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Reviews in Computational Chemistry Volume 18

Reviews in Computational Chemistry Volume 18

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104 Polarizability <strong>in</strong> Computer Simulations<br />

dipoles, there are iterative, adiabatic techniques as well as fully dynamic methods.<br />

In the adiabatic methods, the correspondence between the shell charge<br />

and the effective electronic degrees of freedom is <strong>in</strong>voked, along with the<br />

Born–Oppenheimer approximation. In this case, the slow-mov<strong>in</strong>g nuclei and<br />

core charges are said to move adiabatically <strong>in</strong> the field generated by the shell<br />

charges. In other words, the positions of the shell charges are assumed to<br />

update <strong>in</strong>stantaneously <strong>in</strong> response to the motion of the nuclei, and thus<br />

always occupy the positions <strong>in</strong> which they feel no net force (i.e., the positions<br />

that m<strong>in</strong>imize the total energy of the system). The forces on the core charges<br />

are then used to propagate the dynamics, us<strong>in</strong>g standard numerical <strong>in</strong>tegration<br />

methods. The other alternative is to treat the charges fully dynamically, allow<strong>in</strong>g<br />

them to occupy positions away from the m<strong>in</strong>imum-energy position dictated<br />

by the nuclei, and thus experience nonzero forces.<br />

When the charges are treated adiabatically, a self-consistent method<br />

must be used to solve for the shell displacements, fdig (just as with the dipoles<br />

fl ig <strong>in</strong> the previous section). Comb<strong>in</strong><strong>in</strong>g Eqs. [26], [28], and [29], we can<br />

write the total energy of the shell model system as<br />

U <strong>in</strong>dðfrig; fdigÞ ¼ XN<br />

i ¼ 1<br />

þ 1<br />

2<br />

1<br />

2 kid 2 i þ qi½ri E 0 i ðri þ diÞ E 00<br />

i Š<br />

X n<br />

X<br />

i ¼ 1 j 6¼ i<br />

1<br />

rij<br />

1<br />

jrij djj<br />

1<br />

jrij þ dij þ<br />

1<br />

jrij di þ djj<br />

which is the equivalent of Eq. [<strong>18</strong>] for a model with polarizable po<strong>in</strong>t dipoles,<br />

but with one important difference: Eq. [<strong>18</strong>] is a quadratic function of the fl ig,<br />

guarantee<strong>in</strong>g that its derivative (Eq. [19]) is l<strong>in</strong>ear and that a standard matrix<br />

method can be used to solve for the fl ig. Equation [30] is not a quadratic function<br />

of the fdig. Moreover, the dependence of the short-range <strong>in</strong>teractions on<br />

the displacements of the shell particles further complicates the matter. Consequently,<br />

matrix methods are typically not used to f<strong>in</strong>d the shell displacements<br />

that m<strong>in</strong>imize the energy.<br />

Iterative methods are used <strong>in</strong>stead. In one such approach, 101 the nuclear<br />

(core) positions are updated, and the shell displacements from the previous<br />

step are used as the <strong>in</strong>itial guess for the new shell displacements. The net force,<br />

Fi, on the shell charge is calculated from the gradient of Eq. [30], together with<br />

any short-range <strong>in</strong>teractions. Because the harmonic spr<strong>in</strong>g <strong>in</strong>teraction is, by<br />

far, the fastest vary<strong>in</strong>g component of the potential felt by the shell charge,<br />

the <strong>in</strong>cremental shell displacement ddi ¼ Fi=ki represents a very good estimate<br />

of the equilibrium (energy m<strong>in</strong>imiz<strong>in</strong>g) position of the shells. The forces are<br />

recalculated at this position, and the procedure is iterated until a (nearly)<br />

force-free configuration is obta<strong>in</strong>ed. Alternatively, this steepest descent style<br />

½30Š

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