A note on magnetic generalizations of the Kerr and Kerr–Newman solutions

DOI10.1088/1361-6382/aa80bbzbMath1372.83013OpenAlexW2737358604MaRDI QIDQ5369368

V. S. Man'ko

Publication date: 17 October 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/1361-6382/aa80bb

zbMATH Keywords

electromagnetic fieldKerr solutionmultipole momentsErnst potentialSibgatullin's method

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (1)

Metric of a rotating charged magnetized sphere

Cites Work

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• Multipole moments of stationary space-times
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
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• Corrections and comments on the multipole moments of axisymmetric electrovacuum spacetimes
• A binary system of `antisymmetric' Kerr-Newman masses
• Six-parameter solution of the Einstein–Maxwell equations possessing equatorial symmetry
• The influence of the Lande g -factor in the classical general relativistic description of atomic and subatomic systems
• Note on reflection symmetry in stationary axisymmetric electrovacuum spacetimes
• Equatorial symmetry/antisymmetry of stationary axisymmetric electrovac spacetimes
• Electromagnetic Waves from Very Dense Stars

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