Statistics – Computation
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.239..785k&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 239, Aug. 15, 1989, p. 785-808.
Statistics
Computation
39
Dense Plasmas, Detonation Waves, Shock Wave Propagation, Supernovae, Thermonuclear Explosions, Carbon, Computational Astrophysics, Gas Dynamics, Helium, Oxygen
Scientific paper
The theory of gaseous detonation is applied to thermonuclear detonation waves in supernovae. First, the two-temperature structure of strong shock waves in a dense degenerate plasma is considered. The ion-electron energy transfer rate is calculated for a plasma with arbitrary degeneracy of electrons. It is shown that the non-equilibrium heating of ions is unimportant for detonation. The steady planar one-dimensional structure of detonation waves both in C + O mixtures and in pure helium He-4 is computed for densities from 10 to the 6th to 3 x 10 to the 9th g/cu cm. The thickness of the detonation waves is obtained as a function of the initial density of the matter.
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