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PREPARED BY
Baranitharan
Kings College of Engineering
Nomenclature
For most purposes, it is sufficient to know the En(k) curves - the
dispersion relations - along the major directions of the reciprocal
lattice.
This is exactly what is done when real band diagrams of
crystals are shown. Directions are chosen that lead from the
center of the Wigner-Seitz unit cell - or the Brillouin zones - to
special symmetry points. These points are labeled according to
the following rules:
• Points (and lines) inside the Brillouin zone are denoted with
Greek letters.
• Points on the surface of the Brillouin zone with Roman
letters.
• The center of the Wigner-Seitz cell is always denoted by a Γ
For cubic reciprocal lattices, the points with a high symmetry on the
Wigner-Seitz cell are the intersections of the Wigner Seitz cell with
the low-indexed directions in the cubic elementary cell.
Nomenclature
simple
cubic
Nomenclature
We use the following nomenclature: (red for fcc, blue for bcc):
The intersection point with the [100] direction is
called X (H)
The line Γ—X is called ∆.
The intersection point with the [110] direction is
called K (N)
The line Γ—K is called Σ.
The intersection point with the [111] direction is
called L (P)
The line Γ—L is called Λ.
Brillouin Zone for fcc is bcc
and vice versa.
We use the following nomenclature: (red for fcc, blue for bcc):
The intersection point with the [100] direction is
called X (H)
The line Γ—X is called ∆.
The intersection point with the [110] direction is
called K (N)
The line Γ—K is called Σ.
The intersection point with the [111] direction is
called L (P)
The line Γ—L is called Λ.
Nomenclature
Real crystals are three-dimensional and we must consider
their band structure in three dimensions, too.
Of course, we must consider the reciprocal lattice, and, as
always if we look at electronic properties, use the Wigner-
Seitz cell (identical to the 1st
Brillouin zone) as the unit cell.
There is no way to express quantities that change as a
function of three coordinates graphically, so we look at a
two dimensional crystal first (which do exist in
semiconductor and nanoscale physics).
Electron Energy Bands in 3D
The qualitative recipe for obtaining the band structure
of a two-dimensional lattice using the slightly adjusted
parabolas of the free electron gas model is simple:
LCAO: Linear Combination of Atomic Orbitals
AKA: Tight Binding Approximation
• Free atoms brought together and the Coulomb interaction
between the atom cores and electrons splits the energy levels
and forms bands.
• The width of the band is proportional to the strength of the
overlap (bonding) between atomic orbitals.
• Bands are also formed from p, d, ... states of the free atoms.
• Bands can coincide for certain k values within the Brillouin
zone.
• Approximation is good for inner electrons, but it doesn’t
work as well for the conduction electrons themselves. It can
approximate the d bands of transition metals and the valence
bands of diamond and inert gases.
The lower part (the "cup") is
contained in the 1st Brillouin zone,
the upper part (the "top") comes
from the second BZ, but it is
folded back into the first one. It
thus would carry a different band
index. This could be continued ad
infinitum; but Brillouin zones with
energies well above the Fermi
energy are of no real interest.
These are tracings along major
directions. Evidently, they contain
most of the relevant information
in condensed form. It is clear that
this structure has no band gap.
Electron Energy Bands in 3D
Electronic structure calculations such as our tight-binding method
determine the energy eigenvalues εn at some point k in the first
Brillouin zone. If we know the eigenvalues at all points k, then the
band structure energy (the total energy in our tight-binding method)
is just
LCAO: Linear Combination of Atomic Orbitals
where the integral is over the occupied states of below the Fermi
level.
The full Hamiltonian of the
system is approximated by
using the Hamiltonians of isolated atoms, each one centered at
a lattice point.
The eigenfunctions are assumed to have amplitudes that go to
zero as distances approach the lattice constant.
The assumption is that any necessary corrections to the
atomic potential will be small.
The solution to the Schrodinger equation for this type of single
electron system, which is time-independent, is assumed to be a
linear combination of atomic orbitals.
Band Structure: KCl
We first depict the band structure of an ionic crystal, KCl. The bands are very
narrow, almost like atomic ones. The band gap is large around 9 eV. For alkali
halides they are generally in the range 7-14 eV.
Band Structure: simple cubic
Band Structure: silver (fcc)
Band Structure: tungsten (bcc)
Electron Density of States: Free Electron
Model
+ + + + +
+ + + + +
+ + + + +
+ + + + +
+ + + + +
Schematic model of metallic
crystal, such as Na, Li, K, etc.
The equilibrium positions of
the atomic cores are
positioned on the crystal lattice
and surrounded by a sea of
conduction electrons.
For Na, the conduction
electrons are from the 3s
valence electrons of the free
atoms. The atomic cores
contain 10 electrons in the
configuration: 1s2
2s2
p6
.
Electron Density of States: Free Electron
Model
• Assume N electrons (1 for
each ion) in a cubic solid with
sides of length L – particle in a
box problem.
• These electrons are free to
move about without any
influence of the ion cores,
except when a collision
occurs.
• These electrons do not
interact with one another.
• What would the possible
energies of these electrons
be?
∞
0 L
 How do we know there are free electrons?How do we know there are free electrons?

