In addition, the same options as for CCSD can be used.
BCCD performs a Brueckner coupled-cluster calculation and computes Brueckner orbitals. With these orbitals, the amplitudes of the singles vanish at convergence. Using the BCCD(T) command, the contributions of connected triples are also computed by perturbation theory. Normally, no further input is needed if the BCCD card follows the corresponding HF-SCF. Otherwise, occupancies and orbitals can be specified as in the CI program. BRUECKNER parameters can be modified using the BRUECKNER directive.
The Brueckner orbitals and approximate density matrix can be saved on a MOLPRO dump record using the SAVEORB option. The orbitals are printed if the PRINT option is given. TYPE can be used to specify the type of the approximate density to be computed:
Note: The expectation variables are stored in variables as usual. In the case that both densities are made, the variables contain two values, the first corresponding to REF and the second to TOT (e.g., DMZ(1) and DMZ(2)). If TYPE=REF or TYPE=TOT is give, only the corresponding values are stored.
For avoiding error exits in case of no convergence, see CCSD(T).