Dynamical analysis. Cool-core clusters are shown in blue, and hot-core clusters in orange. Solid lines indicate moving medians, and dashed lines indicate 16% and 84% percentiles (2σ) from the Magneticum simulation (Box2b/hr). Left panel: Freedom ratio for all particles inside the core region (F_c, total). Central panel: Freedom ratio for gas particles inside the core region (F_c, gas). Right panel: Kinetic energy fraction f_{c, gas, kinetic} for gas particles inside the core region. The black bar indicates the first and only measurement of kinetic energy fraction in galaxy clusters, of 10% measured for the Perseus cluster by Hitomi (Hitomi Collaboration 2018).