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handle: 11584/3474
Summary: We adopt here the idea of describing a radiation field by means of the radiation energy density \(E\) and the radiative flux vector \(F\) which must satisfy a set of evolution equations; in these equations an unknown tensorial function \(P(E,F)\) appears that is determined by the methods of extended thermodynamics.
Foundations, constitutive equations, rheology, hydrodynamical models of non-fluid phenomena, Transport processes in time-dependent statistical mechanics, semiconductors, plasmas, neutron transport, radiation energy density, radiative transfer, Radiative transfer in astronomy and astrophysics, QA1-939, extended thermodynamics, electron transport, radiative flux vector, PDEs in connection with optics and electromagnetic theory, Mathematics
Foundations, constitutive equations, rheology, hydrodynamical models of non-fluid phenomena, Transport processes in time-dependent statistical mechanics, semiconductors, plasmas, neutron transport, radiation energy density, radiative transfer, Radiative transfer in astronomy and astrophysics, QA1-939, extended thermodynamics, electron transport, radiative flux vector, PDEs in connection with optics and electromagnetic theory, Mathematics
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