Research Article: Structure and Thermal Stability of Copper Nitride Thin Films
Research Article: Structure and Thermal Stability of Copper Nitride Thin Films
Research Article
Structure and Thermal Stability of Copper Nitride Thin Films
Guangan Zhang,1 Zhibin Lu,1 Jibin Pu,1 Guizhi Wu,1 and Kaiyuan Wang2
1
State Key Laboratory of Solid Lubrication, Lanzhou Institute of Chemical Physics, Chinese Academy of Sciences,
Lanzhou 730000, China
2
School of Materials Science and Engineering, East China University of Science and Technology, Shanghai 200237, China
Copyright © 2013 Guangan Zhang et al. This is an open access article distributed under the Creative Commons Attribution License,
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copper nitride (Cu3 N) thin films were deposited on glass via DC reactive magnetron sputtering at various N2 flow rates and partial
pressures with 150∘ C substrate temperature. X-ray diffraction and scanning electron microscopy were used to characterize the
microstructure and morphology. The results show that the films are composed of Cu3 N crystallites with anti-ReO3 structure. The
microstructure and morphology of the Cu3 N film strongly depend on the N2 flow rate and partial pressure. The cross-sectional
micrograph of the film shows typical columnar, compact structure. The thermal stabilities of the films were investigated using
vacuum annealing under different temperature. The results show that the introducing of argon in the sputtering process decreases
the thermal stability of the films.
1 𝜇m 1 𝜇m
(a) (b)
1 𝜇m
(c)
Figure 3: The SEM image of Cu3 N film deposited under various N2 flow rate 50 sccm; 30 sccm; 10 sccm.
20 min. The XRD spectra of the films prepared at 0.8 Pa N2 (Figure 3(c)), grains on the surface appeared obviously as
partial pressure show a strong [100] orientation. The XRD uniformly nodular-like morphology.
spectra also show that the films prefer [100] orientation, The topography shown in Figure 4 suggests that the film is
but the (111) and (200) peaks become stronger at the N2 prepared with mixture of N2 and Ar. The grain size of the films
partial pressure of 0.6 Pa. For the films prepared at 0.4 Pa N2 increases with the argon introduced in the reactive atmo-
partial pressure, the [100] peaks disappeared. For the films sphere. The copper nitride films prepared at 0.8 Pa N2 partial
prepared at 0.2 Pa N2 partial pressure, the Cu4 N (111) peaks pressure also show pyramid cone morphology (Figure 4(a)).
were observed [12, 20]. The preferred orientation of the However, the film prepared at 0.6 Pa N2 partial pressure is
as-deposited copper nitride films is interpreted to depend composed of large polygonal grains (of up to micrometer
mainly on the mobility of the Cu and N atoms participating scale) with irregular tops separated by a large number of
in the film growth process [2]. Such mobility is expected to porous boundaries (Figure 4(b)). The additional Ar gas can
be a function of the ratio between the number of N and Cu dramatically increase the deposition rate of the films, and
atoms reaching the substrate and also of the kinetic energies high deposition rate may cause larger grain size and sharp
of these atoms. The preferred orientation transformed from grain boundaries.
Cu-rich orientation [111] to N-rich orientation [100] as N2 Difference in crystallite orientation and deposition rate of
partial pressure increased, which indicates that large amount adatoms is believed to be responsible for the great changes
of Cu and N atoms formed N-rich orientation at higher N2 in morphology. For the Cu3 N films prepared at N2 flow
partial pressure. rate of 10 sccm, the crystallite orientation [100] is much
stronger, while other orientations are very weak. This fine
3.2. Morphology. Figure 3 shows the surface morphology of [100] preferred orientation caused nodular-like morphology
the Cu3 N films deposited at different N2 flow rates. It is as a result of isotropic growth. While at higher N2 flow rate
obvious that all the films are extremely smooth, compact, and the argon introduction the pyramid cone morphology
and uniform. It can be found that the N2 flow rates had appeared. This phenomenon can be attributed to the multi-
no significant influence on the grain size of the Cu3 N plicate crystallite orientation. In the deposition process, [111]
films; however, the grain shapes were influenced obviously. and [100] orientation had a competitive growth and thus
Pyramid cone structure was found in Cu3 N films and presented complicated pyramid cone morphology.
