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Gravitationally Induced Neutrino-Oscillation Phases

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arxiv gr-qc/9603008 v6 pith:IY72U4AW submitted 1996-03-08 gr-qc astro-phhep-phquant-ph

D. V. Ahluwalia , C. Burgard This is my paper · ORCID
classification gr-qcastro-phhep-phquant-ph
keywords phasesgravitationallyinducedquantumeffectmechanicalneutrino-oscillationarise
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In this essay, we introduce a new effect of gravitationally induced quantum mechanical phases in neutrino oscillations. These phases arise from an hitherto unexplored interplay of gravitation and the principle of the linear superposition of quantum mechanics. In the neighborhood of a 1.4 solar-mass neutron star, gravitationally induced quantum mechanical phases are roughly 20% of their kinematical counterparts. When this information is coupled with the mass square differences implied by the existing neutrino-oscillation data we find that the new effect may have profound consequences for type-II supernova evolution.

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  1. 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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