The Holographic Principle and the Early Universe

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dc.creatorCanfora, F.
dc.creatorVilasi, G.
dc.date2005-05-18
dc.date2005-08-27
dc.date.accessioned2026-07-07T06:19:04Z
dc.date.available2026-07-07T06:19:04Z
dc.descriptionA scenario is proposed in which the matter-antimatter asymmetry behaves like a seed for the inflationary phase of the universe. The mechanism which makes this scenario plausible is the holographic principle: this scheme is supported by a good prediction of the number of e-folds. It seems that such a mechanism can only work in the presence of a Hagedorn-like phase transition. The issue of the "graceful exit" can also be naturally accounted for.
dc.descriptionRevised version to be pubblished on Physics Letters B: a reference, which provides the results of the paper with further supports, has been added; typos have been corrected; 11 pages no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0505091
dc.identifierhttp://arxiv.org/abs/gr-qc/0505091
dc.identifierPhys.Lett. B625 (2005) 171-176
dc.identifierdoi:10.1016/j.physletb.2005.08.079
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/94948
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleThe Holographic Principle and the Early Universe
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