Surface phenomena and the evolution of radiating fluid spheres in general relativity

Details Surface phenomena and the evolution of radiating fluid spheres in general relativity Surface phenomena and the evolution of radiating fluid spheres in general relativity

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345..918h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 15, 1989, p. 918-924. Research supported by the Direccion General

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Computation

4

Computational Astrophysics, Condensed Matter Physics, Gravitational Collapse, Relativity, Stellar Evolution, Interfacial Tension, Surface Reactions

Scientific paper

A method used to study the evolution of radiating spheres (Herrera,
Jimenez, and Ruggeri) is extended to the case in which surface phenomena
are taken into account. The equations have been integrated numerically
for a model derived from the Schwarzschild interior solution, bringing
out the effects of surface tension on the evolution of the spheres.

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