Gravitating p-Branes

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dc.creatorClark, T. E.
dc.creatorLove, S. T.
dc.creatorNitta, Muneto
dc.creatorter Veldhuis, T.
dc.creatorXiong, C.
dc.date2006-12-14
dc.date2006-12-14
dc.date.accessioned2026-07-07T11:23:24Z
dc.date.available2026-07-07T11:23:24Z
dc.descriptionCoset methods are used to construct the action describing the dynamics associated with the spontaneous breaking of the local Poincare symmetries of D dimensional space-time due to the embedding of a p-brane with codimension N=D-p-1. The resulting action is an ISO(1,p+N) invariant form of the Einstein-Hilbert action, which, in addition to the gravitational vielbein, also includes N massive gauge fields corresponding to the broken space translation symmetries which together carry the fundamental representation of the unbroken SO(N) gauge symmetry and an SO(N) Yang-Mills field localized on the brane. The long wavelength dynamics of the gravitating p-brane is the same as the action of an SO(N) vector massive Proca field and a non-Abelian SO(N) Yang-Mills field all coupled to gravity in d=(1+p) dimensional space-time. The general results are specialized to determine the effective action for the gravitating vortex solution in the D=6 Abelian Higgs-Kibble model.
dc.description28 pages, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/0612147
dc.identifierhttp://arxiv.org/abs/hep-th/0612147
dc.identifierPhys.Rev.D75:065028,2007
dc.identifierdoi:10.1103/PhysRevD.75.065028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194879
dc.subjectHigh Energy Physics - Theory
dc.titleGravitating p-Branes
dc.typetext

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