Angewandte
Communications
Chemie
3
4.24 eV. Reductive MLCT excited-state quenching of both
photosensitizers leading to the TAA+-RuI-AQ-RuI-TAA+
state at 3.90 eV cannot be temporally resolved on our setup.
Subsequently, two-electron transfer steps from the two RuI
centers to AQ occur, going via the TAA+-RuII-AQÀ-RuI-
TAA+ state that is estimated to be at 3.48 eV to finally the
TAA+-RuII-AQ2À-RuII-TAA+ state (CSS2) at 3.56 eV. Due to
the multitude of overlapping processes, we cannot disentangle
them all, nevertheless it is reasonable to assume that the last
electron-accumulating step occurring with a 65 ps time
constant is rate-determining, because it has significantly
smaller driving-force than the preceding electron-transfer
events. Based on the redox potentials (SI page S11) that
electron-accumulating step would even be slightly endergonic
(DGET0 = 0.08 eV), but it should be kept in mind that the
energy estimates in Scheme 2 are associated with uncertain-
ties of Æ 0.1 eV.
Figure 3. Dependence of the AQ bleach at 1322 cmÀ1 and the AQ2À
absorption band at 1366 cmÀ1 on the excitation pulse energy. The data
have been averaged over various time points ranging from 1 to 100 ns
to enhance the signal-to-noise ratio. The inset shows the change in
The TAA+-RuII-AQÀ-RuII-TAA (CSS1) and TAA+-RuII-
AQ2À-RuII-TAA+ (CSS2) states then decay with time con-
stants of 980 and 870 ns, respectively. While the lifetime of
CSS1 is not surprising,[6,9] the relatively long lifetime of CSS2
is remarkable in view of the multitude of decay channels
which in principle are open to a state which is energetically
approximately 3.56 eV above the ground state. However, we
note that relaxation of CSS2 to CSS1 is associated with
optical density (OD) at 1366 cmÀ1 compared to that at 1322 cmÀ1
which reports on the bleaching of AQ and as such is used as an
,
internal standard (which is free of the uncertainty originating from, for
example, the alignment of the spatial overlap between pump- and
probe pulse). The data are fitted to a quadratic function up approx-
imately 0.03 mJ, and to a linear function beyond.
0
DGET ꢀ À2.0 eV, hence it is possible that this reaction is
decelerated by an inverted driving-force effect,[10] similar to
what we observed for the charge-recombination from CSS1 in
donor-bridge-acceptor molecules which are structurally
closely related to triad II.[6b,9]
the largest pump pulse energies tested (Ep = 2 mJ). At this
stage, we do not know what the photo-physical processes are
that give rise to both observations. Double-pulse excitation
experiments with high time-resolution, along the lines of
Ref. [2a], might elucidate these processes.
Since population of CSS2 requires absorption of two
photons, a quadratic dependence of the intensity of the signal
at 1366 cmÀ1 on excitation power is expected. This is indeed
the case, as the data in Figure 3 show. At an excitation energy
of 0.01 mJ, a bleach of the AQ band at 1322 cmÀ1 is already
detectable whereas at 1366 cmÀ1 no trace of AQ2À is
recognizable yet, indicating the exclusive formation of AQÀ
(CSS1) at the lowest pulse energy (Ep). At Ep > 0.01 mJ, the
AQ2À signal at 1366 cmÀ1 (CSS2) becomes observable, and for
Ep > 0.04 mJ the bleach at 1322 cmÀ1 and the signal at
1366 cmÀ1 increase in parallel in essentially a linear fashion.
The inset of Figure 3 highlights this behavior by showing the
expected quadratic power dependence seen up to approx-
imately 0.03 mJ. By comparing the amplitude of the transient
IR response with the spectro-electrochemical difference
spectrum (see SI Figure S4), we estimate that the fractions
of excited pentads, averaged over the excited volume,
amounts to 2% at Ep = 0.03 mJ. As an independent estimate
of the excitation probability, we can also consider the
extinction coefficient of the photosensitizer and the peak
irradiance of the pump pulse, revealing an excitation prob-
ability of 3% at Ep = 0.03 mJ (SI page S12). The second
estimate is somewhat higher, as it refers to the peak, in
contrast to the averaged, excitation probability. In any case,
the changeover to a linear power dependence (see Figure 3,
inset) at such low excitation probabilities is highly surprising.
Likely, the early changeover from a quadratic into a linear
regime has the same origin as the low maximal excitation
probability of CSS2 (15% relative to CSS1) observed even for
In summary, we have achieved long-lived (t = 870 ns)
electron accumulation in a purely molecular system without
sacrificial reagents, using visible light as the only energy input.
This observation is of key importance in the context of solar-
energy conversion, because the generation of so-called solar
fuels (e.g., H2, HCOOH, or CH3OH) from small inert
molecules, such as H2O and CO2, invariably relies on multi-
electron redox reactions. Consequently, it is important to
elucidate the basic principles of photodriven accumulation
and temporary storage of redox equivalents without relying
on sacrificial reagents. Our study reports on an important
proof-of-concept in this regard.
Acknowledgements
This research was funded by the Swiss National Science
Foundation through grant number 200021-146231/1 to O.S.W.
and through grant number CRSII2_160801/1 to P.H., as well
as by the URRP LightChEC of the University of Zꢀrich to
P.H.
Keywords: donor–acceptor systems · electron transfer ·
energy conversion · photochemistry ·
time-resolved spectroscopy
Angew. Chem. Int. Ed. 2016, 55, 1 – 5
ꢀ 2016 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim
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