This document provides an overview of semiconductor theory and band theory of solids. It discusses how band theory can explain the differing electrical properties of conductors, semiconductors, and insulators based on their band structure and energy gaps. Semiconductors have a small energy gap between the valence and conduction bands that can be overcome by thermal excitation, allowing some electrons to reach the conduction band. Doping semiconductors with impurities can create n-type or p-type materials by introducing extra electrons or holes that increase conductivity. The document also covers thermoelectric effects in semiconductors.
1. 1
11.1 Band Theory of Solids
11.2 Semiconductor Theory
11.3 Semiconductor Devices
11.4 Nanotechnology
CHAPTER 11
Semiconductor Theory and Devices
It is evident that many years of research by a great many people, both
before and after the discovery of the transistor effect, has been required
to bring our knowledge of semiconductors to its present development.
We were fortunate to be involved at a particularly opportune time and to
add another small step in the control of Nature for the benefit of mankind.
- John Bardeen, 1956 Nobel lecture
2. 2
11.1: Band Theory of Solids
In Chapter 10 you learned about structural, thermal,
and magnetic properties of solids.
In this chapter we concentrate on electrical
conduction.
3. 3
Categories of Solids
There are three categories of solids, based on their
conducting properties:
conductors
semiconductors
insulators
5. 5
Reviewing the previous table reveals that:
The electrical conductivity at room temperature is
quite different for each of these three kinds of solids
Metals and alloys have the highest conductivities
followed by semiconductors
and then by insulators
6. 6
Semiconductor Conduction
The free-electron model from Chapter 9 does not
apply to semiconductors and insulators, since these
materials simply lack free electrons to conduct in a
free-electron mode, this is due to the nature of the
bond in the crystals
There is a different conduction mechanism for
semiconductors than for normal conductors.
7. 7
Resistivity vs. Temperature
Figure 11.1: (a) Resistivity versus temperature for a typical conductor. Notice the linear rise in
resistivity with increasing temperature at all but very low temperatures. (b) Resistivity versus
temperature for a typical conductor at very low temperatures. Notice that the curve flattens and
approaches a nonzero resistance as T → 0. (c) Resistivity versus temperature for a typical
semiconductor. The resistivity increases dramatically as T → 0.
8. 8
In order to account for decreasing resistivity with
increasing temperature as well as other properties of
semiconductors, a new theory known as the band
theory is introduced.
The essential feature of the band theory is that the
allowed energy states for electrons are nearly
continuous over certain ranges, called energy bands,
with forbidden energy gaps between the bands.
Band Theory of Solids
9. 9
Consider initially the known wave functions of two
hydrogen atoms far enough apart so that they do
not interact.
Band Theory of Solids
10. 10
Band Theory of Solids
Interaction of the wave functions occurs as the atoms get closer:
An electron in the symmetric state has a nonzero probability of
being halfway between the two atoms, while an electron in the
antisymmetric state has a zero probability of being at that location.
Symmetric Antisymmetric
11. 11
Band Theory of Solids
In the symmetric case the binding energy is
slightly stronger resulting in a lower energy
state.
Thus there is a splitting of all possible energy
levels (1s, 2s, and so on).
12. 12
When more atoms are added (as in a real solid), there is
a further splitting of energy levels. With a large number of
atoms, the levels are split into nearly continuous energy
bands, with each band consisting of a number of closely
spaced energy levels.
13. 13
Kronig-Penney Model
An effective way to understand the energy gap in
semiconductors is to model the interaction between
the electrons and the structure of the crystal where
atoms or groups of atoms are arranged on nodes of
a 3D periodic lattice and vibrate around their
equilibrium positions
R. de L. Kronig and W. G. Penney developed a
useful one-dimensional model of the electron lattice
interaction in 1931.
14. 14
Kronig-Penney Model
Kronig and Penney assumed that an electron
experiences an infinite one-dimensional array of finite
potential wells.
Each potential well models attraction to an atom in the
periodic structure, so the size of the wells must
correspond roughly to the lattice spacing in element
semiconductors.
