19.01.2015 Views

MOLPRO

MOLPRO

MOLPRO

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

20 THE CI PROGRAM 149<br />

ROTREF=value<br />

If value=0 the cluster corrections are not printed for the rotated<br />

reference energies (cf. Section 20.7). If value=1 all corrections<br />

are printed. If value=-1 the 2009.1 behaviour is recovered.<br />

20.1 Introduction<br />

The internally contracted MRCI program is called by the CI command. This includes as special<br />

cases single reference CI, CEPA, ACPF, MR-ACPF and MR-AQCC. For closed-shell reference<br />

functions, a special faster code exists, which can be called using the CISD, QCI, or CCSD<br />

commands. This also allows to calculate Brueckner orbitals for all three cases (QCI and CCSD<br />

are identical in this case).<br />

With no further input cards, the wavefunction definition (core, closed, and active orbital spaces,<br />

symmetry) corresponds to the one used in the most recently done SCF or MCSCF calculation.<br />

By default, a CASSCF reference space is generated. Other choices can be made using<br />

the OCC, CORE, CLOSED, WF, SELECT, CON, and RESTRICT cards. The orbitals are taken<br />

from the corresponding SCF or MCSCF calculation unless an ORBITAL directive is given. The<br />

wavefunction may be saved using the SAVE directive, and restarted using START. The EXPEC<br />

directive allows to compute expectation values over one-electron operators, and the TRAN directive<br />

can be used to compute transition matrix elements for one-electron properties. Natural<br />

orbitals can be printed and saved using the NATORB directive.<br />

For excited state calculations see STATE, REFSTATE, and PROJECT.<br />

20.2 Specifying the wavefunction<br />

20.2.1 Occupied orbitals<br />

OCC,n 1 ,n 2 ,...,n 8 ;<br />

n i specifies numbers of occupied orbitals (including CORE and CLOSED) in irreducible representation<br />

number i. If not given, the information defaults to that from the most recent SCF,<br />

MCSCF or CI calculation.<br />

20.2.2 Frozen-core orbitals<br />

CORE,n 1 ,n 2 ,...,n 8 ;<br />

n i is the number of frozen-core orbitals in irrep number i. These orbitals are doubly occupied<br />

in all configurations, i.e., not correlated. If no CORE card is given, the program uses the same<br />

core orbitals as the last CI calculation; if there was none, then the atomic inner shells are taken<br />

as core. To avoid this behaviour and correlate all electrons, specify<br />

CORE<br />

20.2.3 Closed-shell orbitals<br />

CLOSED,n 1 ,n 2 ,...,n 8<br />

n i is the number of closed-shell orbitals in irrep number i, inclusive of any core orbitals. These<br />

orbitals do not form part of the active space, i.e., they are doubly occupied in all reference CSFs;<br />

however, in contrast to the core orbitals (see CORE), these orbitals are correlated through single

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!