作者: Abhik Kumar Sanyal , A. Banerjee
DOI: 10.1007/BF00759320
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摘要: The irrotational Bianchi V cosmological model under the influence of both shear and bulk viscosity, together with heat flux, has been studied. Exact solutions for are obtained three assumptions which first two relate matter density, scalar, expansion scalar third is a barotropic equation state, connecting density thermodynamic pressure. properties studied temperature distribution also given explicitly. It observed that along flux further adds to rate entropy increase.