Sub-GeV dark matter as pseudo-Goldstone from the seesaw scale
Michele Frigerio, Thomas Hambye, Eduard Masso

TL;DR
This paper explores a pseudo-Goldstone boson from the neutrino seesaw sector as a sub-GeV dark matter candidate, generated via Higgs portal interactions or sterile neutrino couplings, with relic density achieved through freeze-in.
Contribution
It introduces a novel dark matter candidate arising from an approximate symmetry in the neutrino seesaw sector, with detailed phenomenology and relic density mechanisms.
Findings
pNGB mass around 3 MeV from Higgs portal
Relic density achievable via freeze-in mechanisms
Decay rates suppressed, ensuring dark matter stability
Abstract
Pseudo Nambu-Goldstone bosons (pNGBs) are naturally light spin-zero particles, which can be interesting dark matter (DM) candidates. We study the phenomenology of a pNGB theta associated with an approximate symmetry of the neutrino seesaw sector. A small coupling of theta to the Higgs boson is induced radiatively by the neutrino Yukawa couplings. By virtue of this Higgs portal interaction (i) the pNGB acquires a mass m_theta proportional to the electroweak scale, and (ii) the observed DM relic density can be generated by the freeze-in of theta-particles with mass m_theta ~ 3 MeV. Alternatively, the coupling of theta to heavy sterile neutrinos can account for the DM relic density, in the 1 keV-3 MeV window. The decays of theta into light fermions are suppressed by the seesaw scale, making such pNGB sufficiently stable to play the role of DM.
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