TABLE I. Fundamental and higher-order bands of aligned CCNTs recorded
spectra. Undoubtedly, the high density of the aligned CCNTs
helps detection of the higher-order Raman spectra.
on a Renishaw Raman system with 514.5 nm laser line I /I ϭ1.3Ϯ0.02.
D
G
In summary, we have successfully synthesized large area
aligned CCNTs, which are perpendicular to the surface of the
substrate. The tubes are around 10–15 nm in diameter and 50
m long. Raman spectra up to fourth order of the aligned
CCNTs have been collected, indicating that CCNTs are
highly graphitized. The appearance of a strong D band shows
that a nanometer scale turbostratic structure may be formed
in carbon nanotubes due to the relatively low growth tem-
perature. The Raman studies are consistent with the results
from SEM and HRTEM. Resonance behavior shows that the
lattice properties of the aligned CCNTs are different from
that of other forms of carbon. Third- and fourth-order Raman
spectra have been detected.
⌬
cmϪ1
⌬
͑cmϪ1
͒
͑
͒
Designation
Designation
1
094
348
581
617
453
697
930
3233
4043
4274
4511
4819
5385
5861
2
DЈ
1
1
1
2
2
2
D
G
3D
2 ϩG
D
ϩ2G
D
DЈ
ϩ2
G
DЈ
2D
4D
D
2 ϩ2G
ϩ
D
G
from a zone–boundary phonon activated by the disorder as-
sociated with finite crystalline size. This assignment is cor-
roborated with the strong peak at ϳ2697 cm ͑i.e., ϳ2
ϫ1348 cm ͒ in the second-order Raman spectrum and the
weak peak at ϳ5385 cm ͑i.e., ϳ4ϫ1348 cm ͒ in the
Ϫ1
The authors thank Wei Liu for the TEM measurements
and Yulong Liu, Yanyong Yang, and David Pitt for the Ra-
man scattering measurements. This work was partially sup-
ported by the National Natural Science Foundation of China.
Ϫ1
Ϫ1
Ϫ1
fourth-order Raman spectrum. While the D line at
348 cm has a counterpart in the second-order spectrum, if
Ϫ1
1
its presence results from the finite crystalline size of nanom-
Ϫ1
eter order, it might be expected that the peak at 1617 cm
also has a counterpart in the second-order spectrum of
CCNTs, namely, 3233 cm . It is important to note that the
1
Ϫ1
S. Iijima, Nature ͑London͒ 354, 56 ͑1991͒.
T. W. Ebbesen and P. M. Ajayan, Nature ͑London͒ 358, 220 ͑1992͒.
M. Endo, K. Takeuchi, S. Igarashi, K. Kobori, M. Shiraishi, and H. W.
Kroto, J. Phys. Chem. Solids 54, 1841 ͑1993͒.
2
differences in frequency between the observed first-order
modes and half the frequency of the corresponding second-
order modes could be due to matrix element effects or to the
region of the k space strongly sampled by the breakdown of
wave–vector conservation.
3
4
P. M. Ajayan, O. Stephan, C. Colliex, and D. Trauth, Science 265, 1212
͑
1994͒.
5
W. A. de Heer, W. S. Bacsa, A. Ch aˆ telain, T. Gerfin, R. H. Baker, L.
Forro, and D. Ugarte, Science 268, 845 ͑1995͒.
H. Dai, E. W. Wong, and C. M. Lieber, Science 272, 523 ͑1996͒.
W. Z. Li, S. S. Xie, L. X. Qian, B. H. Chang, B. S. Zou, W. Y. Zhou, R.
A. Zhao, and G. Wang, Science 274, 1701 ͑1996͒.
H. Hiura, T. W. Ebbesen, K. Tanigaki, and H. Takahashi, Chem. Phys.
Lett. 202, 509 ͑1993͒.
6
7
The second-order Raman spectrum of CCNTs is shown
Ϫ1
in Fig. 3͑a͒. As mentioned above, the peak at 2697 cm
(
D*) is the overtone of the D line, and the peak at
8
9
Ϫ1
2930 cm is attributed to the combination of the D and G
lines. In addition, the second-order scattering at 2453 and
J. M. Holden, P. Zhou, X. X. Bi, P. C. Eklund, S. Bandow, R. A. Jishi, K.
D. Chowdhury, G. Dresselhaus, and M. S. Dresselhaus, Chem. Phys. Lett.
Ϫ1
3
233 cm has also been observed very clearly and attrib-
220, 186 ͑1994͒.
uted to the corresponding fundamental bands, as summarized
10
J. Kastner, T. Pichler, H. Kuzmany, S. Curran, W. Blau, D. N. Weldon,
M. Delamesiere, S. Draper, and H. Zandbergen, Chem. Phys. Lett. 221, 53
Ϫ1
in Table I. The observation of the line at 3233 cm is strong
͑
1994͒.
evidence for overtone scattering from the highest-frequency
11
Ϫ1
W. S. Bacsa, D. Ugarte, A. Ch aˆ telain, and W. A. de Heer, Phys. Rev. B
line at ϳ1617 cm in the density of states.
