Unitarity at Infinity and Topological Holography

dc.creatorMcInnes, Brett
dc.date2006-06-08
dc.date2006-06-16
dc.date.accessioned2026-07-07T10:42:24Z
dc.date.available2026-07-07T10:42:24Z
dc.descriptionRecently it has been suggested that non-gaussian inflationary perturbations can be usefully analysed in terms of a putative dual gauge theory defined on the future conformal infinity generated by an accelerating cosmology. The problem is that unitarity of this gauge theory implies a strong constraint [the "Strominger bound"] on the matter fields in the bulk. We argue that the bound is just a reflection of the equation of state of cosmological matter. The details motivate a discussion of the possible relevance of the ``dS/CFT correspondence" to the resolution of the Big Bang singularity. It is argued that the correspondence may require the Universe to come into existence along a non-singular spacelike hypersurface, as in the theories of ``creation from nothing" discussed by Firouzjahi, Sarangi, and Tye, and also by Ooguri et al. The argument makes use of the unusual properties of gauge theories defined on topologically non-trivial spaces.
dc.description18 pages including 2 eps files
dc.identifierhttps://arxiv.org/abs/hep-th/0606068
dc.identifierhttp://arxiv.org/abs/hep-th/0606068
dc.identifierNucl.Phys.B754:91-106,2006
dc.identifierdoi:10.1016/j.nuclphysb.2006.07.016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181933
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleUnitarity at Infinity and Topological Holography
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