | |
| dc.description | Gravitational waves from inspiralling compact binaries can be reliably extracted from a noisy detector output only if the template used in the detection is a faithful representation of the true signal. In this article we suggest a new approach to constructing faithful signal models. | |
| dc.description | Needs sprocl.sty which is bundled together with the tex file. To appear in the proceedings "Second Edoardo Amaldi Conference on Gravitational Waves", CERN, 1 - 4 July 1997 | |
| dc.identifier | https://arxiv.org/abs/gr-qc/9801014 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/9801014 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/36121 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Modelling Gravitational Waves from Inspiralling Compact Binaries | |
| dc.type | text |