DIFFUSION IN BULK SOLIDS AND THIN FILMS, GUPTA 47
lattice (CSL) and are generally of low energy compared to the bound-
aries with long periodicity; the former may be termed special bound-
aries. In the case of arbitrary misorientation between two crystals, the
grain boundary minimizes its energy by preserving patches of the spe-
cial low-energy-ordered boundary and introducing therein arrays of
intrinsic grain boundary dislocations. It is also possible to have partial
grain boundary dislocations and extrinsic grain boundary dislocations
in the grain boundaries.
There is indirect experimental evidence from which a localized
structure of vacancies may be inferred with little relaxation of the
neighboring atoms. First, there was the measurement of pressure
dependence of the GB self-diffusivities in Ag by Martin et al.,
[80]
which
resulted in a value of ∆V
b
V
o
1.1, where V
o
is the activation volume
for GB self-diffusion defined analogous to Eq. (34) and V
o
is the atomic
volume. The value of ∆V
b
is of the order of atomic volume in grain
boundaries and compares very favorably to its counterpart in the lattice
(Table 1.2).
Second, the isotope effect measurement for self-diffusion in Ag grain
boundaries by Robinson and Peterson
[81]
has also resulted in a relatively
large value of ∆E
b
∼ 0.46, which is temperature-insensitive. The corre-
sponding value of the isotope effect for self-diffusion in lattice is 0.65
∆E
l
0.71; the variation is due to some temperature dependence (Table
1.2). If the mobile defects responsible for GB diffusion were partially dis-
sociated or highly relaxed vacancies, a correlated movement of a number
of atoms would be required for diffusion to occur. Therefore, only a small
isotope effect value would have been observed. The experimental data,
however, neither support nor rule out contribution of interstitial atoms to
grain boundary diffusion. Atomistic computer modeling of point defects
in grain boundaries, using various techniques such as kinetic Monte Carlo
and molecular dynamics, have shown that vacancies as well as interstitial
atoms are stable, depending on the misorientation of the boundary and the
host crystal lattice.
[82]
Both defects have similar attractive binding ener-
gies in the grain boundaries, are mobile, and account for diffusion under
certain conditions. Suzuki and Mishin
[82]
have studied the role of intersti-
tial atoms and vacancies in Cu grain boundaries in detail. They noted
that diffusion in the Σ 5(310) [001], commonly considered a typical
grain boundary, was dominated by the interstitial atoms, whereas other
boundaries, the Σ 5(210)[001], Σ 9(12
–
2)[011], Σ 11(31
–
1)[011],
Σ 7(23
–
1)[111], and Σ 13(34
–
1)[111], were dominated by vacancies. In
any event, grain boundary diffusion is many orders of magnitude faster
than in the lattice. In Sec. 1.5.3, a thermodynamic model is discussed to
explain this difference.