Journal of The Electrochemical Society, 155 ͑9͒ D569-D574 ͑2008͒
D573
Figure 10. Cu island density vs time at −0.8, −0.9, and −1.0 V.
faster than the nickel growth rate, even though the Ni͑II͒ concentra-
tion in solution is almost an order of magnitude larger. At longer
times, the Cu deposition rate decreases, and steady-state growth is
achieved after about 10 s, corresponding to the transition region
described above ͑see Fig. 5͒. The miscibility gap provides the driv-
ing force for phase separation and leads to the formation of a co-
lumnar microstructure.
On the basis of our results, we can summarize the conditions
required to form a core/shell microstructure in a binary alloy system.
First, the system must exhibit a miscibility gap in the composition
range of interest, providing a thermodynamic driving force for phase
separation. Second, to form the core requires a material with a high
initial current and low island density. The fast initial kinetics results
in the formation of a low density of relatively large islands at short
times. Third, the shell requires a material with a relatively low initial
current and high island density, resulting in the formation of rela-
tively small islands. Based on these considerations, it should be
possible to extend the core/shell structure to other systems such as
Co–Cu.
Figure 12. ͑Color online͒ Schematic illustration of the evolution of the
core/shell microstructure. Initially, the growth rate of copper is very fast
compared to nickel and the relatively low island density results in the for-
mation of large copper islands surrounded by smaller nickel islands. As the
copper growth rate slows down, the core/shell microstructure evolves as
steady state is reached.
island density is relatively large, resulting in the formation of a high
density of nickel islands surrounding the larger copper islands. At
longer times, the copper growth and nickel growth reaches steady
state due to the decreased rate of copper deposition. The differences
in nucleation and growth kinetics, coupled with the miscibility gap,
result in this unique core/shell microstructure.
Acknowledgment
This work was supported by the JHU MRSEC ͑NSF grant no.
DMR05-20491͒.
Conclusion
Phase separation in electrodeposited Cu–Ni thin films results in
nodular features with a copper-rich core and nickel-rich shell. We
show that the evolution of this microstructure can be explained by
differences in nucleation and growth between copper and nickel. At
short times, copper deposition is initially fast and exhibits a rela-
tively low island density, resulting in the formation of large hemi-
spherical islands that become the cores in the nodular features. In
contrast, the kinetics of nickel deposition is initially slow but the
Johns Hopkins University assisted in meeting the publication costs of this
article.
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