Modeling 'hydrodynamic phase transitions' in a radiating spherically symmetric distribution of matter

Details Modeling 'hydrodynamic phase transitions' in a radiating spherically symmetric distribution of matter Modeling 'hydrodynamic phase transitions' in a radiating spherically symmetric distribution of matter

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..339h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 1, 1989, p. 339-353. Research supported by the Fundacion Polar a

Physics

Condensed Matter

8

Astronomical Models, Gravitational Collapse, Magnetohydrodynamics, Mass Distribution, Phase Transformations, Condensed Matter Physics, Magnetohydrodynamic Waves, Neutron Stars, Shock Waves, Supernovae

Scientific paper

A method for studying the evolution of discontinuities in radiating spherically symmetric distributions of matter has been extended to model hydrodynamic phase transitions in a composite radiant sphere. In the present scenario, the matter configuration is divided into two regions by a shock wave front, with each side of the interface having a different anisotropic phase. The resultant models are shown to be strongly dependent on the anisotropic jump across the interface and on the luminosity (opacity) of the shock wave.

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