English

Gravity-assisted neutrino masses

High Energy Physics - Phenomenology 2025-12-19 v1

Abstract

Gravity is generally expected to violate global symmetries, including lepton number. However, neutrino masses from the Planck-suppressed Weinberg operator are typically too small to account for oscillation data. We propose a new model-building approach to low-scale neutrino mass generation, in which an intermediate spontaneous symmetry-breaking scale generates masses and mixings in the heavy neutral lepton (HNL) sector, while leaving an unbroken residual symmetry GresG_{\mathrm{res}} that forbids light-neutrino masses. The observed light-neutrino masses then arise because gravity breaks GresG_{\mathrm{res}} via Planck-suppressed operators, inducing the small lepton-number violation required in low-scale seesaw constructions. The HNLs form pseudo-Dirac pairs, with masses potentially within reach of future colliders and complementary tests in precision searches such as charged lepton flavour violation (cLFV). As an illustration, we present a representative realisation of this class of models and show that, for O(1)\mathcal{O}(1) operator coefficients, it predicts a region in the (MRM_R, Θ2\Theta^2)-plane that can be testable via displaced-vertex searches at the High-Luminosity (HL) LHC and the FCC-ee.

Keywords

Cite

@article{arxiv.2512.16862,
  title  = {Gravity-assisted neutrino masses},
  author = {Stefan Antusch and Salvador Centelles Chuliá and Miguel Levy},
  journal= {arXiv preprint arXiv:2512.16862},
  year   = {2025}
}

Comments

5 pages, 1 figure, 1 table

R2 v1 2026-07-01T08:32:03.963Z