Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..631i&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Aug. 1984, p. 631-640) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, July-Aug
Astronomy and Astrophysics
Astronomy
4
Abundance, Carbon Stars, Detonation Waves, Nuclear Fusion, Stellar Cores, Supernovae, White Dwarf Stars, Hydrodynamic Equations, Light Elements, Reaction Kinetics, Stellar Models, Stellar Structure, Thermonuclear Explosions
Scientific paper
The structure of a steady detonation wave in highly degenerate carbon C12 is studied in the density range 106 - 108 g/cm3. A nuclear reaction network for 84 nuclides including protons, neutrons and α-particles and about 600 nuclear reactions is used. Conditions are investigated for existence of all possible regimes of detonation known in hydrodynamical theory of combustion.
Imshennik Vladimir S.
Khokhlov Alexei M.
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