Cosmological magnetic field---the boost-symmetric case

Ji\v{r}\'i Vesel\'y; Martin \v{Z}ofka

Cosmological magnetic field---the boost-symmetric case

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arxiv 2104.02123 v1 pith:XPWCVXR4 submitted 2021-04-05 gr-qc

Jiří Veselý , Martin Žofka This is my paper · ORCID

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keywords fieldmagneticcosmologicaladditionalboost-symmetriccaseclassconstant

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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.

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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.

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