The Energy of a Dynamical Wave-Emitting System in General Relativity
arXiv:gr-qc/0302020 · doi:10.1023/A:1025633817361
Abstract
The problem of energy and its localization in general relativity is critically re-examined. The Tolman energy integral for the Eddington spinning rod is analyzed in detail and evaluated apart from a single term. It is shown that a higher order iteration is required to find its value. Details of techniques to solve mathematically challenging problems of motion with powerful computing resources are provided. The next phase of following a system from static to dynamic to final quasi-static state is described.
36 pages, 2 figures, to appear in Foundations of Physics
References in corpus (2)
Cited by in corpus (4)
- Covariant energy-momentum and an uncertainty principle for general relativity
- The Fully Covariant Energy Momentum Stress Tensor For Gravity and the Einstein Equation in General Relativity
- An observer principle for general relativity
- The Jacobi Curvature Operator in Semi Riemannian Geometry and the Energy Momentum Stress Tensor of the Gravitational Field