Peter A Summers1,2, James A Calladine1, Fabio Ghiotto1, Joe Dawson1, Xue-Z Sun1, Michelle L Hamilton1,3, Michael Towrie4, E Stephen Davies1, Jonathan McMaster1, Michael W George1,2, Martin Schröder1,5. 1. School of Chemistry, The University of Nottingham , University Park, Nottingham NG7 2RD, United Kingdom. 2. Department of Chemical and Environmental Engineering, The University of Nottingham Ningbo China , Ningbo 315100, China. 3. Dynamic Structural Science Consortium, Research Complex at Harwell , Didcot, Oxfordshire OX11 0FA, United Kingdom. 4. Central Laser Facility, Research Complex at Harwell, Science and Technology Facilities Council, Rutherford Appleton Laboratory , Harwell Oxford, Didcot, Oxfordshire OX11 0QX, United Kingdom. 5. School of Chemistry, University of Manchester , Manchester M13 9PL, United Kingdom.
Abstract
The synthesis, photophysics, and photochemistry of a linked dyad ([Re]-[NiFe2]) containing an analogue ([NiFe2]) of the active site of [NiFe] hydrogenase, covalently bound to a Re-diimine photosensitizer ([Re]), are described. Following excitation, the mechanisms of electron transfer involving the [Re] and [NiFe2] centers and the resulting decomposition were investigated. Excitation of the [Re] center results in the population of a diimine-based metal-to-ligand charge transfer excited state. Reductive quenching by NEt3 produces the radically reduced form of [Re], [Re](-) (kq = 1.4 ± 0.1 × 10(7) M(-1) s(-1)). Once formed, [Re](-) reduces the [NiFe2] center to [NiFe2](-), and this reduction was followed using time-resolved infrared spectroscopy. The concentration dependence of the electron transfer rate constants suggests that both inter- and intramolecular electron transfer pathways are involved, and the rate constants for these processes have been estimated (kinter = 5.9 ± 0.7 × 10(8) M(-1) s(-1), kintra = 1.5 ± 0.1 × 10(5) s(-1)). For the analogous bimolecular system, only intermolecular electron transfer could be observed (kinter = 3.8 ± 0.5 × 10(9) M(-1) s(-1)). Fourier transform infrared spectroscopic studies confirms that decomposition of the dyad occurs upon prolonged photolysis, and this appears to be a major factor for the low activity of the system toward H2 production in acidic conditions.
The synthesis, photophysics, and photochemistry of a linked dyad ([Re]-[NiFe2]) containing an analogue ([NiFe2]) of the active site of [NiFe] hydrogenase, covalently bound to a Re-diimine photosensitizer ([Re]), are described. Following excitation, the mechanisms of electron transfer involving the [Re] and [NiFe2] centers and the resulting decomposition were investigated. Excitation of the [Re] center results in the population of a diimine-based metal-to-ligand charge transfer excited state. Reductive quenching by NEt3 produces the radically reduced form of [Re], [Re](-) (kq = 1.4 ± 0.1 × 10(7) M(-1) s(-1)). Once formed, [Re](-) reduces the [NiFe2] center to [NiFe2](-), and this reduction was followed using time-resolved infrared spectroscopy. The concentration dependence of the electron transfer rate constants suggests that both inter- and intramolecular electron transfer pathways are involved, and the rate constants for these processes have been estimated (kinter = 5.9 ± 0.7 × 10(8) M(-1) s(-1), kintra = 1.5 ± 0.1 × 10(5) s(-1)). For the analogous bimolecular system, only intermolecular electron transfer could be observed (kinter = 3.8 ± 0.5 × 10(9) M(-1) s(-1)). Fourier transform infrared spectroscopic studies confirms that decomposition of the dyad occurs upon prolonged photolysis, and this appears to be a major factor for the low activity of the system toward H2 production in acidicconditions.
There is increasing
research interest in the area of solar fuels driven by growing global
issues centered around the supply and demand of depleting energy resources.[1] Solar fuels provide the potential to convert
solar energy into stored energy with applications in transportable
fuels and chemical feedstocks. Thereare several strategies to achieve
this including the photocatalytic splitting of water for the production
of dihydrogen (H2)[2] and the
reduction of carbon dioxide (CO2).[3] Traditionally, photochemical H2 production has been achieved
through the use of a photosensitizer (PS) and a sacrificial electron
donorcoupled with a catalyst able to reduce protons to H2 (Scheme ). In this
scheme the absorption of light by PS generates an excited state (PS*),
which can be reduced by a suitable electron donor (ED) to form the
reduced photosensitizer, PS–. Electron transfer
to the catalyst then generates the intermediates required for the
catalyticreduction of protons. Of particular note in this area was
the recent work from Eisenberg and co-workers, who used a heterogeneous
CdSe nanocrystal PS to deliver electrons to a nickel-based homogeneous
catalyst in water, resulting in continuous H2 production
with little drop in activity over 360 h of photocatalysis.[4] In addition to the bimolecular systems described
in Scheme , photosensitizing
units have been successfully linked to catalysts and electron acceptors
in an effort to facilitate and direct electron transfer and control
charge recombination.[2b,5] Research into the utilization
of homogeneous photocatalytic systems continues to be investigated
widely, and a range of biomimeticcatalysts, inspired by the active
sites of the hydrogenases, have been studied.[2b,6] These
enzymes are naturally occurring catalysts for the interconversion
of protons and H2, with high turnover efficiency at nearly
neutral pH in aqueous environments.[7] Synthetic
efforts have focused on the active sites of the [FeFe] hydrogenase
with complexes such as [Fe2(CO)4X(L1)(L2)] (where X is a dithiolate bridge, and L1 and L2 are either carbonyl or phosphine derived ligands)
acting as the catalyticcenter, with Ru-, Ir-, or Re-derived photosensitizers.[8] The ground state and excited-state properties
of [FeFe] hydrogenase model compounds have been studied in detail
using a range of IR spectroscopies at a variety of excitation wavelengths.
