On stable exponential solutions in Einstein-Gauss-Bonnet cosmology with zero variation of G

被引:18
|
作者
Ivashchuk, V. D. [1 ,2 ]
机构
[1] RUDN Univ, Inst Gravitat & Cosmol, Miklukho Maklaya 6, Moscow 117198, Russia
[2] VNIIMS, Ctr Gravitat & Fundamental Metrol, Ozyornaya 46, Moscow 119361, Russia
来源
GRAVITATION & COSMOLOGY | 2016年 / 22卷 / 04期
基金
俄罗斯基础研究基金会;
关键词
MODEL; SINGULARITY; STABILITY; GRAVITY;
D O I
10.1134/S0202289316040095
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A D-dimensional gravitational model with a Gauss-Bonnet term and the cosmological constant I > is considered. Assuming diagonal cosmological metrics, we find, for certain I > > 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.
引用
收藏
页码:329 / 332
页数:4
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