Detonation-wave structure and nucleosynthesis in exploding carbon-oxygen cores and white dwarfs

Astronomy and Astrophysics – Astronomy

Scientific paper

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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.

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