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Neutrino Oscillations in Gravitational Field

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arxiv 0906.5556 v2 pith:RA7W2MDN submitted 2009-06-30 hep-ph

classification hep-ph
keywords correctiongravitationalfieldneutrinobhattacharycalculatecalculatedclose
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We calculate the gravitational correction to the phase difference between neutrino mass eigenstates. There is a number of papers, where this correction was calculated for the spherically symmetric gravitational field described by the Schwarzschild metric. The results of these papers differ from each other. Our result is close to that of Bhattachary, Habib and Mottola (see ref. [3,6]) and differs only by a coefficient: our correction is twice smaller.

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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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