T₉₀ ∝ (L_iso)^−0.5 correlation (solid blue line) for the GRBs with reported polarization detections (red stars), along with the high-efficiency sample (orange stars; Meng 2022) and the high-energy sample (cyan stars; E_γ, beam ≳10⁵² erg, obtaining a GeV/TeV detection; Sharma et al. 2021). Notably, all three samples roughly exhibit a power-law shape in their X-ray afterglows. The dashed green lines mark a T₉₀ deviation of a factor of two, from the best-fit log (T₉₀) = 1.67–0.5 log (L_iso) relationship. This T₉₀ ∝ (L_iso)^−0.5 correlation aligns closely with the predictions made by the NDAF model (solid red line), which is under the hot fireball framework.