Following excitation, CO loss with geminate or diffusion recombination,
as well as photoproducts assigned to the breaking and recombination
of the Fe–Fe bond, have been observed.[9] Photosensitizing units have been attached directly to the [FeFe]
units, either covalently through a dithiolate bridge integral to the
[FeFe] complex or through ligand substitution reactions at the [FeFe]
center.[10]
Scheme 1
Simplified Schematic
of the One-Electron Reduction of a Catalyst ([Cat]) by a Photosensitiser
([PS]) Proceeding via the Reductive Quenching of [PS]* by an Electron
Donor (ED)
Steady-state and time-resolved
spectroscopic studies have probed the photocatalytic mechanisms in
linked and bimolecular systems, focusing on electron transfer to the
catalyst.[10g,10j,11] Transient absorption (TA) spectroscopy has monitored electron transfer
in bimolecular systems from photogenerated [Ru(bpy)3]+ to [Fe2(CO)4X(L1)(L1)] in CH3CN (X = (μ-SCH2)2CH2, L1 = L2 = CO; X = (μ-SCH2)2NCH2C6H5, L1 = L2 = CO or L1 = L2 = P(Pyr)3 or L1 = CO L2 = P(Pyr)3; X = μ-Cl2bdt2–, L1 = L2 = CO; Pyr = N-pyrrolyl; bdt2– = 3,6-dichlorobenzene-1,2-dithiolate).[8a,10g,11a] Time-resolved measurements have
also been used to study electron transfer in linked systems. TA spectroscopy
was used to observe electron transfer in a self-assembled system consisting
of an [FeFe] hydrogenase mimic functionalized with a pendant pyridine
group, linked to a zinc porphyrin photosensitizer.[10g] Similarly, TA spectroscopy has been used to study a zincporphyrincovalently linked to an [FeFe] hydrogenase model complex,
where rapid electron transfer from the zinc porphyrin to the catalyst
was monitored (τ = 24 ± 1 ps) followed by charge recombination
(τ = 57 ± 1 ps) in CH2Cl2.[10j] Time-resolved infrared (TRIR) spectroscopy
was used to examine electron transfer in the analogous self-assembled
system. Again, electron transfer from the photoexcited porphyrin to
the catalyst was observed (τ = 40 ± 3 ps) with charge recombination
(τ = 205 ± 14 ps) significantly slower than in the covalently
linked system (τ = 57 ± 1 ps).[11b] However, turnover numbers (TON) in linked systems are generally
lower or comparable to the analogous bimolecular, or separated, systems.[2b] For example, in a linked dyad containing an
iridium-based cyclometalated photosensitizer covalently linked to
an [FeFe] hydrogenase mimic, a maximum TON of 127 was reported, which
is similar to the analogous separated system (TON = 138).[10m]We recently reported a detailed mechanistic
study into photocatalyticH2 production from an bimolecular
system using the photosensitizer [ReCl(CO)3(bpy)] and the
catalyst [NiFe2] (Figure ), an analogue of the active site of the [NiFe] hydrogenase,[12] which catalyzes H2 production. In
this paper we report the synthesis of a linked dyad containing a Rediimine based photosensitizer covalently linked to [NiFe2], [Re]-[NiFe2] (Figure ). We investigate the photophysical properties of [Re]-[NiFe2] and monitor excited state formation, electron transfer processes
and H2 production. We compare the results for [Re]-[NiFe2] with an analogous bimolecular system, [Re]/[NiFe2] (a mixture of [ReCl(CO)3(CH3-bpy-COOCH3)] and [NiFe2], Figure ) to evaluate the effects of covalently linking
the [Re] and [NiFe2] units together and to provide valuable
insight for the development of similarcatalytic systems.
Figure 1
Structures
of [NiFe2], [NiFe2]–OH, [ReCl(CO)3(CH3-bpy-COOR)] (R = H or CH3), and
[Re]-[NiFe2].
Structures
of [NiFe2], [NiFe2]–OH, [ReCl(CO)3(CH3-bpy-COOR)] (R = H or CH3), and
[Re]-[NiFe2].
