MOLCAS manual:
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Subsections
10.6 Solvent models.
For isolated molecules of modest size the ab initio methods
have reached great accuracy at present both for ground and
excited states. Theoretical studies on isolated molecules, however,
may have limited value to bench chemists since most of the
actual chemistry takes place in a solvent. If solute-solvent interactions are
strong they may have a large impact on the electronic structure of a
system and then on its excitation spectrum, reactivity, and properties.
For these reasons, numerous models
have been developed to deal with solute-solvent interactions in ab
initio quantum chemical calculations. A microscopic
description of solvation effects can be obtained by a supermolecule
approach or by combining statistical mechanical simulation techniques
with quantum chemical methods.
Such methods, however, demand expensive computations. By contrast, at the
phenomenological level, the solvent can be regarded as a dielectric continuum,
and there are a number of approaches [278,279,280,281,282] based on the classical reaction field concept.
MOLCAS can model the solvent
within the framework of SCF, RASSCF and CASPT2 programs, for the calculation of energies
and properties and also for geometry optimizations. The reaction field formalism
is based on a sharp partition of the system: the solute molecule (possibly
supplemented by some explicit solvent molecules) is placed in a cavity
surrounded by a polarizable dielectric.
The surrounding is characterized mainly by its dielectric constant and density:
an important parameter of the method is the size of the cavity;
the dielectric medium is polarized by the solute, and this polarization creates
a reaction field which perturbs the solute itself.
Two versions of the model are presently available: one is based on the Kirkwood model
[280,281] and uses only spherical cavities; the other is
called PCM (polarizable continuum model) [278,279] and can
use cavities of general shape, modeled on the actual solute molecule. In the former
case, the reaction field is computed as a truncated multipolar expansion and added
as a perturbation to the one-electron Hamiltonian; in the latter case the reaction
field is expressed in terms of a collection of apparent charges (solvation charges)
spread on the cavity surface: the PCM reaction field perturbs both one- and
two-electron Hamiltonian operators. In both cases, the solvent effects can be
added to the Hamiltonian at any level of theory, including MRCI and CASPT2.
This version of the model only uses spherical cavities. In addition,
it includes Pauli repulsion due to the medium by introducing a repulsive
potential representing the exchange repulsion between the solute and the solvent.
This is done by defining a penalty function of Gaussian type, generating
the corresponding spherical well integrals, and adding them to the one-electron
Hamiltonian. When the repulsion potential is used, the size of the cavity should
be optimized for the ground state of the molecule (see below). If the repulsive
potential is not used and the cavity size is chosen to be smaller (molecular
size plus van der Waals radius as is the usual choice in the literature)
one must be aware of the consequences: larger solvent effects but also
an unknown presence of molecular charge outside the boundaries of the
cavity. This is not a consequence of the present model but it is a general
feature of cavity models [281].
The cavities are defined as the envelope of spheres centered on solute
atoms or atomic groups (usually hydrogens are included in the same sphere
of the atoms they are bonded to). Two selection of radii are presently available,
i. e. Pauling radii, and the so-called UATM (united atom topological model) radii:
the latter is the default for PCM calculations; sphere radii can also be provided
by the user in the input file.
The solvation charges are placed
in the middle of small tiles (tesserae) drawn on the surface; the number of
solvation charges can be gauged by changing the average area of tesserae (keyword
AAre in SEWARD).
The program prints some information related to the cavity, where one should
always check carefully the magnitude of sphere radii: the program adjusts them
automatically to the solute topology (each radius depends on
hybridization, bonds, etc.), and sometimes this causes some
problems (for instance, discontinuities could appear during the scan
of a potential energy surface): if this happens, it is preferable to provide
the desired radii in the input file, so that they will be kept at all
geometries.
When doing state-average RASSCF calculations, one has to specify which root is
to be used to generate the solvation charges: this means that the PCM reaction
field will be in equilibrium with a specific electronic state, while it
perturbs all the states included in the calculation.
In electronic transitions (e. g. photon absorption or emission) one has to include
non-equilibrium effects, due to the finite relaxation time of solvent molecules
following a sudden change in electronic distribution. This is done by partitioning the
reaction field in two components (fast and slow, the former always equilibrated,
the latter delayed), whose magnitude is determined by the static dielectric constant
and by a ``fast'' dielectric constant [283] (for very fast processes, like
photon absorption, the fast constant is equal to the square of the refraction index).
