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Автор Luciano Rezzolla
Автор John C Miller
Дата выпуска 1994-07-01
dc.description 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.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Relativistic radiative transfer for spherical flows
Тип paper
DOI 10.1088/0264-9381/11/7/018
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 11
Первая страница 1815
Последняя страница 1832
Выпуск 7

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