Experimental Section
General Procedures
Reagents were used as received from the suppliers (Sigma-Aldrich,
Acros Organic, and Fluka), and all the reactions, manipulations, and
transfers were performed under Ar using standard Schlenk techniques,
unless stated otherwise. For TRIR, luminescence, and H2 production experiments, acetonitrile (99.9%, Merck) and NEt3 (>99.5%, Sigma-Aldrich) were distilled under an inert
atmosphere of Ar from CaH2. For electrochemical measurements,
CH2Cl2 was dried, degassed, and stored under
Ar. Trifluoroacetic acid (TFA) and CDCl3 were degassed
with Ar, stored over 4 Å molecular sieves, and used without further
purification. N(CH2CH2OH)3 (TEOA;
98%, Alfa Aesar) was dried under reduced pressure (160 °C, 1
× 10–1 mbar) for 24 h before being stored under
Ar. High-purity Ar was obtained from BOC. [ReCl(CO)3(bpy)],[13] [NiFe2] (Figure ),[14] [ReCl(CO)3(CH3-bpy-COOH)][15] (CH3-bpy-COOH = 4′-methyl-2,2′-bipyridine-4-carboxylic
acid) and [ReCl(CO)3(CH3-bpy-COOCH3)][16] (Figure , CH3-bpy-COOCH3 =
4′-methyl-2,2′-bipyridine-4-carboxylate) were prepared
according to adapted literature methods. Elemental analyses were performed
by the London Metropolitan University (Carlo Erba CE1108 Elemental
Analyzer). NMR spectra wererecorded on a Brüker DPX 300 spectrometer
running at 300.13 MHz for 1H and at 75.42 MHz for 13C experiments. Electrospray (ES) mass spectrometric data
wererecorded by the Mass Spectrometry Service at the University of
Nottingham using a Brüker Daltonics microTOF Electrospray Mass
Spectrometer. X-band electron paramagneticresonance (EPR) spectra
wererecorded on a Brüker EMX spectrometer. Simulations of
EPR spectra were performed using the Brüker WINEPR SimFonia
package.[17] FTIR spectra wererecorded in
solution cells (Harrick Scientific Products, Inc.) with CaF2 windows using a Nicolet 6700 FTIR spectrometer, typically at 2 cm–1 resolution. Path lengths of 0.25, 0.39, 0.5, or 1
mm were used, and all solutions were prepared under an inert atmosphere
of Ar and degassed by three freeze–pump–thaw cycles.
[Ni]–OH
NaOMe (0.359 g, 6.64 mmol) was added to a solution of toluene-3,4-dithiol
(TDT; 0.520 g, 3.32 mmol) in anhydrous MeOH (30 cm3) under
Ar. The pink solution was stirred for 1 h before dropwise addition
of a concentrated solution of [Ni(OAc)2.4(H2O)] (0.414 g, 1.66 mmol) in MeOH (10 cm3). The dark brown
solution was stirred for 1 h, after which time a concentrated solution
of 1,3-dibromopropan-2-ol (0.542 g, 2.49 mmol) in MeOH (10 cm3) was added. The reaction mixture was stirred for 24 h at
room temperature, after which time a light green precipitate formed.
The powder was collected by filtration and washed with cold anhydrous
MeOH (2 × 5 cm3) and anhydrous isohexane (3 ×
5 cm3) and dried in vacuo. Chromatography of the crude
material on silica gel (Fluka, F60) using CH2Cl2 as eluent yielded one mobile colored fraction, which was isolated.
Evaporation of this solution to dryness yielded a light green powder,
[Ni]–OH. Yield 0.485 g, 69%. Elemental Analysis: Found (Calculated
for C17H18O1S4 Ni1) C, 48.53 (48.01); H, 4.63 (4.27)%. MS (ES+) m/z: 425 (M + H)+, 447 (M +
Na)+. 1HNMR (300 MHz, deuterated dimethyl sulfoxide
(DMSO-d6), 298 K): δH 7.38–6.82 (6H, m, Ph-H), 4.81 (1H,
s, OH), 3.94–3.92 (1H, m, CH), 3.83–3.50 (4H, m, SCH2), 2.23 (6H, s, Ph–CH3) ppm. 13CNMR (75 MHz, DMSO-d6, 298 K): δC 132.68–124.50 (m,
Ph-C), 64.12 (s, C-O),
37.27 (s, SC), 20.92–20.36 (m, Ph-CH3) ppm. IR (solid): 3260 (s), 2919 (s),
2863 (s), 2153 (w), 2011 (w), 1715 (s), 1606 (s), 1579 (s), 1512 (m),
1460 (vs), 1377 (s), 1326 (m), 1280 (s), 1253 (vs), 1196 (m), 1169
(s), 1111 (vs), 1044 (vs), 866 (s), 802 (vs), 772 (m), 689 (m), 638
(m), 577 (w), 563 (w), 535 (s), 521 (vs) cm–1.
[NiFe2]–OH
A mixture of [Ni]–OH
(0.301 g, 0.73 mmol) and Fe3(CO)12 (0.339 g,
0.67 mmol) in anhydrous CH2Cl2 (40 cm3) was heated to reflux for 16 h under Ar. The reaction mixture was
subsequently cooled to room temperature, and the dark brown/red solution
was filtered to remove a dark brown precipitate. The precipitate was
washed with CH2Cl2 (3 × 5 cm3), and the washings werecombined with the filtrate. Concentration
of the filtrate under reduced pressure afforded a dark brown solid,
which was washed with anhydrous isohexane (3 × 5 cm3) and dried in vacuo. Chromatography of the crude material on silica
gel (Fluka, F60) using ethyl acetate and petroleum ether (bp 60–80
°C; 3/2, v/v) as eluent yielded two fractions. A fast-moving
weak orange band was identified as [Fe2(CO)6TDT], an analogue of [Fe2(CO)6BDT] (BDT2– = benzene-1,2-dithiolate) previously reported by
Perra et al.[18] The second slow-moving brown
band was isolated, and removal of the solvent under reduced pressure
afforded a black powder, the target complex [NiFe2]–OH.
