Affleck-Dine Baryogenesis, Split Supersymmetry, and Inflation
arXiv:0802.1328 · doi:10.1103/PhysRevD.80.063519
Abstract
It is shown that, in the context of split supersymmetry, a simple model with a single complex scalar field can produce chaotic inflation and generate the observed amount of baryon asymmetry via the Affleck-Dine mechanism. While the inflaton quantum fluctuations give rise to curvature perturbation, we show that quantum fluctuations of the phase of the scalar field can produce baryonic isocurvature perturbation. Combining with constraints from WMAP data, all parameters in the model can be determined to within a narrow range.
version accepted for publication in PRD
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Cited by in corpus (21)
- Generating the Observed Baryon Asymmetry from the Inflaton Field
- Baryogenesis from the Inflaton Field
- Increasing Temperature toward the Completion of Reheating
- Affleck-Dine inflation
- Affleck-Dine Leptogenesis from Higgs Inflation
- Type II Seesaw Leptogenesis
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