Relativistic SPH Calculations of Compact Binary Mergers
| dc.creator | Rasio, Frederic | |
| dc.creator | Faber, Joshua | |
| dc.creator | Kobayashi, Shiho | |
| dc.creator | Laguna, Pablo | |
| dc.date | 2005-03-01 | |
| dc.date.accessioned | 2026-07-07T02:17:06Z | |
| dc.date.available | 2026-07-07T02:17:06Z | |
| dc.description | We review recent progress in understanding the hydrodynamics of compact binary mergers using relativistic smoothed particle hydrodynamics (SPH) codes. Recent results are discussed for both double neutron stars and black hole - neutron star binaries. The gravitational wave signals from these mergers contain a lot of information about the masses and radii of the stars and the equation of state of the neutron star fluid. For black hole - neutron star mergers, the final fate of the fluid and the gravitational wave emission depend strongly on the mass ratio and the black hole spin. | |
| dc.description | 12 pages, to appear in proceedings of JGRG14 (Yukawa Institute for Theoretical Physics, Kyoto, Japan, Nov 29 - Dec 3, 2004) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0503007 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0503007 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9047 | |
| dc.subject | Astrophysics | |
| dc.title | Relativistic SPH Calculations of Compact Binary Mergers | |
| dc.type | text |