Astrophysically relevant bound trajectories around a Kerr black hole

DOI10.1088/1361-6382/ab004czbMath1476.83017arXiv1901.02730OpenAlexW2909510735MaRDI QIDQ3380502

Arun Mangalam, Prerna Rana

Publication date: 29 September 2021

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

Full work available at URL: https://arxiv.org/abs/1901.02730

zbMATH Keywords

exact solutionsHamiltonian mechanicsphysics of black holesnumerical relativityclassical black holes

Mathematics Subject Classification ID

Black holes (83C57) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Exact solutions to problems in general relativity and gravitational theory (83C15) Orbital mechanics (70M20) Gravitational waves (83C35) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (1)

Spherical orbits around a Kerr black hole

Cites Work

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• ``Golden oldie: On the gravitational field of a mass point according to Einstein's theory
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• Periapsis and gravitomagnetic precessions of stellar orbits in Kerr and Kerr–de Sitter black hole spacetimes
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Celestial mechanics in Kerr spacetime
• Precise relativistic orbits in Kerr and Kerr–(anti) de Sitter spacetimes
• Global Structure of the Kerr Family of Gravitational Fields
• Extreme mass ratio inspirals: LISA's unique probe of black hole gravity
• Computing inspirals in Kerr in the adiabatic regime: I. The scalar case

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