Yield 0.293 g, 62%. Elemental Analysis: Found (Calculated for C23H18O7S4Ni1Fe2) C, 39.98 (39.12); H, 3.12 (2.57)%. MS (ES+) m/z: 727 (M + Na)+. 1HNMR (400 MHz, CDCl3, 298 K): δH 8.17–7.20
(6H, m, Ph-H), 3.89–3.84 (1H, m, CH), 3.74 (1H, m, SCH2), 3.38–3.31 (1H, m, SCH2), 2.99–2.79 (2H, m, SCH2), 2.58–2.49 (6H, s, Ph–CH3), 2.01 (1H, s, OH) ppm. 13CNMR (100 MHz, CDCl3, 298 K): δC 211.92
(s, C≡O), 139.73–128.85 (m, Ph-C), 66.14 (s, C-O), 44.18–42.99
(m, SC), 21.06–20.86 (m, Ph-CH3) ppm. Solution IR (CH2Cl2): νC≡O 2037 (s), 1997 (s) and 1958 (s) cm–1.
[Re]-[NiFe2]
4-Dimethylaminopyridine
(DMAP, 10 mg, 0.08 mmol) and N,N′-dicyclohexylcarbodiimide (DCC, 62 mg, 0.3 mmol) were added
to a solution of [NiFe2]–OH (67 mg, 0.1 mmol) and
ReCl(CO)3(CH3-bpy-COOH) (115 mg, 0.22 mmol)
in CH2Cl2 (40 mL) at 0 °C, and the reaction
was stirred for 48 h at room temperature. The resulting suspension
was filtered, and the filtrate was evaporated to dryness to yield
the crude product, [Re]-[NiFe2], which was purified by
column chromatography on silica gel (Fluka, F60) using ethyl acetate
and petroleum ether (bp 60–80 °C; 2/1, v/v) as eluent.
The intensely colored slow-moving red/brown band was isolated, and
removal of the solvent under reduced pressure afforded the target
complex [Re]-[NiFe2]. Yield 55 mg, 48%. Elemental Analysis:
Found (Calculated for C38H26ClFe2N2NiO11ReS4) C, 37.78 (37.82);
H, 2.19 (2.17); N, 2.36 (2.32)%. MS (ES–) m/z: 1250.7685 [M + HCOO]−, 1240.7342 [M + Cl]−. The adduct [M + COOH]− shows an isotope pattern in good agreement with the
theoretical value (Figure S1). 1HNMR (300 MHz, CDCl3, 298 K) δ: 2.39 (m, 9H, CH3), 3.04 (m, 2H, SCH2CHLCH2S), 3.72 (m,
2H, SCH2CHLCH2S), 4.11 (m, 1H, SCH2CHLCH2S), 6.71–9.38 (m, 12H, Ph-H and Py-H) ppm. 13CNMR (75 MHz,
CDCl3, 298 K) δ: 21.83 (m, CH3), 33.96 (s, SCH2CHLCH2S), 49.19 (s, SCH2CHLCH2S), 118.78–156.05 (m, Ph-C and Py-C), 212.21 (s, CO) ppm. Solution IR: (CH2Cl2)
ν(C≡O) 2037 (s), 2023 (s), 1997 (s), 1957 (s), 1920 (s)
and 1900 (s) cm–1, ν(C=O) 1737 (w)
cm–1; (CH3CN) ν(C≡O) 2036
(s), 2023 (s), 1996 (s), 1957 (s), 1919 (s), 1901 (s) cm–1, ν(C=O) 1742 (w) cm–1.
Time-Resolved
Infrared Spectroscopy
Picosecond and nanosecond TRIR spectra
were obtained using purpose-built equipment based on a pump–probe
approach at both Nottingham and the Rutherford Appleton Laboratory.
Details of the equipment and methods used for the TRIR studies have
been described previously.[19] The results
wererepeated on both instruments, but the data shown in this paper
were obtained using the latter, which used a seeded dual titanium
sapphirechirped pulse amplifier to generate 10 kHz, 40–80
fs, 0.8 mJ pulses at 800 nm. The beam was focused and split into 0.4
mJ beams, which were used to pump a number of different computer-controlled
optical paramagnetic amplifiers (OPAs). These were able to output
a range of synchronized wavelength combinations for use as either
pump or probe beams with a 240 to 15 000 nm spectral coverage.
A high-precision translation stage (Newport IMS600LM) provided a delay
line for the pump beam and generates femtosecond to nanosecond pump–probe
timing. Once through the sample the IR beam was collimated and focused
onto a spectrograph where a 128 mercury cadmium telluride array detector
was used to detect the mid-IR probe. Access to the nanosecond-to-microsecond
time delays was provided by a nanosecond laser system, delivering
1064 nm pulses (10 kHz, 1 ns, 0.05 mJ). Pump energies of 1 μJ
were typically used in experiments reported in this paper. The 355
nm harmonic was used, delivering >5 μJ energy per pulse,
synchronized to the probe beam of the laser system described above.
