Gravitational collapse of a radiating star

Details Gravitational collapse of a radiating star Gravitational collapse of a radiating star

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phla..141..243k&link_type=abstract

Physics Letters A, Volume 141, Issue 5-6, p. 243-248.

Physics

5

Scientific paper

The gravitational collapse of a radiating sphere consisting of a heat conducting fluid with shear-free and radial motion is investigated. The exterior region of the sphere is described by the Vaidya metric while in the interior we suppose that there exists a flux of neutrinos which is described by a null dust term in the energy-momentum tensor. A particular model based on an exact solution of the Einstein field equations for the interior of the sphere is studied.

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