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I am now calculating the CeO8 cluster in EBM. After the the RASSCF calculation, I asked the RASSI>TRDI to give me the transition intensity, but they were not printed out and the programs said "No problematic oscillator strengths above the tolerance have been found". Could you please help me to check the problem. And also one additional questions, is there any way to print quadrupole transition intensities by one key work instead of asking for the transition eigenvalue matrixes.
The RAS1 is 2p, RAS2 is ligand orbitals, RAS3 is 5d
&RASSCF
Spin = 1
HEXS = 1; 1
Symmetry = 2
NActEl * Nel, h RAS1, n RAS3
14 1 1
LUMORB * Read Orb from INPORB
TypeIndex * Read OrbType from INPORB
CIRoot = 48 48 1 * NRoots NDacidsons
Iter
200 100
OrbListing * List all Orbs
All
OrbAppear * OrbList Print Level
Compact
SupSym
0
1; 1 1
1; 1 1
1; 1 6
1; 1 1
1; 1 6
1; 1 6
1; 2 5 6
End of Input
>> COPY $Project.JobIph $CurrDir/$Project.EXC.JobIph
>> COPY $CurrDir/$Project.GS.JobIph JOB001
>> COPY $CurrDir/$Project.EXC.JobIph JOB002
&RASSI
SpinOrbit * SOC Calc
Nr of JobIphs * Input States
2 All
SubSets = 2
TRDI
End of InputLast edited by Sihan Zhang (2025-05-16 11:46:47)
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According to the documentation:
TRDI
Prints out the components and the module of the transition dipole vector. Only vectors with sizes large than 1.0D-4 a.u. are printed. See also the TDMN keyword.
You probably want to use the keywords TDMN and/or DIPR.
For the quadrupole transitions, try QIAL and QIPR
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I tried all of them, even reduce the TDMN to 1.0D-10, still not working. I initially thought it is an input file or version problem, so i just tried the same calculation for CeF6, and got some intensities.
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Maybe they're zero? Try with zero (or negative) thresholds.
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Actually, they are not zero. I later asked for the input file from one paper author. I noticed that it was because of the keywork Symmetry in RASSCF. I need to give a corresponding symmetry of the transition. Then I can get the intensity. I know how to solve it, but still curious about what happened behind.
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I faced with the same problem.
Could you please give me more detail about your solutions?
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I faced with the same problem.
Could you please give me more detail about your solutions?
I put my files here.
&RASSCF
Spin = 1
Symmetry = 5
HEXS = 1; 1
NActEl
8 1 1
LUMORB
TypeIndex
CIRoot = 16 16 1
....
End of Input&RASSI
SpinOrbit
Nr of JobIphs
3 All
SubSets = 3
EJob
DIPrint = 1.0D-8
End of InputIf you defined the symmetry, then you need to specify the state symmetry in RASSCF module, or it will calculate on the default value 1. This can be forbidden by the selection rule depends on the symmetry. For example, my system is in Oh symmetry (C2h in Molcas), ground state is 1 (Ag), excited states are 2/3/5 (B1/2/3u). This is allowed by dipole selection rule.
Last edited by Sihan Zhang (2026-02-28 23:07:15)
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Thanks
Could you please give me more detail about Symmetry =5 in your inout. How can I know the Symmetry?
I have tried Symmetry= from 1 to 8 in my inout, but it did not help.
Below is my input.
###################################
&GATEWAY
COORD
3
C 0.0000000000 0.0000000000 0.0000000000
O1 0.0000000000 0.0000000000 -1.1620000000
O2 0.0000000000 0.0000000000 1.1620000000
BASIS=cc-pVTZ
GROUP=FULL
AMFI
&SEWARD
&SCF
&RASSCF
GUGA
SPIN=1
CIROOT=18 18 1
Inactive = 4 1 1 0 2 1 1 0
Ras2 = 5 5 5 2 15 4 4 2
Symmetry=1
&RASSI
TDMN
1.0D-8
Nr of JobIphs
1 ALL##########################################
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Thanks
Could you please give me more detail about Symmetry =5 in your inout. How can I know the Symmetry?
I have tried Symmetry= from 1 to 8 in my inout, but it did not help.
Below is my input.
1. See this link https://molcas.gitlab.io/OpenMolcas/sph … teway.html
You didn't define the symmetry, therefore, the irrep notation can not work. You can modify in this way:
Suppose you need to calculate in D2h, since I saw you use 8 irreps in the RASSCF module.
COORD
3
C 0.0000000000 0.0000000000 0.0000000000
O1 0.0000000000 0.0000000000 -1.1620000000
SYMMETRY = X Y ZThe second O can be generated by the symmetry.
2. Do calculations in two different irreps. You use RASSI directly after the RASSCF, there is only the states of Ag irrep. The dipole transition between them us forbidden. You need run two calculations for Ag and B1/2/3u to obtain the transition by reading their JobIph/JobMix files, or other irrep combination depending on the state symmetry and tensor product table.
These are carefully written in the manual:
https://molcas.gitlab.io/OpenMolcas/sph … ex-ex.html
Last edited by Sihan Zhang (2026-03-01 17:10:02)
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Thank you very much Sihan Zhang

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