Samples wererecirculated using a peristaltic pump as the sample was
rastered in the x and y planes to
minimize cumulative photodamage to both the sample and window during
repeated photolysis. To analyze the reaction kinetics of transient
species, the spectra were fitted using the minimum number of Lorentzian
bands. In experiments containing [Re]/[NiFe2], the intermediate
growth and decay of the bands associated with [ReCl(CO)3(CH3-bpy-COOCH3)]− overlap
with either the parent bleaches of [NiFe2] or the transient
peaks of [NiFe2]−. As a result, the kinetics
of [ReCl(CO)3(CH3-bpy-COOCH3)]− was measured from the regrowth of the parent
bands of [ReCl(CO)3(CH3-bpy-COOCH3)], as multiple band fitting resulted in more tractable data
analysis. For the same reason, the lifetime of [Re]−-[NiFe2] was measured from the regrowth of the parent
bands of the [Re] moiety in [Re]-[NiFe2].
Luminescence
Spectroscopy
An Edinburgh Instruments FLS920 combined fluorescence
lifetime and steady-state spectrometer was used for all emission measurements.
Samples were held in a l × 1 cm quartz fluorescence cuvette and
either degassed using three freeze–pump–thaw cycles
on a Schlenk line or prepared in a glovebox. Excited-state lifetime
measurements were performed using the time-correlated photon counting
method, with a pulsed diode laser (EPL-405, Edinburgh Instruments)
as an excitation source.
Electrochemical Measurements
Electrochemical
measurements were made using an Autolab PGSTAT20 potentiostat. All
solutions were purged with a stream of Ar prior to use. Cyclic voltammograms
were performed using a three-electrode system, with a glassy carbon
working electrode (6.7 mm diameter), a Pt wire secondary electrode,
and a saturated calomel reference electrode. Before each measurement,
the glassy carbon working electrode was cleaned using a polishing
pad. All potentials are referenced to the Fc+/Fc (Fc =
ferrocene) couple, used as an internal standard. Cyclic voltammograms
of [Re]-[NiFe2] and [NiFe2] (ca. 1 mM) in CH2Cl2 wererecorded with [NBu]4[BF4] (0.4 M) as a supporting electrolyte. Coulometric measurements
were performed using an H-cell at 273 K in CH2Cl2containing [NBu4][BF4] (0.4 M); the cell consisted
of a Pt/Rh gauze basket working electrode separated by a glass frit
from a Pt/Rh gauze secondary electrode. The saturated calomel reference
electrode was placed in a bridge tube containing electrolyte solution,
the tip was positioned at the center of the working electrode, and
the solution was stirred rapidly during electrolysis using a magnetic
stirring bar. Catalyticcyclic voltammetry experiments wereconducted
using a sealed single-compartment electrochemical cell purged with
Ar. Additions of TFA (0.1 mL, 0.5 M in CH2Cl2) to a solution of [Re]-[NiFe2] or [NiFe2]
(5 mL, 1 mM in CH2Cl2) with [NBu4][BF4] (0.4 M) were made using a gastight syringe (Hamilton
TLL, Series 1700, model 1702 and 1705). UV–vis spectro-electrochemical
experiments were performed either at 273 or 243 K with an optically
transparent electrode inserted into a modified quartz cuvette with
a path length of 0.5 mm. A three-electrode configuration consisting
of a Pt/Rh gauze working electrode, a Pt wire secondary electrode
(in a fritted poly(tetrafluoroethylene) sleeve), and a saturated calomel
electrode (chemically isolated from the test solution via a bridge
tube containing electrolyte solution and terminated in a porous frit)
was used in the cell. The potential at the working electrode was controlled
by a Sycopel Scientific Ltd. DD10 M potentiostat. The UV–vis
spectra wererecorded on a PerkinElmer Lambda 16 spectrophotometer
at 1 nm resolution. The spectrometer cavity was purged with N2, and temperaturecontrol at the sample was achieved by flowing
cooled N2 across the surface of the cell. FTIR and EPR
spectroscopic measurements were run on aliquots of solutions following
electrochemical bulk reduction.
H2 Production
H2 production experiments wereconducted on purpose-built
apparatus, the details of which have been reported previously.[12a] Irradiation was performed using a Xe arc lamp
(Oriel Instruments, λ < 420 nm cutoff filter) operating at
250 W and H2 was detected on a gas chromatograph (Shimadzu
2014) using a thermal conductivity detector operating at 50 °C.
Results and Discussion
Electrochemical Studies
Cyclic Voltammetry
The cyclic voltammograms of [Re]-[NiFe2] (1 mM) in CH2Cl2 (Figure ) show two reduction processes at E1/2 = −1.23 V and E1/2 = −1.55
V versus Fc+/Fc. The process at E1/2 = −1.23 V versus Fc+/Fc is an electrochemically
reversible one-electron process and may be assigned to the reduction
of the [NiFe2] unit in [Re]-[NiFe2] by comparison
with the reduction process of [NiFe2] (E1/2 = −1.31 V vs Fc+/Fc).[14] The second process at E1/2 = −1.55 V versus Fc+/Fc occurs at a comparable
potential to [ReCl(CO)3(bpy)] and similar functionalized
bipyridinecompounds, and it is assigned to the reduction of the diimine
ligand within the [Re] unit.[15,20] Coulometric studies
show that this reduction process exhibits multielectron behavior,
which may result from the instability of the diimine radical under
the conditions of the experiment.[21] The
cyclic voltammogram of [Re]-[NiFe2] at 100 mV s–1 shows additional reduction processes at potentials more negative
than −1.9 V versus Fc+/Fc (Figure S2). These reductions and their associated oxidation waves
were not studied further. The reduction processes of [Re]-[NiFe2] at E1/2 = −1.23 V and E1/2 = −1.55 V versus Fc+/Fc
were investigated further with UV–vis, FTIR, and EPR spectroscopic
methods.
