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20 THE CI PROGRAM 151<br />

WF,15,2,1; !define wavefunction symmetry (2)<br />

REF,1; !define additional reference symmetry (1)<br />

For linear geometries the same results can be obtained more cheaply using C 2v symmetry,<br />

WF,15,2,1; !define wavefunction symmetry (2)<br />

REF,1; !define additional reference symmetry (1)<br />

REF,3; !define additional reference symmetry (3)<br />

or<br />

WF,15,3,1; !define wavefunction symmetry (2)<br />

REF,1; !define additional reference symmetry (1)<br />

REF,2; !define additional reference symmetry (2)<br />

Each REF card may be followed by RESTRICT, SELECT, and CON cards, in the given order.<br />

20.2.7 Selecting configurations<br />

SELECT,ref1,ref2,refthr,refstat,mxshrf ;<br />

This card is used to specify a reference configuration set other than a CAS, which is the default.<br />

Configurations can be defined using CON cards, which must appear after the SELECT card.<br />

Alternatively, if ref1 is an existing <strong>MOLPRO</strong> record name, the configurations are read in from<br />

that record and may be selected according to a given threshold.<br />

The select card should normally be placed directly after the WF or REF card(s), or, if present,<br />

the RESTRICT cards. The general order of these cards is<br />

WF (or REF)<br />

RESTRICT (optional)<br />

SELECT (optional)<br />

CON (optional)<br />

ref1=rec1.file:<br />

ref2=rec2.file:<br />

refthr:<br />

(rec1>2000) The configurations are read in from the specified<br />

record. See section 19.5.4 about how to save the configurations<br />

in the MCSCF calculation. If ref1 is not specified, the program<br />

assumes that the configurations are read from subsequent CON<br />

cards (see CON).<br />

(rec2>2000) additional configurations are read from the specified<br />

record. If rec2 is negative, all records between rec1 and<br />

abs(rec2) are read. All configurations found in this way are<br />

merged.<br />

Selection threshold for configurations read from disc (records<br />

rec1–rec2). This applies to the norm of all CSFs for each orbital<br />

configuration.

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