Friedmann Dynamics Recovered from Compactified Einstein–Gauss–Bonnet Cosmology
- Авторлар: Canfora F.1, Giacomini A.2, Pavluchenko S.3, Toporensky A.4,5
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Мекемелер:
- Centro de Estudios Cientificos (CECs), Casilla
- Instituto de Ciencias Físicas y Matemáticas
- Programa de Pós-Graduaзão em Física
- Sternberg Astronomical Institute
- Kazan Federal University
- Шығарылым: Том 24, № 1 (2018)
- Беттер: 28-38
- Бөлім: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176127
- DOI: https://doi.org/10.1134/S0202289318010048
- ID: 176127
Дәйексөз келтіру
Аннотация
Cosmological dynamics is studied in Einstein–Gauss–Bonnet gravity with a perfect fluid source in arbitrary dimension. A systematic analysis is performed for the case that the theory does not admit maximally symmetric solutions. Considering two independent scale factors, namely, one for the 3D space and one for the extra-dimensional space, it is found that a regime exists where the scale factor of extra dimensions tends to a constant value via damped oscillations for not too negative pressure of the fluid, so that asymptotically the evolution of the (3 + 1)-dimensional Friedmann model with perfect fluid is recovered.
Авторлар туралы
F. Canfora
Centro de Estudios Cientificos (CECs), Casilla
Хат алмасуға жауапты Автор.
Email: atopor@rambler.ru
Чили, Valdivia, 1469
A. Giacomini
Instituto de Ciencias Físicas y Matemáticas
Email: atopor@rambler.ru
Чили, Valdivia
S. Pavluchenko
Programa de Pós-Graduaзão em Física
Email: atopor@rambler.ru
Бразилия, São Luís, Maranhão, 65085-580
A. Toporensky
Sternberg Astronomical Institute; Kazan Federal University
Email: atopor@rambler.ru
Ресей, Moscow, 119991; Kazan, 420008