Neutrino fluxes from CNO cycle in the Sun in the non stationary case with mixing

Details Neutrino fluxes from CNO cycle in the Sun in the non stationary case with mixing Neutrino fluxes from CNO cycle in the Sun in the non stationary case with mixing

2009-02-13

arxiv.org/abs/0902.2272v1

JCAP 0908:006,2009

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

6 pages, 3figures

Scientific paper

10.1088/1475-7516/2009/08/006

The computational analyses is presented of the non stationary case with
mixing of the solar model when the neutrino flux $F_{13}$ from the decay of
$^{13}N$ is higher than a standard solar model predicts

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