You apply an electric field across a metal pieceYou apply an electric field across a metal piece
and you can measure a current – a number ofand you can measure a current – a number of
electrons passing through a unit area in unitelectrons passing through a unit area in unit
time.time.

But not all metals have the same current for aBut not all metals have the same current for a
given electric potential. Why not?given electric potential. Why not?
Electron Density of States: Free Electron
Model
The electron density of states is a key parameter in the
determination of the physical phenomena of solids.
Electron Density of States
Knowing the energy levels, we can count how many energy
levels are contained in an interval ∆E at the energy E. This is
best done in k - space.
In phase space, a surface of constant
energy is a sphere as schematically
shown in the picture.
Any "state", i.e. solution of the
Schrodinger equation with a specific k,
occupies the volume given by one of
the little cubes in phase space.
The number of cubes fitting inside the
sphere at energy E thus is the number
of all energy levels up to E.
Electron Density of States: Free Electrons
Counting the number of cells (each containing one possible state
of ψ) in an energy interval E, E + ∆E thus correspond to taking
the difference of the numbers of cubes contained in a sphere with
"radius" E + ∆E and of “radius” E. We thus obtain the density of
states D(E) as
1 ( , ) ( )
( )
1
N E E E N E
D E
V E
dN
V dE
+ ∆ −
=
∆
=
where N(E) is the number of states between E = 0 and E per
volume unit; and V is the volume of the crystal.
Electron Density of States: Free Electrons
The volume of the sphere in k-space is
3
3
4
kV π=
The volume Vk of one unit cell,
containing two electron states is
3
2






=
L
Vk
π
The total number of states is then
( )
3 3 3 3
23
4
2 2
33 8k
V k L k L
N
V
π
ππ
 
 ÷= = =
 ÷
 
Electron Density of States: Free Electrons
2
22
2
2 
 mE
k
m
k
E ±=⇒=
3/2
3 2 2
1 1 2
( )
2
dN m
D E E
L dE π
 
