Neutrino Oscillations Induced by Space-Time Torsion
arXiv:gr-qc/0103046 · doi:10.1088/0264-9381/18/8/307
Abstract
The gravitational neutrino oscillation problem is studied by considering the Dirac Hamiltonian in a Riemann-Cartan space-time and calculating the dynamical phase. Torsion contributions which depend on the spin direction of the mass eigenstates are found. These effects are of the order of Planck scales.
18 pages,LATEX, no figures. To appear in Class.Q.Grav
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