  Einstein Gravitational Field Equations (EFE) of Chaplygin gas dominated
Bianchi-type models are obtained by using metric approximation. The solutions
of equations for a special case, namely Bianchi I model which is a
generalization of isotropic Friedmann-Robertson-Walker (FRW) cosmology, are
obtained. The early and late behaviours of some kinematic parameters in model
are presented in graphically.
