An upper bound on the number of e-foldings

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dc.creatorBanks, T.
dc.creatorFischler, W.
dc.date2003-07-26
dc.date2004-03-07
dc.date.accessioned2026-07-07T02:09:04Z
dc.date.available2026-07-07T02:09:04Z
dc.descriptionIf 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.
dc.description16 pages, latex. New version has extensive modifications to clarify the basic assumptions on which the bound is based and can be viewed as a response to the paper of Lowe and Marolf, correction of typos and added references
dc.identifierhttps://arxiv.org/abs/astro-ph/0307459
dc.identifierhttp://arxiv.org/abs/astro-ph/0307459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6295
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleAn upper bound on the number of e-foldings
dc.typetext

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