Astrophysical Implications of Fusion Reactions at Extremely Low Energies involving 12C and 16O

Details Astrophysical Implications of Fusion Reactions at Extremely Low Energies involving 12C and 16O Astrophysical Implications of Fusion Reactions at Extremely Low Energies involving 12C and 16O

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1304..395m&link_type=abstract

EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (III): From Nuclei to Stars. AIP Conference Proceedings, Volume 1304, pp. 395-4

Astronomy and Astrophysics

Astrophysics

Nuclear Fusion, Nucleosynthesis, Nuclear Fragmentation, Coulomb Blockade, Fusion And Fusion-Fission Reactions, Cosmic Ray Nucleosynthesis, Projectile And Target Fragmentation, Coulomb Energies

Scientific paper

The heavy-ion potential is calculated semi-microscopically within the double folding method with various effective n-n interactions (Gogny, M3Y) and applied to fusion reactions relevant for the carbon and oxygen burning cycles in highly evolved stars. Reaction rates at temperatures relevant for such stellar processes are estimated and upon comparison with traditional and modern extrapolation formulas conclusions are drawn regarding the importance of the employed n-n interactions on the corresponding burning cycle.

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