2021/04/05 by Jiří Veselý, Martin Žofka · 1 citation
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1103/physrevd.100.044059
published as Phys. Rev. D 100, 044059 (2019) · 7 pages, no figures, a reference added
arxiv created 2021/04/05 · arxiv updated 2021/04/07
We find a class of cylindrically symmetric, static electrovacuum spacetimes generated by a non-homogeneous magnetic field and involving the cosmological constant and one additional parameter, which determine uniquely the strength of the magnetic field. We provide a simple model of a source producing the field.