English

Cosmic Solenoids: Minimal Cross-Section and Generalized Flux Quantization

General Relativity and Quantum Cosmology 2009-10-31 v1 Astrophysics High Energy Physics - Theory

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 Φ\Phi of magnetic flux cannot be confined within a cosmic solenoid of circumferential radius smaller than 3G2πc2Φ\frac{\sqrt{3G}}{2\pi c^2}\Phi 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: e/hcΦ+1/eQ=ne/{hc} \Phi + 1/e Q=n with QQ 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.

Keywords

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)

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