| Автор | O B Zaslavskii |
| Дата выпуска | 1995-07-01 |
| dc.description | Explicit formulae are derived for the quasilocal energy of a generic axially-symmetric spacetime with small deviation from spherical symmetry. It is shown that at the horizon the energy reduces to twice the irreducible mass of a black hole. The case of the Ernst--Schwarzschild black hole with a magnetic field is briefly discussed as an illustration. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | On the quasilocal energy of axially-symmetric spacetimes |
| Тип | lett |
| DOI | 10.1088/0264-9381/12/7/002 |
| Electronic ISSN | 1361-6382 |
| Print ISSN | 0264-9381 |
| Журнал | Classical and Quantum Gravity |
| Том | 12 |
| Первая страница | L63 |
| Последняя страница | L67 |
| Аффилиация | O B Zaslavskii; Department of Physics, Kharkov University, Svobody Sq. 4, Kharkov 310077, Ukraine |
| Выпуск | 7 |
