Neutrino oscillations in the Ellis wormhole spacetime
Neutrino oscillations in the Ellis wormhole spacetime
Gravitational lensing is a powerful tool to probe compact astrophysical objects and the distribution of dark matter at large scales. As a counterpart of photons, lensed relativistic neutrinos could also be used to explore properties of curved spacetimes. In the present paper we consider neutrino oscillations in the Ellis wormhole (WH) spacetime in comparison with the widely discussed black hole (BH) spacetimes. We investigate the oscillations involving lensing effects with 2- and 3-flavor neutrinos under the weak-field approximation. In the two-flavor model, the flavor oscillation probabilities display the impacts of the throat radius, neutrino mass hierarchy, and the lightest neutrino mass. In the realistic 3-flavor case, the similar observations are obtained with the up-to-date global fit data of neutrino experiments. The influence of the Ellis WH on the coherence of neutrinos is also studied in the paper. In general, the observations from neutrino oscillations cannot be used to discriminate Ellis WH spacetimes from typical BH spacetimes under the weak-field limit.
Ya-Ru Wang、Shu-Jun Rong
物理学
Ya-Ru Wang,Shu-Jun Rong.Neutrino oscillations in the Ellis wormhole spacetime[EB/OL].(2025-06-30)[2025-07-16].https://arxiv.org/abs/2506.23905.点此复制
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