Radiation hydrodynamics and radiating spheres in general relativity

Details Radiation hydrodynamics and radiating spheres in general relativity Radiation hydrodynamics and radiating spheres in general relativity

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.219..153a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 219, no. 2, p. 153-170

Astronomy and Astrophysics

Astrophysics

3

Diffusion, Equations Of State, Free Flow, Hydrodynamics, Mass Distribution, Mathematical Models, Radiation, Relativity, Spheres, Boltzmann Transport Equation, Boundary Conditions, Einstein Equations, Flux Density, Tensor Analysis

Scientific paper

We comment on a method proposed to study the evolution of General Relativistic Radiating Spheres in both radiation limits, i.e. free streaming out and diffusion, extending it to handle any general radiating spherically symmetric distribution of matter. It is also shown that several dynamic models may emerge from a sole static equation of state. Previous erroneous calculations concerning this method are also commented.

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