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Dynamical tides reexpressed

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The first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range

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Properties of the Binary Black Hole Merger GW150914

(2016) B. P. Abbott et al.   PHYSICAL REVIEW LETTERS

Black Hole Spin via Continuum Fitting and the Role of Spin in Powering Transient Jets

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Compact binary coalescences in the band of ground-based gravitational-wave detectors

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Black Hole Spin Evolution: Implications for Short‐Hard Gamma‐Ray Bursts and Gravitational Wave Detection

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