Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..70..183d&link_type=abstract
Astrophysics and Space Science, vol. 70, no. 1, June 1980, p. 183-190.
Astronomy and Astrophysics
Astrophysics
Carbon Stars, Cores, Stellar Evolution, Stellar Winds, Thermonuclear Reactions, Annihilation Reactions, Bremsstrahlung, Energy Dissipation, Gravitational Collapse, Neutrinos, Supernovae
Scientific paper
Physical conditions prevalent in a degenerate carbon plasma lead to the enhancement of the carbon-carbon thermonuclear reaction rates. Nuclear energy generation rate in the carbon core is thereby augmented. The possible dissipation of energy due to pair-annihilation neutrinos, plasma neutrinos and neutrino bremsstrahlung are considered. Neutral current contribution to these weak processes are also taken into account. It is suggested that the enhanced nuclear generation rate in the evolved core might halt the core collapse for a time, thus necessitating a reassessment of the phenomenon of core collapse as a precursor of carbon detonation supernova events.
Duorah Hira Lal
Duorah Kalpana
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