English

Freeze-In Dark Matter and Leptogenesis: a $\psi'$SM route

High Energy Physics - Phenomenology 2026-04-10 v3 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

We investigate the possibility of \emph{freeze-in} dark matter production and baryogenesis via leptogenesis in a ψ\psi'SM model, which is an E6E_6 extension of the Standard Model, featuring a residual U(1)ψU(1)_{\psi'} gauge symmetry. This symmetry arises from a linear combination of U(1)χU(1)_\chi and U(1)ψU(1)_{\psi}, both of which are subgroups of the E6E_6. The spontaneous breaking of U(1)ψU(1)_{\psi'} symmetry governs the dynamics of a singlet fermion, which serves as a freeze-in dark matter candidate. The dark matter mass arises from dimension-five operators, and a discrete symmetry ensures its stability. We show that freeze-in production from scalar decay can yield the correct relic abundance for dark matter masses between a few MeV to a few hundred GeV. Simultaneously, heavy right-handed neutrinos generate light neutrino masses via the type-I seesaw and produce the observed baryon asymmetry via leptogenesis.

Keywords

Cite

@article{arxiv.2507.01895,
  title  = {Freeze-In Dark Matter and Leptogenesis: a $\psi'$SM route},
  author = {Adeela Afzal and Rishav Roshan},
  journal= {arXiv preprint arXiv:2507.01895},
  year   = {2026}
}

Comments

Accepted for publication in EPJC