Relativistic Radiative Transfer for Spherical Flows

Details Relativistic Radiative Transfer for Spherical Flows Relativistic Radiative Transfer for Spherical Flows

1994-06-18

arxiv.org/abs/astro-ph/9406055v1

Class.Quant.Grav.11:1815-1832,1994

Astronomy and Astrophysics

Astrophysics

28 pages, 9 postscript figs, Plain TeX

Scientific paper

10.1088/0264-9381/11/7/018

We present a new complete set of Lagrangian relativistic hydrodynamical equations describing the transfer of energy and momentum between a standard fluid and a radiation fluid in a general non-stationary spherical flow. The new set of equations has been derived for a particular application to the study of the cosmological Quark--Hadron transition but can also be used in other contexts.

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