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We establish a generic, fully-relativistic formalism to study gravitational-wave emission by extreme-mass-ratio systems in spherically-symmetric, non-vacuum black-hole spacetimes.
1904
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N. Sago, H. Nakano, and M. Sasaki, Gauge problem in the gravitational selfforce. 1. Harmonic gauge approach in the Schwarzschild background, Phys. Rev. D 67
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K. Martel, Gravitational wave forms from a point particle orbiting a Schwarzschild black hole, Phys. Rev. D 69
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K. Martel and E. Poisson, Gravitational perturbations of the Schwarzschild spacetime: A Practical covariant and gauge-invariant formalism, Phys. Rev. D 71
2005
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P. A. Sundararajan, G. Khanna, and S. A. Hughes, Towards adiabatic waveforms for inspiral into Kerr black holes. I. A New model of the source for the time domain perturbation equation, Phys. Rev. D 76
2007
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S. Babak, H. Fang, J. R. Gair, K. Glampedakis, and S. A. Hughes, ’Kludge’ gravitational waveforms for a test-body orbiting a Kerr black hole, Phys. Rev. D 75
2008
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2009
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2020
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2010
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K. Mitman et al. , Nonlinearities in black hole ringdowns, (2022), arXiv:2208.07380 [gr-qc]
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K. G. Arun et al. (LISA), New horizons for fundamental physics with LISA, Living Rev. Rel. 25
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