Possible wormholes in a brane world

The condition [Formula Presented] where R is the four-dimensional scalar curvature, is used for obtaining a large class (with an arbitrary function of [Formula Presented] of static, spherically symmetric Lorentzian wormhole solutions. The wormholes are globally regular and traversable, can have throats of arbitrary size and can be both symmetric and asymmetric. These solutions may be treated as possible wormhole solutions in a brane world since they satisfy the vacuum Einstein equations on the brane where effective stress-energy is induced by interaction with the bulk gravitational field. Some particular examples are discussed. © 2003 The American Physical Society.

Авторы
Bronnikov K.A. 1, 2 , Kim S.W.3
Редакторы
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Издательство
-
Номер выпуска
6
Язык
Английский
Страницы
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Статус
Опубликовано
Подразделение
-
Номер
-
Том
67
Год
2003
Организации
  • 1 VNIIMS, 3-1 M. Ulyanovoy St., Moscow, 117313, Russian Federation
  • 2 Institute of Gravitation and Cosmology, PFUR, 6 Miklukho-Maklaya St., Moscow, 117198, Russian Federation
  • 3 Department of Science Education, Ewha Womans University, Seoul, 120-750, South Korea
Ключевые слова
article; cosmos; energy; gravity; mathematical analysis; mathematical model; theory; vacuum
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/109/