Generalized coulomb barrier transmission coefficient for solar neutrino and astrophysical problems

Details Generalized coulomb barrier transmission coefficient for solar neutrino and astrophysical problems Generalized coulomb barrier transmission coefficient for solar neutrino and astrophysical problems

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ijtp...33.1861k&link_type=abstract

International Journal of Theoretical Physics, Volume 33, Issue 9, pp.1861-1867

Physics

Scientific paper

For astrophysical calculations, it is customary to extrapolate higher-energy (≳20keV) data using the Gamow transmission coefficient in estimating the nonresonance nuclear fusion reaction cross sections σ(E) for charged particles at low energies (<20 keV). We present a general extrapolation method based on a more realistic Coulomb barrier transmission coefficient, which can accommodate simultaneously both nonresonance and resonance contributions.

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