Unsteady flow of a relativistic radiating gas in a gravitational field

Details Unsteady flow of a relativistic radiating gas in a gravitational field Unsteady flow of a relativistic radiating gas in a gravitational field

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.192..201b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 192, no. 2, June 1992, p. 201-207.

Statistics

Computation

Gravitational Fields, Interstellar Gas, Neutrinos, Relativistic Plasmas, Unsteady Flow, Computational Astrophysics, Perturbation Theory, Radiative Heat Transfer

Scientific paper

The unsteady flow of a relativistic radiating neutrino gas is studied in
a gravitational field. The curved body is assumed to be a vertical flat
plate on which is imposed a time-dependent perturbations on a basic
flow. For small perturbations, the ill-posed problem is reduced to a
well-posed one and analytical solutions are developed.

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