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We estimate the accuracy in the measurement of the tidal Love number of a supermassive compact object through the detection of an extreme mass ratio inspiral~(EMRI) by the future LISA mission.
1903
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A. Le Tiec and M. Casals, “Spinning Black Holes Fall in Love,” Phys. Rev. Lett
2007
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L. Barack and C. Cutler, “Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes,” Phys. Rev
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M. Vallisneri, “Use and abuse of the Fisher information matrix in the assessment of gravitational-wave parameter-estimation prospects,” Phys. Rev. D
2008
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T. Binnington and E. Poisson, “Relativistic theory of tidal Love numbers,” Phys. Rev. D
2009
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T. Damour and A. Nagar, “Relativistic tidal properties of neutron stars,” Phys. Rev. D
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L. Barack, “Gravitational self force in extreme mass-ratio inspirals,” Class. Quant. Grav
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A. Le Tiec, M. Casals, and E. Franzin, “Tidal Love Numbers of Kerr Black Holes,” Phys. Rev. D
2010
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H. S. Chia, “Tidal deformation and dissipation of rotating black holes,” Phys. Rev. D
2010
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C. Posada, “Slowly rotating supercompact Schwarzschild stars,” Mon. Not. Roy. Astron. Soc
2017
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2011
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2012
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2012
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S. A. Hughes, “Evolution of circular, nonequatorial orbits of Kerr black holes due to gravitational wave emission. II. Inspiral trajectories and gravitational wave forms,” Phys. Rev. D
2013
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Cambridge University Press, 2014
E. Poisson and C. Will, Gravity: Newtonian, Post-Newtonian, Relativistic · 2014
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2018
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G. Raposo, P. Pani, and R. Emparan, “Exotic compact objects with soft hair,” Phys. Rev. D
2019
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2019
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S. A. Hughes, “Bound orbits of a slowly evolving black hole,” Phys. Rev. D
2019
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2019
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