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Neutrino flavor oscillations in a curved space-time

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arxiv 1410.1523 v2 pith:WGEA7YJM submitted 2014-10-05 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords curvedexpressionmetricneutrinospace-timeapplyapproximationblack
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Using a WKB approximation of the Dirac equation in a curved spacetime, we obtain the expression for the phase shift between two neutrino mass eigenstates in a generic gravitational field. We apply this expression to two specific space-time geometries, namely the Kerr-Newman metric describing a rotating and charged black hole, and the Friedmann-Robertson-Walker metric.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Quantum Correlations of Neutrinos in the Kerr-Newman Space-time

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Neutrino quantum correlations in Kerr-Newman spacetime differ from Schwarzschild case, with black hole spin and charge modulating periods and amplitudes for radial and non-radial paths.

  2. Effects of gravitational lensing on neutrino oscillation in Hu-Sawicki f(R) gravity

    hep-ph 2025-06 conditional novelty 4.0 of 10

    Neutrino oscillation probabilities from lensed paths in Hu-Sawicki f(R) gravity are derived, showing sensitivity to λ and to neutrino mass parameters.

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