Comment on the BDT-Bianchi type-VI(0) stiff matter solution

Details Comment on the BDT-Bianchi type-VI(0) stiff matter solution Comment on the BDT-Bianchi type-VI(0) stiff matter solution

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.108..419l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 108, no. 2, Jan. 1985, p. 419-421.

Statistics

Computation

1

Computational Astrophysics, Cosmology, Mass Distribution, Relativity, Scalars, Vacuum, Asymptotic Series, Relativistic Theory, Series Expansion, Stiffness

Scientific paper

The author points out that the Brans-Dicke-Bianchi type VI0 stiff matter solution recently given by Ram and Singh is not the most general solution of the corresponding field equations. Moreover, this solution has no vacuum limit and the general relativistic limit is obtained only after making an asymptotic expansion. In this paper the author rediscusses the entire problem in a different way. In the limit φ = const., ω→∞, he obtains both the stiff matter and the vacuum relativistic limit first given by Ellis and MacCallum (1969) in analytic form.

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