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The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux from binary systems are derived to next-to-next-to-leading order in the Post-Newtonian (PN) expansion of general relativity, including finite-size and tail effects.
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M. Maggiore et al. , Science Case for the Einstein Telescope, JCAP 03
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D. Baumann, H. S. Chia, R. A. Porto, and J. Stout, Gravitational Collider Physics, Phys. Rev. D 101
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H. Tagoshi, M. Shibata, T. Tanaka, and M. Sasaki, PostNewtonian expansion of gravitational waves from a particle in circular orbits around a rotating black hole: Up to O ( v 8 ) O(v^{8}) beyond the quadrupole formula, Phys. Rev. D 54
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I. Z. Rothstein, TASI lectures on effective field theories, (2003), arXiv:hep-ph/0308266 [hep-ph]
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M. Punturo et al. , The einstein telescope: A third-generation gravitational wave observatory, Class. Quant. Grav. 27
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T. Dietrich et al. , CoRe database of binary neutron star merger waveforms, Class. Quant. Grav. 35
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