English

Lepton parity dark matter and naturally unstable domain walls

High Energy Physics - Phenomenology 2026-05-11 v2 Cosmology and Nongalactic Astrophysics

Abstract

We propose a simple and predictive setup that connects neutrino masses, dark matter (DM), and gravitational waves. A minimal lepton parity DM scenario is considered where the residual symmetry (1)L(-1)^L from the type I seesaw acts as the dark parity D=(1)L+2jD=(-1)^{L+2j}, ensuring DM stability without imposing any new symmetry. A singlet Majorana fermion SS with even lepton parity serves as the DM candidate, interacting via a real scalar σ\sigma which is also even lepton parity. The scalar potential possesses an accidental Z2\mathcal{Z}_2 symmetry, whose spontaneous breaking gives rise to unstable domain walls (DW) in the presence of explicit Z2\mathcal{Z}_2 breaking terms allowed by the lepton parity. The subsequent DW annihilation generates a stochastic gravitational wave (GW) background potentially observable at different GW experiments.

Keywords

Cite

@article{arxiv.2508.02642,
  title  = {Lepton parity dark matter and naturally unstable domain walls},
  author = {Ernest Ma and Partha Kumar Paul and Narendra Sahu},
  journal= {arXiv preprint arXiv:2508.02642},
  year   = {2026}
}

Comments

v2: 5+5 pages, 2+4 captioned figures, 1+2 tables, version accepted for publication in Phys. Rev. D