Radiating spherical collapse with shear and heat flow

Details Radiating spherical collapse with shear and heat flow Radiating spherical collapse with shear and heat flow

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.199..215t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 199, no. 2, p. 215-223.

Statistics

Computation

5

Computational Astrophysics, Gravitational Collapse, Heat Flux, Relativity, Shear, Astronomical Models, Gravitational Fields

Scientific paper

We consider a spherical body consisting of a fluid with heat flow which radiates in its exterior a null fluid described by the outgoing Vaidya's metric, we prove that this solution matched with the outgoing Vaidya's metric represents a physically reasonable collapsing model. Our model has the remarkable property: it is shear-free and the motion of the fluid is geodesic.

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