The May 2026 preprint arXiv:2605.30369 presents a Constrained Evolutionary TOV Discovery (CETD) pipeline that identifies a narrow basin of ~1.4×10^4 causal equations of state capable of satisfying both the low tidal deformability of GW170817 and the 2.5–2.67 M⊙ secondary in GW190814 within general relativity. Unlike monotonic sound-speed models that force a trade-off between radius and maximum mass, the recovered EoS exhibit a double-peaked sound-speed profile reaching cs²/c² = 0.86–0.99, allowing radii of 11.97–12.29 km at 1.4 M⊙ while still supporting Mmax up to 2.8 M⊙. This non-monotonic structure was missed in earlier analyses that treated the two events as separate constraints rather than joint boundary conditions on the same dense-matter phase space. The CETD search is entirely theoretical; it does not incorporate new observational data and remains a preprint without peer review. Its principal limitation is the assumption of a single unified EoS across both events, ignoring possible first-order phase transitions or temperature effects in merger remnants. When placed alongside the original LIGO-Virgo publications (Abbott et al. 2017, PRL 119, 161101; Abbott et al. 2020, ApJ 896, L44) and the 2023 Bayesian EoS meta-analysis by Huth et al. (Nature 606, 276), the new basin suggests that the apparent tension was largely an artifact of overly restrictive monotonic priors rather than a fundamental conflict with nuclear theory. The work therefore reframes the 2.6 M⊙ object in GW190814 as a plausible neutron star whose existence demands a temporary softening followed by stiffening of the speed of sound near 3–4 times nuclear saturation density.