Non-static fluid spheres in general relativity

Details Non-static fluid spheres in general relativity Non-static fluid spheres in general relativity

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.108..415m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 108, no. 2, Jan. 1985, p. 415-417.

Statistics

Computation

Density Distribution, Fluid Pressure, Gravitational Collapse, Relativity, Spheres, Static Stability, Computational Astrophysics, Mass Distribution

Scientific paper

A few years ago, Banerjee and Banerji had given a class of exact interior solutions for a perfect spherically-symmetric fluid distribution with inhomogeneous density and pressure. This class serves as a simple model for gravitational collapse with inhomogeneous matter and, therefore, may be of an essential astrophysical importance. It is proved that these solutions are, in fact, identical with Faulkes' earlier solutions.

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