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.
In this paper, we propose a physics-based method of prediction high-energy solar flares (SFs) with the help of neutrino detectors utilizing coherent elastic neutrino-nucleus scattering (CEνNS). The behavior of neutrino beams passing through coupled sunspots (CSs) being the sources of future SFs is investigated. We consider the evolution of left-handed electron neutrino νeL and muon neutrino νμL beams formed in the convective zone after the passage of the Micheev – Smirnov – Wolfenstein resonance. It is assumed that the neutrinos possess the charge radius, the magnetic and anapole moments while the CS magnetic field is vortex, nonhomogeneous and has twisting. Estimations of the weakening of the neutrino beams after traversing the resonant layers are given. It is shown that for SFs this weakening could be registered by neutrino detectors of the second generation only when neutrinos have the Dirac nature.
Consideration is being given to the neutrino system governed by the wave function Ψ T = (ν eL , ν XL , ν eL , ν XL ) traveling in the region of the solar flare (SF). Our treatment of the problem holds for any standard model (SM) extensions in which massive neutrinos possess nonzero dipole magnetic and anapole moments. The possible resonance conversions of the electron neutrinos are examined. Since the ν eL → ν XL and ν eL → ν XL -resonances take place in the convective zone, their existence can in no way be connected with the SF. However, when the solar neutrino flux moves through the SF region in the preflare period, then it undergoes the additional resonance conversions resulting in appearance of the ν eL and ν XL neutrinos. On the other hand, according to the hypothesis of the ν e -induced β-decays weakening the electron neutrinos flux leads to the decrease of the β-decay rate for some elements. So, under passage of the electron neutrino flux through the region of the SF, the following four phenomena could be detected: (i) decreasing the number of the electron neutrinos; (ii) appearance of the ν eL neutrinos; (iii) increasing the amount of the ν XL -neutrinos; (iv) reduction of the β-decay rate for some elements of the periodic table.The possible influence of the electron antineutrino flux produced in the superflares on the regime of the hypothetical georeactor is considered.
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