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arXiv · 0811.4053

Nuclear electron capture rate in stellar interiors and the case of 7Be

P. Quarati·A. M. Scarfone
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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.

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P. Quarati, A. M. Scarfone. 2008-11-25. Nuclear electron capture rate in stellar interiors and the case of 7Be. https://doi.org/10.1088/0954-3899%2F36%2F2%2F025203

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