Right-Handed Neutrino Dark Matter with Forbidden Annihilation
arXiv:2304.02997 · doi:10.1103/PhysRevD.107.123013
Abstract
The seesaw mechanism with three right-handed neutrinos has one as a well-motivated dark matter candidate if stable and the other two can explain baryon asymmetry via the thermal leptogenesis scenario. We explore the possibility of introducing additional particles to make the right-handed neutrino dark matter in thermal equilibrium and freeze out through a forbidden annihilation channel. Nowadays in the Universe, this forbidden channel can be reactivated by a strong gravitational potential such as the supermassive black hole in our galaxy center. The Fermi-LAT gamma ray data and dark matter relic density require this right-handed neutrino dark matter to have mass below GeV and the existence of an additional boson that can be tested at future lepton colliders.
7 pages, 1 figures
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- WIMP Dark Matter from a Natural Discrete Gauge Symmetry in the Standard Model
- On the existence of quaternion-handedness for the spinor solutions of the Dirac and Majorana neutrinos