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Reviews in Computational Chemistry Volume 18

Reviews in Computational Chemistry Volume 18

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λ i /eV<br />

4<br />

3<br />

2<br />

1<br />

0<br />

0 10 20 30 40<br />

Both the free energy gap and the Stokes shift <strong>in</strong>clude two contributions: one<br />

aris<strong>in</strong>g from the variation of the solute dipole (the first term) and one due to<br />

the polarizability change (the second term). The Stokes shift is hence nonzero<br />

even if the charge distribution does not change <strong>in</strong> the course of the transition<br />

(m02 ¼ m01).<br />

The polarizability difference determ<strong>in</strong>es the relative change <strong>in</strong> the<br />

frequency of the solvent driv<strong>in</strong>g mode given by the parameter a1 of the Q<br />

model<br />

a1 ¼<br />

fe1<br />

2ap f1 ~a0<br />

The fact that the parameter a1 is connected to spectroscopic moments for<br />

absorption and emission transitions opens an <strong>in</strong>terest<strong>in</strong>g opportunity to derive<br />

the polarizability change of optical chromophores from spectroscopic first and<br />

second moments. The equation for the polarizability change is as follows:<br />

~a0 ¼ 1<br />

2l1<br />

l<br />

h nst þ l2<br />

α 01<br />

α 02 /Å 3<br />

Beyond the Parabolas 179<br />

Figure 8 Dependence of the solvent reorganization energy <strong>in</strong> the neutral (1, m01) and<br />

charge-separated (2, m02) states on the polarizability of the f<strong>in</strong>al state a02. The solvent<br />

response coefficients are estimated from the cont<strong>in</strong>uum dielectric model (Eq. [95]).<br />

Solute and solvent parameters are m01 ¼ 0, m02 ¼ 15 D, a01 ¼ 20 A ˚ 3 , R0 ¼ 4A ˚ , E1 ¼ 2,<br />

Es ¼ 30. In this and subsequent figures, some of the axes are labeled as the ratios shown<br />

<strong>in</strong> order to make the quantities dimensionless. For example, the ord<strong>in</strong>ate <strong>in</strong> this plot<br />

is <strong>in</strong> units of electron volts, and the abscissa is <strong>in</strong> units of cubic angstroms.<br />

h nst þ l1<br />

~m02 ~m01<br />

h nst þ l2<br />

2<br />

1<br />

2<br />

½99Š<br />

½100Š

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