Modeling ``Hydrodynamic Phase Transitions'' in a Radiating Spherically Symmetric Distribution of Matter
Abstract
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.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 1989
- DOI:
- Bibcode:
- 1989ApJ...339..339H
- Keywords:
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- Astronomical Models;
- Gravitational Collapse;
- Magnetohydrodynamics;
- Mass Distribution;
- Phase Transformations;
- Condensed Matter Physics;
- Magnetohydrodynamic Waves;
- Neutron Stars;
- Shock Waves;
- Supernovae;
- Astrophysics;
- DENSE MATTER;
- HYDRODYNAMICS;
- SHOCK WAVES