On stable exponential solutions in Einstein–Gauss–Bonnet cosmology with zero variation of G
- Authors: Ivashchuk V.D.1,2
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Affiliations:
- Institute of Gravitation and Cosmology
- Center for Gravitation and Fundamental Metrology
- Issue: Vol 22, No 4 (2016)
- Pages: 329-332
- Section: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176045
- DOI: https://doi.org/10.1134/S0202289316040095
- ID: 176045
Cite item
Abstract
A D-dimensional gravitational model with a Gauss–Bonnet term and the cosmological constant Λ is considered. Assuming diagonal cosmological metrics, we find, for certain Λ > 0, new examples of solutions with an exponential time dependence of two scale factors, governed by two Hubble-like parameters H > 0 and h < 0, corresponding to submanifolds of dimensions m and l, respectively, with (m, l) = (4, 2), (5, 2), (5, 3), (6, 7), (7, 5), (7, 6) and D = 1 + m + l. Any of these solutions describes an exponential expansion of our 3-dimensional factor space with the Hubble parameter H and zero variation of the effective gravitational constant G. We also prove the stability of these solutions in the class of cosmological solutions with diagonal metrics.
About the authors
V. D. Ivashchuk
Institute of Gravitation and Cosmology; Center for Gravitation and Fundamental Metrology
Author for correspondence.
Email: ivashchuk@mail.ru
Russian Federation, Miklukho-Maklaya 6, Moscow, 117198; Ozyornaya 46, Moscow, 119361