Milne–Eddington Solutions for Relativistic Spherical Flows
نویسندگان
چکیده
منابع مشابه
Relativistic Radiative Transfer for Spherical Flows
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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ژورنال
عنوان ژورنال: Publications of the Astronomical Society of Japan
سال: 2010
ISSN: 0004-6264,2053-051X
DOI: 10.1093/pasj/62.2.255