Astrophysical S factors for fusion reactions involving C, O, Ne, and Mg isotopes

Using the São Paulo potential and the barrier penetration formalism we have calculated the astrophysical factor S(E)S(E) for 946 fusion reactions involving stable and neutron-rich isotopes of C, O, Ne, and Mg for center-of-mass energies E varying from 2 to ≈18–30 MeV (covering the range below and above the Coulomb barrier). We have parameterized the energy dependence, S(E)S(E), by an accurate universal 9-parameter analytic expression and present tables of fit parameters for all the reactions. We also discuss the reduced 3-parameter version of our fit which is highly accurate at energies below the Coulomb barrier, and outline the procedure for calculating the reaction rates. The results can be easily converted to thermonuclear or pycnonuclear reaction rates to simulate various nuclear burning phenomena, in particular, stellar burning at high temperatures and nucleosynthesis in high density environments.