Multidimensional cosmology with anisotropic fluid: acceleration and   variation of G
  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. 
J.-M. Alimi, V.D. Ivashchuk, S.A. Kononogov and V.N. Melnikov