Spin-up and mass-gain in hyperbolic encounters of spinning black holes

Healey Kogan; Frederick C. L. Pardoe; Helvi Witek

doi:10.1103/j7ch-t96d

paper

Spin-up and mass-gain in hyperbolic encounters of spinning black holes

arXiv:2511.00307 · doi:10.1103/j7ch-t96d

Abstract

Scattering black holes spin up and gain mass through the re-absorption of orbital angular momentum and energy radiated in gravitational waves during their encounter. In this work, we perform a series of numerical relativity simulations to investigate the spin-up and mass-gain for equal-mass black holes with a wide range of equal initial spins, $χ_{i} \in [- 0.7, 0.7]$ , aligned (or anti-aligned) to the orbital angular momentum. We also consider a variety of initial momenta. Furthermore, we explore a range of incident angles and identify the threshold between scattering and merging configurations. The spin-up and mass-gain are typically largest in systems with incident angles close to the threshold value, large momenta, and negative (i.e. anti-aligned) initial spins. When evaluated at the threshold angle, we find that the spin-up decreases linearly with initial spin. Intriguingly, systems with initial spin $χ_{i} = 0.7$ sometimes experience a spin-down, in spite of an increase in the black-hole angular momentum, due to a corresponding gain in the black-hole mass. Across the simulation suite, we find a maximum spin-up of $0.3$ and a maximum increase in the black-hole mass of $15%$ .

arXiv comment23 pages, 23 figures; matches version published in PRD

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Cited by in corpus (1)

Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results