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60 CHAPTER 4. ELECTRONIC STRUCTURE<br />

Plane wave expansion <strong>of</strong> a Bloch state<br />

Knowing that Bloch’s theorem follows from general symmetry considerations, we can now rederive (4.4)<br />

more quickly, by constructing a state which conforms with Bloch’s theorem from the outset:<br />

|ψ k 〉 = ∑ G<br />

c k−G |k − G〉; , (4.8)<br />

where the sum runs over all reciprocal lattice vectors G. Where does this come from Bloch’s<br />

theorem states that ψ k (r) is a product <strong>of</strong> a plane wave e ikr and a function u k (r) with the periodicity<br />

<strong>of</strong> the lattice. We can Fourier-expand the periodic function as a sum over all reciprocal lattice vectors,<br />

u k (r) = ∑ G c k−Ge −iGr . This gives for ψ k (r) = 〈r|ψ k 〉 = ∑ G c k−Ge i(k−G)r = ∑ G c k−G〈r|k − G〉.<br />

In this form, the electron wavefunction appears as a superposition <strong>of</strong> harmonics, whose wavevectors are<br />

related by reciprocal lattice vectors G.<br />

Writing the Hamiltonian as Ĥ = Ĥ0 + V , where Ĥ0 gives the kinetic energy and V is the periodic<br />

potential <strong>of</strong> the lattice, we are looking for the eigenvalues E k in<br />

Left multiply with a plane wave state 〈k|:<br />

Ĥ|ψ k 〉 = E k |ψ k 〉 . (4.9)<br />

〈k|Ĥ|ψ k〉 = E k c k = 〈k|Ĥ0|k〉c k + ∑ G<br />

〈k|V |k − G〉c k−G (4.10)<br />

We can identify 〈k|V |k − G〉 as the Fourier component V G <strong>of</strong> the periodic potential, defined in (4.1).<br />

We immediately obtain the key equation:<br />

( )<br />

E (0)<br />

k<br />

− E k c k + ∑ V G c k−G = 0 , (4.11)<br />

G<br />

where the kinetic energy E (0)<br />

k<br />

= h¯ 2<br />

2m k2 . This is the same as (4.3), which we derived from a more<br />

general plane wave expansion for |ψ〉.<br />

It is <strong>of</strong>ten convenient to rewrite q = k + G ′ , where G ′ is a reciprocal lattice vector chosen so that<br />

q lies in the first Brillouin zone, and to write G ′′ = G + G ′ in the second summation. This gives back<br />

(4.4): [ ( ) h¯2<br />

2m (q − G′ ) 2 − E c q−G ′ + ∑ ]<br />

U G ′′ −G ′c q−G ′′ = 0 (4.12)<br />

G ′′<br />

4.3 Nearly free electron theory<br />

Although we have, with Eqn. (4.3), reduced the problem <strong>of</strong> finding the eigenstates <strong>of</strong> the<br />

electronic hamiltonian to that <strong>of</strong> solving an eigenvector/eigenvalue problem, this still looks<br />

rather intractable: we are stuck with an infinite set <strong>of</strong> basis functions and therefore with<br />

having to diagonalise, in principle, an infinitely-dimensional matrix. Recall that the singleelectron<br />

state was obtained from the plane wave expansion |ψ k 〉 = ∑ G c k−G |k − G〉, in which<br />

we have to fix all the coefficients c −G . However, it should be possible to find approximate<br />

eigenstates by reducing the size <strong>of</strong> the basis set. 1<br />

1 There are lengthy descriptions <strong>of</strong> this approach in all the textbooks. A nice treatment similar to the one<br />

given her can be found in the book by Singleton.

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