Gauge invariant cosmological perturbation theory for braneworlds

Simple item page
dc.creatorRiazuelo, Alain
dc.creatorVernizzi, Filippo
dc.creatorSteer, Danièle
dc.creatorDurrer, Ruth
dc.date2002-05-21
dc.date.accessioned2026-07-07T04:13:34Z
dc.date.available2026-07-07T04:13:34Z
dc.descriptionWe derive the gauge invariant perturbation equations for a 5-dimensional bulk spacetime in the presence of a brane. The equations are derived in full generality, without specifying a particular energy content of the bulk or the brane. We do not assume Z_2 symmetry, and show that the degree of freedom associated with brane motion plays a crucial role. Our formalism may also be used in the Z_2 symmetric case where it simplifies considerably.
dc.description73 pages, 11 figures, submitted to PRD
dc.identifierhttps://arxiv.org/abs/hep-th/0205220
dc.identifierhttp://arxiv.org/abs/hep-th/0205220
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51306
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGauge invariant cosmological perturbation theory for braneworlds
dc.typetext

Files

Collections

arXiv