摘要

We have investigated general Bianchi type I cosmological models which containing a perfect fluid and dark energy with time varying G and I > that have been presented. The perfect fluid is taken to be one obeying the equation of state parameter, i.e., p=omega I; whereas the dark energy density is considered to be either modified polytropic or the Chaplygin gas. Cosmological models admitting both power-law which is explored in the presence of perfect fluid and dark energy too. We reconstruct gravitational parameter G, cosmological term I >, critical density rho (c) , density parameter Omega, cosmological constant density parameter Omega (I >) and deceleration parameter q for different equation of state. The present study will examine non-linear EOS with a general nonlinear term in the energy density.

  • 出版日期2012-8