Maximally localized Wannier functions: Theory and applications
Maximally localized Wannier functions: Theory and applications
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