50, 15 473 ͑1994͒.
The third- and fourth-order Raman spectra are shown in
Fig. 3͑b͒. To our knowledge, this is the first report on the
detection of such higher-order Raman spectra of carbon
12
P. V. Huong, R. Cavagnat, P. M. Ajayan, and O. Stephan, Phys. Rev. B
51, 10 048 ͑1995͒.
1
1
3
4
P. C. Eklund, J. M. Holden, and R. A. Jishi, Carbon 33, 959 ͑1995͒.
A. M. Rao, E. Richter, Shunji Bandow, Bruce Chase, P. C. Eklund, K. A.
Williams, S. Fang, K. R. Subbaswamy, M. Menon, A. Thess, R. E. Smal-
ley, G. Dresselhaus, and M. S. Dresselhaus, Science 275, 187 ͑1997͒.
T. W. Ebbesen, H. Hiura, J. Fujita, Y. Ochiai, S. Matsui, and K. Tanigaki,
Chem. Phys. Lett. 209, 83 ͑1993͒.
Y. Saito, T. Yoshikawa, M. Inagaki, M. Tomita, and T. Hayashi, Chem.
Phys. Lett. 204, 277 ͑1993͒.
R. S. Ruoff and D. C. Lorents, Carbon 33, 925 ͑1995͒.
V. Ivanov, A. Fonseca, J. B. Nagy, A. Lucas, D. Lambin, D. Bernaerts,
and X. B. Zhang, Carbon 33, 1727 ͑1995͒.
nanotubes. The very clear and strong third-order peak at
Ϫ1
4
274 cm can be safely attributed to a combination of 2
Ϫ1
15
ϫ1348ϩ1581 cm . However, this peak shows a large
downshift in frequency with respect to both the 4320 cm
peak of HOPG and the 4305 cm peak of PG. Further-
Ϫ1
1
1
6
7
Ϫ1
25
Ϫ1
more, the third-order peaks at 4043, 4511, and 4819 cm
have also been observed and assigned to 3ϫ1348 cmϪ1,
18
Ϫ1
Ϫ1
1
348ϩ2ϫ1581 cm , and 1581ϩ2ϫ1617 cm , respec-
tively. The fourth-order Raman band at 5861 cm is also
1
2
2
9
0
1
G. Vitali, M. Rossi, M. L. Terranova, and V. Sessa, J. Appl. Phys. 77,
Ϫ1
4307 ͑1995͒.
observed clearly in Fig. 3͑b͒ and can be assigned to the com-
D. G. McCulloch, S. Prawer, and A. Hoffman, Phys. Rev. B 50, 5905
͑1994͒.
V. Barbarossa, F. Galluzzi, R. Tomaciello, and A. Zanobi, Chem. Phys.
Lett. 185, 53 ͑1991͒.
F. Tuinstra and J. L. Koenig, J. Chem. Phys. 53, 1126 ͑1970͒.
R. J. Nemanich and S. A. Solin, Phys. Rev. B 20, 392 ͑1979͒.
R. Tsu, J. H. Gonzalez, and I. G. Hernandez, Solid State Commun. 27,
Ϫ1
bination of 2ϫ1348ϩ2ϫ1581 cm , while the fourth-order
Ϫ1
Raman spectrum at 5392 cm seems to appear and can be
Ϫ1
assigned to 4ϫ1348 cm
.
22
23
Basically, all the Raman features of aligned CCNTs are
similar to those of PG.25 This indicates that the microstruc-
ture of individual tubes of CCNTs is composed of many
crystalline domains, which possess a high degree of crystal-
line order, as shown by the appearance of high-order Raman
24
507 ͑1978͒.
25
Y. Kawashima and G. Katagiri, in International Conference on Raman
Spectroscopy, 14th, Hong Kong, 1994, edited by N. T. Yu and X. Y. Li
͑Wiley, New York͒, p. 752.
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