15. 15
Kronig-Penney Model
Since the electrons are not free their energies are less
than the height V0 of each of the potentials, but the
electron is essentially free in the region 0 < x < a,
where it has a wave function of the form
where the wave number k is given by the usual
relation:
16. 16
Tunneling
In the region between a < x < a + b the electron can
tunnel through and the wave function loses its
oscillatory solution and becomes that of an
evanescent wave
18. 18
The left-hand side is limited to values between +1 and
−1 for all values of K.
Plotting this it is observed there exist restricted (shaded)
forbidden zones for solutions.
Kronig-Penney Model
19. 19
Figure 11.5 (a) Plot of the left side of
Equation (11.3) versus ka for κ2ba / 2 =
3π / 2. Allowed energy values must
correspond to the values of k for
for which the plotted
function lies between -1 and +1.
Forbidden values are shaded in light
blue. (b) The corresponding plot of
energy versus ka for κ2ba / 2 = 3π / 2,
showing the forbidden energy zones
(gaps).
The Forbidden Zones
20. 20
Important differences between the Kronig-
Penney model and the single potential well
1) For an infinite crystal structure (translation periodic lattice)
the allowed energies within each band are continuous
rather than discrete. In a real crystal the lattice is not
infinite, but even if chains are thousands of atoms long,
the allowed energies are nearly continuous.
2) In a real three-dimensional crystal it is appropriate to
speak of a wave vector . The allowed ranges for
constitute what are referred to in solid state theory as
Brillouin zones.
k
k
21. 21
And…
3) In a real crystal the potential function is more
complicated than the Kronig-Penney squares. Thus, the
energy gaps are by no means uniform in size. The gap
sizes can be changed by the introduction of impurities
or imperfections of the lattice.
These facts concerning the energy gaps are of
paramount importance in understanding the electronic
behavior of semiconductors.
22. 22
Band Theory and Conductivity
Band theory helps us understand what makes a
conductor, insulator, or semiconductor.
1) Good conductors like copper can be understood using the free
electron
2) It is also possible to make a conductor using a material with its
highest band filled, in which case no electron in that band can be
considered free.
3) If this filled band overlaps with the next higher band, however (so that
effectively there is no gap between these two bands) then an applied
electric field can make an electron from the filled band jump to the
higher level.
This allows conduction to take place, although typically
with slightly higher resistance than in normal metals. Such
materials are known as semimetals.
23. 23
Valence and Conduction Bands
The band structures of insulators and semiconductors
resemble each other qualitatively. Normally there exists in
both insulators and semiconductors a filled energy band
(referred to as the valence band) separated from the next
higher band (referred to as the conduction band) by an
energy gap.
If this gap is at least several electron volts, the material is
an insulator. It is too difficult for an applied field to
overcome that large an energy gap, and thermal excitations
lack the energy to promote sufficient numbers of electrons
to the conduction band.
24. 24
For energy gaps smaller than about 1 electron volt,
it is possible for enough electrons to be excited
thermally into the conduction band, so that an
applied electric field can produce a modest current.
The result is a semiconductor.
Smaller energy gaps create semiconductors
25. 25
11.2: Semiconductor Theory
At T = 0 we expect all of the atoms in a solid to be in the
ground state. The distribution of electrons (fermions) at
the various energy levels is governed by the Fermi-Dirac
distribution of Equation (9.34):
β = (kT)−1 and EF is the Fermi energy.
26. 26
Temperature and Resistivity
When the temperature is increased from T = 0, more and more
atoms are found in excited states.
The increased number of electrons in excited states explains the
temperature dependence of the resistivity of semiconductors.
Only those electrons that have jumped from the valence band to
the conduction band are available to participate in the
conduction process in a semiconductor. More and more
electrons are found in the conduction band as the temperature is
increased, and the resistivity of the semiconductor therefore
decreases.
27. 27
Some Observations
Although it is not possible to use the Fermi-Dirac factor to derive an exact
expression for the resistivity of a semiconductor as a function of
temperature, some observations follow:
1) The energy E in the exponential factor makes it clear why the band gap is
so crucial. An increase in the band gap by a factor of 10 (say from 1 eV to
10 eV) will, for a given temperature, increase the value of exp(βE) by a
factor of exp(9βE).
This generally makes the factor FFD so small
that the material has to be an insulator.
2) Based on this analysis, the resistance of a semiconductor is expected to
decrease exponentially with increasing temperature.
