Author Topic: Including COSMO in two-photon absorption calculations  (Read 6055 times)

pharmd

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Including COSMO in two-photon absorption calculations
« on: November 29, 2025, 10:49:14 AM »
Hello,

I cannot find definitive information on whether COSMO is taken into account when computing two-photon absorption properties in TURBOMOLE. I enabled COSMO with $cosmo_correlated using the cosmoprep command after running define, but the TPA results change very little.
Should I add or modify anything in the control file (below)? Any advice on the correct control-file settings or on how to force COSMO into the TPA workflow would be much appreciated.

Many thanks in advance!

Code: [Select]
$cosmo
  rsolv= 1.30
$reaction_field
   econv=  1.0000E-06
   qmaxconv=  1.0000E-05
   qrmsconv=  1.0000E-06
$cosmo_atoms
# radii in Angstrom units
c  1-6,8,10-15,17,19                                                           \
   radius=  2.0000
o  7,9,16,18,20                                                                \
   radius=  1.7200
h  21-30                                                                       \
   radius=  1.3000
$cosmo_out file=out.ccf
$cosmo_data file=cosmo_transfer.tmp
$cosmo_correlated
$title
$symmetry c1
$user-defined bonds    file=coord
$coord    file=coord
$optimize
 internal   off
 redundant  off
 cartesian  on
 global     off
 basis      off
$atoms
c  1-6,8,10-15,17,19                                                           \
   basis =c aug-cc-pVDZ                                                        \
   cbas  =c aug-cc-pVDZ
o  7,9,16,18,20                                                                \
   basis =o aug-cc-pVDZ                                                        \
   cbas  =o aug-cc-pVDZ
h  21-30                                                                       \
   basis =h aug-cc-pVDZ                                                        \
   cbas  =h aug-cc-pVDZ
$basis    file=basis
$scfmo   file=mos
$closed shells
 a       1-70                                   ( 2 )
$scfiterlimit      100
$scfconv        7
$thize     0.10000000E-04
$thime        5
$scfdamp   start=0.300  step=0.050  min=0.100
$scfdump
$scfintunit
 unit=30       size=0        file=twoint
$scfdiis
$maxcor    500 MiB  per_core
$scforbitalshift  automatic=.1
$drvopt
   cartesian  on
   basis      off
   global     off
   hessian    on
   dipole     on
   nuclear polarizability
$interconversion  off
   qconv=1.d-7
   maxiter=25
$coordinateupdate
   dqmax=0.3
   interpolate  on
   statistics    5
$forceupdate
   ahlrichs numgeo=0  mingeo=3 maxgeo=4 modus=<g|dq> dynamic fail=0.3
   threig=0.005  reseig=0.005  thrbig=3.0  scale=1.00  damping=0.0
$forceinit on
   diag=default
$energy    file=energy
$grad    file=gradient
$forceapprox    file=forceapprox
$denconv     0.10000000E-06
$freeze
 implicit core=   20 virt=    0
$cbas    file=auxbasis
$laplace
  conv=5
$ricc2
$excitations
    irrep=a  multiplicity=  1  nexc=  5
    twophoton  states=all  operators=(diplen,diplen)
$rundimensions
   natoms=30
   nbf(CAO)=590
   nbf(AO)=550
$last step     ricc2
$orbital_max_rnorm 0.58544120061808E-04
$last SCF energy change = -948.33859
$charge from dscf
         -0.000 (not to be modified here)
$dipole from dscf
  x     0.41711971769947    y     1.05211810132355    z     0.27435875240447    a.u.
   | dipole | =    2.9600540161  debye
$excitation_energies_CC2_____1^a___ file=exstates
$t2_norm_of_re0_CC2_____1^a___ file=exstates
$t2_norm_of_le0_CC2_____1^a___ file=exstates
$<le0|re0>-overlap_CC2_____1^a___ file=exstates
$<le01|re01>-overlap_CC2_____1^a___ file=exstates
$<le02|re02>-overlap_CC2_____1^a___ file=exstates
$end