ROTO-TRANSLATIONAL EFFECTS ON DEFLECTION OF LIGHT AND PARTICLE BY MOVING KERR BLACK HOLE

DOI10.1142/S021827181450031XzbMath1284.83081arXiv2007.12317OpenAlexW2058288573MaRDI QIDQ5411384

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Publication date: 23 April 2014

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2007.12317

zbMATH Keywords

relativitygravitationgravitational lensing

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

Second post-Minkowskian metric for a moving Kerr black hole ⋮ Kerr–Schild form of the exact metric for a constantly moving Kerr black hole and null gravitational deflection ⋮ Weak and strong deflection gravitational lensings by a charged Horndeski black hole

Cites Work

• Harmonic metric for Kerr black hole and its post-Newtonian approximation
• Gravimagnetism, causality, and aberration of gravity in the gravitational light-ray deflection experiments
• Lensing by Kerr black holes. II: Analytical study of quasi-equatorial lensing observables
• Deflection of highly relativistic particles in a gravitational field
• Wave and particle scattering properties of high-speed Kerr black holes
• GRAVITOMAGNETISM AND THE SPEED OF GRAVITY

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