Figure 2
Cyclic voltammogram of [Re]-[NiFe2] (1 mM) in CH2Cl2 containing [NBu4][BF4] (0.4
M) as a supporting electrolyte showing the two reduction processes
at E1/2 = −1.23 V and E1/2 = −1.55 V vs Fc+/Fc.
Cyclic voltammogram of [Re]-[NiFe2] (1 mM) in CH2Cl2containing [NBu4][BF4] (0.4
M) as a supporting electrolyte showing the two reduction processes
at E1/2 = −1.23 V and E1/2 = −1.55 V vs Fc+/Fc.
UV–vis Spectroelectrochemical Studies
The one-electron reduction process at E1/2 = −1.23 V versus Fc+/Fc of [Re]-[NiFe2] (1 mM) in CH2Cl2 was monitored by UV–vis
spectroelectrochemistry at 243 K. During the reduction the intensity
of the peaks at 372, 485, and 700 nm decrease with the simultaneous
growth of new absorbances at 364, 420, 497, and 620 nm (Figure a and Table S1). These new bands are assigned to the reduction of the [NiFe2] center to form [Re]-[NiFe2]− through comparison with previously reported spectroelectrochemical
studies on [NiFe2].[14] The presence
of isosbestic points (Figure a and Table S1) are diagnostic
of a conversion between [Re]-[NiFe2] and [Re]-[NiFe2]− occurring with no long-lived intermediates
on the time scale of the experiment. Reoxidation of [Re]-[NiFe2]− resulted in the quantitative regeneration
of the UV–vis spectrum of [Re]-[NiFe2], and thus,
the reduction process is chemically reversible on the time scale of
the experiment. The second reduction process at E1/2 = −1.55 V versus Fc+/Fc (Figure ) was investigated
by in situ bulk reduction of [Re]-[NiFe2] at −1.65
V versus Fc+/Fc (243 K, Figure b). This reduction process is associated
with the development of bands at 374, 488, 520, and 699 nm (Figure b, Table S1), and these bands are assigned to reduction processes
that are localized on both the bipyridine ligand of the [Re] unit
and the [NiFe2] moiety to generate [Re]−-[NiFe2]−. Electrochemical oxidation
of this solution generated an almost identical profile to [Re]-[NiFe2] but with a decreased spectral intensity at ca. 370 nm. This
difference is most likely due to the instability of the reduced bipyridine
radical about the [Re] center observed previously in the coulometric
experiments (see above).
Figure 3
UV–vis spectra observed during the electrochemical
reduction of [Re]-[NiFe2] (1 mM) in CH2Cl2 (containing 0.4 M [NBu4][BF4] as a
supporting electrolyte) at 243 K. (a) Reduction of [Re]-[NiFe2] (black) to [Re]-[NiFe2]− (red).
(b) Reduction of [Re]-[NiFe2] (black) to [Re]−-[NiFe2]− (blue).
UV–vis spectra observed during the electrochemical
reduction of [Re]-[NiFe2] (1 mM) in CH2Cl2 (containing 0.4 M [NBu4][BF4] as a
supporting electrolyte) at 243 K. (a) Reduction of [Re]-[NiFe2] (black) to [Re]-[NiFe2]− (red).
(b) Reduction of [Re]-[NiFe2] (black) to [Re]−-[NiFe2]− (blue).
FTIR and EPR Spectroscopic Studies
The FTIR spectrum
of [Re]-[NiFe2] (1 mM) in CH2Cl2 shows
six distinct peaks (Figure ) in the metalcarbonyl region, which can be assigned to the
[Re] (2023, 1920, and 1900 cm–1) and [NiFe2] (2037, 1997, and 1957 cm–1) units. One electron
reduction at −1.23 V versus Fc+/Fc is associated
with a decrease in intensity of bands at 2037, 1997, and 1957 cm–1 and the growth of new bands at 1972, 1925, and 1890
cm–1 (Figure , green line), which are associated with a one-electron reduced
[NiFe2] unit. The down shift of ca. 67 cm–1 for the CO bands in [Re]-[NiFe2]− relative
to those in [Re]-[NiFe2] is in good agreement with shifts
reported for other [NiFe2] centers and is indicative of
an increased electron density on the Fecenters.[10a,12] A small reduction in the intensity of a band associated with the
[Re] unit (2025 cm–1) can also be observed in the
spectrum along with the growth of a band at 2020 cm–1. It appears that during bulk electrolysis partial reaction at the
[Re] center occurs. X-band EPR spectra of electrochemically generated
[Re]-[NiFe2]− wererecorded as fluid
(293 K) and frozen (77 K) solutions (Figure ). The simulated Hamiltonian parameters (giso = 2.043; g11 = 2.014; g22 = 2.018; and g33 = 2.098) are in good agreement with the those reported
for [NiFe2]− (giso = 2.042; g11 = 2.099; g22 = 2.015; and g33 = 2.015).[14]
Figure 4
FTIR spectra of [Re]-[NiFe2] before and after bulk reduction to [Re]-[NiFe2]− in CH2Cl2 (containing
0.4 M [NBu4][BF4] as a supporting electrolyte)
at 293 K. (a) FTIR spectrum of [Re]-[NiFe2]. (b) FTIR difference
spectrum recorded following the reduction of [Re]-[NiFe2] to [Re]-[NiFe2]−.
