CCL: correction of my comment on MO's in Solvent
- From: Andreas Klamt <klamt(!)cosmologic.de>
- Subject: CCL: correction of my comment on MO's in Solvent
- Date: Fri, 05 Apr 2013 08:13:06 +0200
Sent to CCL by: Andreas Klamt [klamt[*]cosmologic.de]
Dear colleagues,
after some critical questions by colleagues, I need to correct myself
with respect to my previous statement on the meaning of the MOs in
continuum solvents:
The MOs do make sense and they will be the same in both of the two
implementations, i.e by either considering the total polarization
charges as prividing an external field and aditing the penalty for the
polarization energy costs at the end, or by considering the solvent
response as an indirect charge-charge iteractions (in addition to the
direct Coulomb interaction), i.e. representing it as additional
nuclei-nuclei, nuclei-electron, and electron-electron interaction. As
long as we are on the SCF level (i.e. Hartree-Fock or DFT) in both
cases
the final FOCK matrix is identical and hence orbitals and orbital
energies will be identical. Just for subsequent perturbation treatment
it is useful to realize that the continuum interaction has one-electron
and two-electron contributions.
Sorry for any confusion which I may have caused
Andreas
Am 31.03.2013 16:17, schrieb Andreas Klamt klamt,,cosmologic.de:
Sent to CCL by: Andreas Klamt [klamt{=}cosmologic.de]
Since my first two attempts were not posted yet, here again my comment:
Dear Ramesh,
this is a good question. In the way as most continuum models are
implemented nowadays, the orbitals do not make much sense, because the
polarization charges are completely treated as external field, and the
energy for generatig the field is added to the total energy of the
molecule after the SCF has achieved. In my original COSMO
implementation in MOPAC I followed a different concept, considering
the continuum contribution as an indirect charge-charge interaction.
In that way you have additional nuclei-nuclei-interactions, additional
nuclei-electron-interactions (added to the one electron Hamiltonian,
and additional electron-electron interactions, added to the
two-electron-interactions. Thus the continuum interactions enter the
orbitals in a perfectly analogous way to the Coulomb interactions. A
post-correction for the self energy of the polarization field is not
required, since all energy contributions already take it into account
by the factor 1/2. While the total energy, and all expectation values
will be exactly the same in both implementations, the orbital energies
produced in that way are considerably different from thse in the
standard way, but I am convinced they make more sense. (Without
understand it in detail, Zerner and coworker had earlier called the
models as model A and B, see Szafran, et al. J. Comp. Chem 1993 ....)
Please note the difference of the models for the orbitals: In the
standard implementation, the electrons in the LUMO "see" the
polarization charge polarization charges produced by the ground state
electron density, i.e. the change of the polarization charges due to
the excitation to the LUMO is missing.
But I am afraid, currently no implementation of PCM or COSMO following
the Coulomb energy analogy is available. While writing this I realize
that I may be wrong: The GAMESS COSMO implementation may still have
it. Kim Baldridge should know about this best.
Best regards
Andreashttp://www.ccl.net/chemistry/sub_unsub.shtmlConferences:
http://server.ccl.net/chemistry/announcements/conferences/>