EFFICIENT CALCULATION OF ROVIBRATIONAL EIGENSTATES OF SEQUENTIALLY BONDED 4-ATOM MOLECULES

A new efficient and fully symmetry-adapted finite-basis variational method for calculating the rovibrational eigenstates (J greater-than-or-equal-to 0) of any sequentially bonded four-atom molecule is presented. The exact kinetic-energy operator T(VR) in valence coordinates is used in a scheme of successive basis-set contractions. The success of the method is demonstrated with new results for the molecules HCCH, HOOH, and HCNO, respectively linear, nonlinear, and quasilinear. The complexity Of T(VR) contributes little to the computational cost, yielding a Hamiltonian matrix whose elements can all be cheaply calculated from products of arbitrarily accurate one-dimensional integrals; the dominant cost is that of matrix diagonalization. Matrices of up to 6000 X 6000 are used to obtain low-lying levels converged to small fractions of 1 cm-1, even for the difficult case of HOOH. The generalization to J greater-than-or-equal-to 0 allows the calculation of PI states for HCCH and HCNO and effective rotational constants for HCCH, all usefully converged. For the first time nine-dimensional rovibrational wave functions for four-atom systems are calculated without dynamical approximation and with basis sets well completed in all degrees of freedom. For HCCH it is straightforward to obtain hundreds of rovibrational (J=0,1,2) levels converged to better than 1.5 cm-1, opening up the possibility of the systematic refinement of the nuclear potential function V(N).