The modified Lagrangian equations of general-relativistic hydrodynamics for a nonideal fluid

Details The modified Lagrangian equations of general-relativistic hydrodynamics for a nonideal fluid The modified Lagrangian equations of general-relativistic hydrodynamics for a nonideal fluid

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.145..355m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 145, no. 2, June 1988, p. 355-376.

Astronomy and Astrophysics

Astronomy

3

Euler-Lagrange Equation, Hydrodynamics, Quasars, Relativistic Effects, Seyfert Galaxies, Black Holes (Astronomy), Navier-Stokes Equation, Newtonian Fluids, Radiative Transfer, Thermal Conductivity, Viscous Fluids

Scientific paper

The general-relativistic equations of hydrodynamics for a nonideal fluid are derived in the modified Lagrangian form. Together with the zeroth and first moment equations of radiative transfer derived by Morita and Kaneko (1986), the equations provide a complete set of the modified Lagrangian equations of radiation hydrodynamics. The equations of hydrodynamics are specialized for a thermally conducting, Newtonian viscous fluid in the modified Lagrangian form, which are the generalization of the special-relativistic equations of hydrodynamics derived by Greenberg (1975).

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