The fluxes of CN neutrinos from the Sun in case of mixing in a spherical layer in the solar core

TL;DR

This paper calculates how mixing in a spherical layer of the solar core affects CN neutrino fluxes, showing a significant increase in $^{13}N$ neutrinos and discussing experimental implications.

Contribution

It introduces a model of mixing in the solar core that aligns with seismic and neutrino data, predicting increased $^{13}N$ neutrino fluxes.

Findings

Significant increase in $^{13}N$ neutrino flux due to core mixing.

Model consistent with seismic and solar neutrino measurements.

Implications for future neutrino detection experiments.

Abstract

The results of the calculation are presented for the fluxes of CN neutrinos from the Sun in case of mixing in a spherical layer in the solar core, consistent with the seismic data and with the measured solar neutrino fluxes. It is shown that a substantial increase of the flux of $^{13}N$ neutrinos can be gained in this case. The possible implications for experiment are discussed.