Cosmic Solenoids: Minimal Cross-Section and Generalized Flux Quantization
Abstract
A self-consistent general relativistic configuration describing a finite cross-section magnetic flux tube is constructed. The cosmic solenoid is modeled by an elastic superconductive surface which separates the Melvin core from the surrounding flat conic structure. We show that a given amount of magnetic flux cannot be confined within a cosmic solenoid of circumferential radius smaller than without creating a conic singularity. Gauss-Codazzi matching conditions are derived by means of a self-consistent action. The source term, representing the surface currents, is sandwiched between internal and external gravitational surface terms. Surface superconductivity is realized by means of a Higgs scalar minimally coupled to projective electromagnetism. Trading the 'magnetic' London phase for a dual 'electric' surface vector potential, the generalized quantization condition reads: with denoting some dual 'electric' charge, thereby allowing for a non-trivial Aharonov-Bohm effect. Our conclusions persist for dilaton gravity provided the dilaton coupling is sub-critical.
Cite
@article{arxiv.gr-qc/9901002,
title = {Cosmic Solenoids: Minimal Cross-Section and Generalized Flux Quantization},
author = {Aharon Davidson and David Karasik},
journal= {arXiv preprint arXiv:gr-qc/9901002},
year = {2009}
}
Comments
Revtex, 11 twocolumn pages, 3 eps figures (accepted for publication in Phys. Rev. D)