Statistical comparisons show good agreement between higher-order PN and perturbation schemes for million-solar-mass black holes but divergences and unreliable orbital decay in pairwise PN for billion-solar-mass cases.
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A benchmark for binary star interaction with a supermassive black hole in general relativity
Statistical comparisons show good agreement between higher-order PN and perturbation schemes for million-solar-mass black holes but divergences and unreliable orbital decay in pairwise PN for billion-solar-mass cases.