Curvature invariants for accelerating Kerr–Newman black holes in (anti-)de Sitter spacetime

DOI10.1088/1361-6382/ac750azbMath1498.83028arXiv2112.01235OpenAlexW3214886901MaRDI QIDQ5084139

Georgios V. Kraniotis

Publication date: 23 June 2022

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

Full work available at URL: https://arxiv.org/abs/2112.01235

zbMATH Keywords

cosmological constantcurvature invariantsgravitomagnetismKerr-Newman-(anti-)de Sitteraccelerating rotating and charged black holeschiral photon anomaly

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Motion of charged particles (78A35) Einstein-Maxwell equations (83C22) Electro- and magnetostatics (78A30) Motion of the gyroscope (70E05)

Related Items (1)

Motion equations in a Kerr–Newman–de Sitter spacetime: some methods of integration and application to black holes shadowing in Scilab

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