Extended bodies in a Kerr spacetime: exploring the role of a general quadrupole tensor
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Publication:5416489
DOI10.1088/0264-9381/31/7/075024zbMath1291.83130arXiv1408.5484OpenAlexW3102782021WikidataQ62560795 ScholiaQ62560795MaRDI QIDQ5416489
Publication date: 20 May 2014
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1408.5484
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 (4)
Spin Dynamics of Moving Bodies in Rotating Black Hole Spacetimes ⋮ Dynamics of extended bodies with spin-induced quadrupole in Kerr spacetime: generic orbits ⋮ The effective field theorist's approach to gravitational dynamics ⋮ Extended bodies moving on geodesic trajectories
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