= =  ÷
 
3 23 3 3
2 2 2
2
3 3
/
k L L mE
N
π π
 
= =  ÷
 
Electron Density of States: Free Electrons
D(E)
Electron Density of States: Free Electron
Model
From
thermodynamics,
the chemical
potential, and thus
the Fermi Energy, is
related to the
Helmholz Free
Energy:
where
VT
NFNF ,
)()1( −+=µ
F U TS= −
Electron Density of States: Free Electron
Model
If an electron is added, it
goes into the next available
energy level, which is at the
Fermi energy. It has little
temperature dependence.
( )/
( )/
1
( )
1
1
1
B
F B
k T
k T
f
e
e
ε µ
ε ε
ε −
−
=
+
=
+
Fermi-Dirac Distribution
For lower energies,
f goes to 1.
For higher energies,
f goes to 0.
Free Electron Model: QM Treatment
where nx, ny, and nz are integers
Free Electron Model: QM Treatment
and similarly for y and z, as well
2 4
0, , , ...
2 4
0, , , ...
2 4
0, , , ...
x
y
z
k
L L
k
L L
k
L L
π π
π π
π π
= ± ±
= ± ±
= ± ±
( )i k r
k eψ ×
=
Free Electron Model: QM Treatment
m
k
m
p
v

==
m
k
2
2
F
2
F

=ε
Free Electron Model: QM Treatment
B
F
F
k
T
ε
=
1/32
F F
3 N
v k
m m V
π 
= =  ÷
 
h h
( )
3/2
F2 2
3
2
2
3
ln ln constant
then
3
2
V m
N
N
dN N
D
d
ε
π
ε
ε
ε ε
 
=  ÷
 
⇒ = +
= =
h
Free Electron Model: QM Treatment
The number of orbitals per
unit energy range at the Fermi
energy is approximately the
total number of conduction
electrons divided by the Fermi
energy.
Free Electron Model: QM Treatment
As the temperature
increases above T = 0
K, electrons from region
1 are excited into region
2.
This represents how
many energies are
occupied as a function of
energy in the 3D
k-sphere.
Electron Density of States: LCAO
If we know the band structure at every point in the Brillouin zone, then the
DOS is given by the formula
( )
1
3
( ) k
4
n
n
dS
D ε ε
π
−
= ∇∑∫
where the integral is over the surface Sn(ε) is the surface in k space at
which the nth eigenvalue has the value εn.
Obviously we can not evaluate this integral directly, since we don't
know εn(k) at all points; and we can only guess at the properties of its
gradient. One common approximation is to use the tetrahedron method,
which divides the Brillouin zone into (surprise) tetrahedra, and then
linearly interpolate within the tetrahedra to determine the gradient. This
method is an approximation, but its accuracy obviously improves as we
increase the number of k-points.
When the denominator in the integral is zero, peaks due to van Hove
singularities occur. Flat bands give rise to a high density of states. It is also
higher close to the zone boundaries as illustrated for a two dimensional
lattice below.
Electron Density of States: LCAO
( )
1
3
( ) k
4
n
n
dS
D ε ε
π
−
= ∇∑∫
Leon van Hove
• For the case of metals, the
bands are very free electron-
like (remember we compared
with the empty lattice) and the
conduction bands are partly
filled.
• The figure shows the DOS for
the cases of a metal , Cu, and a
semiconductor Ge. Copper has
a free electron-like s-band,
upon which d-bands are
superimposed. The peaks are
due to the d-bands. For Ge the
valence and conduction bands
are clearly seen.
Electron Density of States: LCAO
Electron Density of States: LCAO
fcc
The basic shape of
the density of states
versus energy is
determined by an
overlap of orbitals. In
this case s and d
orbitals…
Electron Density of States: LCAO
bcc
tungsten

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Energy band theory of solids

