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Complete waveform models able to account for arbitrary non-planar orbits represent a holy grail in current gravitational-wave astronomy.
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Thibault Damour, Piotr Jaranowski, and Gerhard Schaefer, “On the determination of the last stable orbit for circular general relativistic binaries at the third postNewtonian approximation,” Phys. Rev. D62
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Thibault Damour, “Coalescence of two spinning black holes: An effective one- body approach,” Phys. Rev. D64
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Jeremy D. Schnittman, “Spin-orbit resonance and the evolution of compact binary systems,” Phys. Rev. D 70
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Raoul-Martin Memmesheimer, Achamveedu Gopakumar, and Gerhard Schaefer, “Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits,” Phys. Rev. D 70
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Alessandra Buonanno, Yan-bei Chen, and Michele Vallisneri, “Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit,” Phys. Rev. D67
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