The origin of the correlation between the effective spins () and mass ratios () of LIGO-Virgo-KAGRA’s binary black holes (BBHs) is still an open question. Motivated by the recent identification of two subpopulations of the BBHs, in this work we investigate the potential correlation for each subpopulation. Surprisingly, the - correlation {either significantly weakens or disappears} for the low-mass subpopulation if we introduce a second distribution for the high-mass subpopulation, which likely originates from hierarchical mergers. {This suggests that the - correlation in the overall population can be explained by the superposition of two distinct subpopulations.} {We find Bayesian evidence strongly favoring two separate distributions over a single mass-ratio-dependent distribution, with Bayes factors .} The first subpopulation has a narrow distribution peaking at , whose primary-mass function {showing a rapid decline beyond} , in agreement with first-generation BBHs. The second distribution is broad and peaks at , aligning with predictions for hierarchical mergers in active galactic nucleus (AGN) disks. {However, we cannot exclude negative values in the second subpopulation, suggesting hierarchical mergers might occur both in AGN disks and stellar clusters. Furthermore, the inferred second distribution might alternatively arise from other formation channels, such as stable mass transfer or chemically homogeneous evolution, if not interpreted as hierarchical mergers.}

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