To perform a non-equilibrium calculation, for example to study a ground-to-excited state
transition, one has to perform a regular calculation at equilibrium for the ground state,
followed by a calculation for the excited state specifying the keyword NONEQ in the
RASSCF program. Failing to include the keyword NONEQ will cause the program
to compute equilibrium solvation also for the excited state, what would be appropriate
for an adiabatic, instead of a vertical, transition.
CASPT2 calculations can be performed as usual for isolated molecules, specifying
the keyword RFPERT. Geometry optimizations can be performed as usual: note that
the arrangement of solvation charges around the solute molecule is likely
to break the molecular symmetry. If the symmetry was explicitly requested in
SEWARD, the system will keep it through the optimization even in the
presence of the solvent, otherwise the convergence could be more difficult, and
the final geometry could result of a lower symmetry.
We begin by performing a CASSCF/CASPT2 reaction field calculation
on the ground state of a molecule.
To use the Kirkwood model, the keyword
REACtion field
is needed; if no repulsive potential is going to be used the input
simply consists in adding the
appropriate data (dielectric constant of the medium, cavity size, and
angular quantum number of the highest multipole moment of the charge
distribution) into the SEWARD input:
&SEWARD &END
...
...
RF-Input
Reaction field
80 8.0 4
End of RF-Input
...
...
End of Input
This will compute the reaction field at those levels. The dielectric
constant 80.0 correspond to water as solvent. The radius of the cavity
is 8.0 in atomic units. Finally 4 is the maximum angular moment
number used in the multipole expansion. The cavity origin is the
coordinate origin, thus the molecule must be placed accordingly.
If we want to include the reaction field (either PCM or Kirkwood
model)
at other levels of theory the keyword RFPErt must be
added to the MOTRA or CASPT2 inputs.
We are, however, going to explain the more complicated situation where
a repulsive well potential has to be added to the model. In this case
it is convenient to optimize the size of the cavity, although
in so doing we obtain large cavity sizes and therefore
smaller solvent effects. More realistic results can be obtained if
additional and specific solvent molecules are added inside the cavity.
To define the well potential we have to add the keyword
WELL Integrals to the SEWARD input to compute and add the
Pauli repulsion integrals to the bare Hamiltonian.
The requirements considered to build this potential
are that it shall reproduce solvation energies for spherical particles,
ions, and that it must be wide enough so that the electrons in the
excited state of the molecules are also confined to the cavity. Negative ions
have the property that their electrons are loosely bound and they are thus suited
for parametrizing the repulsive potential.
The final result of different calibration calculations
[284,281] is a penalty function which includes four
Gaussians. If a is
the radius of the cavity the Gaussians are placed at distances a+2.0,
a+3.0, a+5.0 and a+7.0 a.u. from the cavity's center with
exponents 5.0, 3.5, 2.0 and 1.4, respectively.
As an example we will use the N,N-dimethylaminobenzonitrile (DMABN) molecule
(see Figure ).
This is a well known system with large dipole moments both in ground and
excited states which suffer important effects due to the polar environment.
Figure 10.13:
N,N-dimethylaminobenzonitrile (DMABN)
|
&SEWARD &END
Title
para-DMABN molecule. Cavity size: 10 au.
Symmetry
X XY
Basis set
N.ANO-S...3s2p1d.
N1 0.0000000000 0.0000000000 4.7847613288
N2 0.0000000000 0.0000000000 -8.1106617786
End of basis
Basis set
C.ANO-S...3s2p1d.
C1 0.0000000000 0.0000000000 2.1618352923
C2 0.0000000000 2.2430930886 0.7747833630
C3 0.0000000000 2.2317547910 -1.8500321252
C4 0.0000000000 0.0000000000 -3.1917306021
C5 0.0000000000 0.0000000000 -5.9242601761
C6 0.0000000000 2.4377336900 6.0640991723
End of basis
Basis set
H.ANO-S...2s.
H1 0.0000000000 4.0043085530 -2.8534714086
H2 0.0000000000 4.0326542950 1.7215314260
H3 0.0000000000 2.1467175630 8.0879851846
H4 1.5779129980 3.6622699270 5.5104123361
End of basis
RF-Input
reaction field
38.8 10.0 4
End of RF-Input
Well Int
4
1.0 5.0 12.0
1.0 3.5 13.0
1.0 2.0 15.0
1.0 1.4 17.0
End of Input
&SCF &END
TITLE
DMABN molecule
OCCUPIED
20 2 12 5
ITERATIONS
50
END OF INPUT
&RASSCF &END
TITLE
p-DMABN
SYMMETRY
1
SPIN
1
NACTEL
10 0 0
FROZEN
8 0 3 0
INACTIVE
12 1 9 1
RAS2
0 2 0 7
THRS
1.0E-06,1.0E-03,1.0E-03
ITER
50,25
LUMORB
END OF INPUT
In the SEWARD input the WELL Integrals must include
first the number of Gaussians used (four), followed by the
coefficient and exponent of the Gaussian and the radius of
the cavity in the sequence explained above: first the most
compact Gaussian with the radius plus 2.0 au, and so on
to the least compact Gaussian.
