Relativistic Radiative Transfer for Spherical Flows
Astrophysics
2010-04-06 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/9406055,
title = {Relativistic Radiative Transfer for Spherical Flows},
author = {Luciano Rezzolla and John C. Miller},
journal= {arXiv preprint arXiv:astro-ph/9406055},
year = {2010}
}
Comments
28 pages, 9 postscript figs, Plain TeX