arXiv · gr-qc/0211072
Spin polarised magnetized cylinder in torsioned spacetime
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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L. C. Garcia de Andrade. 2002-11-22. Spin polarised magnetized cylinder in torsioned spacetime. https://doi.org/10.1023/a%3A1024406009917
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