Thermodynamics of a model of nonadiabatic spherical gravitational collapse

Details Thermodynamics of a model of nonadiabatic spherical gravitational collapse Thermodynamics of a model of nonadiabatic spherical gravitational collapse

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.211...31g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 211, no. 1, p. 31-40

Physics

6

Gravitational Collapse, Nonadiabatic Conditions, Stellar Evolution, Thermodynamics, Diffusion, Dissipation, Field Theory (Physics), Fluid Flow, Radiation Transport

Scientific paper

In this work, a thermodynamic treatment of a Friedmann-like model of nonadiabatic spherical gravitational collapse is presented. The calculations have been performed according to Eckart's theory of dissipative relativistic fluids, while the diffusion approximation has been adopted for the radiation transport. The conclusions deduced are in agreement with the predictions of the theory of late stellar evolution.

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