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Neutrino spin oscillations in gravitational fields

机译:引力场中的中微子自旋振荡

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摘要

We study neutrino spin oscillations in gravitational fields. The quasi-classical approach is used to describe the neutrino spin evolution. First we examine the case of a weak gravitational field. We obtain the effective Hamiltonian for the description of neutrino spin oscillations. We also receive the neutrino transition probability when a particle propagates in the gravitational field of a rotating massive object. Then we apply the general technique to the description of neutrino spin oscillations in the Schwarzschild metric. The neutrino spin evolution equation for the case of the neutrino motion in the vicinity of a black hole is obtained. The effective Hamiltonian and the transition probability are also derived. We examine the neutrino oscillations process on different circular orbits and analyze the frequencies of spin transitions. The validity of the quasi-classical approach is also considered.
机译:我们研究引力场中的中微子自旋振荡。准经典方法用于描述中微子自旋演化。首先,我们研究弱引力场的情况。我们获得了描述中微子自旋振荡的有效哈密顿量。当粒子在旋转的​​大质量物体的引力场中传播时,我们还会收到中微子跃迁概率。然后,我们将通用技术应用于Schwarzschild度量中中微子自旋振荡的描述。得到了黑洞附近中微子运动情况下的中微子自旋演化方程。还推导出有效的哈密顿量和转移概率。我们研究了不同圆形轨道上的中微子振荡过程,并分析了自旋跃迁的频率。还考虑了准经典方法的有效性。

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