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We discuss the effects of the black holes' spin-multipole structure in the orbital dynamics of binary black holes according to general relativity, focusing on the leading-post-Newtonian-order couplings at each order in an expansion in the black holes' spins.
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K. Kyrian and O. Semerak, “Spinning test particles in a Kerr field,” Mon. Not. Roy. Astron. Soc. 382
2007
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2008
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2008
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2008
L. Barack, “Gravitational self-force: Orbital mechanics beyond geodesic motion,” in General Relativity, Cosmology and Astrophysics , Fundamental Theories of Physics, Vol. 177 (Springer International Publishing, 2014) pp. 147–168
2014
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2014
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I. Z. Rothstein, “Progress in effective field theory approach to the binary inspiral problem,” Gen. Rel. Grav. 46
2014
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2015
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T. Damour and A. Nagar, “Relativistic tidal properties of neutron stars,” Phys. Rev. D80
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