On black holes and wormholes in a brane world

The general solution to the trace of the 4-dimensional Einstein equations for static, spherically symmetric configurations is used for finding general classes of black hole (BH) and wormhole metrics which may be asymptotically flat or have any other prescribed asymptotics. The procedure generically leads to families of solutions unifying globally regular BHs with a Kerr-like global structure and symmetric wormholes. The BH event horizons are generically simple or double, but inside matter distributions, they can be of any order under some special conditions. A few simple examples are discussed. A natural application of the above results, is the brane world concept, in which the trace of the 4D gravity equations is the only unambiguous equation for the 4D metric, and its solutions can be continued into the 5D bulk according to the embedding theorems.

Авторы
Bronnikov K.A. 1, 2 , Kim S.-W.3
Сборник материалов конференции
Номер выпуска
SUPPL.
Язык
Английский
Страницы
S81-S85
Статус
Опубликовано
Том
45
Год
2004
Организации
  • 1 VNIIMS, 3-1 M. Ulyanovoy St., Moscow 117313, Russian Federation
  • 2 Inst. of Gravitation and Cosmology, PFUR, 6 Miklukho-Maklaya St., Moscow 117198, Russian Federation
  • 3 Dept. of Science Education, Ewha Womans University, Seoul 120-750, South Korea
Ключевые слова
Black holes; Exact solutions; Large extra dimensions; Multidimensional gravity; Wormholes
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/3593/