Symmetric Hyperbolic System in the Self-dual Teleparallel Gravity
arXiv:gr-qc/0408047 · doi:10.1103/PhysRevD.70.044009
Abstract
In order to discuss the well-posed initial value formulation of the teleparallel gravity and apply it to numerical relativity a symmetric hyperbolic system in the self-dual teleparallel gravity which is equivalent to the Ashtekar formulation is posed. This system is different from the ones in other works by that the reality condition of the spatial metric is included in the symmetric hyperbolicity and then is no longer an independent condition. In addition the constraint equations of this system are rather simpler than the ones in other works.
8 pages, no figures
References in corpus (14)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- New Formalism for Numerical Relativity
- Gravitational Lorentz Force and the Description of the Gravitational Interaction
- Gravitational Energy-Momentum Density in Teleparallel Gravity
- Pseudotensors and quasilocal energy-momentum
- Fixing Einstein's equations
- First-order symmetric-hyperbolic Einstein equations with arbitrary fixed gauge
- First order hyperbolic formalism for Numerical Relativity
- Einstein and Yang-Mills theories in hyperbolic form without gauge-fixing
- Hamiltonian structure of the teleparallel formulation of GR
- Symmetric hyperbolic system in the Ashtekar formulation
- Teleparallel Equivalent of the Kaluza-Klein Theory
- Einstein's equations in Ashtekar's variables constitute a symmetric hyperbolic system
- Teleparallel Equivalent of Non-Abelian Kaluza-Klein Theory