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Maximally localized Wannier functions: Theory and applications

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17<br />

Problems associated with reaching local minima of the<br />

spread functional, <strong>and</strong> with obtaining <strong>Wannier</strong> <strong>functions</strong><br />

that are not real-valued, are more pronounced in the case<br />

of entangled b<strong>and</strong>s. They are usually alleviated by careful<br />

reconsideration of the energy windows used, in order<br />

to include higher energy states of the appropriate<br />

symmetry, <strong>and</strong>/or by using a better initial guess for the<br />

projections. We infer, therefore, that such problems are<br />

associated not with the wannierization part of the procedure,<br />

but rather with the initial selection of the smooth<br />

subspace from the full manifold of entangled b<strong>and</strong>s.<br />

It is worth noting that the Γ-point formulation<br />

(Sec. II.F.2) appears to be less affected by these problems.<br />

In cases where it is not intuitive or obvious what<br />

the MLWFs should be, therefore, it can often be a fruitful<br />

strategy to use the Γ-point formulation to obtain approximate<br />

MLWFs that may then be used to inform the initial<br />

guess for a subsequent calculation with a full k-point<br />

mesh.<br />

J. Many-body generalizations<br />

The concept of WFs is closely tied to the framework<br />

of single-particle Hamiltonians. Only in this case can we<br />

define J occupied single-particle Bloch <strong>functions</strong> at each<br />

wavevector k <strong>and</strong> treat all J of them on an equal footing,<br />

allowing for invariance with respect to unitary mixing<br />

among them. Once the two-particle electron-electron<br />

interaction is formally included in the Hamiltonian, the<br />

many-body wavefunction cannot be reduced to any simple<br />

form allowing for the construction of WFs in the usual<br />

sense.<br />

One approach is to consider the reduced one-particle<br />

density matrix<br />

∫<br />

n(r, r ′ ) = Ψ ∗ (r, r 2 ...) Ψ(r ′ , r 2 , ...) dr 2 dr 3 ... (54)<br />

for a many-body insulator. Since n(r, r ′ ) is periodic in<br />

the sense of n(r + R, r ′ + R) = n(r, r ′ ), its eigenvectors –<br />

the so-called “natural orbitals” – have the form of Bloch<br />

<strong>functions</strong> carrying a label n, k. If the insulator is essentially<br />

a correlated version of a b<strong>and</strong> insulator having J<br />

b<strong>and</strong>s, then at each k there will typically be J occupation<br />

eigenvalues ν nk that are close to unity, as well as some<br />

small ones that correspond to the quantum fluctuations<br />

into conduction-b<strong>and</strong> states. If one focuses just on the<br />

subspace of one-particle states spanned by the J valencelike<br />

natural orbitals, one can use them to construct oneparticle<br />

WFs following the methods described earlier,<br />

as suggested by Koch <strong>and</strong> Goedecker (2001). However,<br />

while such an approach may provide useful qualitative<br />

information, it cannot provide the basis for any exact<br />

theory. For example, the charge density, or expectation<br />

value of any other one-particle operator, obtained<br />

by tracing over these WFs will not match their exact<br />

many-body counterparts.<br />

A somewhat related approach, adopted by Hamann<br />

<strong>and</strong> V<strong>and</strong>erbilt (2009), is to construct WFs out of the<br />

quasiparticle states that appear in the GW approximation<br />

(Aryasetiawan <strong>and</strong> Gunnarsson, 1998). Such an approach<br />

will be described more fully in Sec. VI.A.3. Here<br />

again, this approach may give useful physical <strong>and</strong> chemical<br />

intuition, but the one-electron quasiparticle wave<strong>functions</strong><br />

do not have the physical interpretation of occupied<br />

states, <strong>and</strong> charge densities <strong>and</strong> other ground-state<br />

properties cannot be computed quantitatively from them.<br />

Finally, a more fundamentally exact framework for a<br />

many-body generalization of the WF concept, introduced<br />

in Souza et al. (2000), is to consider a many-body system<br />

with twisted boundary conditions applied to the manybody<br />

wavefunction in a supercell. For example, consider<br />

M electrons in a supercell consisting of M 1 × M 2 × M 3<br />

primitive cells, <strong>and</strong> impose the periodic boundary condition<br />

Ψ q (..., r j + R, ...) = e iq·R Ψ q (..., r j , ...) (55)<br />

for j = 1, ..., M, where R is a lattice vector of the superlattice.<br />

One can then construct a single “many-body<br />

WF” in a manner similar to Eq. (3), but with k → q <strong>and</strong><br />

|ψ nk ⟩ → |Ψ q ⟩ on the right side. The resulting many-body<br />

WF is a complex function of 3M electron coordinates,<br />

<strong>and</strong> as such it is unwieldy to use in practice. However, it<br />

is closely related to Kohn’s theory of the insulating state<br />

(Kohn, 1964), <strong>and</strong> in principle it can be used to formulate<br />

many-body versions of the theory of electric polarization<br />

<strong>and</strong> related quantities, as shall be mentioned in<br />

Sec. V.A.4.<br />

III. RELATION TO OTHER LOCALIZED ORBITALS<br />

A. Alternative localization criteria<br />

As we have seen, WFs are inherently non-unique <strong>and</strong>,<br />

in practice, some strategy is needed to determine the<br />

gauge. Two possible approaches were already discussed<br />

in Sec. II, namely, projection <strong>and</strong> maximal localization.<br />

The latter approach is conceptually more satisfactory, as<br />

it does not depend on a particular choice of trial orbitals.<br />

However, it still does not uniquely solve the problem of<br />

choosing a gauge, as different localization criteria are possible<br />

<strong>and</strong> there is, a priori, no reason to choose one over<br />

another.<br />

While MLWFs for extended systems have been generated<br />

for the most part by minimizing the sum of<br />

quadratic spreads, Eq. (17), a variety of other localization<br />

criteria have been used over the years for molecular<br />

systems. We will briefly survey <strong>and</strong> compare some of<br />

the best known schemes below. What they all have in<br />

common is that the resulting <strong>localized</strong> molecular orbitals

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