Coalescence of a strange star with a black hole
| dc.creator | Lee, William H. | |
| dc.creator | Nix, Jon | |
| dc.creator | Kluzniak, Wlodzimierz | |
| dc.date | 2001-03-22 | |
| dc.date.accessioned | 2026-07-07T01:57:59Z | |
| dc.date.available | 2026-07-07T01:57:59Z | |
| dc.description | We present the first numerical results on the binary coalescence of a quark star with a black hole, obtained with a 3-D Newtonian smooth particle hydro (SPH) code. The star is initially represented by 17,000 particles modeling a self-gravitating fluid with the equation of state P= (rho - rho0)c**2/3, and the black hole by a point mass with an absorbing boundary at the Schwarzschild radius. As in similar calculations carried out for a stiff polytrope, the stellar core survives the initial episode of mass transfer, but here an accretion disk is clearly formed as well. | |
| dc.description | 3 pages, to appear in the proceedings of the 4th INTEGRAL workshop, "Exploring the extreme universe", Alicante, September 2000. Uses esapub.cls | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0103380 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0103380 | |
| dc.identifier | 2001, ESA SP--459, p. 227 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2601 | |
| dc.subject | Astrophysics | |
| dc.title | Coalescence of a strange star with a black hole | |
| dc.type | text |