“…At the low collision energies, E coll , typical of orbiting resonances, the number of partial waves implied in the dynamics is relatively small and this circumstance facilitates the performance of precise fundamental calculations, as a consequence there is a growing interest, both experimental and theoretical, in the stereodynamics of collisions in this low E coll range. [19][20][21][22][23][24][25][26] The pioneering work of Balakrishnan and Dalgarno [27] on reactivity at ultra-low temperatures was performed for the F + H 2 system and, at temperatures down to a few K, the reaction is also of interest in astrophysics, where the HF molecule is used to estimate the depletion of fluorine from ice mantles in dense clouds, and as a tracer of H 2 in the diffuse interstellar medium [28,29]. This reaction, which has been a prototype in the field of reaction dynamics since the seventies, is very well known in many respects.…”