HEAL DSpace

Anisotropic extra dimensions

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dc.contributor.author Papantonopoulos, E en
dc.contributor.author Papazoglou, A en
dc.contributor.author Tsoukalas, M en
dc.date.accessioned 2014-03-01T01:35:18Z
dc.date.available 2014-03-01T01:35:18Z
dc.date.issued 2011 en
dc.identifier.issn 1550-7998 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/20991
dc.subject Cosmological Constant en
dc.subject Extra Dimension en
dc.subject Spectrum en
dc.subject randall sundrum en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other VELTMAN-ZAKHAROV DISCONTINUITY en
dc.subject.other GRAVITATIONAL HIGGS MECHANISM en
dc.subject.other DARK ENERGY en
dc.subject.other GRAVITY en
dc.subject.other MASS en
dc.subject.other MILLIMETER en
dc.subject.other HIERARCHY en
dc.subject.other FIELDS en
dc.subject.other SPACE en
dc.title Anisotropic extra dimensions en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevD.84.025016 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevD.84.025016 en
heal.identifier.secondary 025016 en
heal.language English en
heal.publicationDate 2011 en
heal.abstract We consider the scenario where, in a five-dimensional theory, the extra spatial dimension has different scaling than the other four dimensions. We find background maximally symmetric solutions, when the bulk is filled with a cosmological constant and at the same time it has a three-brane embedded in it. These background solutions are reminiscent of Randall-Sundrum warped metrics, with bulk curvature depending on the parameters of the breaking of diffeomorphism invariance. Subsequently, we consider the scalar perturbation sector of the theory and show that it has certain pathologies and the striking feature that in the limit where the diffeomorphism invariance is restored, there remain ghost scalar mode(s) in the spectrum. © 2011 American Physical Society. en
heal.publisher AMER PHYSICAL SOC en
heal.journalName Physical Review D - Particles, Fields, Gravitation and Cosmology en
dc.identifier.doi 10.1103/PhysRevD.84.025016 en
dc.identifier.isi ISI:000292875600008 en
dc.identifier.volume 84 en
dc.identifier.issue 2 en


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