Gravitational radiation fields in teleparallel equivalent of general relativity and their energies
arXiv:1101.1012 · doi:10.1088/1674-1056/19/11/110402
Abstract
We derive two new retarded solutions in the teleparallel theory equivalent to general relativity (TEGR). One of these solutions gives a divergent energy. Therefore, we used the regularized expression of the gravitational energy-momentum tensor, which is a coordinate dependent. A detailed analysis of the loss of the mass of Bondi space-time is carried out using the flux of the gravitational energy-momentum.
Latex 12 pages
References in corpus (17)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Gravitational Lorentz Force and the Description of the Gravitational Interaction
- Gravitational Energy-Momentum Density in Teleparallel Gravity
- Pseudotensors and quasilocal energy-momentum
- Energy and angular momentum of the gravitational field in the teleparallel geometry
- Hamiltonian formulation of general relativity in the teleparallel geometry
- Teleparallel Spin Connection
- Regularized expression for the gravitational energy-momentum in teleparallel gravity and the principle of equivalence
- Energy-momentum and angular momentum densities in gauge theories of gravity
- The quadratic spinor Lagrangian is equivalent to the teleparallel theory
- Generalized Equivalence Principle in Extended New General Relativity
- Rotating Black Holes in Metric-Affine Gravity
- Space-time defects and teleparallelism
- Static Bondi Energy in the Teleparallel Equivalent of General Relativity
- On gravitational radiation and the energy flux of matter
- Gravitational energy of conical defects
- Black Holes in 2+1 Teleparallel Theories of Gravity