“…5,10,13 However, it has been shown to break down in NO(X) + Kr and Xe scattering, attributed to the stronger attractive forces in these more polarizable systems. [14][15][16] In these measurements of NO(A) + Kr scattering, there is good agreement between QS and KA models for backward scattering for all N 0 , indicating that collisions at low-l that probe the repulsive wall are well described by the KA model. In contrast, significant disagreements are seen between QS and KA models for forward scattering, which the PCSs show is arising for all N 0 from the attractive regions of the PES.…”