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 in the study of the cosmological quark - hadron transition, but can also be used in other contexts.
Relativistic radiative transfer for spherical flows / Rezzolla, L.; Miller, J. C.. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - 11:7(1994), pp. 018.1815-018.1832. [10.1088/0264-9381/11/7/018]
Relativistic radiative transfer for spherical flows
MILLER J. C.
1994-01-01
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 in the study of the cosmological quark - hadron transition, but can also be used in other contexts.File in questo prodotto:
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