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

TL;DR

This paper analyzes the non-stationary solar model with mixing, focusing on how it affects neutrino fluxes, particularly the flux from $^{13}N$ decay, which exceeds standard model predictions.

Contribution

It introduces a computational approach to model non-stationary solar conditions with mixing, highlighting its impact on neutrino flux predictions.

Findings

Neutrino flux $F_{13}$ exceeds standard model predictions in the non-stationary case.

Mixing in the solar model significantly alters neutrino fluxes.

The model provides insights into solar neutrino observations.

Abstract

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