On stable exponential solutions in Einstein–Gauss–Bonnet cosmology with zero variation of G
- 作者: Ivashchuk V.D.1,2
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隶属关系:
- Institute of Gravitation and Cosmology
- Center for Gravitation and Fundamental Metrology
- 期: 卷 22, 编号 4 (2016)
- 页面: 329-332
- 栏目: Article
- URL: https://journals.rcsi.science/0202-2893/article/view/176045
- DOI: https://doi.org/10.1134/S0202289316040095
- ID: 176045
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详细
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.
作者简介
V. Ivashchuk
Institute of Gravitation and Cosmology; Center for Gravitation and Fundamental Metrology
编辑信件的主要联系方式.
Email: ivashchuk@mail.ru
俄罗斯联邦, Miklukho-Maklaya 6, Moscow, 117198; Ozyornaya 46, Moscow, 119361
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