Input: oh_runmrci1.com Output: oh_runmrci1.out
The following table is printed at the end of the output:
RESULTS METHOD STATE S ENERGY DIPX DIPY DIPZ CASSCF 1.2 0.5 -75.41331789 0.0 0.0 0.67158730 CASSCF 1.3 0.5 -75.41331789 0.0 0.0 0.67158730 CASSCF 1.1 0.5 -75.24125256 0.0 0.0 0.69975340 MRCI 1.2 0.5 -75.55518444 0.0 0.0 0.66457191 MRCI+D 1.2 0.5 -75.56014871 0.0 0.0 0.66457191 MRCI+P 1.2 0.5 -75.55853208 0.0 0.0 0.66457191 MRCI 1.3 0.5 -75.55518444 0.0 0.0 0.66457191 MRCI+D 1.3 0.5 -75.56014871 0.0 0.0 0.66457191 MRCI+P 1.3 0.5 -75.55853208 0.0 0.0 0.66457191 MRCI 1.1 0.5 -75.39442202 0.0 0.0 0.70484623 MRCI+D 1.1 0.5 -75.40040680 0.0 0.0 0.70484623 MRCI+P 1.1 0.5 -75.39846312 0.0 0.0 0.70484623
This calculation performs MRCI calculations for both and . The procedure is not clever enough to recognize that they are degenerate. However, one can easily modify the input to eliminate this drawback.
Input: oh_runmrci2.com Output: oh_runmrci2.out
This produces
RESULTS METHOD STATE S ENERGY DIPX DIPY DIPZ CASSCF 1.2 0.5 -75.41331789 0.0 0.0 0.67158730 CASSCF 1.3 0.5 -75.41331789 0.0 0.0 0.67158730 CASSCF 1.1 0.5 -75.24125256 0.0 0.0 0.69975340 MRCI 1.2 0.5 -75.55518444 0.0 0.0 0.66457191 MRCI+D 1.2 0.5 -75.56014871 0.0 0.0 0.66457191 MRCI+P 1.2 0.5 -75.55853208 0.0 0.0 0.66457191 MRCI 1.1 0.5 -75.39442202 0.0 0.0 0.70484623 MRCI+D 1.1 0.5 -75.40040680 0.0 0.0 0.70484623 MRCI+P 1.1 0.5 -75.39846312 0.0 0.0 0.70484623
You may want to extend the active space to include the orbitals. This can be achieved by setting the variable OCC.
Input: oh_runmrci3.com Output: oh_runmrci3.out
For accurate calculations of the electronic transition moment, also the orbitals contribute significantly. These are in symmetry 1 ( ) and 4 (). In order to force the orbital to become the , we must use the SYM directive in the SCF calculation. Since it is not possible to insert this into the procedure, we must write the SCF input explicitly.
Input: oh_runmrci4.com Output: oh_runmrci4.out
Note that this calculation is quite expensive!
P.J. Knowles and H.-J. Werner