
energy states that constitute the silicon conduction band are derived from the
higher excited states of the silicon atoms but relate to motion of the electrons
throughout the crystal. This contrasts with the organic molecular crystals in
which all the electrons remain bound within individual molecules and are only
transferred from one molecule to another under exceptional conditions.
Magnesium oxide can be regarded as typical of an ionic solid. In this case the
valence electrons attached to anions have minimal interactions with the electrons
attached to the cations. The energy states that constitute the conduction band are
derived from the higher excited 3s state of the magnesium atoms; the valence
band is derived from the 2p states of the oxygen atoms. An energy diagram of the
form shown in Fig. 2.8(b) is applicable for both covalent and ionic crystals.
If the temperature dependence of the electronic conductivity of a semi-
conductor is to be accounted for, it is necessary to analyse how the density of
charge carriers and their mobilities each depend upon T (see Eq. (2.25)). In the
first place attention will be confined to the density n of electrons in the conduction
band and the density p of ‘holes’ in the valence band. When the ‘intrinsic’
properties of the crystal are under consideration, rather than effects arising from
impurities or, in the case of compounds, from departures from stoichiometry, the
corresponding conductivity is referred to as ‘intrinsic conductivity’. The approach
to the calculation of n and p in this instance is as follows.
Figure 2.9 illustrates the situation in which a small fraction of the valence
electrons in an intrinsic semiconductor have been thermally excited into the
conduction band, with the system in thermal equilibrium. Since the only source
of electrons is the valence band p
i
¼ n
i
, where the subscript indicates intrinsic.
Formally, the electron density in the conduction band can be written
n
i
¼
ð
E
top
E
c
ZðEÞFðEÞdEð2:28Þ
in which ZðEÞdE represents the total number of states in the energy range dE
around E per unit volume of the solid, and the Fermi–Dirac function FðEÞ
represents the fraction of states occupied by an electron. FðEÞ has the form
FðEÞ ¼ exp
EE
F
kT
þ 1
1
ð2:29Þ
where E
F
is the Fermi energy, which is a characteristic of the particular system
under consideration.
The evaluation of n
i
is readily accomplished under certain simplifying
assumptions. The first is that EE
F
kT, which is often the case since kT is
approximately 0.025 eV at room temperature and EE
F
is commonly greater
than 0.2 eV. If this condition is met the term þ1 can be omitted from Eq. (2.29);
if it is not met then the electron distribution is said to be degenerate and the full
Fermi function must be used. The second assumption is that the excited electrons
30 ELEMENTARY SOLID STATE SCIENCE