Input: h2o_casscf.com Output: h2o_casscf.out
This could be extended, for instance, by the following input cards
OCC,4,1,2; ! specify occupied space CLOSED,2 ! specify closed-shell (inactive) orbitals CORE,1; ! specify frozen core orbitals WF,10,1; ! define wavefunction symmetry START,2100.2; ! read guess orbitals from record 2100, file 2 ORBITAL,2140.2; ! save final orbitals to record 2140, file 2 NATORB,PRINT,CI ! print natural orbitals and diagonalize the hamiltonian ! for the natural orbitals. The largest CI coefficients ! are printed.
Example for a state-averaged calculation for CN, and states, and , states averaged. A full valence CASSCF calculation is performed
Input: cn_sa_casscf.com Output: cn_sa_casscf.out
Example for an RASSCF (restricted active space) calculation for N, including SCF determinant plus all double excitations into valence orbitals. The single excitations are excluded. symmetry, CSF method used:
Input: n2_rasscf.com Output: n2_rasscf.out