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Neutrino-antineutrino Asymmetry of C$\nu$B on the Surface of the Round Earth

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arxiv 2401.07347 v2 pith:FPHV4I74 submitted 2024-01-14 hep-ph hep-ex

classification hep-phhep-ex
keywords asymmetryearthmathcalneutrino-antineutrinoroundsurfaceaboveachieve
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

It has been claimed that the coherent scattering of relic neutrinos with the Earth will result in a neutrino-antineutrino asymmetry of $\mathcal{O}(10^{-4})$ on the Earth surface, which is five orders of magnitude larger than the naive model expectation. In this work we show that this overdensity was overestimated for the perfectly round Earth by solving the exact solution with partial waves. The maximal asymmetry after summing over all the angular modes is only around $10^{-8}$ above the ground. To achieve the proposed asymmetry of $\mathcal{O}(10^{-4})$, a special geography may be needed as the experimental site.

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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. Detection prospects for the Cosmic Neutrino Background using matter interferometers

    hep-ph 2025-11 conditional novelty 6.0 of 10

    The Cosmic Neutrino Background is predicted to induce phase shifts of ~1e-22 to 1e-14 rad in matter interferometers, far below current and near-future sensitivity.

  2. Probing Terrestrial Relic Neutrino Charge with Mach-Zehnder Interferometer

    hep-ph 2025-06 reject novelty 5.0 of 10

    A Mach-Zehnder interferometer with one vertical arm is proposed to probe relic neutrino charge, with claimed sensitivity down to epsilon_nu ~ 10^-22, but the signal calculation is flawed.

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