Generating the Baryon Asymmetry of the Universe in Split Fermion Models
arXiv:hep-ph/0511244 · doi:10.1103/PhysRevD.73.103517
Abstract
The origin of the matter-antimatter asymmetry of the universe is one of the major unsolved problems in cosmology and particle physics. In this paper, we investigate the recently proposed possibility that split fermion models -- extra dimensional models where the standard model fermions are localized to different points around the extra dimension -- could provide a means to generate this asymmetry during the phase transition of the localizing scalars. After setting up the scenario that we consider, we use a single fermion toy model to estimate the reflection coefficients for scattering off the phase boundary using a more realistic scalar profile than previous work resulting in a different Kaluza Klein spectrum. The value we calculate for is consistent with the mechanism being the source of the baryon asymmetry of our universe provided the violating processes have an efficiency of order .
17 pages, 3 figures; References added; Minor changes, Accepted for publication in Phys. Rev. D
References in corpus (8)
- Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)
- Flavor Constraints on Split Fermion Models
- Twisted Split Fermions
- Neutrino Mass Patterns within the See-saw Model from Multi-localization along Extra Dimensions
- Kaluza-Klein Structure Associated With Fat Brane
- Low-energy effective theory from a non-trivial scalar background in extra dimensions
- Split Fermions Baryogenesis from the Kobayashi-Maskawa Phase
- Leptogenesis from Split Fermions