
220
9 Point Defects
The defectons can collide with one another at finite concen trations, and collisions
with other crystal excitations (e. g., phonons) are also possible at finite temperatures.
An increasing number of collisions fundamentally affects the character of defecton
motion. If the frequency of collisions is small enough, we practically have a freely
moving defecton. With increasing frequency of collisio ns the defecton can approach
equilibrium with the lattice during the time when it stays within a unit cell. We then
speak about a practically localized defect.
In most cases the tunneling probability is relatively small. Therefore, to calculate
the defecton dispersion law, we may use the strong coupling approximation known in
electron theory. The function ε
D
(k) is found in this case explicitly at all values of k.
For instance, for a simple cubic lattice we h ave
ε
D
(k)=ε
1
−ε
2
(cos ka
1
+ cos ka
2
+ cos ka
3
), (9.2.1)
where ε
1
, ε
2
are constant values, |ε
2
| is proportional to the quantum-tunneling proba-
bility; a
α
are the fundamental lattice translation vectors, α = 1, 2, 3. The width of the
defecton energy band is ∆ε = 6 |ε
2
|.
In an isotropic approximation, the expansion (9.2.1) near the minimum value of ε
0
(the energy band bottom) has the form
ε
D
= ε
0
+
¯h
2
k
2
2m
∗
, ε
0
= ε
1
−3ε
2
, (9.2.2)
where m
∗
is the defecton effective mass (of order of magnitude ¯h
2
/m
∗
∼ a
2
∆ε).
The presence of a defecton in a quantum crystal allows one to explain the physical
nature of quantum dilatatio n (Chapter 8). We assume that in a crystal free of impurities
the “defectiveness” arises only due to the excitation of vacancies. The possibility of
tunneling transforms a vacancy into a defecton, or a vacancy wave with the dispersion
relation (9.2.2).
Vacancy wave generation with k = 0 does not break the ideal periodicity of a
crystal. However, the number of crystal lattice sites becomes unequal to the number
of atoms. The defecton energy with k = 0,i.e.,ε
0
, is dependent on the state of
a crystal, in particular on its volume V changing under the influence of an external
pressure. It may turn out that at a certain volume V
k
the parameter ε
0
vanishes. We
assume that near this point
ε
0
= λ
V
k
−V
V
k
. (9.2.3)
We shall set, for definiteness, λ > 0 and consider the defectons obeying Bose
statistics (such as vacancies in solid
4
He).
It then follows from (9.2.3) that for V < V
k
, ε
0
> 0 and the energy spectrum of
defectons is separated from the ground-state energy (without defectons) by a gap. A
finite activation energy is needed to form a vacancy and thus at T = 0 the number of
defectons equals zero.