Here, we have defined a cavity size of 10 au
(cavity centered at coordinate origin). The RASSCF program will read
the RCTFLD input, prepared this time for acetonitrile
( = 38.8 ), a cavity size of 10.0 au (the same
as in the SEWARD input) and a multipole expansion up to the fourth order
which is considered sufficient [281].
The active space includes the space over
the molecular plane, excluding the orbital of the CN
group which lies in the molecular plane.
We repeat the calculation for different cavity sizes in order
to find the radius which gives the lowest absolute energy at the CASSCF
level. The presence of the repulsive terms allows the cavity
radius to be computed by energy minimization. For the calculations
using different cavity sizes it is not necessary to repeat the
calculation of all the integrals, just those related to the
well potential. Therefore, the keyword ONEOnly can be
included in the SEWARD input. The ONEINT file will be modified
and the ORDINT file is kept the same for each molecular
geometry. The energies obtained are in Table .
Table 10.17:
Ground state CASSCF energies for DMABN with different cavity sizes.
Radius (au) |
CASSCF energies (au) |
no cav. |
-455.653242 |
10.0 |
-455.645550 |
11.0 |
-455.653486 |
12.0 |
-455.654483 |
14.0 |
-455.654369 |
16.0 |
-455.654063 |
|
Taking the gas-phase value (no cav.) as the reference, the CASSCF
energy obtained with a 10.0 au cavity radius is higher. This is an
effect of the repulsive potential, meaning that the molecule is too close to
the boundaries. Therefore we discard this value and use the values
from 11.0 to 16.0 to make a simple second order fit and obtain a
minimum for the cavity radius at 13.8 au.
Once we have this value we also need to optimize the position of the
molecule in the cavity. Some parts of the molecule, especially those
with more negative charge, tend to move close to the
boundary. Remember than the sphere representing the cavity has
its origin in the cartesian coordinates origin. We use the radius of
13.8 au and compute the CASSCF energy at different displacements
along the coordinate axis. Fortunately enough, this molecule has
C2v symmetry. That means that displacements along two of the
axis (x and y) are restricted by symmetry. Therefore it is
necessary to analyze only the displacements along the z coordinate.
In a less symmetric molecule all
the displacements should be studied even including combination of the displacements.
The result may even be a three dimensional net, although no
great accuracy is really required. The results for DMABN n C2v symmetry are compiled
in Table .
Table 10.18:
Ground state CASSCF energies for different translations with respect to the initial position of of the DMABN molecule in a 13.8 au cavity.
Disp. in z (au) |
CASSCF energies (au) |
+0.5 |
-455.654325 |
0.0 |
-455.654400 |
-0.5 |
-455.654456 |
-1.0 |
-455.654486 |
-1.5 |
-455.654465 |
|
Fitting these values to a curve we obtain an optimal displacement of -1.0 au. We move the
molecule and reoptimize the cavity radius at the new position of the
molecule. The results are listed in Table .
Table 10.19:
Ground state CASSCF energies for DMABN with different cavity sizes. The molecule position in the cavity has been optimized.
Radius (au) |
CASSCF energies (au) |
11.8 |
-455.653367 |
12.8 |
-455.654478 |
13.8 |
-455.654486 |
14.8 |
-455.654318 |
|
There is no significant change. The cavity radius is then selected as 13.8 au and the
position of the molecule with respect to the cavity is kept as in
the last calculation. The calculation is carried out with the new values.
The SCF or RASSCF outputs will contain the information about the
contributions to the solvation energy. The CASSCF energy obtained will
include the reaction field effects and an analysis of the
contribution to the solvation energy for each value of the multipole
expansion:
Reaction field specifications:
------------------------------
~
Dielectric Constant : .388E+02
Radius of Cavity(au): .138E+02
Truncation after : 4
~
Multipole analysis of the contributions to the dielectric solvation energy
~
--------------------------------------
l dE
--------------------------------------
0 .0000000
1 -.0013597
2 -.0001255
3 -.0000265
4 -.0000013
--------------------------------------
The reaction field parameters are added to the
SEWARD program input through the keyword
RF-Input
To invoke the PCM model the keyword
PCM-model
is required. A possible input is
RF-input
PCM-model
solvent
acetone
AAre
0.2
End of rf-input
which requests a PCM calculation with acetone as solvent, with tesserae
of average area
. Note that the default parameters are
solvent=water, average area
; see the SEWARD
manual section for further PCM keywords. By default the PCM adds
non-electrostatic terms (i. e. cavity formation energy, and dispersion
and repulsion solute-solvent interactions) to the computed free-energy
in solution.
