Holonomy and Symmetry in M-theory

dc.creatorHull, Chris
dc.date2003-05-05
dc.date2003-05-07
dc.date.accessioned2026-07-07T04:15:11Z
dc.date.available2026-07-07T04:15:11Z
dc.descriptionSupersymmetric solutions of 11-dimensional supergravity can be classified according to the holonomy of the supercovariant derivative arising in the Killing spinor condition. It is shown that the holonomy must be contained in $\SL(32,\R)$. The holonomies of solutions with flux are discussed and examples are analysed. In extending to M-theory, account has to be taken of the phenomenon of ` supersymmetry without supersymmetry'. It is argued that including the fermionic degrees of freedom in M-theory requires a formulation with a local $\SL(32,\R)$ symmetry, analogous to the need for local Lorentz symmetry in coupling spinors to gravity.
dc.description26 pages. 31/32 supersymmetries might occur after all
dc.identifierhttps://arxiv.org/abs/hep-th/0305039
dc.identifierhttp://arxiv.org/abs/hep-th/0305039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51908
dc.subjectHigh Energy Physics - Theory
dc.titleHolonomy and Symmetry in M-theory
dc.typetext

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