The ultrarelativistic Reissner-Nordstrom field in the Colombeau algebra
arXiv:gr-qc/9606059 · doi:10.1063/1.531819
Abstract
The electromagnetic field of the ultrarelativistic Reissner-Nordstrom solution shows the physically highly unsatisfactory property of a vanishing field tensor but a nonzero, i.e., delta-like, energy density. The aim of this work is to analyze this situation from a mathematical point of view, using the framework of Colombeau's theory of nonlinear generalized functions. It is shown that the physically unsatisfactory situation is mathematically perfectly defined and that one cannot aviod such situations when dealing with distributional valued field tensors.
final version, minor grammatical changes
Cited by in corpus (17)
- The use of Generalised Functions and Distributions in General Relativity
- A rigorous solution concept for geodesic and geodesic deviation equations in impulsive gravitational waves
- Geodesics and geodesic deviation for impulsive gravitational waves
- A note on the Penrose junction conditions
- Pre-Equilibrium Radial Flow from Central Shock-Wave Collisions in AdS5
- Ultrarelativistic black hole in an external electromagnetic field and gravitational waves in the Melvin universe
- Interpolating Between Asymptotic and Near Horizon Symmetries
- Invariance of the distributional curvature of the cone under smooth diffeomorphisms
- Ultrarelativistic limits of boosted dilaton black holes
- Generalized Kerr Schild metrics and the gravitational field of a massless particle on the horizon
- Ultrarelativistic boost of spinning and charged black rings
- The classical point-electron in Colombeau's theory of nonlinear generalized functions
- Distributional Metrics and the Action Principle of Einstein-Hilbert Gravity
- A nonlinear theory of distributional geometry
- Weak second Bianchi identity for static, spherically symmetric spacetimes with timelike singularities
- Light bending by a Coulomb field and the Aichelburg-Sexl ultraboost
- Generalized regularly discontinuous solutions of the Einstein equations