Stress-energy tensor in the Bel-Szekeres space-time
arXiv:gr-qc/9802050 · doi:10.1103/PhysRevD.58.104010
Abstract
In a recent work an approximation procedure was introduced to calculate the vacuum expectation value of the stress-energy tensor for a conformal massless scalar field in the classical background determined by a particular colliding plane wave space-time. This approximation procedure consists in appropriately modifying the space-time geometry throughout the causal past of the collision center. This modification in the geometry allows to simplify the boundary conditions involved in the calculation of the Hadamard function for the quantum state which represents the vacuum in the flat region before the arrival of the waves. In the present work this approximation procedure is applied to the non-singular Bel-Szekeres solution, which describes the head on collision of two electromagnetic plane waves. It is shown that the stress-energy tensor is unbounded as the killing-Cauchy horizon of the interaction is approached and its behavior coincides with a previous calculation in another example of non-singular colliding plane wave space-time.
17 pages, LaTex file, 2 PostScript figures
References in corpus (8)
- Constant magnetic field in closed string theory: an exactly solvable model
- Four Dimensional Plane Wave String Solutions with Coset CFT Description
- Finite sigma models and exact string solutions with Minkowski signature metric
- Strings in Plane Wave Backgrounds Revisited
- Particle creation in a colliding plane wave spacetime: wave packet quantization
- Particle Creation in the Bell-Szekeres Spacetime
- Quantum fields interacting with colliding plane waves: the stress-energy tensor and backreaction
- Stress-energy tensor in colliding plane wave space-times: An approximation procedure