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    • Distinguishing Black-Hole Spin-Orbit Resonances by their Gravitational-Wave Signatures 

      Gerosa, D.; O'Shaughnessy, R.; Kesden, Michael; Berti, E.; Sperhake, U. (American Physical Society, 2014-06-24)
      If binary black holes form following the successive core collapses of sufficiently massive binary stars, precessional dynamics may align their spins, S₁ and S₂, and the orbital angular momentum L into a plane in which they ...