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76 CHAPTER 5. BANDSTRUCTURE OF REAL MATERIALS<br />

• You will also <strong>of</strong>ten see particular bands labelled either along lines or at points by greek<br />

or latin capital letters with a subscript. These notations label the group representation<br />

<strong>of</strong> the state (symmetry) and we won’t discuss them further here.<br />

Density <strong>of</strong> states<br />

We have dealt earlier with the density <strong>of</strong> states <strong>of</strong> a free electron band in 2. The maxima<br />

E max and minima E min <strong>of</strong> all bands must have a locally quadratic dispersion with respect to<br />

momenta measured from the minima or maxima. Hence the density <strong>of</strong> states (in 3D) near the<br />

minima will be the same<br />

g(E > ∼ E min ) = V (<br />

m ∗ 2m ∗ (E − E min )<br />

π 2 h¯ 2 h¯ 2<br />

) 1<br />

2<br />

. (5.10)<br />

as before, with now however the replacement <strong>of</strong> the bare mass by an effective mass m ∗ =<br />

(m ∗ xm ∗ ym ∗ z) 1/3 averaging the curvature <strong>of</strong> the bands in the three directions 3 . A similar form<br />

must apply near the band maxima, but with now g(E) ∝ (E max − E) 1 2 . Notice that the flatter<br />

the band, the larger the effective mass, and the larger the density <strong>of</strong> states 4 .<br />

Since every band is a surface it will have saddle points (in two dimensions or greater) which<br />

are points where the bands are flat but the curvature is <strong>of</strong> opposite signs in different directions.<br />

Examples <strong>of</strong> the generic behaviour <strong>of</strong> the density <strong>of</strong> states in one, two and three dimensions<br />

are shown in Fig. 5.1. The saddle points give rise to cusps in the density <strong>of</strong> states in 3D, and<br />

a logarithmic singularity in 2D.<br />

For any form <strong>of</strong> E(k), the density <strong>of</strong> states is<br />

g(E) = ∑ n<br />

g n (E) = ∑ n<br />

∫<br />

dk<br />

4π 3 δ(E − E n(k)) , (5.11)<br />

Because <strong>of</strong> the δ-function in (5.11), the momentum integral is actually over a surface in k-space S n<br />

which depends on the energy E; S n (E F ) is the Fermi surface. We can separate the integral in k into<br />

a two-dimensional surface integral along a contour <strong>of</strong> constant energy, and an integral perpendicular to<br />

this surface dk ⊥ (see Fig. 5.2). Thus<br />

g n (E) =<br />

=<br />

∫<br />

∫<br />

S n(E)<br />

S n(E)<br />

∫<br />

dS<br />

4π 3<br />

dk ⊥ (k) δ(E − E n (k))<br />

where ∇ ⊥ E n (k) is the derivative <strong>of</strong> the energy in the normal direction. 5<br />

dS<br />

4π 3 1<br />

|∇ ⊥ E n (k)| , (5.12)<br />

Notice the appearance <strong>of</strong> the gradient term in the denominator <strong>of</strong> (5.12), which must vanish at the<br />

edges <strong>of</strong> the band, and also at saddle points, which exist generically in two and three dimensional bands.<br />

Maxima, minima, and saddle points are all generically described by dispersion (measured relative to the<br />

3 Since the energy E(k) is a quadratic form about the minimum, the effective masses are defined by h¯ 2<br />

m ∗ α<br />

∣<br />

along the principal axes α <strong>of</strong> the ellipsoid <strong>of</strong> energy.<br />

∂ 2 E(k)<br />

∂k<br />

∣<br />

α<br />

2 kmin<br />

4 The functional forms are different in one and two dimensions.<br />

5 We are making use <strong>of</strong> the standard relation δ(f(x) − f(x 0 )) = δ(x − x 0 )/|f ′ (x 0 )|<br />

=

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