  • 2. Nomenclature For most purposes, it is sufficient to know the En(k) curves - the dispersion relations - along the major directions of the reciprocal lattice. This is exactly what is done when real band diagrams of crystals are shown. Directions are chosen that lead from the center of the Wigner-Seitz unit cell - or the Brillouin zones - to special symmetry points. These points are labeled according to the following rules: • Points (and lines) inside the Brillouin zone are denoted with Greek letters. • Points on the surface of the Brillouin zone with Roman letters. • The center of the Wigner-Seitz cell is always denoted by a Γ
  • 3. For cubic reciprocal lattices, the points with a high symmetry on the Wigner-Seitz cell are the intersections of the Wigner Seitz cell with the low-indexed directions in the cubic elementary cell. Nomenclature simple cubic
  • 4. Nomenclature We use the following nomenclature: (red for fcc, blue for bcc): The intersection point with the [100] direction is called X (H) The line Γ—X is called ∆. The intersection point with the [110] direction is called K (N) The line Γ—K is called Σ. The intersection point with the [111] direction is called L (P) The line Γ—L is called Λ. Brillouin Zone for fcc is bcc and vice versa.
  • 5. We use the following nomenclature: (red for fcc, blue for bcc): The intersection point with the [100] direction is called X (H) The line Γ—X is called ∆. The intersection point with the [110] direction is called K (N) The line Γ—K is called Σ. The intersection point with the [111] direction is called L (P) The line Γ—L is called Λ. Nomenclature
  • 6. Real crystals are three-dimensional and we must consider their band structure in three dimensions, too. Of course, we must consider the reciprocal lattice, and, as always if we look at electronic properties, use the Wigner- Seitz cell (identical to the 1st Brillouin zone) as the unit cell. There is no way to express quantities that change as a function of three coordinates graphically, so we look at a two dimensional crystal first (which do exist in semiconductor and nanoscale physics). Electron Energy Bands in 3D The qualitative recipe for obtaining the band structure of a two-dimensional lattice using the slightly adjusted parabolas of the free electron gas model is simple:
  • 7. LCAO: Linear Combination of Atomic Orbitals AKA: Tight Binding Approximation • Free atoms brought together and the Coulomb interaction between the atom cores and electrons splits the energy levels and forms bands. • The width of the band is proportional to the strength of the overlap (bonding) between atomic orbitals. • Bands are also formed from p, d, ... states of the free atoms. • Bands can coincide for certain k values within the Brillouin zone. • Approximation is good for inner electrons, but it doesn’t work as well for the conduction electrons themselves. It can approximate the d bands of transition metals and the valence bands of diamond and inert gases.
  • 8.
  • 9. The lower part (the "cup") is contained in the 1st Brillouin zone, the upper part (the "top") comes from the second BZ, but it is folded back into the first one. It thus would carry a different band index. This could be continued ad infinitum; but Brillouin zones with energies well above the Fermi energy are of no real interest. These are tracings along major directions. Evidently, they contain most of the relevant information in condensed form. It is clear that this structure has no band gap. Electron Energy Bands in 3D
  • 10. Electronic structure calculations such as our tight-binding method determine the energy eigenvalues εn at some point k in the first Brillouin zone. If we know the eigenvalues at all points k, then the band structure energy (the total energy in our tight-binding method) is just LCAO: Linear Combination of Atomic Orbitals where the integral is over the occupied states of below the Fermi level.
  • 11. The full Hamiltonian of the system is approximated by using the Hamiltonians of isolated atoms, each one centered at a lattice point. The eigenfunctions are assumed to have amplitudes that go to zero as distances approach the lattice constant. The assumption is that any necessary corrections to the atomic potential will be small. The solution to the Schrodinger equation for this type of single electron system, which is time-independent, is assumed to be a linear combination of atomic orbitals.
  • 12. Band Structure: KCl We first depict the band structure of an ionic crystal, KCl. The bands are very narrow, almost like atomic ones. The band gap is large around 9 eV. For alkali halides they are generally in the range 7-14 eV.
  • 16. Electron Density of States: Free Electron Model + + + + + + + + + + + + + + + + + + + + + + + + + Schematic model of metallic crystal, such as Na, Li, K, etc. The equilibrium positions of the atomic cores are positioned on the crystal lattice and surrounded by a sea of conduction electrons. For Na, the conduction electrons are from the 3s valence electrons of the free atoms. The atomic cores contain 10 electrons in the configuration: 1s2 2s2 p6 .
  • 17. Electron Density of States: Free Electron Model • Assume N electrons (1 for each ion) in a cubic solid with sides of length L – particle in a box problem. • These electrons are free to move about without any influence of the ion cores, except when a collision occurs. • These electrons do not interact with one another. • What would the possible energies of these electrons be? ∞ 0 L
