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The AGN Channel in 3D: Scattering Belts and the Importance of Eccentricity in the Black Hole Population
Active galactic nuclei (AGN) are a promising origin for observed gravitational wave mergers. Current population synthesis models are limited to 1D N-body or Monte Carlo methods which rely on statistical approaches to resolving dynamical scatterings. We present three-dimensional hybrid $N$-body simul
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