Dynamics of extended bodies with spin-induced quadrupole in Kerr spacetime: generic orbits

DOI10.1007/s10714-017-2214-yzbMath1380.83142arXiv1611.07602OpenAlexW2551032740MaRDI QIDQ682418

Wen-Biao Han, Ran Cheng

Publication date: 2 February 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1611.07602

zbMATH Keywords

Kerr spacetimegravitational wavesKerr black holeextended bodygeneric orbitsquadrupoleextreme-mass-ratio inspiralsMathisson-Papapetrou-Dixon equations

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)

Related Items (2)

Spin Dynamics of Moving Bodies in Rotating Black Hole Spacetimes ⋮ The distributional stress–energy quadrupole

Cites Work

• Unnamed Item
• Chaos and dynamics of spinning particles in Kerr spacetime
• Dynamics of extended bodies in general relativity center-of-mass description and quasirigidity
• Fast Lyapunov indicators. Application to asteroidal motion
• Gravitational self-force in extreme mass-ratio inspirals
• Spinning test particles and clock effect in Kerr spacetime
• A covariant multipole formalism for extended test bodies in general relativity
• Extended bodies in a Kerr spacetime: exploring the role of a general quadrupole tensor
• Spinning test-particles in general relativity. I
• The motion of point particles in curved spacetime
• On the structure of symplectic mappings. The fast Lyapunov indicator: A very sensitive tool

This page was built for publication: Dynamics of extended bodies with spin-induced quadrupole in Kerr spacetime: generic orbits