Sub-GeV dark matter as Pseudo-Nambu-Goldstone bosons from the seesaw scale

Michele Frigerio, Thomas Hambye, Eduard Masso

Producció científica: Contribució a una revistaArticleRecercaAvaluat per experts

65 Cites (Scopus)

Resum

Pseudo-Nambu-Goldstone bosons (pNGBs) are naturally light, spin-zero particles that can be interesting dark-matter (DM) candidates. We study the phenomenology of a pNGBΘ associated with an approximate symmetry of the neutrino seesaw sector. A small coupling of Θ 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 Θ proportional to the electroweak scale, and (ii) the observed DM relic density can be generated by the freeze-in of Θ particles with mass m Θ ~ 3 MeV. Alternatively, the coupling of Θ to heavy sterile neutrinos can account for the DM relic density, in the window 1 keV ≤ m Θ ≤ 3 MeV. The decays of Θ into light fermions are suppressed by the seesaw scale, making such pNGBs sufficiently stable to play the role of DM.
Idioma originalEnglish
Número d’article021026
RevistaPhysical Review X
Volum1
Número2
DOIs
Estat de la publicacióPublicada - 1 de des. 2011

Fingerprint

Navegar pels temes de recerca de 'Sub-GeV dark matter as Pseudo-Nambu-Goldstone bosons from the seesaw scale'. Junts formen un fingerprint únic.

Com citar-ho