On stable exponential cosmological solutions with two factor spaces in (1+ m + 2)-dimensional Einstein–Gauss–Bonnet model with Λ-term

V. Ivashchuk, A. A. Kobtsev
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引用次数: 0

Abstract

A (m+3)-dimensional Einstein–Gauss–Bonnet gravitational model including the Gauss–Bonnet term and the cosmological term Λ is considered. Exact solutions with exponential time dependence of two scale factors, governed by two Hubble-like parameters H>0 and h≠H, corresponding to factor spaces of dimensions m>2 and l=2, respectively, are found. Under certain restrictions on x=h/H, the stability of the solutions in a class of cosmological solutions with diagonal metrics is proved. A subclass of solutions with small enough variation of the effective gravitational constant G is considered and the stability of all solutions from this subclass is shown. This article is part of the theme issue ‘The future of mathematical cosmology, Volume 1’.
具有Λ-term的(1+ m + 2)维Einstein-Gauss-Bonnet模型中具有两因子空间的稳定指数宇宙学解
考虑了一个(m+3)维爱因斯坦-高斯-邦纳引力模型,其中包括高斯-邦纳项和宇宙学项Λ。得到了由两个类哈勃参数H>0和H≠H控制的两个尺度因子分别对应于维数m b> 2和l=2的因子空间的指数时间依赖的精确解。在x=h/ h的一定限制下,证明了一类具有对角度量的宇宙学解解的稳定性。考虑了有效引力常数G变化足够小的一类解,并证明了该类所有解的稳定性。本文是主题问题“数学宇宙学的未来,第一卷”的一部分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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