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Gravitational Effects on the Neutrino Oscillation

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arxiv hep-ph/9611231 v2 pith:EJW3TTBM submitted 1996-11-05 hep-ph gr-qc

N. Fornengo , C. Giunti , C.W. Kim , J. Song (The Johns Hopkins University , USA , INFN , Sezione di Torino , Italy) This is my paper · ORCID
classification hep-phgr-qc
keywords gravitationalpropagationeffectsfieldneutrinoneutrinososcillationapplication
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The propagation of neutrinos in a gravitational field is studied. A method of calculating a covariant quantum-mechanical phase in a curved space-time is presented. The result is used to calculate gravitational effects on the neutrino oscillation in the presence of a gravitational field. We restrict our discussion to the case of the Schwartzschild metric. Specifically, the cases of the radial propagation and the non-radial propagation are considered. A possible application to gravitational lensing of neutrinos is also suggested.

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Cited by 3 Pith papers

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

  1. Neutrino Constraints on Scalar-Tensor Gravity

    hep-ph 2025-12 conditional novelty 6.0 of 10

    Spatially varying scalar fields rescale neutrino masses and arrival times, and neutrino data bound these rescaling parameters for Symmetron and Chameleon models.

  2. 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.

  3. 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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