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We compute the linear metric perturbation to a Schwarzschild black hole generated by a spinning compact object, specialising to circular equatorial orbits with an (anti-)aligned spin vector.
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S. Detweiler, A consequence of the gravitational self-force for circular orbits of the schwarzschild geometry, Physical Review D - Particles, Fields, Gravitation and Cosmology 77
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N. Warburton, T. Osburn, and C. R. Evans, Evolution of small-mass-ratio binaries with a spinning secondary, Phys. Rev. D 96
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A. Pound, Nonlinear gravitational self-force: second-order equation of motion, Phys. Rev. D 95
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2017
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S. Hopper and C. R. Evans, Gravitational perturbations and metric reconstruction: Method of extended homogeneous solutions applied to eccentric orbits on a schwarzschild black hole, Phys. Rev. D 82
2010
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A. Pound, Self-consistent gravitational self-force, Phys. Rev. D 81
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A. I. Harte, Mechanics of extended masses in general relativity, Class. Quant. Grav. 29
2012
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2013
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2013
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2018
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2018
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2019
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2019
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2019
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2019
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J. E. Thompson, B. Wardell, and B. F. Whiting, Gravitational self-force regularization in the regge-wheeler and easy gauges, Phys. Rev. D 99
2019
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D. Bini, A. Geralico, and J. Steinhoff, Detweiler’s redshift invariant for extended bodies orbiting a schwarzschild black hole, Phys. Rev. D 102
2020
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2021
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2021
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2021
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I. Timogiannis, G. Lukes-Gerakopoulos, and T. A. Apostolatos, Spinning test body orbiting around a schwarzschild black hole: Comparing spin supplementary conditions for circular equatorial orbits, Phys. Rev. D 104
2021
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2021
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V. Skoupý and G. Lukes-Gerakopoulos, Spinning test body orbiting around a kerr black hole: Eccentric equatorial orbits and their asymptotic gravitational-wave fluxes, Phys. Rev. D 103
2021
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2021
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V. Witzany, (private communications) (2021)
2021
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