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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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It is believed that the running (for instance, COHERENT) and forthcoming terrestrial neutrino experiments will be sensitive to the neutrino charge radius [1] that is one of the neutrino fundamental electromagnetic characteristics [2] predicted [3] to be non-zero even in the Standard Model. In this work we continue our studies [4] on neutrino oscillations in environment with large electric currents accounting for diagonal and non-diagonal neutrino charge radii and anapole moments. We derive neutrino evolution equation in moving matter with electric currents and consider spin and spin-flavor neutrino oscillations. We also study conditions for possible resonances of neutrino oscillations engendered by the neutrino charge radii and compare these conditions with real astrophysical environment. [1] M.Cadeddu, F.Dordei, C.Giunti, K.Kouzakov, E.Picciau, A.Studenikin, Phys.Rev.D 100 (2019) 073014. [2] C.Giunti, A.Studenikin, Rev.Mod.Phys. 87 (2015) 531. [3] J.Bernabeu, L.G.Cabral-Rosetti, J.Papavassiliou, J.Vidal, Phys.Rev.D 62 (2000) 113012. [4] K.Kouzakov, F.Lazarev, V.Shakhov, K.Stankevich, A.Studenikin, PoS ICHEP2020 (2021) 217.