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• W3100956032 abstract "The Planck data on cosmic microwave background indicates that the Starobinsky-type model with concave inflation potential is favored over the convex-type chaotic inflation. Is there any reason for that? Here we argue that if our universe began with a Euclidean wormhole, then the Starobinsky-type inflation is probabilistically favored. It is known that for a more generic choice of parameters than that originally assumed by Hartle and Hawking, the Hartle-Hawking wave function is dominated by Euclidean wormholes, which can be interpreted as the creation of two classical universes from nothing. We show that only one end of the wormhole can be classicalized for a convex potential, while both ends can be classicalized for a concave potential. The latter is therefore more probable." @default.
• W3100956032 created "2020-11-23" @default.
• W3100956032 creator A5009067151 @default.
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• W3100956032 date "2018-10-01" @default.
• W3100956032 modified "2023-10-17" @default.
• W3100956032 title "Why concave rather than convex inflaton potential?" @default.
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• W3100956032 doi "https://doi.org/10.1140/epjc/s10052-018-6357-0" @default.
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