  • 18.  How do we know there are free electrons?How do we know there are free electrons?  You apply an electric field across a metal pieceYou apply an electric field across a metal piece and you can measure a current – a number ofand you can measure a current – a number of electrons passing through a unit area in unitelectrons passing through a unit area in unit time.time.  But not all metals have the same current for aBut not all metals have the same current for a given electric potential. Why not?given electric potential. Why not?
  • 19. Electron Density of States: Free Electron Model
  • 20. The electron density of states is a key parameter in the determination of the physical phenomena of solids. Electron Density of States Knowing the energy levels, we can count how many energy levels are contained in an interval ∆E at the energy E. This is best done in k - space. In phase space, a surface of constant energy is a sphere as schematically shown in the picture. Any "state", i.e. solution of the Schrodinger equation with a specific k, occupies the volume given by one of the little cubes in phase space. The number of cubes fitting inside the sphere at energy E thus is the number of all energy levels up to E.
  • 21. Electron Density of States: Free Electrons Counting the number of cells (each containing one possible state of ψ) in an energy interval E, E + ∆E thus correspond to taking the difference of the numbers of cubes contained in a sphere with "radius" E + ∆E and of “radius” E. We thus obtain the density of states D(E) as 1 ( , ) ( ) ( ) 1 N E E E N E D E V E dN V dE + ∆ − = ∆ = where N(E) is the number of states between E = 0 and E per volume unit; and V is the volume of the crystal.
  • 22. Electron Density of States: Free Electrons The volume of the sphere in k-space is 3 3 4 kV π= The volume Vk of one unit cell, containing two electron states is 3 2       = L Vk π The total number of states is then ( ) 3 3 3 3 23 4 2 2 33 8k V k L k L N V π ππ    ÷= = =  ÷  
  • 23. Electron Density of States: Free Electrons 2 22 2 2   mE k m k E ±=⇒= 3/2 3 2 2 1 1 2 ( ) 2 dN m D E E L dE π   = =  ÷   3 23 3 3 2 2 2 2 3 3 / k L L mE N π π   = =  ÷  
  • 24. Electron Density of States: Free Electrons D(E)
  • 25. Electron Density of States: Free Electron Model
  • 26. From thermodynamics, the chemical potential, and thus the Fermi Energy, is related to the Helmholz Free Energy: where VT NFNF , )()1( −+=µ F U TS= −
  • 27. Electron Density of States: Free Electron Model If an electron is added, it goes into the next available energy level, which is at the Fermi energy. It has little temperature dependence. ( )/ ( )/ 1 ( ) 1 1 1 B F B k T k T f e e ε µ ε ε ε − − = + = + Fermi-Dirac Distribution For lower energies, f goes to 1. For higher energies, f goes to 0.
  • 28. Free Electron Model: QM Treatment where nx, ny, and nz are integers
  • 29. Free Electron Model: QM Treatment and similarly for y and z, as well 2 4 0, , , ... 2 4 0, , , ... 2 4 0, , , ... x y z k L L k L L k L L π π π π π π = ± ± = ± ± = ± ± ( )i k r k eψ × =
  • 30. Free Electron Model: QM Treatment m k m p v  == m k 2 2 F 2 F  =ε
  • 31. Free Electron Model: QM Treatment B F F k T ε = 1/32 F F 3 N v k m m V π  = =  ÷   h h
  • 32. ( ) 3/2 F2 2 3 2 2 3 ln ln constant then 3 2 V m N N dN N D d ε π ε ε ε ε   =  ÷   ⇒ = + = = h Free Electron Model: QM Treatment The number of orbitals per unit energy range at the Fermi energy is approximately the total number of conduction electrons divided by the Fermi energy.
  • 33. Free Electron Model: QM Treatment As the temperature increases above T = 0 K, electrons from region 1 are excited into region 2. This represents how many energies are occupied as a function of energy in the 3D k-sphere.
  • 34.
  • 35. Electron Density of States: LCAO If we know the band structure at every point in the Brillouin zone, then the DOS is given by the formula ( ) 1 3 ( ) k 4 n n dS D ε ε π − = ∇∑∫ where the integral is over the surface Sn(ε) is the surface in k space at which the nth eigenvalue has the value εn. Obviously we can not evaluate this integral directly, since we don't know εn(k) at all points; and we can only guess at the properties of its gradient. One common approximation is to use the tetrahedron method, which divides the Brillouin zone into (surprise) tetrahedra, and then linearly interpolate within the tetrahedra to determine the gradient. This method is an approximation, but its accuracy obviously improves as we increase the number of k-points.
  • 36. When the denominator in the integral is zero, peaks due to van Hove singularities occur. Flat bands give rise to a high density of states. It is also higher close to the zone boundaries as illustrated for a two dimensional lattice below. Electron Density of States: LCAO ( ) 1 3 ( ) k 4 n n dS D ε ε π − = ∇∑∫ Leon van Hove
  • 37. • For the case of metals, the bands are very free electron- like (remember we compared with the empty lattice) and the conduction bands are partly filled. • The figure shows the DOS for the cases of a metal , Cu, and a semiconductor Ge. Copper has a free electron-like s-band, upon which d-bands are superimposed. The peaks are due to the d-bands. For Ge the valence and conduction bands are clearly seen. Electron Density of States: LCAO
  • 38. Electron Density of States: LCAO fcc The basic shape of the density of states versus energy is determined by an overlap of orbitals. In this case s and d orbitals…
  • 39. Electron Density of States: LCAO bcc tungsten

