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A spinorial Hamiltonian approach to gravity

James D E Grant

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We give a spinorial set of Hamiltonian variables for general relativity in any dimension greater than 2. This approach involves a study of the algebraic properties of spinors in higher dimensions, and of the elimination of second-class constraints from the Hamiltonian theory. In four dimensions, when restricted to the positive spin-bundle, these variables reduce to the standard Ashtekar variables. In higher dimensions, the theory can either be reduced to a spinorial version of the ADM formalism, or can be left in a more general form which seems useful for the investigation of some spinorial problems such as Riemannian manifolds with reduced holonomy group. In dimensions 0 (mod 4), the theory may be recast solely in terms of structures on the positive spin-bundle BbbV+, but such a reduction does not seem possible in dimensions 2 (mod 4), due to algebraic properties of spinors in these dimensions.


PACS

04.20.Cv Fundamental problems and general formalism

02.40.-k Geometry, differential geometry, and topology

04.25.-g Approximation methods; equations of motion

MSC

83C10 Equations of motion

83C60 Spinor and twistor methods; Newman-Penrose formalism

Subjects

Mathematical physics

Gravitation and cosmology

Dates

Issue 11 (November 1999)

Received 22 December 1998, in final form 15 July 1999



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