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Creators/Authors contains: "Lima, Alicia"

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  1. Free, publicly-accessible full text available May 1, 2026
  2. In the post-Newtonian regime, the time it takes two black holes to orbit each other is much shorter than the time it takes their spins and the orbital angular momentum to precess about the direction of the total angular momentum, which in turn is shorter than the orbital decay time. We use the parameters quantifying the component black hole spins in and out of the orbital plane to build an interactive 3D visualization to explore the phenomenology of spin precession over these different time scales. 
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