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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Format: | Article |
Language: | English |
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SpringerOpen
2022-10-01
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Series: | Journal of High Energy Physics |
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Online Access: | https://doi.org/10.1007/JHEP10(2022)018 |