The Bogomolny Equations and Solutions for Einstein-Yang-Mills-Dilaton- $σ$ Models

dc.creatorBraden, H. W.
dc.creatorVarela, V.
dc.date1998-04-30
dc.date1998-09-11
dc.date.accessioned2026-07-07T10:53:55Z
dc.date.available2026-07-07T10:53:55Z
dc.descriptionWe derive Bogomolny equations for an Einstein-Yang-Mills-dilaton-$σ$ model (EYMD-$σ$) on a static spacetime, showing that the Einstein equations are satisfied if and only if the associated (conformally scaled) three-metric is flat. These are precisely the static metrics for which super-covariantly constant spinors exist. We study some general properties of these equations and then consider the problem of obtaining axially symmetric solutions for the gauge group SU(2).
dc.description24 pages LaTex, 1 Figure, revised text for publication
dc.identifierhttps://arxiv.org/abs/hep-th/9804204
dc.identifierhttp://arxiv.org/abs/hep-th/9804204
dc.identifierPhys.Rev.D58:124020,1998
dc.identifierdoi:10.1103/PhysRevD.58.124020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185645
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe Bogomolny Equations and Solutions for Einstein-Yang-Mills-Dilaton- $σ$ Models
dc.typetext

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