Dissipative relativistic radiative hydrodynamics

Details Dissipative relativistic radiative hydrodynamics Dissipative relativistic radiative hydrodynamics

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1198i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Nov.-Dec. 1989, p. 1198-1207. In Russian.

Statistics

Computation

1

Computational Astrophysics, Dissipation, Hydrodynamics, Relativistic Theory, Compton Effect, Differential Equations, Lorentz Transformations, Radiation Absorption, Radiative Heat Transfer

Scientific paper

Using a noninertial comoving reference frame, equations of relativistic radiative hydrodynamics are derived, taking account of dissipative properties of matter and interaction (effects of absorption and Compton scattering) of nearly equilibrium (Planckian) radiation with matter. The system of equations obtained can be considered a relativistic generalization of the well-known equations of radiative hydrodynamics in Lagrangian coordinates. The most interesting result is the appearance of several types of coefficients of bulk radiative viscosity, in addition to the coefficients of radiative heat conduction and shear radiative viscosity.

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