On Preserving a B+L Asymmetry Produced in the Early Universe
arXiv:hep-ph/9403259 · doi:10.1016/0370-2693(94)91490-7
Abstract
One of the most efficient mechanisms for producing the baryon asymmetry of the Universe is the decay of scalar condensates in a SUSY GUT as was first suggested by Affleck and Dine. We show that given a large enough asymmetry, the baryon number will be preserved down to low temperatures even if B - L = 0, because the baryon number carrying scalars form bose condensates that give the W a mass. We derive the conditions on the condensate needed to suppress electroweak sphaleron interactions which would otherwise drive the baryon asymmetry to zero when B - L = 0.
10 pages, LaTeX, UMN-TH-1240, CfPA-TH-94-13, LBL-35275
References in corpus (7)
- Progress in Electroweak Baryogenesis
- Nucleon Decay in the Minimal Supersymmetric Grand Unification
- Sphaleron Erasure of Primordial Baryogenesis
- On the Baryon, Lepton-Flavour and Right-Handed Electron Asymmetries of the Universe
- Leptogenesis in Supersymmetric Standard Model with Right-handed Neutrino
- Inflation, Neutrino Baryogenesis, and (S)Neutrino-Induced Baryogenesis
- On the Erasure and Regeneration of the Primordial Baryon Asymmetry by Sphalerons
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- The Cold Big-Bang Cosmology as a Counter-example to Several Anthropic Arguments
- Generation of cosmological large lepton asymmetry from a rolling scalar field
- Large Lepton Asymmetry for Small Baryon Asymmetry and Warm Dark Matter
- On large lepton number asymmetries of the Universe
- Cosmological Moduli Problem in a Supersymmetric Model with Direct Gauge Mediation
- TeV Right-handed Neutrinos and the Flavor-symmetry-improved Seesaw Mechanism
- Constraints on Baryogenesis from the Decay of Superstring Axions