Asymptotic scalar field cosmology in string theory

Abstract Asymptotic (late-time) cosmology depends on the asymptotic (infinite-distance) limits of scalar field space in string theory. Such limits feature an exponentially decaying potential V ~ exp(−cϕ) with corresponding Hubble scale H ~ ϕ ̇ 2 + 2 V $$ \sqrt{{\dot{\phi}}^2+2V} $$ ~ exp(−λ Hϕ ), an...

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Bibliographic Details
Main Author: Tom Rudelius
Format: Article
Language:English
Published: SpringerOpen 2022-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP10(2022)018