Exact Bianchi type V imperfect fluid solutions

Details Exact Bianchi type V imperfect fluid solutions Exact Bianchi type V imperfect fluid solutions

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996gregr..28..251n&link_type=abstract

General Relativity and Gravitation, Volume 28, Issue 3, pp.251-261

Physics

4

Scientific paper

It is shown that it is sufficient to solve a single first order differential equation to determine exact Bianchi type V imperfect fluid solutions of Einstein's field equations. Two exact solutions are presented in this paper. One of these two solutions corresponds to the case when the anisotropic pressure tensor is proportional to the shear tensor. This proportionality, it is shown, is a necessary but not a sufficient condition for the absence of heat flow in a Bianchi type V universe. It is also observed that the presence of heat flow necessarily introduces anisotropy in a Bianchi type V universe.

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