Einstein Rosen Universe in a Scalar-Tensor Theory of Gravitation

Details Einstein Rosen Universe in a Scalar-Tensor Theory of Gravitation Einstein Rosen Universe in a Scalar-Tensor Theory of Gravitation

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.301...79r&link_type=abstract

Astrophysics and Space Science, Volume 301, Issue 1-4, pp. 79-82

Astronomy and Astrophysics

Astrophysics

1

Perfect Fluid, Scalar-Tensor Theory, Stiff Fluid

Scientific paper

Field equations in the presence of a perfect fluid distribution are obtained in a scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. 113, 1985, 467) with the aid of Einstein Rosen cylindrically symmetric metric. A static vacuum model and a non-static stiff fluid model are presented. The physical and geometrical properties of the stiff fluid model are studied.

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