The H-3 potential energy surface has been calculated using the Cashion-Hers
hbach (CH) potential which contains all orders of two-body Coulomb, exchang
e, and overlap terms. For collinear configurations, the dominant three-body
contribution comes from the Axilrod-Teller-Muto triple-dipole dispersion e
nergy. By adding only this term, properly damped, the saddle point region p
otential agrees with recent ab initio calculations to within 9 x 10(-5) a.u
. (0.06 kcal/mole). (C) 2000 Elsevier Science B.V. All rights reserved.