Galactic dynamo seeds from non-superconducting spin-polarised strings
Abstract
Earlier Enqvist and Olesen have shown that formation of ferromagnetic planar walls in vacuum at GUT scales in comoving plasmas may generate a large scale magnetic field of . In this paper we show that starting from classical Einstein-Cartan-Maxwell strong gravity, a spin-polarised ferromagnetic cylinder gives rise to a cosmological magnetic field of the order . Vorticity of cylinder is used to obtain galactic magnetic fields. Magnetic fields up to can be obtained from the spin density of the cylinder. If matching conditions are used cosmological magnetic fields of the order of where is the radius of the cosmic strings. For a cosmic string with the radius of an hydrogen atom the cosmic magnetic field is which is enough to seed galactic dynamos.
Keywords
Cite
@article{arxiv.1401.2587,
title = {Galactic dynamo seeds from non-superconducting spin-polarised strings},
author = {L. C. Garcia de Andrade},
journal= {arXiv preprint arXiv:1401.2587},
year = {2015}
}
Comments
arXiv admin note: substantial text overlap with arXiv:gr-qc/0211072