Stealth Acceleration and Modified Gravity

dc.creatorCharmousis, Christos
dc.creatorGregory, Ruth
dc.creatorPadilla, Antonio
dc.date2007-06-06
dc.date.accessioned2026-07-07T13:04:27Z
dc.date.available2026-07-07T13:04:27Z
dc.descriptionWe show how to construct consistent braneworld models which exhibit late time acceleration. Unlike self-acceleration, which has a de Sitter vacuum state, our models have the standard Minkowski vacuum and accelerate only in the presence of matter, which we dub ``stealth-acceleration''. We use an effective action for the brane which includes an induced gravity term, and allow for an asymmetric set-up. We study the linear stability of flat brane vacua and find the regions of parameter space where the set-up is stable. The 4-dimensional graviton is only quasi-localised in this set-up and as a result gravity is modified at late times. One of the two regions is strongly coupled and the scalar mode is eaten up by an extra symmetry that arises in this limit. Having filtered the well-defined theories we then focus on their cosmology. When the graviton is quasi-localised we find two main examples of acceleration. In each case, we provide an illustrative model and compare it to LambdaCDM.
dc.description32 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/0706.0857
dc.identifierhttp://arxiv.org/abs/0706.0857
dc.identifierJCAP 0710:006,2007
dc.identifierdoi:10.1088/1475-7516/2007/10/006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/227172
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleStealth Acceleration and Modified Gravity
dc.typetext

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