Spin polarised magnetized cylinder in torsioned spacetime
General Relativity and Quantum Cosmology
2015-06-25 v1
Abstract
A Spin-polarised cylindrically symmetric exact class of solutions endowed with magnetic fields in Einstein-Cartan-Maxwell gravity is obtained. Application of matching conditions to this interior solution having an exterior as Einstein's vacuum solution shows that for this class of metrics the Riemann-Cartan (RC) rotation vanishes which makes the solution static. Therefore we end up with a magnetized static spin polarised cylinder where the pressure along the symmetry axis is negative.
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Cite
@article{arxiv.gr-qc/0211072,
title = {Spin polarised magnetized cylinder in torsioned spacetime},
author = {L. C. Garcia de Andrade},
journal= {arXiv preprint arXiv:gr-qc/0211072},
year = {2015}
}
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