An upper bound on the number of e-foldings
classification
🌌 astro-ph
gr-qchep-phhep-th
keywords
cosmologicale-foldingsnumberuniverseaccelerationasymptoticallyboundbounded
read the original abstract
If the present acceleration of the universe is due to an asymptotically de Sitter universe with small cosmological constant, and the principle of Cosmological Complementarity is valid, then the number of e-foldings during inflation is bounded.
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