An equation of state for radiating dissipative spheres in general relativity

Details An equation of state for radiating dissipative spheres in general relativity An equation of state for radiating dissipative spheres in general relativity

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.193..201b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 193, no. 2, July 1992, p. 201-215.

Astronomy and Astrophysics

Astrophysics

11

Anisotropy, Energy Dissipation, Equations Of State, Relativity, Spheres, Thermal Conductivity, Navier-Stokes Equation, Schwarzschild Metric, Stellar Models, Viscosity

Scientific paper

The paper studies the effects of viscosity and thermal conduction on the evolution of radiating fluid spheres. The present proposition for examining dissipative fluids in a general relativistic approach consists of a prescription of an equation of state which specifies the degree of anisotropy induced by the viscosity. The Herrera-Jimenez-Ruggeri method extended to the case of dissipative radiating fluids is used to elaborate an explicit Schwarzschild-like model.

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