Inertial Effects on Berry's Phase of Neutrino Oscillations
arXiv:gr-qc/0003086 · doi:10.1007/s100520050011
Abstract
The Berry phase of mixed states, as neutrino oscillations, is calculated in a accelerating and rotating reference frame. It turns out to be depending on the vacuum mixing angle, the mass--squared difference and on the coupling between the momentum of the neutrino and the spinorial connection. Berry's phase for solar neutrinos and its geometrical aspects are also discussed.
11 pages, LaTex file, 1 table, to appear in Europ. Phys. J. C
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