Rates for some reactions in the mass range 39 is less than or equal to A which is less than or equal to 45
Abstract
Groundstate reaction rates have been deduced from recent cross section measurements for the ^{39}K(α, p)^{42}Ca, ^{42}Ca(α, p)^{45}Sc, ^{42}Ca(α, n)^{45}Ti, ^{42}Ca(p, γ)^{43}Sc, and ^{44}Ca(p, n)^{44}Sc reactions. Stellar reaction rates have been derived from the groundstate rates by multiplying by the ratio of stellar to groundstate rates obtained from statistical model calculations. Stellar rates for the four exoergic reverse reactions have been derived using the procedures of Woosley et al.
 Publication:

The Astrophysical Journal
 Pub Date:
 January 1983
 DOI:
 10.1086/160595
 Bibcode:
 1983ApJ...264..278B
 Keywords:

 Ground State;
 Nuclear Fusion;
 Reaction Kinetics;
 Stars;
 Calcium;
 Oxygen;
 Silicon;
 Stellar Mass;
 Stellar Temperature;
 Astrophysics