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Probing the Local Dark Matter Halo with Neutrino Oscillations

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arxiv 2305.06441 v2 pith:KWACQDZM submitted 2023-05-10 hep-ph hep-th

classification hep-phhep-th
keywords halodarkearthmatterneutrinooscillationsdependinginterior
verification ladder T0 review T1 audit T2 compute T3 formal

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Dark matter particles can form halos gravitationally bound to massive astrophysical objects. The Earth could have such a halo where depending on the particle mass, the halo either extends beyond the surface or is confined to the Earth's interior. We consider the possibility that if dark matter particles are coupled to neutrinos, then neutrino oscillations can be used to probe the Earth's dark matter halo. In particular, atmospheric neutrinos traversing the Earth can be sensitive to a small size, interior halo, inaccessible by other means. Depending on the halo mass and neutrino energy, constraints on the dark matter-neutrino couplings are obtained from the halo corrections to the neutrino oscillations.

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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. Oscillating Neutrinos vs. Oscillating Scalars: Constraining Scalar Dark Matter-Induced Neutrino Mass

    hep-ph 2026-08 conditional novelty 6.0 of 10

    Using T2K, RENO and JUNO data, a virialised ultralight scalar dark matter background can provide at most about 9% to 54% of neutrino masses for scalar masses between 2x10^-21 and 3x10^-8 eV.

  2. Probing the quantum speed limit and entanglement in flavor oscillations of neutrino-antineutrino system in curved spacetime

    gr-qc 2025-04 reject novelty 5.0 of 10

    Gravity-induced neutrino-antineutrino oscillations near a rotating primordial black hole are computed in Kerr-Schild polar coordinates, with quantum speed limit and entanglement entropy estimated.

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