Inflationary Baryogenesis
arXiv:hep-ph/0103348 · doi:10.1103/PhysRevD.64.063511
Abstract
In this letter we explore the possibility of creating the baryon asymmetry of the universe during inflation and reheating due to the decay of a field associated with the inflaton. CP violation is attained by assuming that this field is complex with a phase that varies as the inflaton evolves. We consider chaotic and natural inflation scenarios. In the former case, the complex decaying field is the inflaton itself and, in the latter case, the phase of the complex field is the inflaton. We calculate the asymmetry produced using the Bogolyubov formalism that relates annihilation and creation operators at late time to the annihilation and creation operators at early time.
17 pages, Revtex
References in corpus (2)
Cited by in corpus (14)
- End of inflation, oscillons and matter-antimatter asymmetry
- Quintessential Baryogenesis
- The exact WKB for cosmological particle production
- Leptogenesis from a sneutrino condensate revisited
- Naturalness of the relaxion mechanism
- The Exact WKB and the Landau-Zener transition for asymmetry in cosmological particle production
- Dynamical CP Violation in the Early Universe
- Leptogenesis due to oscillating Higgs field
- Complex Hybrid Inflation and Baryogenesis
- Dilution of dark matter relic density in singlet extension models
- Dynamical CP Violation in the Early Universe and Leptogenesis
- Spontaneous baryogenesis in spiral inflation
- QCD preheating: New frontier of baryogenesis
- Baryon asymmetry from higher-order matter contributions in gravity