Polarization effects in Kerr black hole shadow due to the coupling between photon and bumblebee field

DOI10.1007/JHEP07(2020)054zbMath1451.83007arXiv2004.08857MaRDI QIDQ2215350

Jiliang Jing, Mingzhi Wang, Songbai Chen

Publication date: 11 December 2020

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.08857

zbMATH Keywords

black holesclassical theories of gravity

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05)

Related Items (5)

Kerr black holes with synchronised Proca hair: lensing, shadows and EHT constraints ⋮ Periastron precession due to a Janis–Newman–Winicour wormhole in the weak field limit ⋮ Black holes with scalar hair in light of the Event Horizon Telescope ⋮ Chaotic shadows of black holes: a short review ⋮ Schwarzschild-like black hole with a topological defect in bumblebee gravity

Cites Work

• Black hole physics. Basic concepts and new developments
• Propagation of vacuum polarized photons in topological black hole spacetimes
• Gravitational lensing under the effect of Weyl and bumblebee gravities: applications of Gauss-Bonnet theorem
• ``Faster than light photons and charged black holes.
• Shadow of a black hole surrounded by dark matter
• GUP modified Hawking radiation in bumblebee gravity
• Shadows of Kerr black holes with and without scalar hair
• Binary black hole shadows, chaotic scattering and the Cantor set
• Quantum gravitational optics: the induced phase
• Geodesic structure of the Born–Infeld black hole

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