On stability of exponential cosmological solutions with non-static volume factor in the Einstein–Gauss–Bonnet model

A (n+ 1) -dimensional gravitational model with Gauss–Bonnet term and a cosmological constant term is considered. When ansatz with diagonal cosmological metrics is adopted, the solutions with an exponential dependence of the scale factors, ai∼ exp (vit) , i= 1 , ⋯ , n, are analyzed for n> 3. We study the stability of the solutions with non-static volume factor, i.e. if K(v)=∑k=1nvk≠0. We prove that under a certain restriction R imposed solutions with K(v) > 0 are stable, while solutions with K(v) < 0 are unstable. Certain examples of stable solutions are presented. We show that the solutions with v1= v2= v3= H> 0 and zero variation of the effective gravitational constant are stable if the restriction R is obeyed. © 2016, The Author(s).

Авторы
Издательство
Springer New York LLC
Номер выпуска
8
Язык
Английский
Статус
Опубликовано
Номер
431
Том
76
Год
2016
Организации
  • 1 Center for Gravitation and Fundamental Metrology, VNIIMS, 46 Ozyornaya ul., Moscow, 119361, Russian Federation
  • 2 Institute of Gravitation and Cosmology, Peoples’ Friendship University of Russia (RUDN University), 6 Miklukho-Maklaya ul., Moscow, 117198, Russian Federation
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/3862/
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