“…Any slight potential barrier would be of paramount importance in low-temperature environments. Second, in cold interstellar clouds, typical temperatures of 10-30 K correspond to mean translational energies for collisions, E T = 3/2 RT, of 0.12-0.4 kJ mol −1 , respectively, and branching ratios of the integral cross sections R1 = σ (1b)/σ (1a+1b) and R2 = σ (1c)/σ (1) have only been determined above a relative translational energy (collision energy) of E T = 3.5 kJ mol −1 except for a preliminary measurement of R1 at E T = 0.8 kJ mol −1 (Costes et al 2006). In this paper, we report high-level ab initio electronic structure calculations of c-C 3 H and l-C 3 H performed with the coupledcluster method and high-resolution, differential cross-section measurements in crossed-beam experiments at low energies that allow, with the aid of previous low-temperature kinetic results, determination of the branching ratios R1 and R2 as a function of collision energy.…”