Expressions for the 14O(α,p)17F and 17F(p,γ)18Ne astrophysical reaction rates

Details Expressions for the 14O(α,p)17F and 17F(p,γ)18Ne astrophysical reaction rates Expressions for the 14O(α,p)17F and 17F(p,γ)18Ne astrophysical reaction rates

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvc..56.1647b&link_type=abstract

Physical Review C (Nuclear Physics), Volume 56, Issue 3, September 1997, pp.1647-1650

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Transfer Reactions, Radiative Capture, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables

Scientific paper

The 14O(α,p)17F and 17F(p,γ)18Ne astrophysical reaction rates are needed to determine the breakout conditions from the hot CNO cycle into the rapid proton capture process in hot stellar environments. We have examined recent indirect experimental measurements of these reactions and generated analytical expressions for the reaction rates as a function of temperature. We also present a correction to the previously reported calculation of the 17F(p,γ) rate.

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