On stable exponential solutions in Einstein–Gauss–Bonnet cosmology with zero variation of G-dimensional factor space with the Hubble parameter H and
zero variation of the effective gravitational
On Multidimensional Cosmology with Anisotropic Fluid: Asymptotical Acceleration and Zero Variation of G to the density: pi = wiρ, i = 0,…,n.
Solutions with accelerated expansion of our 3-space M0 and
zero variation Bi-Variationality, Symmetries and Approximate SolutionsBy a bi-
variational system we mean any system of equations generated by two different Hamiltonian