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Cylindrical spacetimes due to radial magnetic fields

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arxiv 2104.01557 v1 pith:ZVIXP7CS submitted 2021-04-04 gr-qc

Jiří Veselý , Martin Žofka This is my paper · ORCID
classification gr-qc
keywords magneticspacetimesfieldsaxisclassesconstantcontinuecosmological
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We continue our previous study of cylindrically symmetric, static electrovacuum spacetimes generated by a magnetic field, involving optionally the cosmological constant, and investigate several classes of exact solutions. These spacetimes are due to magnetic fields that are perpendicular to the axis of symmetry.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Magnetising de Sitter and Anti-de Sitter spacetimes

    gr-qc 2026-07 conditional novelty 5.5 of 10

    A Harrison-type map plus fluid rescaling produces spherical Melvin analogues of dS and AdS that reduce to ordinary (A)dS when the magnetic field vanishes.

  2. Properties of the magnetic universe with positive cosmological constant

    gr-qc 2025-09 conditional novelty 5.0 of 10

    The paper works out the geometry, flux, and geodesics of the Melvin magnetic universe with a positive cosmological constant, showing its two-sphere section is compact and carries a conical singularity, with a Freund-R...

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