Neutrino oscillations in vortex and twisting magnetic fields

Abstract

The behavior of the neutrino flux in vortex and twisting magnetic fields is considered within the left-right symmetric model. By way of illustration of the magnetic fields we discuss the magnetic fields of the coupled sunspots (CS's) which are the sources of the future solar flares. It is expected that the neutrinos have such multipole moments as the charge radius, the magnetic and anapole moments. The evolution equation in the Schrodinger-like form is found and all magnetic-induced resonance conversions are analyzed. It is demonstrated that in the case of the super flares one may detect the depletion of the ν eL neutrinos caused by their resonance absorptions when they travel through the CS magnetic fields. Observations of this phenomena could be carried out at neutrino telescopes of the next generation whose work is based on the reaction of the coherent elastic neutrino-nucleus scattering.

Prediction of solar flares using neutrino detectors of the second generation

“…The aim of our work is to investigate the possibility of forecasting the high energy SF with the help of the neutrino detectors utilizing the CEνNS. The work represents continuation of the papers [16,17,18,19] in which the correlation between the SF and behavior of the electron neutrino beam in the CS magnetic field during the initial stage of the SF was discussed. In contrast to the previous works, we take into account all the neutrino multipole moments and carry out the analysis for the Dirac and Majorana neutrinos.…”