Nuclear electron capture rate in stellar interiors and the case of 7Be
Nuclear Theory
2009-03-04 v1
Abstract
Nuclear electron capture rate from continuum in an astrophysical plasma environment (like solar core) is calculated using a modified Debye-Huckel screening potential and the related non-Gaussian q-distribution of electron momenta. For q=1 the well-known Debye-Huckel results are recovered. The value of q can be derived from the fluctuation of number of particles and temperature inside the Debye sphere. For 7Be continuum electron capture in solar core, we find an increase of 7 -- 10 percent over the rate calculated with standard Debye-Huckel potential. The consequence of this results is a reduction of the same percentage of the SSM 8B solar neutrino flux, leaving unchanged the SSM 7Be flux.
Cite
@article{arxiv.0811.4053,
title = {Nuclear electron capture rate in stellar interiors and the case of 7Be},
author = {P. Quarati and A. M. Scarfone},
journal= {arXiv preprint arXiv:0811.4053},
year = {2009}
}
Comments
8 pages, 1 figure, IOP macro style, submitted to JPG