07.04.2013 Views

Essentials of Computational Chemistry

Essentials of Computational Chemistry

Essentials of Computational Chemistry

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

396 11 IMPLICIT MODELS FOR CONDENSED PHASES<br />

where ε is the exterior dielectric constant. Taking r on the surface <strong>of</strong> the sphere, i.e., |r| =a,<br />

Eq. (11.3) becomes<br />

G =− 1<br />

q<br />

2 4πa2 <br />

− q <br />

ds =<br />

εa<br />

q2<br />

2εa<br />

(11.11)<br />

As the square <strong>of</strong> the charge, the dielectric constant, and the ionic radius must all be positive,<br />

work must be expended to charge the sphere, but the work is less for higher exterior dielectric<br />

constants, as expected. Recalling that the polarization energy is the difference in the required<br />

work in the gas phase and solution, we may write<br />

GP =− 1<br />

<br />

1 −<br />

2<br />

1<br />

2 q<br />

(11.12)<br />

ε a<br />

which is the so-called Born equation for the polarization energy <strong>of</strong> a monatomic ion in<br />

atomic units.<br />

If instead <strong>of</strong> carrying a charge, our sphere appears to be characterized by a perfectly<br />

dipolar distribution having dipole moment µ, an analogous analysis provides<br />

GP =− 1<br />

2<br />

2<br />

2 (ε − 1) µ<br />

(2ε + 1) a3 (11.13)<br />

which is the so-called Kirkwood–Onsager equation in atomic units.<br />

An important difference between the Born and Kirkwood–Onsager formulae is that the<br />

former depends on the charge, which is a property <strong>of</strong> the system restricted to integral values,<br />

while the latter depends on the dipole moment, which can potentially vary in different<br />

environments. In the context <strong>of</strong> quantum mechanical calculations, let us define the Kirkwood–Onsager<br />

polarization energy operator by invoking µ as the dipole moment operator<br />

in Eq. (11.13). In that case, the Schrödinger equation in solution becomes<br />

<br />

H − 1<br />

2<br />

<br />

2(ε − 1) 〈|µ|〉<br />

(2ε + 1) a3 <br />

µ = E (11.14)<br />

where H is the usual gas-phase Hamiltonian. Written in this fashion, the components <strong>of</strong> the<br />

second term on the l.h.s. that precede the final dipole moment operator may be regarded as<br />

the reaction field.<br />

Equation (11.14) is an example <strong>of</strong> a non-linear Schrödinger equation. It can be solved in<br />

the usual HF fashion by construction <strong>of</strong> a Slater determinant formed from MOs ψ that are<br />

optimized using a modified Fock operator according to<br />

<br />

2(ε − 1) 1<br />

Fi −<br />

〈|µ|〉2 ψi = eiψi<br />

(11.15)<br />

(2ε + 1) a3 where Fi is the usual gas-phase Fock operator for MO i (Ángyán 1992). A critical feature<br />

<strong>of</strong> Eq. (11.15) is that it involves an additional level <strong>of</strong> iteration compared to the standard<br />

HF approach. Not only must the final wave function render the density matrix and Fock

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!