Radiating spheres in general relativity with a mixed transport energy flow

Details Radiating spheres in general relativity with a mixed transport energy flow Radiating spheres in general relativity with a mixed transport energy flow

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.178..261b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 178, no. 2, April 1991, p. 261-275. Research supported by International Ce

Astronomy and Astrophysics

Astrophysics

9

Gravitational Collapse, Radiative Transfer, Relativity, Supernova Remnants, Explosions, Hydrodynamics, Spheres

Scientific paper

The evolution of general relativistic spheres is studied analytically for the case where diffusion and free streaming radiation are simultaneously present. The seminumerical method, based on the work of Herrera et al. (1990), assumes that free streaming processes are proportional to diffusive ones, and the initial data and the radiation profile are given at the surface of matter distribution. The mixed-mode radiation is found to be responsible for a unique hydrodynamic process, and the dynamic of the matter distribution depends primarily on the equation of state of the model.

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