arXiv:0707.3500·v1·Astrophysics
Coulomb tunneling for fusion reactions in dense matter: Path integral Monte Carlo versus mean field
A.I. Chugunov (1)🇷🇺 · H.E. DeWitt (2)🇺🇸 · D.G. Yakovlev (1) ((1) Ioffe Institute; (2) LLNL)🇷🇺
Abstract
We compare Path Integral Monte Carlo calculations by Militzer and Pollock (Phys. Rev. B 71, 134303, 2005) of Coulomb tunneling in nuclear reactions in dense matter to semiclassical calculations assuming WKB Coulomb barrier penetration through the radial mean-field potential. We find a very good agreement of two approaches at temperatures higher than ~1/5 of the ion plasma temperature. We obtain a simple parameterization of the mean field potential and of the respective reaction rates. We analyze Gamow-peak energies of reacting ions in various reaction regimes and discuss theoretical uncertainties of nuclear reaction rates taking carbon burning in dense stellar matter as an example.
Comments: 13 pages, 7 figures, to appear in Phys. Rev. D