Reviews in Computational Chemistry Volume 18
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