Editor's Notes

  1. Calculated electron wave functions for atomic sodium, plotted around two nuclei separated by the nearest-neighbor distance in metallic sodium of 3.7 angstroms. Overlap of the 1s wave functions is negligible – no alteration in the solid. Overlap of the 2s and 2p orbitals is small – so you would find bands associated with these. The overlap is strongest for the 3s – where the valence electrons are. In the tight binding approximation we do not expect cases of strong overlap to make significant contribution to the band structure.
  2. Every solid contains electrons. How those electrons respond to an electric field – whether they are conducting, insulating, or semi-conducting – is determined by the filling of available energy bands – separated by forbidden regions where no wavelike orbitals exist – these are the band gaps.
  3. When an electron is confined to a cube-shaped box, the wavefunction is a standing wave. Since we’ll also need this wavefunction to satisfy periodic boundary conditions, like we did for phonons, the wavefunctions will also be periodic in x, y, and z with period L. Of course, we want to deal with free-particles, so Mr. Schrodinger with periodic conditions gives us wavefunctions that are traveling plane waves...
  4. The traveling plane wave solution is valid as long as the components of the wavevector satisfy these relations...any component of k is of the form 2n/L where n is our positive or negative quantum number. This arises because when you satisfy the periodic boundary conditions, you find Just as in the case of phonons...only certain wavelengths are possible for these electrons confined to the box.
  5. The momentum i quantum mechanics is an operator In the ground state of a system of N particles, the occupied orbitals may be represented as points inside a sphere in k space... The energy at the surface of the sphere is the Fermi energy and the wavevectors have a maximum value kF.
  6. We can define a velocity at the Fermi surface... This is for an electron at the highest occupied energy level, which can have a k-vector pointing in any direction. We can also define what is called a Fermi temperature, but this is not a temperature of the electron gas. It is a measure of where the Fermi energy is at (typically on the order of ~ 10000 K) So, for most metals say at room temperature, not many electrons are excited above the Fermi energy.
  7. The red curve is the square root of the energy. The black curve is the red curve multiplied by the Fermi-Dirac distribution. The blue line represents the Fermi energy, filled levels at 0 K.