String Cosmology: Concepts and Consequences

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dc.creatorVeneziano, G.
dc.date1995-12-13
dc.date.accessioned2026-07-07T04:21:44Z
dc.date.available2026-07-07T04:21:44Z
dc.descriptionAfter recalling a few basic concepts from cosmology and string theory, I will discuss the main ideas/assumptions underlying string cosmology and show how these lead to a two-parameter family of ``minimal" models. I will then explain how to compute, in terms of those parameters, the spectrum of scalar, tensor and electromagnetic perturbations, point at their ($T$ and $S$-type) duality symmetries, and mention their most relevant physical consequences.
dc.description21p, latex, epsf, 3 figures in uuencoded file
dc.identifierhttps://arxiv.org/abs/hep-th/9512091
dc.identifierhttp://arxiv.org/abs/hep-th/9512091
dc.identifierHelv.Phys.Acta 69 (1996) 553-569
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54443
dc.subjectHigh Energy Physics - Theory
dc.titleString Cosmology: Concepts and Consequences
dc.typetext

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