Lepton parity dark matter and naturally unstable domain walls
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 from the type I seesaw acts as the dark parity , ensuring DM stability without imposing any new symmetry. A singlet Majorana fermion with even lepton parity serves as the DM candidate, interacting via a real scalar which is also even lepton parity. The scalar potential possesses an accidental symmetry, whose spontaneous breaking gives rise to unstable domain walls (DW) in the presence of explicit breaking terms allowed by the lepton parity. The subsequent DW annihilation generates a stochastic gravitational wave (GW) background potentially observable at different GW experiments.
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