Communication
(CO)3Cl] in wet acetonitrile;[19] H2 was formed directly at the
surface of the semiconducting Si even when no Re complex
was present. Maeda and co-workers reported a porous semi-
conducting C3N4 and a Ru complex that combined to photoca-
talyze the reduction of CO2 to H2, CO, and HCO2H in CH3CN/
N((CH2)2OH)3.[20] In the case of 1-Re, ligand 1 was a likely
source of mobile electrons that did not reside (at least in part)
on Re, as the ligand alone absorbed UV and visible light (see
the Supporting Information, Figure S5). Luminescence from
1 was most intense upon irradiation at 270 nm (see the Sup-
porting Information, Figure S6); however, 1 was somewhat lu-
minescent when irradiated with near-UV light. Thus, when sus-
pensions of 1 in CO2- and Ar-saturated CH3CN/NEt3 were irradi-
ated (lꢀ300 nm), H2 (but not CO) was generated (see the Sup-
porting Information, Figure S10). Thus, although adventitious
H2O is the likely source of H2, it could apparently not react di-
rectly with photoexcited 1-Re, as no H2 was formed when 1-Re
was irradiated in CO2-saturated CH3CN without NEt3 (see the
Supporting Information, Figure S9). Similarly, the reported
C3N4–Ru system did not produce H2 in the absence of an
amine.[20]
Figure 3. Effect of adding 2 during the photocatalytic reduction of CO2 over
1-Re in NEt3/CH3CN.
was due to soluble [(a-diimine)Re(CO)3Cl] analogues. Consis-
tent with this, the induction period was observed even for the
formation of H2 upon irradiation of Re-free 1 in CO2-saturated
NEt3/CH3CN.
Overall, 1-Re was a photocatalyst for the generation of
syngas (H2/CO=1.4–2.2) under the reaction conditions. Both
H2 and CO were generated slowly at first, with the rates of
their generation increasing over time. Whereas the rate of CO
formation over 1-Re was highly stable after 100 min [d(CO)/
To test our hypothesis that the porous structure of 1-Re con-
ferred stability by preventing interactions between Re centers,
we performed an additional test (Figure 3). The photocatalytic
reduction of CO2 over 1-Re was repeated as before for around
2 h. Then, 20 mg of 2 was added. Initially, both CO and H2 pro-
duction spiked, but both declined quickly. Importantly, the rate
of CO production fell below the level seen before 2 was
added. In fact, after a total of 325 min (206 min after 2 was
added), CO production ceased completely. Thus the introduc-
tion of a soluble [(a-diimine)Re(CO)3Cl] catalyst for the photo-
catalytic reduction of CO2 actually inactivated the immobilized
catalyst 1-Re. H2 formation, in contrast, stabilized again at
a rate similar to that observed before 2 was added, demon-
strating that both the photoexcitation of the unmetalated con-
jugated polymer 1 and electron abstraction from the sacrificial
donor NEt3 continued unabated. Only the Re catalyst, which
coordinates and reduces the CO2 molecule, was inactivated,
suggesting that the deactivation usually observed in [(a-diimi-
ne)Re(CO)3Cl]-type catalysts is frustrated in 1-Re until a soluble
small-molecule analogue is added. This is, to our knowledge,
the most unambiguous demonstration to date that [(a-diimi-
ne)Re(CO)3Cl] catalysts for photocatalytic CO2 reduction de-
compose via a bimetallic pathway. Thus, although 1-Re shows
lower initial activity for the photocatalytic reduction of CO2 in
the presence of a sacrificial donor than the soluble catalyst 2
does, the isolation of the Re active sites within the POP yielded
a more stable catalyst. Furthermore, POP 1 itself was a photoca-
talyst for H2 generation (presumably from H2O reduction), so
1-Re catalyzed the photocatalytic generation of H2 and CO. Ad-
ditional experiments will be required in order to understand
(and potentially control) the relative rates of H2 and CO forma-
tion.
À1
dt=4.6Æ0.5 mmolminÀ1 mmolRe over t=110–1200 min], that
of H2 actually increased slightly, causing the ratio of H2 to CO
in the gas phase to increase over time (Figure 2, inset). Al-
though the source of the observed induction period for photo-
catalyst 1-Re is still being investigated, the similar profiles of
H2 and CO formation suggest that a single phenomenon ac-
counts for both. Especially interesting, however, was the very
stable rate of CO generation by 1-Re. This was in contrast to
the case of 2, over which the rate of CO production quickly
reached a peak before declining significantly. After 2 h, cata-
lysts 1-Re and 2 were producing CO at similar rates, but CO
generation over catalyst 2 had nearly ceased after 4 h. Thus it
was clear that 1-Re was a more stable photocatalyst for CO2 re-
duction than 2. Over 20 h, catalyst 1-Re yielded 5.0 mol CO
and 8.9 mol H2 per mol Re (i.e. TONCO =5, TONH2 =8.8; Fig-
ure S13). Therefore, the slower but more stable 1-Re produced
more CO than 2 had before losing activity (TONCO over 2 was
3.5).
The reaction mixture from CO2 reduction over 1-Re was
sampled after 60 and 120 min and the aliquots were analyzed
by inductively coupled plasma (ICP) and optical emission spec-
troscopy detection. Each contained around 7 ppm Re, which
represents roughly a third of the Re originally present in 1-Re.
However, this Re was not photocatalytically active; when the
catalyst was used for 120 min, then filtered from solution, the
filtrate was not an active photocatalyst for CO2 reduction, al-
though it produced a small amount of H2 upon irradiation (see
the Supporting Information, Figure S14). Therefore, CO produc-
tion over 1-Re was stable despite the loss of some Re to solu-
tion. Moreover, the slow build-up of catalyst activity in 1-Re
could not be explained by assuming that all catalytic activity
Chem. Eur. J. 2015, 21, 18576 – 18579
18578
ꢀ 2015 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim