Full Paper
exhibits “bowl chirality”, arising from the three-dimensional ge-
ometry. Attempts were made herein to produce enantiopure
forms from the racemates of 4ac by chiral resolution. The
chiral resolution of 4ac was performed with HPLC by using
a DAICEL CHIRALPAK IA chiral column. A mixed eluent system
composed of methanol and 2-propanol (1:1) gave the best re-
sults, clearly yielding two well-resolved peaks (see the Support-
ing Information). Owing to its very low solubility in the eluent
system, the chiral resolution of 4ac in useful amounts is im-
practical.
Table 7. Photophysical properties of buckybowls.[a]
[b]
Compound
labs [nm]
lem [nm]
3aa
3ba
4aa
4ba
5aa
5ba
C60
287, 337, 374 (sh), 405 (sh)
228, 268, 293, 336, 378 (sh), 400 (sh)
238, 288, 297, 308, 354 (sh)
252 (sh), 274, 300, 314, 370 (sh)
362, 421, 436 (sh), 461 (sh), 502 (sh)
345, 362, 416, 439, 466, 502 (sh)
336, 407
416, 436, 463 (sh)
414, 437, 462 (sh)
438, 466, 493 (sh)
467, 550 (sh)
528, 560 (sh)
528, 560 (sh)
C70
336, 366, 383, 470, 551 (sh)
[a] Samples (concentration ꢀ10À5 m) measured in CH2Cl2; sh=shoulder.
Wavelengths shown in italics represent excitation wavelengths.
Conclusion
A simple method for synthesizing highly curved buckybowls
was developed. These products can be directly generated from
easily obtained planar precursors under mild reaction condi-
tions. The bowl-shaped molecules thus formed exhibit a large
bowl depth and a high bowl-to-bowl inversion barrier. These
p-bowls can be used to study
C60 and C70 is known to be very weak because of the highly ef-
ficient intersystem crossing,[45] whereas 3 and 5 both exhibit
strong fluorescence at approximately 416/436 and 528 nm, re-
spectively. The photoluminescence of 4 is very weak.
bowl-to-bowl inversion dynam-
ics because they have planar or
S-shaped transition structures. It
is noteworthy that compounds
4 should be suitable starting
materials for constructing the
smallest
corannulene-based
carbon nanotube (C40H10).[31] The
electron mobility of polar bucky-
bowl crystals and the chiral aux-
iliary-assisted resolution of buck-
ybowls are currently being ex-
amined.
Figure 10. HOMO and LUMO distributions of compounds 3–5.
Figure 10 demonstrates that ethylene bridges of 3ba and
5ba participate similarly in establishing their HOMOs and
LUMOs, explaining why the photophysical properties of 3ba
and 5ba are similar to those of their parent compounds. How-
ever, the ethylene bridge in 4ba influences the HOMO more
strongly than it does the LUMO, increasing the potential of the
HOMO more than it does that of the LUMO (Table S1 in the
Supporting Information). The consequently reduced band gap
is responsible for the redshifting of the UV and PL spectra of
4ba relative to those of 4aa. Like C70, bowls 5 have longer-
wavelength absorptions than 3 and 4, although 3, 4 and 5 can
all map onto C70. The extent of p-conjugation of both HOMOs
and LUMOs of the three compound classes follows the order
5>3/4 (Figure 10). Accordingly, bowls 5 have the smaller band
gap. Time-dependent density functional theory (TD-DFT) calcu-
lations demonstrate that the strongest vertical excitation wave-
lengths for 3aa, 4aa, and 5aa are 306, 345, and 439 nm, re-
spectively (Table S2 in the Supporting Information).
Experimental Section
General procedures
1H and 13C NMR: Bruker 300 (300 and 75 MHz), 400 (400 and
100 MHz) and 500 (500 and 125 MHz). MS: High-resolution mass
spectra (HRMS) were obtained on Finnigan MAT-95XL high-resolu-
tion mass spectrometer. X-ray crystal structure determination:
Single-crystal X-ray diffraction was performed on a Bruker APEX
DUO at 100(2) K. Data were collected and processed by using
APEX II 4 K CCD detector. Melting points were determined with
a Bꢃchi melting point apparatus B545 and are uncorrected. UV
spectra were recorded with VARIAN CARY 50 Probe. Photolumines-
cence experiments were accomplished with Jasco FP-6300.
Procedure for the preparation of buckybowls
The procedures for preparing buckybowls 3/4[17] and 5[18] have
been described previously. The Supporting Information provides
analytic data concerning new compounds generated herein.
The high inversion barriers of 3–5 cannot be measured
using common NMR techniques, such as variable-temperature
and 2D EXSY methods, owing to instrumental limitations. Since
bowl inversion of an enantiopure bowl corresponds to the rac-
emization process, the racemization at high temperature may Acknowledgements
help to confirm experimentally the value of the inversion barri-
er. Numerous chiral buckybowls have been synthesized and ex-
amined.[46] Mono-substituted 4ac is a chiral buckybowl, which
This work was supported by the National Science Council of
Taiwan (NSC 101-2628-M-006-002-MY3 and NSC 99-2113-M-
Chem. Eur. J. 2014, 20, 598 – 608
606
ꢀ 2014 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim