Ultraviolet freeze-in baryogenesis
arXiv:2204.13554 · doi:10.1103/PhysRevD.106.023515
Abstract
We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath particles which are responsible for the production of feebly-interacting dark matter. The same processes violate , which further leads to an asymmetry between matter and antimatter being generated in the visible sector. We focus on the possibility that these interactions are described through non-renormalizable operators, which leads to both dark matter and the baryon asymmetry being produced at high temperatures. The mechanism is exemplified by studying two concrete scenarios, one involving scalar and one involving fermion dark matter. We find that in both cases it is, indeed, possible to achieve a common explanation for the dark matter content and the matter-antimatter asymmetry of the Universe, provided that dark matter is in the keV mass range.
26 pages, 8 figures, v2: Matches the published version
References in corpus (12)
- Leptogenesis
- The Sphaleron Rate in the Minimal Standard Model
- Enhancement of the Dark Matter Abundance Before Reheating: Applications to Gravitino Dark Matter
- How warm are non-thermal relics? Lyman- bounds on out-of-equilibrium dark matter
- The Minimal Phantom Sector of the Standard Model: Higgs Phenomenology and Dirac Leptogenesis
- Particle-antiparticle asymmetries from annihilations
- The role of CP violating scatterings in baryogenesis - case study of the neutron portal
- Towards Cogenesis via Asymmetric Freeze-in: The Who Came-in from the Cold
- Baryogenesis and Dark Matter from Freeze-In
- Mechanism for baryogenesis via feebly interacting massive particles
- Dark Freeze-out Cogenesis
- Freeze-in Leptogenesis via Dark-Matter Oscillations