Solar Neutrinos from CNO Electron Capture

Details Solar Neutrinos from CNO Electron Capture Solar Neutrinos from CNO Electron Capture

2003-09-23

arxiv.org/abs/hep-ph/0309266v3

Phys.Rev. C69 (2004) 015801

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 1 figure, submitted to Phys. Rev. C; v2 has minor changes including integration over solar volume and addition of mis

Scientific paper

10.1103/PhysRevC.69.015801

The neutrino flux from the sun is predicted to have a CNO-cycle contribution as well as the known pp-chain component. Previously, only the fluxes from beta+ decays of 13N, 15O, and 17F have been calculated in detail. Another neutrino component that has not been widely considered is electron capture on these nuclei. We calculate the number of interactions in several solar neutrino detectors due to neutrinos from electron capture on 13N, 15O, and 17F, within the context of the Standard Solar Model. We also discuss possible non-standard models where the CNO flux is increased.

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