We introduce a novel estimator to quantify statistical tensions among multiple cosmological datasets simultaneously. This estimator generalizes the Difference-in-Means statistic, $Q_{ \rm DM}$, to the multi-dataset regime. Our framework enables the detection of dominant tension directions in the shared parameter space. It further provides a geometric interpretation of the tension for the two- and three-dataset cases in two dimensions. According to this approach, the previously reported increase in tension between DESI and Planck from $1.9\sigma$ (DR1) to $2.3\sigma$(DR2) is reinterpreted as a more modest shift from $1.18\sigma^{ \rm eff}$ (DR1) to $1.45\sigma^{ \rm eff}$ (DR2). These new tools may also prove valuable across research fields where dataset discrepancies arise.
Categories: astro-ph.CO astro-ph.IM hep-ex hep-ph physics.data-an