Journal
PHYSICAL REVIEW D
Volume 102, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.102.043511
Keywords
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Funding
- JSPS KAKENHI [JP17H01131]
- MEXT [JP15H05889, JP18H04594, JP19H05114]
- Ministry of Science and Technology (MOST) of Taiwan [MOST 109-2112-M-167-001]
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In this paper, we investigate the parameter space in the framework of hilltop supernatural inflation in which the inflaton field can play the role of Affleck-Dine field to produce successful baryogenesis. The suitable value of reheating temperature could coincide with the reheating temperature required to produce lightest supersymmetric particle dark matter. The baryon isocurvature perturbation is shown to be negligible. We consider p = 3, p = 4, and p = 6 type III hilltop inflation and discuss how to connect the models to supersymmetric theories.
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