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arXiv · gr-qc/9511060

The Symplectic Structure of General Relativity in the Double-Null (2+2) Formalism

Abstract

In the (2+2) formulation of general relativity spacetime is foliated by a two-parameter family of spacelike 2-surfaces (instead of the more usual one-parameter family of spacelike 3-surfaces). In a partially gauge-fixed setting (double-null gauge), I write down the symplectic structure of general relativity in terms of intrinsic and extrinsic quantities associated with these 2-surfaces. This leads to an identification of the reduced phase space degrees of freedom. In particular, I show that the two physical degrees of freedom of general relativity are naturally encoded in a quantity closely related to the twist of the pair of null normals to the 2-surfaces. By considering the characteristic initial-value problem I establish a canonical transformation between these and the more usually quoted conformal 2-metric (or shear) degrees of freedom. (This paper is based on a talk given at the Fifth Midwest Relativity Conference, Milwaukee, USA.)

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BibTeXRIS

Richard J. Epp. 1995-11-22. The Symplectic Structure of General Relativity in the Double-Null (2+2) Formalism. https://arxiv.org/abs/gr-qc/9511060

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