This is approximately true—although not exactly, because the function
FFD is not a simple exponential, and because the band gap does vary
somewhat with temperature.
28. 28
Clement-Quinnell Equation
A useful empirical expression developed by Clement
and Quinnell for the temperature variation of standard
carbon resistors is given by
where A, B, and K are constants.
29. 29
Test of the Clement-Quinnell Equation
Figure 11.7: (a) An experimental test of the Clement-Quinnell equation, using resistance versus
temperature data for four standard carbon resistors. The fit is quite good up to 1 / T ≈ 0.6,
corresponding to T ≈ 1.6 K. (b) Resistance versus temperature curves for some thermometers used in
research. A-B is an Allen-Bradley carbon resistor of the type used to produce the curves in (a). Speer
is a carbon resistor, and CG is a carbon-glass resistor. Ge 100 and 1000 are germanium resistors.
From G. White, Experimental Techniques in Low Temperature Physics, Oxford: Oxford University
Press (1979).
30. 30
Holes and Intrinsic Semiconductors
When electrons move into the conduction band, they leave behind
vacancies in the valence band. These vacancies are called holes.
Because holes represent the absence of negative charges, it is useful
to think of them as positive charges.
Whereas the electrons move in a direction opposite to the applied
electric field, the holes move in the direction of the electric field.
A semiconductor in which there is a balance between the number of
electrons in the conduction band and the number of holes in the
valence band is called an intrinsic semiconductor.
Examples of intrinsic semiconductors include pure carbon and
germanium.
31. 31
Impurity Semiconductor
It is possible to fine-tune a semiconductor’s properties by adding a small
amount of another material, called a dopant, to the semiconductor
creating what is a called an impurity semiconductor.
As an example, silicon has four electrons in its outermost shell (this
corresponds to the valence band) and arsenic has five.
Thus while four of arsenic’s outer-shell electrons participate in covalent
bonding with its nearest neighbors (just as another silicon atom would),
the fifth electron is very weakly bound.
It takes only about 0.05 eV to move this extra electron into the
conduction band.
The effect is that adding only a small amount of arsenic to silicon greatly
increases the electrical conductivity.
32. 32
n-type Semiconductor
The addition of arsenic to silicon creates what is known as an n-
type semiconductor (n for negative), because it is the electrons
close to the conduction band that will eventually carry electrical
current.
The new arsenic energy levels just below the conduction band
are called donor levels because an electron there is easily
donated to the conduction band.
33. 33
Acceptor Levels
Consider what happens when indium is added to silicon.
Indium has one less electron in its outer shell than silicon. The result is
one extra hole per indium atom. The existence of these holes creates
extra energy levels just above the valence band, because it takes
relatively little energy to move another electron into a hole
Those new indium levels are called acceptor levels because they can
easily accept an electron from the valence band. Again, the result is an
increased flow of current (or, equivalently, lower electrical resistance)
as the electrons move to fill holes under an applied electric field
It is always easier to think in terms of the flow of positive charges
(holes) in the direction of the applied field, so we call this a p-type
semiconductor (p for positive).
acceptor levels p-Type semiconductors
In addition to intrinsic and impurity semiconductors, there are many
compound semiconductors, which consist of equal numbers of
two kinds of atoms.
34. 34
Thermoelectric Effect
In one dimension the induced electric field E in a
semiconductor is proportional to the temperature gradient,
so that
where Q is called the thermoelectric power.
The direction of the induced field depends on whether the
semiconductor is p-type or n-type, so the thermoelectric
effect can be used to determine the extent to which n- or p-
type carriers dominate in a complex system.
35. 35
Thermoelectric Effect
When there is a temperature gradient in a thermoelectric
material, an electric field appears.
This happens in a pure metal since we can assume the
system acts as a gas of free electrons.
As in an ideal gas, the density of free electrons is greater at
the colder end of the wire, and therefore the electrical
potential should be higher at the warmer end and lower at the
colder end.
The free-electron model is not valid for semiconductors;
nevertheless, the conducting properties of a semiconductor
are temperature dependent, as we have seen, and therefore
it is reasonable to believe that semiconductors should exhibit
a thermoelectric effect.
This thermoelectric effect is sometimes called the Seebeck
effect.