| Автор | E Gourgoulhon |
| Дата выпуска | 1992-12-01 |
| dc.description | A complete system of equations sufficient to handle the fully general relativistic hydrodynamics in the case of spherical symmetry is presented, as well as its numerical implementation in a pseudo-spectral code. This code is able to follow tiny radial perturbations of a neutron star near the maximum mass, and especially to show the growth of their fundamental mode as the central density increases, as well as to describe a complete collapse towards a black hole when the instability threshold is passed. In other respects, the code is employed to address the problem of the minimum mass of a black hole formed via gravitational collapse. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | 1D numerical relativity applied to neutron star collapse |
| Тип | paper |
| DOI | 10.1088/0264-9381/9/S/005 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 9 |
| Первая страница | S117 |
| Последняя страница | S125 |
| Аффилиация | E Gourgoulhon; Dept. d'Astrophys. Relativiste et de Cosmologie, Obs. de Paris, Meudon, France |
| Выпуск | S |
