Other
Scientific paper
May 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230..223l&link_type=abstract
Astrophysical Journal, Part 1, vol. 230, May 15, 1979, p. 223-229.
Other
Detonation Waves, Dwarf Stars, Nonuniform Plasmas, Stellar Evolution, Stellar Models, Carbon, Electron Energy, Shock Fronts, Stellar Structure, Supernovae, Wave Equations
Scientific paper
The microstructure of detonation waves is investigated under the conditions expected to obtain in 4- to 8-solar mass degenerate carbon dwarfs. A two-component plasma composed of ions and degenerate electrons is considered, and the case of a high-ion-temperature precursor with subsequent transfer via Coulomb interactions is treated in order to see whether such a nonequilibrium situation can affect the self-consistency of the detonation wave. It is found that, in an actual situation, this more exact treatment does not significantly alter the conditions and conclusions obtained by other authors for a thermal-equilibrium detonation.
Buchler Jean-Robert
Littleton J. E.
Truran Jame. W.
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