Generating the baryon asymmetry of the universe in split fermion models
Creators
- 1. School of Physics, Research Centre for High Energy Physics, University of Melbourne, Victoria 3010 (Australia)
Description
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 nB/s is consistent with the mechanism being the source of the baryon asymmetry of our universe provided the B-L violating processes have an efficiency of order 10-5
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.73.103517;
- arXiv
- arXiv:hep-ph/0511244v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 73
- Journal Issue
- 10
- Journal Page Range
- p. 103517-103517.10
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37078252
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANTIMATTER; ASYMMETRY; BARYONS; COSMOLOGY; EFFICIENCY; KALUZA-KLEIN THEORY; PHASE TRANSFORMATIONS; SCALARS; STANDARD MODEL; UNIVERSE
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; HADRONS; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; QUANTUM FIELD THEORY; UNIFIED GAUGE MODELS; UNIFIED-FIELD THEORIES
Optional Information
- Notes
- (c) 2006 The American Physical Society