“…As a consequence, the HO 2 system has been the topic of numerous electronic structure calculations of its potential energy surface [10,11,12,13,14,15] as well as dynamics calculations to evaluate its temperature dependent rate coefficients [13,14,16,17,18,19,20,21,22,23,24,25,26]. The reaction has also been the focus of a large number of experimental measurements [27,28,29,30,31,32,33,34,35,36]. However, there still remains significant discrepancy between measured and computed values of its rate coefficients for temperatures below 200 K, which is the most important region for astrophysical and upper atmospheric applications.…”