A complete input for a ground state CASPT2 calculation on formaldehyde
() in water is
&GATEWAY
Title
formaldehyde
Coord
4
H 0.000000 0.924258 -1.100293 Angstrom
H 0.000000 -0.924258 -1.100293 Angstrom
C 0.000000 0.000000 -0.519589 Angstrom
O 0.000000 0.000000 0.664765 Angstrom
Basis set
6-31G*
Group
X Y
RF-input
PCM-model
solvent
water
end of rf-input
End of input
&SEWARD
End of input
&SCF
Title
formaldehyde
Occupied
5 1 2 0
End of input
&RASSCF
Title
formaldehyde
nActEl
4 0 0
Inactive
4 0 2 0
Ras2
1 2 0 0
LumOrb
End of input
&CASPT2
Frozen
4 0 0 0
RFPErt
End of input
In the PCM picture, the solvent reaction field is
expressed in terms of a polarization charge density spread
on the cavity surface, which, in the most recent version of the method,
depends on the electrostatic potential
generated by the solute on the cavity according to
|
= |
|
(10.5) |
where is the solvent dielectric constant and
is the (electronic+nuclear) solute potential at point
on the cavity surface.
The and operators are related respectively to
the electrostatic potential
and to the normal component of the
electric field
generated by the surface charge density .
It is noteworthy that in this PCM formulation the polarization charge
density is designed to take into account implicitly
the effects of the fraction of solute electronic density lying outside the
cavity.
In the computational practice, the surface charge distribution
is expressed in terms of a set of point charges placed
at the center of each surface tessera, so that operators are replaced by the
corresponding square matrices.
Once the solvation charges (q) have been determined,
they can be used to compute energies and properties in solution.
The interaction energy between the solute and the solvation charges
can be written
|
(10.6) |
where Vi is the solute potential calculated at the representative point
of tessera i. The charges act as
perturbations on the solute electron density : since the charges
depend in turn on through the electrostatic potential, the solute
density and the charges must be adjusted until self consistency.
It can be shown[282] that for any SCF procedure including a
perturbation linearly depending on the electron density,
the quantity that is variationally minimized corresponds to a free energy
(i.e. Eint minus the work spent to polarize the dielectric and to create
the charges).
If
is the solute energy in vacuo, the free energy
minimized in solution is
|
(10.7) |
where VNN is the solute nuclear repulsion energy, is the
solute electronic density for the isolated molecule, and is the
density perturbed by the solvent.
The inclusion of non-equilibrium solvation effects, like those
occurring during electronic excitations, is introduced in the model by
splitting the solvation charge on each surface element into
two components: qi,f is the charge due to electronic (fast) component
of solvent polarization, in equilibrium with the solute electronic density
upon excitations, and qi,s, the charge arising from the orientational
(slow) part, which is delayed when the solute undergoes a sudden transformation.
The photophysics and photochemistry of
acrolein are mainly controlled by the relative position of the
, and states, which is,
in turn, very sensitive to the presence and the nature of the solvent.
We choose this molecule in order to show an example of how to
use the PCM model in a CASPT2 calculation of vertical excitation
energies.
The three states we want to compute are low-lying singlet
and triplet excited states of the s-trans isomer.
The space (4 MOs /4 -electrons)
with the inclusion of the lone-pair MO (ny) is a suitable choice
for the active space in this calculation.
For the calculation in aqueous solution, we need first to compute the CASPT2
energy of the ground state in presence of the solvent water.
This is done by including in the SEWARD input for the corresponding gas-phase
calculation the section
RF-input
PCM-model
solvent
water
DIELectric constant
78.39
CONDuctor version
AARE
0.4
End of rf-input
If not specified, the default solvent is chosen to be water.
Some options are available. The value of the dielectric constant
can be changed for calculations at temperatures other than 298 K.
For calculations in polar solvents like water, the use of the conductor
model (C-PCM) is recommended.
This is an approximation that employs conductor rather than dielectric
boundary conditions. It works very well for polar solvents
(i. e. dielectric constant greater than about 5), and is based
on a simpler and more robust implementation. It can be useful also in cases when
the dielectric model shows some convergence problems.
