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| .. | ||
| c2h6-ri00.nwc | ||
| c2h6-ri00.out | ||
| c2h6-rifc00.nwc | ||
| c2h6-rifc00.out | ||
| c2h6-rifc01.nwc | ||
| c2h6-rifc01.out | ||
| c2h6-rifc02.nwc | ||
| c2h6-rifc02.out | ||
| c2h6-scf.nwc | ||
| fit.lib | ||
| h2o-rifc02.nwc | ||
| h2o-rifc02.out | ||
| h2o-scf.nwc | ||
| hf-rifc02.nwc | ||
| hf-rifc02.out | ||
| hf-scf.nwc | ||
| README | ||
$Id: README,v 1.3 1999-09-29 23:27:06 gg502 Exp $ Here are a few small examples of RI-MP2 calculations, along with the associated SCF input decks. Most of them freeze a couple of core orbitals, but one of the C2H6 ones doesn't. They all take the fitting basis sets from fit.lib. First run the *-scf.nwc calculation, then run any of the corresponding *-ri*.nwc calculations. The numbers used at the end of the input deck names (00, 01, 02) indicate the use of different fitting basis sets, and you should be able to run more than one such calculation without re-doing the SCF calculation. Note, however, that frozen core specifications (*-rifc*.nwc jobs) stay in the .db file, and so will effect future calculations restarted from the same .db file. This means if you run the sequence c2h6-scf.nwc, c2h6-rifc00.nwc, c2h6-ri00.nwc the frozen core directive from the second job will also effect the third one! The simplest approach is to do any all-electron calculations BEFORE any of the frozen core ones. These jobs were run on an SGI PowerChallenge (1 CPU) 12 February 1997