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duce the most desirable dispersion strengthening
as discussed in Chapter 11:
9
The matrix should be relatively soft and
ductile and the precipitate, or second
phase, should be strong;
9
the precipitate particles should be round
and discontinuous;
9
the second-phase particles should be small
and numerous; and
9
in general, the more precipitate phase we
have, the stronger the alloy will be.
As in Chapter 11, we will concentrate on how
phase transformations influence the strength of
the materials and how heat treatments can influ-
ence other properties. Since we will be dealing
with solid-state phase transformations, we will
begin with a discussion on the nucleation and
growth of second-phase particles in solid-state
phase transformations.
12-1 Nucleation and Growth in Solid-State Reactions
In Chapter 9, we discussed nucleation of a solid nucleus from a melt. We also discussed
the concepts of supersaturation, undercooling, and homogeneous and heterogeneous
nucleation. Let’s now see how these concepts apply to solid-state phase transformations
such as the eutectoid reaction. In order for a precipitate of phase b to form from a solid
matrix of phase a, both nucleation and growth must occur. The total change in free
energy required for nucleation of a spherical solid precipitate from the matrix is:
DG ¼
4
3
pr
3
DG
vða!bÞ
þ 4pr
2
s
ab
þ
4
3
pr
3
e ð 12-1Þ
The first two terms include the free energy change per unit volume (DG
v
), and the en-
ergy change needed to create the unit area of the interface (s
ab
), just as in solidification.
However, the third term takes into account the strain energy per unit volume (e), the
energy required to permit a precipitate to fit into the surrounding matrix during the
nucleation and growth of the precipitate, introduced when the precipitate forms in a
solid, rigid matrix. The precipitate does not occupy the same volume that is displaced,
so additional energy is required to accommodate the precipitate in the matrix.
Nucleation As in solidification, nucleation occurs most easily on surfaces already
present in the structure, thereby minimizing the surface energy term. Thus, the precip-
itates heterogeneously nucleate most easily at grain boundaries and other defects.
Growth Growth of the precipitates normally occurs by long-range di¤usion and redis-
tribution of atoms. Di¤using atoms must be detached from their original locations
(perhaps at lattice points in a solid solution), move through the surrounding material
to the nucleus, and be incorporated into the crystal structure of the precipitate. In some
cases, the di¤using atoms might be so tightly bonded within an existing phase that the
detachment process limits the rate of growth. In other cases, attaching the di¤using
atoms to the precipitate—perhaps because of the lattice strain—limits growth. This
result sometimes leads to the formation of precipitates that have a special relationship
to the matrix structure that minimizes the strain at the interface between the parent
phase and the precipitate particles. In most cases, however, the controlling factor is the
di¤usion step.
C H A P T E R 12 Dispersion Stren gthening by Phase Transfor mations and Heat Treatment358