English

Minimal Majoron Dark Matter

High Energy Physics - Phenomenology 2026-05-14 v1 Cosmology and Nongalactic Astrophysics

Abstract

We study Majoron dark matter (DM) in its minimal realization, based on the Type-I seesaw framework extended by a SM-singlet complex scalar. Remaining agnostic about the origin and value of the Majoron mass, we evaluate the DM abundance from both the freeze-in and misalignment mechanisms, and identify the viable parameter space consistent with observational constraints. Without fine-tuning of the initial misalignment angle, we find that the Majoron mass is bounded by mJO(10) MeVm_J \lesssim \mathcal{O}(10)~\mathrm{MeV}. We also discuss compatibility with thermal leptogenesis. Successful leptogenesis with two right-handed neutrinos favors misalignment-dominated production with the Majoron mass mJO(100) eVm_J \lesssim \mathcal{O}(100)~\mathrm{eV}, while freeze-in dominated production is compatible with leptogenesis only with a mild fine-tuning of the initial misalignment angle, θiO(0.01)\theta_i \lesssim \mathcal{O}(0.01).

Keywords

Cite

@article{arxiv.2605.12946,
  title  = {Minimal Majoron Dark Matter},
  author = {Kensuke Akita and Koichi Hamaguchi and Haruto Kitagawa and Tatsuya Yokoyama},
  journal= {arXiv preprint arXiv:2605.12946},
  year   = {2026}
}

Comments

18 pages, 7 figures