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Binary black hole spin measurements from gravitational wave observations can reveal the binary's evolutionary history.
1904
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1905
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1912
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1961
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1973
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M. J. Fitchett, “The influence of gravitational wave momentum losses on the centre of mass motion of a Newtonian binary system,” Monthly Notices of the Royal Astronomical Society 203
1983
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1994
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Oleg Y. Gnedin, HongSheng Zhao, J. E. Pringle, S. Michael Fall, Mario Livio, and Georges Meylan, “The unique history of the globular cluster omega centauri,” Astrophys. J. Lett. 568
2002
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Jeremy D. Schnittman, “Spin-orbit resonance and the evolution of compact binary systems,” Phys. Rev. D 70
2004
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David Merritt, Milos Milosavljevic, Marc Favata, Scott A. Hughes, and Daniel E. Holz, “Consequences of gravitational radiation recoil,” Astrophys. J. 607
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Eric Poisson, “Absorption of mass and angular momentum by a black hole: Time-domain formalisms for gravitational perturbations, and the small-hole / slow-motion approximation,” Phys. Rev. D 70
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2007
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J. A. Gonzalez, M. D. Hannam, U. Sperhake, Bernd Bruegmann, and S. Husa, “Supermassive recoil velocities for binary black-hole mergers with antialigned spins,” Phys. Rev. Lett. 98
2007
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2009
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LIGO Scientific Collaboration and Virgo Collaboration, “GWTC-1,” https://doi.org/10.7935/82H3-HH23 (2018)
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LIGO Scientific Collaboration and Virgo Collaboration, “GWTC-2,” https://doi.org/10.7935/99gf-ax93 (2020)
2020
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