columns as a result of thermal motion. Importantly, the
apparent CD spectrum at 100 1C reveals that the helical
structure of 1 is exceptionally thermally stable. Subsequent
cooling to 25 1C restored the original CD spectrum. In
addition, the chiral anisotropy g factor (De307/e300 = 0.0044)
scarcely changes from low concentrations (4.20 Â 10À7 M) to
higher concentrations (4.20 Â 10À4 M; Fig. 3, inset), suggest-
ing strong association among the molecules.
This work was partly supported by the Sasakawa Scientific
Research Grant from The Japan Science Society.
Notes and references
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To further investigate the differences in the intermolecular
interactions, fluorescence (FL) spectra (4.20 Â 10À7 M) were
measured at an excitation of 360 nm (Fig. 4). Emission maxima
in CHCl3 and TCE solutions at 25 1C were observed at 457 nm
(fluorescence quantum yield, f = 0.26) and 459 nm (f = 0.32),
respectively. In contrast to the blue fluorescence observed for
these nonhelicogenic solutions, the emission in helicogenic n-
hexane and n-dodecane solutions was orange, and their max-
ima were observed at 604 (f = 0.020) and 607 nm (f = 0.036),
respectively. For the helicogenic solutions, the broad peaks at
around 605 nm are approximately 1/9–1/16 the intensity and
are considerably red-shifted with respect to the emission peaks
at around 458 nm for the nonhelicogenic solutions. This
behavior also indicates that the molecules form columnar
structures by strong p–p stacking in the helicogenic solvents.9
In addition, close stacking of 1 in n-alkanes is also supported
from the fact that the non-aggregated hexakis[4-(hexyloxycar-
bonyl)phenylethynyl]benzene, 2, which does not include amide
groups, shows no solvatochromism (Fig. S3w) and its UV-vis
and FL spectra in n-hexane were essentially the same as those
of L-1 in nonhelicogenic solutions.10 Consequently, the FL
property is clearly dependent on the aggregation state of 1, and
the emission changes from blue in the molecularly dispersed
state to orange in the helical columnar state. Here, the broad
emission in the helical columnar state is shifted by approxi-
mately 5300 cmÀ1 to lower energy compared to that of mono-
mer emission, considered to be excimer emission, because this
energy difference is comparable to those of other excimers
generated among the phenylethynyl units.11 With heating, the
excimer emission peak hypsochromically shifts by about 4 nm
and the intensity gradually decreases; the monomer emission
was not observed at all (Fig. 4, inset). This result also supports
the strong association of 1 in n-alkane. The decrease in
fluorescence intensity is probably due to several factors in
combination: (1) a decrease in positional order of the molecules
within the columns by thermal motion, (2) breaking of larger
columnar stacks into smaller stacks but not monomers,12a and
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In summary, we have succeeded in the synthesis of a
C6-symmetric hydrogen-bonded discotic molecule. Stacking
among large central cores of 1 is enforced by six intermolecular
hydrogen bonds, resulting in a highly stable supramolecular helical
structure, which exhibits excimer emission due to strong inter-
molecular interactions. In addition, the type of intermolecular
association is dependent on the solvent, and the observed fluor-
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a molecularly dispersed state. Detailed investigations into aspects
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ꢀc
This journal is The Royal Society of Chemistry 2008
Chem. Commun., 2008, 3447–3449 | 3449