Pith. sign in

REVIEW 2 cited by

Neutrino-antineutrino Asymmetry of CνB on the Surface of the Round Earth

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

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

Neutrino-antineutrino Asymmetry of CνB on the Surface of the Round Earth

classification hep-ph hep-ex
keywords asymmetryearthmathcalneutrino-antineutrinoroundsurfaceaboveachieve
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original 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.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Background-Induced Forces from Quadratically Coupled Ultralight Dark Matter

    hep-ph 2026-06 unverdicted novelty 7.0

    Earth screening of quadratically coupled ultralight dark matter produces a multi-band frequency structure in the induced force whose sideband amplitudes vary annually, enabling improved constraints from MICROSCOPE and...

  2. Detection prospects for the Cosmic Neutrino Background using matter interferometers

    hep-ph 2025-11 conditional novelty 6.0

    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.