The Holographic Approach to Cosmology

Simple item page
dc.creatorBanks, T.
dc.creatorFischler, W.
dc.date2004-12-09
dc.date.accessioned2026-07-07T04:17:49Z
dc.date.available2026-07-07T04:17:49Z
dc.descriptionWe review the successes and challenges of the holographic approach to cosmology. The model predicts an exactly scale invariant fluctuation spectrum with long and short distance cut-offs. It can account for the observed fluctuations in the CMB and might explain the low power at large scales. We outline various cosmological histories compatible with holographic initial conditions. This paper is based on talks given by the authors at Cosmo 04 in Toronto, and the 2004 Tamura Symposium in Austin
dc.description9 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0412097
dc.identifierhttp://arxiv.org/abs/hep-th/0412097
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/52921
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Holographic Approach to Cosmology
dc.typetext

Files

Collections

arXiv