Can Reissner-Nordström wormholes be considered for Spacetime Foam formation?
Remo Garattini
Abstract
A simple model of spacetime foam, made by N Reissner-Nordström wormholes with a magnetic and electric charge in a semiclassical approximation, is taken under examination. The Casimir-like energy of the quantum fluctuation of such a model is computed and compared with that one obtained with a foamy space modeled by N Schwarzschild wormholes. The comparison leads to the conclusion that a foamy spacetime cannot be considered as a collection of N Reissner-Nordström wormholes but that such a collection can be taken as an excited state of the foam.
Create a lesson
Related papers
Non-Commutativity in Geodesic Congruences
Aarav Shah, Louis H. Kauffman
Scalar wave dark matter imprints on binary black hole mergers: dependence on field mass and density
Yu-Peng Zhang, Shao-Wen Wei, Yu-Xiao Liu
Quantum Energy Inequalities with a twist: rotating frames along stationary worldlines
Christopher J. Fewster, Daniel Lomax Ford
Analytic Electromagnetic Effective Source for Geodesic Orbit in Schwarzschild Spacetime
Xuchen Lu, Yungui Gong, Bokai Zhang et al.
Stability conditions for light rings in circular stationary axisymmetric spacetimes
Jake O. Shipley
Post-Newtonian secular dynamics of hierarchical triples II. Canonical derivation of the 1PN\,×\,quadrupole cross terms and of the quadrupole-squared term
Hideyoshi Arakida