Abstract
We present pycnonuclear reaction calculations for a one-component ionic crystal at zero temperature considering different theoretical approaches. The rates depend directly on the determination of the astrophysical S-factor at low energies, which has been obtained through the barrier penetration formalism. A totally parameter-free model for the real part of the nuclear interaction has been employed in the calculation of 12C+12C fusion cross sections.
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Schedule a callMore From: Journal of Physics G: Nuclear and Particle Physics
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