6037
Wang, Rittby, and Graham: Detection of cyclic C6
with the simulated spectrum shows a good match for the
dominant singly C-substituted bands.
sured for the first time based on the excellent agreement of
the frequency, isotopic shifts, and their relative intensities
1
3
Additional, weaker features in the simulated spectrum in
Fig. 3͑b͒ belong to the doubly substituted isotopomers. Cor-
responding absorptions observed in the FTIR spectrum are
clearly observable in the spectrum of Fig. 4 at 1652.4 ͑H͒,
with the predictions from DFT calculations. Cyclic C is the
first cyclic carbon cluster so far discovered spectroscopically.
6
ACKNOWLEDGMENTS
1
1
657.4 ͑F͒, 1658.7 ͑L͒, 1679.4 ͑J͒, 1681.9 ͑I͒, and
682.7 cm ͑K͒. Under a variety of conditions they also
Grants from the Welch Foundation ͑Graham, No.
P-0786; Rittby, No. P-1259͒ and the TCU Research Fund in
support of this research, and from the W. M. Keck Founda-
tion for the purchase of the Bomem spectrometer, are grate-
fully acknowledged. The authors are grateful to Mike Mur-
dock for his skill and advice in the construction of the laser
evaporation and rod fabrication systems.
Ϫ1
exhibit intensity behavior which is similar to that for the
three singly substituted isotopomer bands. As shown in
Table III, these weaker absorptions are readily assigned to
isotopomers with double 13C substitutions. The experimental
frequency values are in reasonably good agreement with the
DFT predicted values despite the fact that some of the iso-
topomer bands overlap. For example, a band was not as-
signed to the ͑M͒ isotopomer because it is overlapped by the
singly substituted 13C isotopomer ͑D͒ band. Similarly, an
1
W. Weltner, Jr. and R. J. Van Zee, Chem. Rev. 89, 1713 ͑1989͒.
J. M. L. Martin, J. P. Franc c¸ ois, and R. J. Gijbels, Mol. Struct. 294, 21
2
͑1993͒.
3
K. R. Thompson, R. L. DeKock, and W. Weltner, Jr., J. Am. Chem. Soc.
assignment for ͑G͒ was not made because it is overlapped by
a band at 1687.6 cm
Ϫ1
93, 4688 ͑1971͒.
.
4
M. Vala, T. M. Chandrasekhar, J. Szcepanski, and R. Pellow, High Temp.
Additional bands appearing at 1667.4, 1671.1, 1675.9,
Sci. 27, 19 ͑1990͒.
R. H. Kranze and W. R. M. Graham, J. Chem. Phys. 98, 71 ͑1993͒.
D. W. Arnold, S. E. Bradforth, T. N. Kitsopoulos, and D. M. Neumark, J.
Ϫ1
5
and 1687.6 cm in Fig. 4 are not, however, related to the
1
the evidence of their different behavior during annealing and
on the correlation of their intensities with other bands to the
high-frequency side of the 1694.9 cm absorption. The in-
6
Ϫ1
694.9 cm absorption. This conclusion is based both on
Chem. Phys. 86, 5212 ͑1986͒.
J. Kurtz and D. P. Huffman, J. Chem. Phys. 92, 30 ͑1990͒.
H. J. Hwang, A. Van Orden, K. Tanaka, E. W. Kuo, J. R. Heath, and R. J.
7
8
Ϫ1
Saykally, Mol. Phys. 79, 769 ͑1993͒.
T. F. Giesen, A. Van Orden, H. J. Hwang, R. S. Fellers, R. A. Proven c¸ al,
9
Ϫ1
tensity of the band at 1687.6 cm decreases slightly on an-
nealing while the intensities of the 1694.9 cm band and its
and R. J. Saykally, Science 265, 756 ͑1994͒.
K. Raghavachari, R. A. Whiteside, and J. A. Pople, J. Chem. Phys. 85,
Ϫ1
10
associated isotopic shift bands all increase. Although appar-
ently not a member of the 1694.9 cm band group, the
6623 ͑1986͒.
