| Автор | Sean A Hayward |
| Дата выпуска | 1994-12-01 |
| dc.description | General laws of black hole dynamics, some of which are analogous to the laws of thermodynamics, have recently been found for a general definition of a black hole in terms of a future outer trapping horizon, a hypersurface foliated by marginal surfaces of a certain type. This theory is translated here into spin coefficient language. Most of the following results assume an energy condition. Second law: the area form of a future outer trapping horizon is generically increasing, otherwise constant. First law: the rate of change of the area form is given by an energy flux and the trapping gravity. Zeroth law: the total trapping gravity of a compact outer marginal surface has an upper bound, attained if and only if the trapping gravity is constant. Topology law: a compact future outer marginal surface has spherical topology. Signature law: an outer trapping horizon is generically spatial, otherwise null. Trapping law: spatial surfaces sufficiently close to a compact future outer marginal surface are trapped if they lie inside the trapping horizon. Confinement law: if the interior and exterior of a future outer trapping horizon are disjoint, an observer inside the horizon cannot get outside. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Spin coefficient form of the new laws of black hole dynamics |
| Тип | paper |
| DOI | 10.1088/0264-9381/11/12/016 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 11 |
| Первая страница | 3025 |
| Последняя страница | 3035 |
| Аффилиация | Sean A Hayward; Department of Physics, Kyoto University, Kyoto 606--01, Japan and Faculty of Mathematical Studies, University of Southampton, Southampton SO9 5NH, UK |
| Выпуск | 12 |