deposited at 50 sccm N2 flow rate (Figure 3(a)). Figure 3(b) is In order to understand more details of the grains, we use
also the pyramid cone morphology of Cu3 N film deposited atomic force microscopy images. Figure 5 shows the image of
at 30 sccm N2 flow rate. For the N2 flow rate of 10 sccm film deposited under N2 flow rate of 50 sccm. We can clearly
4 Indian Journal of Materials Science
1.5
(𝜇m)
1
1 𝜇m
0.5
(a)
0
0 0.5 1 1.5 2
(𝜇m)
0.00 116.02
(nm)
(a)
1 𝜇m
80
(nm)
(b)
0
Figure 4: The SEM image of Cu3 N film deposited under various N2
partial pressure 0.8 Pa; 0.6 Pa. 0.5
(𝜇m) 1.0
1.5 0
0.5
see that several small grains of size ∼50 nm agglomerated 1.5
1.0
together and formed a big grain boundary (grains as seen in (𝜇m)
SEM images). (b)
A typical cross-sectional micrograph is also shown in
Figure 6, where the formation of columnar grains perpen- Figure 5: The AFM image of Cu3 N film deposited under N2 flow
dicular to the substrate surface and a smooth film surface rate of 50 sccm.
morphology is clearly shown. It is known that the columnar
structure formed due to the high deposition rate and low
lateral adatoms mobility. The columnar boundary is due to evolution of the phase structure and decomposition temper-
an accumulation effect of the crystallographic flaws that are ature of the film deposited at mixed N2 and Ar atmosphere is
built into the thin films during deposition and then enriched unlike the film deposited at pure N2 atmosphere (Figure 8).
in the boundary. When the heating temperature at 150∘ C, the intensity of Cu3 N
(111) diffraction peaks increased and the intensity closed to
3.3. Thermal Stability. The Cu3 N films deposited at N2 that of (100). At 200∘ C heating temperature, the intensity
flow rate of 10 sccm and N2 partial pressure of 0.8 Pa were of (100) peaks is stronger than the (111) peaks. However,
annealed in vacuum (pressure = 3.0 × 10−3 Pa) for 1 h at at 250∘ C heating temperature, Cu peaks appeared without
a temperature ranging from 150∘ C to 300∘ C. Figures 7 and obvious Cu3 N peaks. This indicates that Cu3 N phase has been
8 show the XRD spectra of the heat treated Cu3 N films transformed into Cu phase completely through annealing
compared with as prepared films. For the film prepared at treatment at a temperature of 250∘ C. The color change of
pure nitrogen atmosphere (Figure 7), it is found that as the Cu3 N films also can provide information of phase transform.
heating temperature at 150∘ C, the intensity of Cu3 N (111) and The decomposition temperature of Cu3 N in our experiment
(200) diffraction peaks decreased and almost disappeared, is higher than Cu3 N annealing in vaccum as reported [5].
and when the heating temperature reached 200∘ C and 250∘ C, One possibility of this difference of decomposition tem-
the diffraction peaks did not show obviously changes. Further perature is the structure. The films prepared at pure nitrogen
increase the heating temperature to 300∘ C, the Cu (111) peaks atmosphere show a small particle size with a relative compact
appeared, which indicated that decomposition took place at texture, while the films prepared at mixed nitrogen and argon
the temperature ranges from 250∘ C to 300∘ C, lower than the atmosphere show a larger particle size with obvious large
decomposition temperature (about 360∘ C) [6]. However, the number of void boundaries with a looser texture. And the
Indian Journal of Materials Science 5
Cu (200)
Cu (111)
300∘ C
250∘ C
Cu3 N (100)
Cu3 N (111)
Intensity (a.u.)
Cu3 N (200)
1 𝜇m
200∘ C
Figure 6: The typical cross-sectional SEM image of Cu3 N film.
150∘ C
Sample
20 30 40 50 60 70 80
2𝜃 (deg)
References
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