Spin polarised magnetized cylinder in torsioned spacetime
L.C. Garcia de Andrade (Departamento de Fisica Teorica-IF-UERJ)

TL;DR
This paper derives exact solutions for a magnetized, spin-polarized cylindrical spacetime in Einstein-Cartan-Maxwell gravity, revealing a static configuration with specific pressure characteristics.
Contribution
It introduces a new class of exact solutions for magnetized, spin-polarized cylinders in Einstein-Cartan-Maxwell gravity, analyzing their static nature and matching conditions.
Findings
Riemann-Cartan rotation vanishes, making the solution static.
The interior solution has negative pressure along the axis.
Matching conditions with vacuum solutions are satisfied.
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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