Hamilton-Jacobi equation for spinning particles near black holes

A compact stellar-mass object inspiraling onto a massive black hole deviates from geodesic motion due to radiation-reaction forces as well as finite-size effects. Such postgeodesic deviations need to be included with sufficient precision into wave-form models for the upcoming space-based gravitation...

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Veröffentlicht in:	Physical review. D 2019-11, Vol.100 (10), p.1, Article 104030
1. Verfasser:	Witzany, Vojtěch
Format:	Artikel
Sprache:	eng
Schlagworte:	Black holes Geodesy Gravitational waves Hamilton-Jacobi equation Resonant frequencies Size effects Two body problem Waveforms
Online-Zugang:	Volltext
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