Transition from inspiral to plunge into a highly spinning black hole

DOI10.1088/1361-6382/ab79d3zbMath1479.83126arXiv1909.12848OpenAlexW3102152584MaRDI QIDQ5161988

Caroline Jonas, Geoffrey Compère, Kwinten Fransen

Publication date: 1 November 2021

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

Full work available at URL: https://arxiv.org/abs/1909.12848

zbMATH Keywords

ISCOrapidly rotating black holebinary black hole dynamicsextreme mass ratio inspiraltransition from inspiral to plunge

Mathematics Subject Classification ID

Black holes (83C57) KdV equations (Korteweg-de Vries equations) (35Q53) Painlevé and other special ordinary differential equations in the complex domain; classification, hierarchies (34M55) Two-body problems (70F05) Orbital mechanics (70M20) Gravitational waves (83C35) Motion of the gyroscope (70E05)

Related Items (2)

Kerr-fully diving into the abyss: analytic solutions to plunging geodesics in Kerr ⋮ Gravitational perturbations from NHEK to Kerr

Cites Work

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• Whirling orbits around twirling black holes from conformal symmetry
• Fast plunges into Kerr black holes
• Inspiral into Gargantua
• Gravitational waves from plunges into Gargantua
• Slowly Varying Jump and Transition Phenomena Associated with Algebraic Bifurcation Problems
• Spin and quadrupole couplings for high spin equatorial intermediate mass-ratio coalescences
• Particle motion near high-spin black holes
• Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
• The Kerr/CFT correspondence and its extensions

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