is linked directly to the carbon of the pyrrolidine skeleton.3a 355 nm
excitation was chosen, although it populates the singlet excited
states of C60 (1.76 eV) and that of the oPPE (2.6 eV), due to over-
lapping absorptions. We know, however, from past experiments
with C60–oPPE that when the oPPEs are excited, a rapid
intramolecular transduction of energy funnels the excited state
energy to the fullerene core, generating 1*C60 quantitatively.8
Excitation of C60, on the other hand, leads directly to 1*C60.
Overall the quantum yield of C60 fluorescence amounts to 6.0 6
1024—identical to that of a C60-reference that lacks the oPPE
however, clear that no radical ion pair is formed for the 3-mer—
2
?
vide infra. Both radical ion pair features, that is, C60 and
+
6
exTTF , decay in the 0-mer (4.9 6 10 s21), 1-mer (1.1 6
?
106 s21), and 2-mer (3.8 6 105 s21) with similar rates (2DGCR
1.0 eV) to reinstate the singlet ground states.
#
Relating the charge separation and charge recombination
dynamics in THF to the electron donor acceptor separation (i.e.,
center-to-center—RCC) enabled us to evaluate the damping factor
of the oPPE bridges—see Fig. 2.10 Both relationships reveal linear
dependences and provided damping factors (b) that are in perfect
agreement with each other: 0.21 ¡ 0.05 A21 for charge separation
bridge—ruling out any endothermic electron transfer (2DGCS
.
˚
20.24 eV) between C60 (Ered: 0.61 ¡ 0.02 V versus Ag/Ag+)8
and oPPE (Eox: 1-mer: 2.09 V, 2-mer: 2.04 V; 3-mer: 1.96 V versus
Ag/Ag+).8
versus 0.2 ¡ 0.05 A21 for charge recombination. Please note that
˚
these values are more than an order of magnitude higher than
what we have established earlier for oPPV bridges (i.e., 0.01 ¡
0.005 A21).3
In stark contrast to C60–oPPE and the C60 reference, the
fullerene fluorescence is appreciably quenched in 9a–c (i.e., as low
as 0.55 6 1024 in THF)—Fig. S2.{ Moreover, the fluorescence
quantum yields depend strongly on the length of the oPPE bridge:
0-mer: 0.18 6 1024; 1-mer: 0.55 6 1024; 2-mer: 1.8 6 1024.§
Setting these quantum yields in context to the C60-reference and its
lifetime, the C60 fluorescence deactivation rates in the 0-mer,
1-mer, and 2-mer were determined as 2.1 6 1010 s21, 6.6 6 109 s21
and 1.3 6 109 s21, respectively. Additionally, we followed the
fluorescence at 710 nm, but found only measurable decay rates for
the C60 reference (6.6 6 108 s21) and the 2-mer (2.6 6 109 s21).
˚
˚
Extrapolating the relationships to RCC of 28.46 A, which
corresponds to the center-to-center distance in the 3-mer, helps to
explain the lack of electron transfer activation in the latter: The
rate of electron transfer would be with 3.9 6 108 s21, notably
slower than the intrinsic deactivation of the C60 singlet excited state
(6.6 6 108 s21)—see marked data point (i.e, large square) in Fig. 2.
To shed light on this observation we conducted calculations on
the topological and electronic structure of C60–oPPE–exTTF.
Theoretical calculations at DFT and semiempirical AM1 levels
revealed that the dihedral angle formed by the phenyl ring adjacent
to the pyrolidine and the benzene moiety of the exTTF connected
to the oligomer is not planar, and this deviation from planarity
increased significantly when semiempirical PM3 was used
(Fig. S3{). This lack of planarity could break the electronic
coupling between the donor and acceptor units in 9c, thus
accounting for the photophysical outcome.
1
We must conclude at this point of the investigation that *C60,
populated either directly or indirectly, powers an exothermic
electron transfer (2DGCS # 0.7 eV) to yield the radical ion pair
state, C60 –oPPE–exTTF .
2
?
+
?
The aforementioned hypothesis, namely, formation of the
radical ion pair state, was corroborated through transient
absorption spectroscopy. Importantly, Fig. 1 corroborates the
The investigation of the electronic structure revealed significant
differences between the oPPE and oPPV systems. The HOMO in
both systems is strongly localized on the exTTF and the LUMO
on the C60. According to the common, but oversimplified, one-
electron concept, the HOMO–LUMO transition would represent a
complete charge-transfer excitation with a very low extinction
coefficient. In addition, the HOMO in the C60–oPPV–exTTF triad
reaches into the oPPE bridge, whereas the HOMO in the C60–
oPPE–exTTF triad is completely localized on the exTTF. This
+
?
spectral signatures of the one-electron oxidized exTTF and the
one-electron reduced C60 2, which were detected as new transient
?
maxima at 660 and 1000 nm, respectively.3,9 The spectral
identification holds for the 0-mer, 1-mer, and 2-mer, while for
the 3-mer only a very broad transient, whose identity remains
unknown to us at this stage, dominates the region of interest. It is,
Fig. 1 Differential absorption spectrum (visible and near-infrared)
obtained upon nanosecond flash photolysis (355 nm) of y1.0 6 1025
M
Fig. 2 Center-to-center distances (RCC) dependence of electron transfer
rate constants (ln kCR) in C60–oPPV–exTTF in nitrogen saturated THF at
room temperature. The dotted line represents the singlet lifetime of C60.
solutions of C60–oPPV–exTTF (2-mer) in nitrogen saturated THF with a
time delay of 200 ns at room temperature. Insert shows charge
recombination dynamics at 660 nm.
This journal is ß The Royal Society of Chemistry 2006
Chem. Commun., 2006, 3202–3204 | 3203