Ϫ1
11
K. Raghavachari and J. S. Binkley, J. Chem. Phys. 87, 2191 ͑1987͒.
1
1
2
3
Ϫ1
V. Parasuk and J. Alml o¨ f, J. Chem. Phys. 91, 1137 ͑1989͒.
J. Hutter, and H. P. L u¨ thi, J. Am. Chem. Soc. 101, 2213 ͑1994͒.
J. Hutter, H. P. L u¨ thi, and F. Diederich, J. Am. Chem. Soc. 116, 750
͑1994͒.
J. Szcepanski, and M. J. Vala, J. Phys. Chem. 95, 2792 ͑1991͒.
C. M. L. Rittby ͑unpublished͒.
R. H. Kranze ͑unpublished͒.
J. M. L. Martin and P. R. Taylor, J. Phys. Chem. 100, 6047 ͑1996͒; J. M.
L. Martin ͑private communication͒.
1
687.6 cm band remains unidentified. The intensities of
Ϫ1
the bands at 1667.4, 1671.1, and 1675.9 cm seem corre-
lated to other moderately intense bands located to the high-
frequency side of the 1694.9 cm absorption ͑e.g., 1705.7,
14
Ϫ1
15
1
1
6
7
Ϫ1
1
710.6, and 1714.2 cm ͒, but not shown in both Figs. 3͑a͒
and 4, and may belong to unidentified carbon clusters
trapped in the matrix.
18
19
J. M. L. Martin, J. El-Yazal, and J. P. Fran c¸ ois, Chem. Phys. Lett. 242,
Table III, comparing the observed frequencies and cor-
responding shifts with the values calculated at two different
levels of DFT calculations, summarizes the proposed assign-
5
70–579 ͑1995͒.
20
W. Kr a¨ tschmer and K. Nachtigall, in Polycyclic Aromatic Hydrocarbons
and Astrophysics, edited by A. Leger et al. ͑Reidel, Dordrecht, 1987͒, p.
´
13
ments. It can be seen that all of the single C shifts and
75.
2
2
1
2
¯
almost all of the doubly 13C substituted isotopic shifts, ex-
Z. Slanina, J. M. Rudzi n´ ski, and E. Osawa, Z. Phys. D 19, 431 ͑1991͒.
R. H. Kranze, P. A. Withey, C. M. L. Rittby, and W. R. M. Graham, J.
Chem. Phys. 103, 6841 ͑1995͒.
R. H. Kranze, C. M. L. Rittby, and W. R. M. Graham, J. Chem. Phys. 105,
5313 ͑1996͒.
cept for one singly and two doubly substituted shifts which
are overlapped by other bands, can be unambiguously as-
signed to isotopomers of cyclic C (D ).
2
2
3
4
6
3h
D. Han, C. M. L. Rittby, and W. R. M. Graham, J. Chem. Phys. 106, 6222
͑
1997͒.
V. CONCLUSION
25
M. J. Frisch, G. W. Trucks, H. B. Schlegel, P. M. W. Gill, B. G. Johnson,
M. A. Robb, J. R. Cheeseman, T. Keith, G. A. Petersson, J. A. Montgom-
ery, K. Raghavachari, M. A. Al-Laham, V. G. Zakrzewski, J. V. Ortiz, J.
B. Foresman, J. Cioslowski, B. B. Stefanov, A. Nanayakkara, M. Challa-
combe, C. Y. Peng, P. Y. Ayala, W. Chen, M. W. Wong, J. L. Andres, E.
S. Replogle, R. Gomperts, R. L. Martin, D. J. Fox, J. S. Binkley, D. J.
Defrees, J. Baker, J. P. Stewart, M. Head-Gordon, C. Gonzalez, and J. A.
Pople, GAUSSIAN 94, Revision D.2, Gaussian, Inc., Pittsburgh, PA, 1995.
L. N. Shen, T. J. Doyle, and W. R. M. Graham, J. Phys. Chem. 93, 1597
͑1990͒.
FTIR measurements in an Ar matrix combined with pre-
dictions from a new B3LYP/cc-pVTZ DFT calculation per-
formed in the present work, and previous B3LYP/cc-pVDZ
calculations by Martin and Taylor,18 have resulted in the first
spectroscopic identification of cyclic C . The most intense
6
Ϫ1
infrared active mode, (eЈ)ϭ1694.9 cm of the cyclic C6
26
4
structure with D3h symmetry, has been assigned and mea-
J. Chem. Phys., Vol. 107, No. 16, 22 October 1997
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