Electromagnetic Dirac Cogenesis
Preprint
Abstract
We propose a novel cogenesis mechanism by utilising the two-body decay of heavy vector-like fermions to dark matter (DM) $χ$ and right chiral part of light Dirac neutrino $ν_R$ via the electromagnetic dipole operator. This leads to generation of asymmetry in dark fermion $χ$ as well as $ν_R$ with the latter getting transferred to left-handed lepton doublets via Yukawa interactions with a neutrinophilic Higgs doublet. While lepton asymmetry is converted into baryon asymmetry of the Universe via electroweak sphalerons, the dark fermion asymmetry results in asymmetric dark matter. Since CP asymmetries in lepton and dark sector are equal and opposite due to net lepton number conservation, DM mass is restricted to a fixed value $\sim \mathcal{O}(1)$ GeV. Long-lived nature of DM keeps indirect detection prospects at gamma-ray telescopes alive while thermalised light Dirac neutrinos lead to observable dark radiation at cosmic microwave background (CMB) experiments. Heavy vector-like fermions can be probed at terrestrial experiments via their electromagnetic dipole interactions.
Keywords
All Related Versions
This publication has 67 references indexed in Scilit:
- Affleck-Dine cogenesis of baryon and dark matterJournal of High Energy Physics, 2023
- Leptogenesis and dark matter through relativistic bubble walls with observable gravitational wavesJournal of High Energy Physics, 2022
- Baryogenesis via relativistic bubble wallsJournal of High Energy Physics, 2021
- Helicitogenesis: WIMPy baryogenesis with sterile neutrinos and other realizationsJournal of High Energy Physics, 2014
- Constraining light dark matter with diffuse X-ray and gamma-ray observationsJournal of High Energy Physics, 2013
- A WIMPy baryogenesis miracleJournal of High Energy Physics, 2012
- Supersymmetric dark matterPhysics Reports, 1996
- Barygenesis without grand unificationPhysics Letters B, 1986
- Technocosmology — could a technibaryon excess provide a “natural” missing mass candidate?Physics Letters B, 1985
- Baryon number generation in the early universeNuclear Physics B, 1980