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