Scale invariant theory for Bianchi Type VIII and IX space-times with perfect fluid

Details Scale invariant theory for Bianchi Type VIII and IX space-times with perfect fluid Scale invariant theory for Bianchi Type VIII and IX space-times with perfect fluid

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.283...67m&link_type=abstract

Astrophysics and Space Science, v. 283, Issue 1, p. 67-74 (2003).

Astronomy and Astrophysics

Astrophysics

3

Perfect Fluid, Energy-Density, Isotropy, Dirac Gauge, Space-Time Ms Classification Number (1991): 83D05 Pacs Number (1983): 04.50+H

Scientific paper

In this paper we have taken an attempt to study the feasibility of scale invariant theory (Wesson, 1981a,b) in Bianchi type VIII and IX space-times with a time dependent gauge function (Dirac Gauge i.e. βα{1}/{t}) and a matter field in the form of a perfect fluid. It is found that Bianchi type VIII (δ=1) space-time is feasible in this theory whereas Bianchi type IX (δ=-1) space-time is not feasible. In this feasible case a radiating model is constructed and its physical behaviour is discussed.

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