  The article is devoted to cosmology. It deals with homogeneous anisotropic
cosmological models. Scale factors have been evaluated for the multicomponent
models with perfect fluid, taking account of its expansion, rotation and shear.
The cosmological fluid components are as follows: phantom matter, de Sitter
vacuum, domain walls, strings, dust, radiation, perfect gas, stiff matter and
ekpyrotic matter. The scale factor dependences on the equation of state and
kinematic invariants of the perfect fluid have been analysed. The paper is
aimed at finding exact solutions of Friedmann and Raychaudhuri equations for
different combination of matter components and kinematic invariants.
