Relativistic Radiative Transfer for Spherical Flows

Preprint

18 June 1994

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9406055

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.

Keywords

RELATIVISTIC RADIATIVE
RADIATIVE TRANSFER
RADIATION FLUID
SPHERICAL FLOWS
NEW COMPLETE
COMPLETE SET

All Related Versions

Version 1, 1994-06-18, ArXiv
Published version: Classical and Quantum Gravity, 11 (7), 1815.

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