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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

Gravitational Effects on the Neutrino Oscillation

N. Fornengo , C. Giunti , C.W. Kim , J. Song (The Johns Hopkins University , USA , INFN , Sezione di Torino , Italy) This is my paper
classification hep-ph gr-qc
keywords gravitationalpropagationeffectsfieldneutrinoneutrinososcillationapplication
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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

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  1. Neutrino Constraints on Scalar-Tensor Gravity

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    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

    Kerr-Newman parameters M, a, and Q modulate neutrino survival probabilities, entanglement, and coherence differently from the Schwarzschild case, with spin lengthening and charge shortening oscillation periods in outw...

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

    gr-qc 2026-05 unverdicted novelty 5.0

    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.