The main input groups (those with the "*" prompt) are listed here and the full descriptions are given in the designated sections.
The first input group is always required to specify the type of calculation, and follows immediately after the **WAVE FUNCTIONS keyword.
The remaining input groups may be specified in any order. In this chpater they are grouped alphabetcially, although the short presentation below gather them according to purpose.
The following two input groups are used to modify the molecular environment by adding field-dependent terms in the Hamiltonian and by invoking the self-consistent reaction field model for solvent effects, respectively:
The following input group describes additional field-dependent terms in the Hamiltonian :
The next input group specifies the configurations included in the MCSCF and CI wave functions:
The two next groups are used to specify initial orbitals and initial guess for the CI vector:
The two following input groups control the second-order MCSCF optimization:
The next three groups have special input only relevant for the respective calculation types:
The next section is used to select some types of analysis of the final MCSCF or CI wave function:
The next section is used to change the default integral transformation and specify any final integral transformation after convergence (a program following SIRIUS may need a higher transformation level):
The final two input groups control the amount of printed output and collect options not fitting in any of the other groups:
The wave function input is finished when a line is encountered beginning with two stars, for example
**END OF INPUTor
**MOLORB ... formatted molecular orbitals coefficients **END OF INPUT
The **MOLORB keyword or the **NATORB keyword must be somewhere on the input file and be followed by molecular orbital coefficients if the option for formatted input of molecular orbitals has been specified. Apart from this requirement, arbitrary information can be written to the following lines of the input file.