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Relativistic Radiative Transfer for Spherical Flows

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arxiv astro-ph/9406055 v1 pith:ICL4GNCP submitted 1994-06-18 astro-ph

Luciano Rezzolla , John C. Miller This is my paper · ORCID
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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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