Extrinsic Curvature and the Einstein Constraints
Abstract
The Einstein initial-value equations in the extrinsic curvature (Hamiltonian) representation and conformal thin sandwich (Lagrangian) representation are brought into complete conformity by the use of a modified decomposition of symmetric tensors.Keywords
All Related Versions
- Version 1, 2002-07-24, ArXiv
- Version 2, 2002-11-07, ArXiv
- Published version: Physical Review D, 67 (4).
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