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Similar

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2005
Cited alongside, same era.
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Then

T. Osburn, N. Warburton, and C. R. Evans, Highly eccentric inspirals into a black hole, Phys. Rev. D 93
Original
2016
Later among the works it cites.
C. Merlin, A. Ori, L. Barack, A. Pound, and M. van de Meent, Completion of metric reconstruction for a particle orbiting a Kerr black hole, Phys. Rev. D 94
Original
2016
Later among the works it cites.
C. P. Berry, R. H. Cole, P. Cañizares, and J. R. Gair, Importance of transient resonances in extreme-mass-ratio inspirals, Phys. Rev. D 94
2016
Later among the works it cites.
R. Fujita, S. Isoyama, A. Le Tiec, H. Nakano, N. Sago, and T. Tanaka, Hamiltonian Formulation of the Conservative Self-Force Dynamics in the Kerr Geometry, Class. Quant. Grav. 34
Original
2017
Later among the works it cites.
D. P. Mihaylov and J. R. Gair, Transition of EMRIs through resonance: corrections to higher order in the on-resonance flux modification, J. Math. Phys. 58

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2023

Self-forced inspirals with spin-orbit precession

Lynch, Philip, van de Meent, Maarten, Warburton, Niels

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We develop the first model for extreme mass-ratio inspirals (EMRIs) with misaligned angular momentum and primary spin, and zero eccentricity -- also known as quasi-spherical inspirals -- evolving under the influence of the first-order in mass ratio gravitational self-force.

The forcing terms are provided by an efficient spectral interpolation of the first-order gravitational self-force in the outgoing radiation gauge.
In order to speed up the calculation of the inspiral we apply a near-identity (averaging) transformation to eliminate all dependence of the orbital phases from the equations of motion while maintaining all secular effects of the first-order gravitational self-force at post-adiabatic order.
The resulting solutions are defined with respect to `Mino time' so we perform a second averaging transformation so the inspiral is parametrized in terms of Boyer-Lindquist time, which is more convenient of LISA data analysis.