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(2+1) sector of (3+1) gravity

Jerzy Lewandowski, +1 more
- 01 Mar 1997 - 
- Vol. 14, Iss: 3, pp 775-782
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TLDR
In this article, the rank-2 sector of classical (3 + 1)-dimensional Ashtekar gravity is considered and it is found that the consistency of the evolution equations with the reality of the volume requires that the 3-surface of initial data is foliated by 2-surfaces tangential to degenerate triads.
Abstract
The rank-2 sector of classical (3 + 1)-dimensional Ashtekar gravity is considered. It is found that the consistency of the evolution equations with the reality of the volume requires that the 3-surface of initial data is foliated by 2-surfaces tangential to degenerate triads. In turn, the degeneracy is preserved by the evolution. The 2-surfaces behave like (2 + 1)-dimensional empty spacetimes with a massless complex field propagating along each of them. The results provide some evidence for the issue of evolving a non-degenerate gravitational field into a degenerate sector of Ashtekar's phase space.

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Citations
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Degenerate metric phase boundaries

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References
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Journal ArticleDOI

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TL;DR: A Hamiltonian formulation of general relativity based on certain spinorial variables is introduced that enables one to imbed the constraint surface in the phase space of Einstein's theory into that of Yang-Mills theory.
Journal ArticleDOI

New Hamiltonian formulation of general relativity

TL;DR: An important feature of the new form of constraints is the natural embedding of the constraint surface of the Einstein phase space into that of Yang-Mills phase space, which provides new tools to analyze a number of issues in both classical and quantum gravity.
Book

Lectures on Non-Perturbative Canonical Gravity

TL;DR: In this article, the authors present an up-to-date account of a non-perturbative, canonical quantization program for gravity, which was highlighted in virtually every major conference in gravitational physics over the past three years.
Journal ArticleDOI

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TL;DR: In this paper, the connection between the lagrangian and the hamiltonian is partially worked out, and it is shown how to identify the space-time metric in terms of them.
Journal ArticleDOI

New constraints for canonical general relativity

TL;DR: In this article, a fully 4-diffeo invariant canonical theory in Ashtekar's variables, derived from Plebanski's action, was shown to be invariant under a number of new constraints.
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