“…At the higher end, we are in the regime of intermediate velocities, where the orbiting velocity of the bound H(ls) electron matches the collision velocity; excitation takes places via so-called 'direct' processes at large internuclear separations, resulting in a large transition probability and in a preferred orientation of the excited electronic charge cloud after the collision (propensity rule) [8]. In the two regimes, calculations based on different theoretical models, for example, molecular orbital [9], close-coupling [10][11][12], optical potential [13], and first Born calculations [143 are available to compare our results with.…”