Diffusion processes in the collapse of a radiating spherical body

Details Diffusion processes in the collapse of a radiating spherical body Diffusion processes in the collapse of a radiating spherical body

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...382..255c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 382, Nov. 20, 1991, p. 255-260.

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Conductive Heat Transfer, Diffuse Radiation, Gravitational Collapse, Stellar Models, Supernovae, Adiabatic Conditions, Computational Astrophysics, Radiative Heat Transfer, Spheres, Stellar Cores

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The model considered by Barreto et al. (1989) to study the heat conduction and photon processes in the collapse of a radiating spherical system is further developed. The spherical body is divided into two regions: the core, modeled with a nonadiabatic fluid that can produce radiation, and the envelope of dust and radiation that surrounds the core. The effective adiabatic index, the shear, and the temperature are analyzed for the heat conduction and the photon diffusion limits.

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