Second post-Minkowskian metric for a moving Kerr black hole
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Publication:2921598
DOI10.1142/S0218271814500795zbMath1296.83040arXiv2007.13329OpenAlexW1974762188MaRDI QIDQ2921598
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Publication date: 13 October 2014
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2007.13329
Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
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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
- On the efficient computation of the quadrupole light deflection
- Light propagation in the gravitational field of moving bodies by means of Lorentz transformation I. Mass monopoles moving with constant velocities
- Exact Harmonic Metric for a Uniformly Moving Schwarzschild Black Hole
- ROTO-TRANSLATIONAL EFFECTS ON DEFLECTION OF LIGHT AND PARTICLE BY MOVING KERR BLACK HOLE
- The effect of the motion of the Sun on the light-time in interplanetary relativity experiments
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