Bianchi Type VI1 Cosmological Model in Scale-Invariant Theory

Details Bianchi Type VI1 Cosmological Model in Scale-Invariant Theory Bianchi Type VI1 Cosmological Model in Scale-Invariant Theory

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002czjph..52..765m&link_type=abstract

Czechoslovak Journal of Physics, vol. 52, Issue 6, p.765-773

Physics

2

Space-Time - Scale-Invariant - Dirac Gauge - Perfect Fluid

Scientific paper

An attempt has been taken to study the feasibility of scale-invariant theory in Bianchi type VI h space-time with a time dependent gauge function (Dirac gauge) and a matter field in the form of a perfect fluid with isotropic matter pressure. It is found that Bianchi type VI h (h = 1) space-time is feasible in this theory whereas Bianchi type VI h (h = -1) and VI h (h = 0) space-times are not feasible. In the feasible case a non-singular model for the universe filled with disorder radiation is constructed and some of its physical behaviors are studied.

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