Interplay of neutrino spin and three-flavour oscillations in a magnetic field

A. Popov, A. Lichkunov, A. Studenikin
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Abstract

We develop the approach to the problem of neutrino oscillations in a magnetic field introduced in [1] and extend it to the case of three neutrino generations. The theoretical framework suitable for computation of the Dirac neutrino spin, flavour and spin-flavour oscillations probabilities in a magnetic field is given. The closed analytic expressions for the probabilities of oscillations are obtained accounting for the normal and inverted hierarchies and the possible effect of CP violation. In general, the neutrino oscillation probabilities exhibit quite a complicated interplay of oscillations on the magnetic ωB = μνB and vacuum ωvac = Δm2 ik 4p frequencies. The obtained results are of interest in applications to neutrino oscillations under the influence of extreme astrophysical environments, for example peculiar to magnetars and supernovas, as well as in studying neutrino propagation in interstellar magnetic fields (see [2]).
磁场中中微子自旋和三味振荡的相互作用
我们发展了在[1]中引入的磁场中中微子振荡问题的方法,并将其扩展到三代中微子的情况。给出了适用于计算磁场中狄拉克中微子自旋、风味和自旋风味振荡概率的理论框架。得到了考虑正、倒层次和CP违和可能影响的振荡概率的封闭解析表达式。一般来说,中微子振荡概率在磁ωB = μνB和真空ωvac = Δm2 ik 4p频率上表现出相当复杂的振荡相互作用。所获得的结果对于在极端天体物理环境(例如磁星和超新星特有的环境)影响下的中微子振荡应用以及研究中微子在星际磁场中的传播具有重要意义(见[2])。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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