Deflagration-front structure in a degenerate carbon core

Details Deflagration-front structure in a degenerate carbon core Deflagration-front structure in a degenerate carbon core

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..302k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, May 1983, p. 302-306) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, May-June 19

Astronomy and Astrophysics

Astronomy

2

Carbon Stars, Deflagration, Nuclear Reactions, Stellar Evolution, Thermonuclear Explosions, Nuclides, Reaction Kinetics, Supernovae

Scientific paper

The structure of a nonsteady deflagration front determined by nuclear kinetics is calculated in the density range ρ0 = 107-109 g/cm3 assuming constant pressure. It is found that at ρ0 > ρe ≅ 5×107 g/cm3 burning of C12 leads to nuclear statistical equilibrium. When ρ < ρe the products of burning are nuclides with A ≤ 30. An approximate description of nuclear kinetics is discussed.

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