"Phantom" Inflation in Warped Compactification

dc.creatorPiao, Yun-Song
dc.date2007-12-20
dc.date2008-09-04
dc.date.accessioned2026-07-07T10:16:06Z
dc.date.available2026-07-07T10:16:06Z
dc.descriptionIn this paper, in a class of warped compactifications with the brane/flux annihilation, we find that the inflation may be driven by a flat direction identified as that along the number p of anti D3-branes located at the tip of the Klebanov-Strassler throat. The spectrum of adiabatic perturbation generated during inflation is nearly scale invariant, which may be obtained by using the results shown in the phantom inflation, since in a four-dimension effective description the evolution of energy density along the $p$ direction is slowly increasing.
dc.description5 pages, 2 figures, some arguments on the reliability of our resulits added, ref. added, to publish in PRD, matched to published version
dc.identifierhttps://arxiv.org/abs/0712.3328
dc.identifierhttp://arxiv.org/abs/0712.3328
dc.identifierPhys.Rev.D78:023518,2008
dc.identifierdoi:10.1103/PhysRevD.78.023518
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/173393
dc.subjectGeneral Relativity and Quantum Cosmology
dc.title"Phantom" Inflation in Warped Compactification
dc.typetext

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