Statistics – Computation
Scientific paper
Apr 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..345m&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, April 1987, p. 345-351. In Russian. In Russian.
Statistics
Computation
1
Electron-Positron Pairs, Gas Dynamics, Interstellar Gas, Pair Production, Relativistic Velocity, Shock Wave Luminescence, Thermal Radiation, Computational Astrophysics, Gas Density, Gas Temperature
Scientific paper
Calculations of Taub's equations with allowance for equilibrium radiation and equations of state with allowance for the production of electron-positron pairs are carried out for a wide range of undisturbed-gas densities, 10 to the -13th to 10 to the 7th g/cu cm. The shock velocity is defined as a parameter in a range from 0.0001 to 0.99 of light velocity. The main features of gas-state changes behind the shock front are examined as a function of the undisturbed-gas density and the shock velocity. Conditions for the occurrence of the radiation-domination regime of the shock wave are established. The results are of interest in connection with the study of relativistic shock waves in stars or the interstellar gas.
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