Supersymmetric M3-branes and G_2 Manifolds

dc.creatorCvetic, M.
dc.creatorGibbons, G. W.
dc.creatorLu, H.
dc.creatorPope, C. N.
dc.date2001-06-03
dc.date2001-06-11
dc.date.accessioned2026-07-07T10:34:07Z
dc.date.available2026-07-07T10:34:07Z
dc.descriptionWe obtain a generalisation of the original complete Ricci-flat metric of G_2 holonomy on R^4\times S^3 to a family with a non-trivial parameter λ. For generic λthe solution is singular, but it is regular when λ={-1,0,+1}. The case λ=0 corresponds to the original G_2 metric, and λ={-1,1} are related to this by an S_3 automorphism of the SU(2)^3 isometry group that acts on the S^3\times S^3 principal orbits. We then construct explicit supersymmetric M3-brane solutions in D=11 supergravity, where the transverse space is a deformation of this class of G_2 metrics. These are solutions of a system of first-order differential equations coming from a superpotential. We also find M3-branes in the deformed backgrounds of new G_2-holonomy metrics that include one found by A. Brandhuber, J. Gomis, S. Gubser and S. Gukov, and show that they also are supersymmetric.
dc.descriptionLatex, 29 pages. This corrects a previous version in which it was claimed that the M3-brane solutions were pseudo-supersymmetric rather than supersymmetric
dc.identifierhttps://arxiv.org/abs/hep-th/0106026
dc.identifierhttp://arxiv.org/abs/hep-th/0106026
dc.identifierNucl.Phys.B620:3-28,2002
dc.identifierdoi:10.1016/S0550-3213(01)00534-X
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179367
dc.subjectHigh Energy Physics - Theory
dc.titleSupersymmetric M3-branes and G_2 Manifolds
dc.typetext

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