12 DIFFUSION PROCESSES IN ADVANCED TECHNOLOGICAL MATERIALS
where ∆H
f
and ∆H
m
are enthalpies for the formation and motion of the
defect, and S
f
and S
m
are the corresponding entropy terms, respectively.
The temperature dependence of the diffusion coefficient is generally of
the Arrhenius type and is written as:
D D
o
e
(QkT)
, (28)
with
D
o
1
6
a
2
Z f v
o
exp[(S
m
S
f
)k]. (29)
From the measurement of the diffusion coefficient, knowledge of the
crystal geometry (the coordination number and the lattice parameter), v
o
(related to Debye q
D
), and an independent measurement of the correla-
tion factor, f, it is possible to evaluate the total entropy factor. For the
separation of formation and motion components of the entropy and
enthalpy, separate experiments are needed, such as the resistance studies
of the quenched-in defects, the positron annihilation, and the simultane-
ous length and lattice parameters.
[10, 22]
Note that the diffusion coeffi-
cient and the various factors involved therein are basic properties of the
solids.
Table 1.1 lists self-diffusion data for several important pure elements.
While most metals diffuse by a vacancy mechanism, self-interstitial atoms
are important for diffusion in covalently bonded solids like Ge and Si, at
least at high temperatures.
[23]
When an interstitial atom is formed and a
vacancy is left behind, it is known as a Frenkel defect. Anotable example
for the formation of Frenkel defects is radiation damage in solids. The
energy involved in Frenkel defect formation equals the sum of the vacancy
and interstitial formation energies less the binding energy. The Frenkel
defect is usually very mobile and is accompanied by mass transport. The
interstitial atoms may also be of the impurity type, which fit into the inter-
stices in lattice easily by virtue of their small size. Consequently, their for-
mation energy is negligible, and in Eq. (27), the terms S
f
and ∆H
f
may be
omitted. Hence, diffusion of the foreign or impurity interstitials may be
very fast. Gas atoms such as H, C, O, and N commonly occur as intersti-
tials in BCC metals such as Fe, W, Nb, and Ta, and in HCPmetals such as
Ti, Zr, and Hf. In the Si lattice as well, most transition metal impurities
enter as interstitial atoms, although their solubilities rarely exceed one
part per million.
[14, 23, 24]