2016/12/31 by K. K. Ernazarov, V. D. Ivashchuk · 1 citation
Physics and Astronomy · #gr-qc #hep-th
paper · pdf · doi:10.1140/epjc/s10052-017-4669-0
14 pages, 2 figures, LaTex., 2nd revised version, several words and phrases are changed or added, eq. (3.1) is modified, Remark on p. 4 is inserted. To be published in Eur. Phys. J. C. arXiv admin note: substantial text overlap with arXiv:1612.07178
arxiv created 2017/01/30 · arxiv updated 2017/03/08
A D-dimensional gravitational model with a Gauss-Bonnet term and the cosmological term Lambda is considered. By assuming diagonal cosmological metrics, we find, for certain fine-tuned Lambda, a class of solutions with exponential time dependence of two scale factors, governed by two Hubble-like parameters H >0 and h < 0, corresponding to factor spaces of dimensions m > 3 and l > 1, respectively, with (m,l) non-equal to (6,6), (7,4), (9,3) and D = 1 + m + l. Any of these solutions describes an exponential expansion of 3-dimensional subspace with Hubble parameter H and zero variation of the effective gravitational constant G. We prove the stability of these solutions in a class of cosmological solutions with diagonal metrics.