Fundamentals of Materials Science and Engineering: An Integrated Approach, 3e

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GTBL042-11 GTBL042-Callister-v3 October 4, 2007 11:59


2nd Revised Pages

11.3 The Kinetics of Phase Transformations • 409

Surface or interface

Solid

Liquid



SL

IL
SI

Figure 11.5 Heterogeneous
nucleation of a solid from a liquid.
The solid–surface (γSI), solid–liquid
(γSL), and liquid–surface (γIL)
interfacial energies are represented
by vectors. The wetting angle (θ)is
also shown.

energy (i.e., energy barrier) for nucleation (G∗of Equation 11.4) is lowered when
nuclei form on preexisting surfaces or interfaces, since the surface free energy (γ
of Equation 11.4) is reduced. In other words, it is easier for nucleation to occur at
surfaces and interfaces than at other sites. Again, this type of nucleation is termed
heterogeneous.
In order to understand this phenomenon, let us consider the nucleation, on a
flat surface, of a solid particle from a liquid phase. It is assumed that both the liquid
and solid phases “wet” this flat surface, that is, both of these phases spread out and
cover the surface; this configuration is depicted schematically in Figure 11.5. Also
noted in the figure are three interfacial energies (represented as vectors) that exist
at two-phase boundaries—γSL,γSI, andγIL—as well as the wetting angleθ(the angle
between theγSIandγSLvectors). Taking a surface tension force balance in the plane
of the flat surface leads to the following expression:

γIL=γSI+γSLcosθ (11.12)

For heterogeneous
nucleation of a solid
particle, relationship
among solid-surface,
solid-liquid, and
liquid-surface
interfacial energies
and the wetting angle

Now, using a somewhat involved procedure similar to the one presented above
for homogeneous nucleation (which we have chosen to omit), it is possible to derive
equations forr∗andG∗; these are as follows:

r∗=−

2 γSL
Gv

(11.13)


For heterogeneous
nucleation, critical
radius of a stable
solid particle nucleus

G∗=


(


16 πγSL^3
3 Gv^2

)


S(θ) (11.14)

For heterogeneous
nucleation, activation
free energy required
for the formation of a
stable nucleus TheS(θ) term of this last equation is a function only ofθ(i.e., the shape of the
nucleus), which will have a numerical value between zero and unity.^1
From Equation 11.13, it is important to note that the critical radiusr∗for het-
erogeneous nucleation is the same as for homogeneous, inasmuch asγSLis the same
surface energy asγin Equation 11.3. It is also evident that the activation energy
barrier for heterogeneous nucleation (Equation 11.14) is smaller than the homoge-
neous barrier (Equation 11.4) by an amount corresponding to the value of thisS(θ)
function, or

G∗het=G∗homS(θ) (11.15)

(^1) For example, forθangles of 30◦and 90◦, values ofS(θ) are approximately 0.01 and 0.5,
respectively.

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