| Автор | Abhay Ashtekar |
| Автор | Christopher Beetle |
| Автор | Stephen Fairhurst |
| Дата выпуска | 1999-02-01 |
| dc.description | A set of boundary conditions defining a non-rotating isolated horizon are given in Einstein-Maxwell theory. A spacetime representing a black hole which itself is in equilibrium but whose exterior contains radiation admits such a horizon. Physically motivated, (quasi-)local definitions of the mass and surface gravity of an isolated horizon are introduced. Although these definitions do not refer to infinity, the quantities assume their standard values in Reissner-Nordström solutions. Finally, using these definitions, the zeroth and first laws of black hole mechanics are established for isolated horizons. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Isolated horizons: a generalization of black hole mechanics |
| Тип | lett |
| DOI | 10.1088/0264-9381/16/2/027 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 16 |
| Первая страница | L1 |
| Последняя страница | L7 |
| Аффилиация | Abhay Ashtekar; Center for Gravitational Physics and Geometry, Department of Physics, The Pennsylvania State University, University Park, PA 16802, USA |
| Аффилиация | Christopher Beetle; Center for Gravitational Physics and Geometry, Department of Physics, The Pennsylvania State University, University Park, PA 16802, USA |
| Аффилиация | Stephen Fairhurst; Center for Gravitational Physics and Geometry, Department of Physics, The Pennsylvania State University, University Park, PA 16802, USA |
| Выпуск | 2 |