Figure 5
X-band EPR spectra in
CH2Cl2 (black) and the simulated spectra (red)
for [Re]-[NiFe2]− (a) as a fluid solution
at 293 K (simulation parameters: giso =
2.043; Wiso = 20 G) and (b) as a frozen
solution at 77 K (simulation parameters: g11 = 2.014; g22 = 2.018; g33 = 2.098; W11 = 11 G; W22 = 12 G; W33 =
14 G).
FTIR spectra of [Re]-[NiFe2] before and after bulk reduction to [Re]-[NiFe2]− in CH2Cl2 (containing
0.4 M [NBu4][BF4] as a supporting electrolyte)
at 293 K. (a) FTIR spectrum of [Re]-[NiFe2]. (b) FTIR difference
spectrum recorded following the reduction of [Re]-[NiFe2] to [Re]-[NiFe2]−.
Electrocatalytic Studies
The electrocatalytic activity
of the first reduction process of [Re]-[NiFe2] (E1/2 = −1.23 V vs Fc+/Fc) was
investigated using the same procedure that has been employed previously
for [NiFe2] and related compounds.[12b,14] The cyclic voltammogram of [Re]-[NiFe2] shows an increased
cathodic peak current and a reduction in the current of the anodic
wave (Figure S3), as aliquots of TFAare
added to a solution of [Re]-[NiFe2] (1 mM) in CH2Cl2 (containing 0.4 M [NBu4][BF4] as a supporting electrolyte). This reduction in the current of
the anodic wave is consistent with the removal of [Re]-[NiFe2]− from the diffusion layer of the working electrode
by a method other than that of heterogeneous electron transfer to
the electrode and is diagnostic of an electrocatalytic process.[22]The electrochemical and spectrochemical
results are consistent with a first reduction process that is localized
at the [NiFe2] center and a second process that is localized
at the [Re] center in [Re]-[NiFe2]. Thus, the photoreduction
of the [Re] unit could provide a route to the photochemical production
of [Re]-[NiFe2]−, a desired intermediate
required for catalyticH2 formation.X-band EPR spectra in
CH2Cl2 (black) and the simulated spectra (red)
for [Re]-[NiFe2]− (a) as a fluid solution
at 293 K (simulation parameters: giso =
2.043; Wiso = 20 G) and (b) as a frozen
solution at 77 K (simulation parameters: g11 = 2.014; g22 = 2.018; g33 = 2.098; W11 = 11 G; W22 = 12 G; W33 =
14 G).
Luminescence Spectroscopic
Studies
The excited-state properties of the linked dyad [Re]-[NiFe2] and of the analogous uncoupled [Re]/[NiFe2] system
were examined by luminescence spectroscopy. Luminescence spectra of
solutionscontaining [Re]-[NiFe2], [ReCl(CO)3(CH3-bpy-COOCH3)], [NiFe2], and
[Re]/[NiFe2] (each at 17 μM) in CH3CNare shown in Figure (λex = 406 nm).
Figure 6
Luminescence spectra for [Re]/[NiFe2], [ReCl(CO)3(CH3-bpy-COOCH3)], [Re]-[NiFe2], and [NiFe2] (each at 17 μM)
in CH3CN (λex = 406 nm).
Luminescence spectra for [Re]/[NiFe2], [ReCl(CO)3(CH3-bpy-COOCH3)], [Re]-[NiFe2], and [NiFe2] (each at 17 μM)
in CH3CN (λex = 406 nm).The observed emission for each solution (except
[NiFe2]) was normalized to the absorbance at 406 nm in
the UV–vis spectrum. For solutions of [Re]/[NiFe2] and [Re]-[NiFe2] the spectral bands of [NiFe2] were subtracted before normalization. [ReCl(CO)3(CH3-bpy-COOCH3)] exhibits a broad emission (λmax = 678 nm, τ = 25 ± 0.5 ns, Figure , green line), and the addition
of an equimolar amount of [NiFe2] to the solution resulted
in no observable drop in the emission intensity or lifetime of the 3MLCT excited state ([Re]/[NiFe2], Figure , black line). This suggests
that at concentrations of ca. 17 μM, [NiFe2] does
not quench the 3MLCT excited state of [ReCl(CO)3(CH3-bpy-COOCH3)] to a detectable extent. In
contrast, the emission from [Re]-[NiFe2] is ca. 60% lower
in intensity (λmax = 650 nm, τ = 24 ±
0.5 ns, Figure , red
line) when compared to [Re]/[NiFe2]. The drop in emission
intensity could suggest quenching of the [Re]-based excited state
in [Re]-[NiFe2] by the covalently bound [NiFe2] moiety. However, the lifetimes are not significantly different,
and the emission maximum for [Re]-[NiFe2] is at a higher
energy than for [ReCl(CO)3(CH3-bpy-COOCH3)].We estimated the quenching rate constant (kq) for the reductive quenching of the 3MLCT excited states of [Re]-[NiFe2] and [ReCl(CO)3(CH3-bpy-COOCH3)] by NEt3, through construction of Stern–Volmer plots generated from
the 3MLCT lifetime (Figure S4).[23] The second-order quenching rate constants
are kq = 4.3 ± 0.2 × 107 M–1 s–1 (Figure S4, black dots) and kq = 1.4 ± 0.1 × 107 M–1 s–1 (Figure S4, black
squares) for the 3MLCT excited state of [ReCl(CO)3(CH3-bpy-COOCH3)] and [Re]-[NiFe2], respectively.
