2017/11/25 by O. M. Boyarkin, Boyarkin, O. M., Iren Boyarkina +2
Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #Geophysics and Gravity Measurements #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Solar and Space Plasma Dynamics #hep-ph
paper · pdf · doi:10.48550/arxiv.1711.09247
11 pages. arXiv admin note: text overlap with arXiv:hep-ph/0401221 by other authors
openalex publication_date 2017/11/25 · arxiv created 2017/12/03 · arxiv updated 2017/12/06 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The evolution of the solar neutrino flux which is described by the wave function ΨT=(νeL,νXL, νeL, νXL) is examined. Our treatment of the problem holds for any standard model (SM) extensions possessing nonzero dipole magnetic and anapole moments. When the solar neutrino flux moves through the solar flare (SF) region in the preflare period, then it undergoes the additional (compared with the SM) resonance conversions. As a result, the weakening the electron neutrinos flux takes place. On the other hand, existence of the additional resonances lead to appearance of the νeL and νXL neutrinos that could be detected by the terrestrial detectors. The hypothesis of the νe-induced β-decays is also discussed. According to it, before the large SF, decreasing the β-decay rate for some elements takes place. The possible influence of the electron antineutrino flux produced in the superflares on the regime of the hypothetical georeactor is considered.