Multidimensional cosmology with anisotropic fluid: acceleration and variation of G

Details Multidimensional cosmology with anisotropic fluid: acceleration and variation of G Multidimensional cosmology with anisotropic fluid: acceleration and variation of G

2006-11-02

arxiv.org/abs/gr-qc/0611015v3

Grav.Cosmol.12:173-178,2006

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, Latex, corrected typos, Proceedings of the International Conference on Gravitation, Cosmology, Astrophysics and Nonst

Scientific paper

A multidimensional cosmological model describing the dynamics of n+1 Ricci-flat factor-spaces M_i in the presence of a one-component anisotropic fluid is considered. The pressures in all spaces are proportional to the density: p_i = w_i \rho, i = 0,...,n. Solutions with accelerated expansion of our 3-space M_0 and small enough variation of the gravitational constant G are found. These solutions exist for two branches of the parameter w_0. The first branch describes superstiff matter with w_0 > 1, the second one may contain phantom matter with w_0 < - 1, e.g., when G grows with time.

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