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I am calculating SA-CASSCF+MS-CASPT2. I would like to know the character of the MS-CASPT2 roots. I find the following output. Do the u,d and 2 represent the occupation of SA-CASSCF natural orbitals, which could be visualized with GRID_IT and Luscus?
Thanks a lot!
THE ORIGINAL CI ARRAYS ARE NOW MIXED AS LINEAR
COMBINATIONS, GIVEN BY THE EIGENVECTORS.
A NEW JOBIPH FILE NAMED 'JOBMIX' IS PREPARED.
********************************************************************************
++ Mixed CI coefficients:
The CI coefficients for the MIXED state nr. 1
--------------------------------------------------------------------------------
CI COEFFICIENTS LARGER THAN 0.50D-01
Occupation of active orbitals, and spin coupling
of open shells. (u,d: Spin up or down).
SGUGA info is (Midvert:IsyUp:UpperWalk/LowerWalk)
Conf SGUGA info Occupation Coefficient Weight
87 ( 2:1: 1/ 11) u22222222222d0 0.804559 0.647316
88 ( 2:1: 2/ 11) u2222222222d20 0.108204 0.011708
90 ( 2:1: 4/ 11) u2222222222dud 0.060648 0.003678
91 ( 2:1: 5/ 11) u2222222222udd -0.151888 0.023070
92 ( 2:1: 6/ 11) u222222222202d -0.070944 0.005033
94 ( 2:1: 8/ 11) u22222222220d2 0.105945 0.011224
155 ( 3:1: 1/ 11) u222222222d220 0.504303 0.254322
156 ( 3:1: 2/ 11) u222222222d2ud -0.073604 0.005418
188 ( 4:1: 1/ 10) u222222222u2dd -0.073096 0.005343
190 ( 4:1: 3/ 10) u222222222udd2 0.058539 0.003427
218 ( 5:1: 1/ 10) u222222222022d 0.090245 0.008144
219 ( 5:1: 2/ 10) u22222222202d2 0.109157 0.011915
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If I'm not mistaken, those should be the same orbitals as the RASSCF: average pseudo-natural orbitals. The mixed CI vectors should be just a linear combination (according to the MS eigenvectors) of the input CI vectors.
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Dear Ignacio,
Thanks so much for your reply!
I have to identify the orbitals that contribute to certain MS-CASPT2 roots. Now I am trying to visualize the CASPT2 orbitals with the following script.
&GATEWAY
coord = geom.xyz
basis = 6-31g*; group= E
RICD
&GRID_IT
FILEORB=input.Pt2Orb.1
all
I used ALTER and SUPSYM to calculate XAS with the core-excited state. But the output *.lus file doesn't show me any core orbitals. All of them look like valence orbitals.
However, the *lus file generated from the RASSCF orbital (*.RasOrb) does show core orbitals.
Do you mean that I could use the RASSCF natural orbitals to analyze the MS-CASPT2 roots?
Thanks a lot!
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The Pt2Orb files should contain the PT2 natural orbitals, i.e., they contain the perturbation correction. I'm not sure they contain the MS mixing. Are they different when you include the NOMULT keyword? The "Mixed CI coefficients" table, on the other hand, contains the mixing, but not the PT2 correction.
The Pt2Orb files should contain the core orbitals, even if they are fully occupied... If they don't, it might be a bug in GRID_IT or Luscus. Note that if you have core orbitals in the active space, you may want to change the number of frozen orbitals in CASPT2.
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