Another parameter that can be varied in presence of convergency problem
is the average area of the tesserae of which the surface of the cavity is composed.
However, a lower value for this parameter may give poorer results.
Specific keywords are in general needed for the other modules to work with PCM, except for
the SCF. The keyword NONEquilibrium is
necessary when computing excited states energies in RASSCF.
For a state specific calculation of the ground state CASSCF energy, the solvent effects
must be computed with an equilibrium solvation approach, so this keyword must be omitted.
None the less, the keyword RFpert must be included in the CASPT2 input
in order to add
the reaction field effects to the one-electron hamiltonian as a constant perturbation.
&RASSCF &END
Title
Acrolein GS + PCM
Spin
1
Symmetry
1
nActEl
6 0 0
Frozen
4 0
Inactive
8 0
Ras2
1 4
LUMORB
THRS
1.0e-06 1.0e-04 1.0e-04
ITERation
100 100
End of input
&CASPT2 &END
Title
ground state + PCM
RFpert
End of Input
Information about the reaction field calculation employing
a PCM-model appear first in the SCF output
Polarizable Continuum Model (PCM) activated
Solvent:water
Version: Conductor
Average area for surface element on the cavity boundary: 0.4000 Angstrom2
Minimum radius for added spheres: 0.2000 Angstrom
Polarized Continuum Model Cavity
================================
Nord Group Hybr Charge Alpha Radius Bonded to
1 O sp2 0.00 1.20 1.590 C [d]
2 CH sp2 0.00 1.20 1.815 O [d] C [s]
3 CH sp2 0.00 1.20 1.815 C [s] C [d]
4 CH2 sp2 0.00 1.20 2.040 C [d]
------------------------------------------------------------------------------
The following input is used for the CASPT2 calculation of the
state.
Provided that the same $WorkDir has been using, which contains all the files of of the
calculation done for the ground state, the excited state calculation is done
by using inputs for the RASSCF
and the CASPT2 calculations:
&RASSCF &END
Title
Acrolein n->pi* triplet state + PCM
Spin
3
Symmetry
2
nActEl
6 0 0
Frozen
4 0
Inactive
8 0
Ras2
1 4
NONEquilibrium
LUMORB
ITERation
100 100
End of input
&CASPT2 &END
Title
triplet state
RFpert
End of Input
Note the RASSF keyword NONEQ, requesting that the slow part of the reaction
field be frozen as in the ground state, while the fast part is
equilibrated to the new electronic distribution. In this case the fast
dielectric constant is the square of the refraction index, whose value
is tabulated for all the allowed solvents (anyway, it can be modified by
the user through the keyword ``DIELectric'' in SEWARD).
The RASSCF output include the line:
Calculation type: non-equilibrium (slow component from JobOld)
Reaction field from state: 1
This piece of information means that the program computes the solvent
effects on the energy of the
by using a non-equilibrium approach.
The slow component of the solvent response is kept frozen in terms of the charges
that have been computed for the previous equilibrium calculation of
the ground state. The remaining part of the solvent response,
due to the fast charges, is instead computed self-consistently for the
state of interest (which is state 1 of the specified spatial and spin symmetry in this case).
The vertical excitations to the lowest valence states
in aqueous solution for s-trans acrolein are
listed in the Table and compared
with experimental data.
As expected by qualitative reasoning, the vertical excitation energy to the
state exhibits a blue shift in water.
The value of the vertical transition energy computed with the inclusion of the
PCM reaction field is computed to be 3.96 eV at the CASPT2 level of theory.
The solvatochromic shift is thus of +0.33 eV.
Experimental data are available for the
excitation energy to the
state. The band shift in
going from isooctane to water is reported to be +0.24 eV which is in fair
agreement with the PCM result.
No experimental data are available for the excitation energies to the triplet
states of acrolein in aqueous solution. However it is of interest to see how
the ordering of these two states depends on solvent effects.
The opposing solvatochromic shifts produced by the solvent on these two electronic transitions
place the two triplet states closer in energy.
This result might suggest that a dynamical interconversion between
the and may occur more favorable in solution.
Table 10.20:
Vertical excitation energies/eV (solvatochromic shifts) of s-trans acrolein in gas-phase and in aqueous solution
State |
Gas-phase |
Water |
Expt.a |
|
3.63 |
3.96 (+0.33) |
3.94 (+0.24)b |
T1
|
3.39 |
3.45 (+0.06) |
|
T2
|
3.81 |
3.71 (-0.10) |
|
aRef.[285] |
bSolvatochromic shifts derived by comparison of the
absorption wave lengths in water and isooctane |
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