We report a comparative dynamics study of the title reaction using a realis
tic double many-body expansion potential energy surface (DMBE I) for ground
-state HO3 [Mol. Phys. 91 (1997) 301], and a recently reported DMBE II [Che
m. Phys. Lett. 334 (2001) 173] surface obtained by modifying DMBE I to fit
extensive ab initio calculations corrected for the complete basis set limit
. The comparison provides strong evidence that the title reaction can be a
significant source of ozone under stratospheric conditions. (C) 2001 Elsevi
er Science B.V. All rights reserved.