Rotating black holes without ℤ2 symmetry and their shadow images

DOI10.1088/1475-7516/2020/05/040zbMath1492.85010arXiv2004.01440OpenAlexW3101760964MaRDI QIDQ5069142

Che-Yu Chen

Publication date: 8 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.01440

zbMATH Keywords

gravitymodified gravityastrophysical black holes

Mathematics Subject Classification ID

Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Geodesics in global differential geometry (53C22) Galactic and stellar structure (85A15) Gravitational waves (83C35) Motion of the gyroscope (70E05)

Related Items (7)

Kerr black holes with synchronised Proca hair: lensing, shadows and EHT constraints ⋮ Gravitational footprints of black holes and their microstate geometries ⋮ Black holes with scalar hair in light of the Event Horizon Telescope ⋮ Black hole shadow with soft hairs ⋮ Superentropic AdS black hole shadows ⋮ Generating rotating spacetime in Ricci-based gravity: naked singularity as a black hole mimicker ⋮ From a locality-principle for new physics to image features of regular spinning black holes with disks

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