Axially symmetric cosmological models for the perfect fluid

Families of metrics are found in synchronous coordinates generalising Tolman's spherically symmetric solutions, both for non-coherent dust and for special cases of perfect fluid with non-zero pressure. New metrics depend on an additional arbitrary function of R, theta , and they lead specifically to solutions of the Schwarzschild and Friedmann types (but differing from them in general, especially in their Petrov types and isometries).

Авторы
Редакторы
-
Издательство
-
Номер выпуска
11
Язык
Английский
Страницы
2335-2343
Статус
Опубликовано
Подразделение
-
Номер
027
Том
17
Год
1984
Организации
  • 1 Dept. of Theoretical Phys., P. Lumumba Peoples' Friendship Univ., Moscow, Russian Federation
Ключевые слова
-
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/1376/