Stringy Model of Cosmological Dark Energy

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dc.creatorAref'eva, Irina Ya.
dc.date2007-10-16
dc.date.accessioned2026-07-07T10:57:39Z
dc.date.available2026-07-07T10:57:39Z
dc.descriptionA string field theory(SFT) nonlocal model of the cosmological dark energy providing w<-1 is briefly surveyed. We summarize recent developments and open problems, as well as point out some theoretical issues related with others applications of the SFT nonlocal models in cosmology, in particular, in inflation and cosmological singularity.
dc.descriptionTalk at PASCOS 2007, to appear in the proceedings, 5 pages, latex
dc.identifierhttps://arxiv.org/abs/0710.3017
dc.identifierhttp://arxiv.org/abs/0710.3017
dc.identifierAIPConf.Proc.957:297-300,2007
dc.identifierdoi:10.1063/1.2823785
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186826
dc.subjectHigh Energy Physics - Theory
dc.titleStringy Model of Cosmological Dark Energy
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