Study computes 1-post-Newtonian coefficients in binary black holes, indicating coherence with general relativity.
TQNT-V5.10b applies the Kerr-V5 foundation (V5.10a) to compute the leading 1-post-Newtonian coefficients and the dominant quasi-normal-mode (QNM) frequencies of the ringdown. Within the precision of the V5-inherited G (V5.8, 0.05%), the V5 results are coherent with general relativity at the level tested by LIGO-Virgo binary black hole events. No tuning is introduced: the comparison is honest, with residuals at the level of V5.8 κ_g uncertainty. Companion to V5.10a. Complements the V5 monograph (10.5281/zenodo.19131538).
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Lilian Cariou (2026) studied this question.
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