Time-Resolved Infrared Spectroscopic Studies
We used picosecond- and nanosecond-TRIR spectroscopies to probe
the mechanisms of the decay of the excited states in [Re]-[NiFe2] and [Re]/[NiFe2] in CH3CN, where the
reaction kinetics can be elucidated and used to monitor electron transfer
processes.
Time-Resolved Infrared Studies on [Re]-[NiFe2]
The FTIR spectrum of [Re]-[NiFe2] in CH3CN
possesses six ν(CO) bands associated with the [Re] (2023, 1919,
and 1901 cm–1) and [NiFe2] (2036, 1996,
and 1957 cm–1) units of the molecule (Figure a). The picosecond-TRIR spectrum
of [Re]-[NiFe2] (0.3 mM) obtained 50 ps after flash photolysis
(λ = 400 nm) shows that all parent bands are bleached and that
new bands are observed at 2065, 2009, 1985, and 1945 cm–1 (Figure b). The
transient species in this spectrum can be divided into two components,
those associated with the [Re] and those with the [NiFe2] units. The parent bands associated with the [NiFe2]
center rapidly reform (τ = 70 ps, Figure S5) as the bands at 2009 and 1985 cm–1 decay,
which is similar to processes observed in the control experiment following
the photolysis of [NiFe2], in which a short-lived transient
is formed (τ = 90 ps) with bands shifted to lower wavenumber.[12a] This species is tentatively assigned to the
homolysis of the Fe–Fe bond in [NiFe2], which has
also been observed after photolysis of synthetic analogues of the
active sites of the [FeFe] hydrogenases.[5d,9a] The nanosecond-TRIR spectrum of [Re]-[NiFe2] recorded
2 ns after photolysis (λ = 355 nm) only shows depletion of the
parent bands associated with the [Re] moiety (2023, 1919, and 1901
cm–1) and transient bands at 2065, 1995, and 1960
cm–1 (Figurec, blue line). The species formed is characteristic of the
production of a Re-diimine 3MLCT excited state where the
ν(CO) bands shift up in energy due to the oxidation of the Recenter ([Re]*-[NiFe2]).[24] Such
behavior has been reported for numerous [ReCl(CO)3(diimine)] 3MLCT excited states, and the shift in the ν(CO) bands
to higher wavenumber has been well-documented.[25] Following photolysis, the 3MLCT bands decay
(τ = 20 ± 1 ns, Figure d, blue dots), and the parent bands reform (Figure d, black dots). This
lifetime (τ = 20 ± 1 ns) is of the same magnitude as the 3MLCT emission lifetime at 650 nm (τ = 24 ± 0.5
ns), measured using luminescence spectroscopy (see above) and suggests
that the excited state [Re]*-[NiFe2] is not quenched by
electron transfer to the [NiFe2] unit.
Figure 7
FTIR, ps-TRIR, and ns-TRIR
spectra of [Re]-[NiFe2] in CH3CN. (a) FTIR ground-state
spectrum. (b) ps-TRIR difference spectrum taken 50 ps after flash
photolysis at 400 nm. (c) ns-TRIR difference spectrum taken 2 ns after
flash photolysis at 355 nm. (d) TRIR kinetic traces for the decay
of the [Re]* center (blue dots) and regrowth of the ground-state bands,
[Re] (black dots). The solid blue line is a monoexponential best-fit
of the data.
FTIR, ps-TRIR, and ns-TRIR
spectra of [Re]-[NiFe2] in CH3CN. (a) FTIR ground-state
spectrum. (b) ps-TRIR difference spectrum taken 50 ps after flash
photolysis at 400 nm. (c) ns-TRIR difference spectrum taken 2 ns after
flash photolysis at 355 nm. (d) TRIR kinetic traces for the decay
of the [Re]* center (blue dots) and regrowth of the ground-state bands,
[Re] (black dots). The solid blue line is a monoexponential best-fit
of the data.Figure shows the nanosecond-TRIR spectra obtained
following excitation (λ = 355 nm) of [Re]-[NiFe2]
(0.3 mM) in a solution of CH3CNcontaining NEt3 (2 M). The spectrum obtained 2 ns after photolysis (Figure b) is identical to the spectra
obtained above in the absence of NEt3 (Figurec) and shows the formation
of a 3MLCT excited state at the [Re] center. However, in
this experiment the 3MLCT bands decay (Figure e, blue dots, τ = 12
± 0.5 ns) as 60% of the parent [Re] moiety bands recover (Figure e, black dots) to
form a new species with bands at 2004, 1896, and 1897 cm–1 (Figurec), which
accounts for the remaining 40% of the parent bleach. Through comparison
with similar experiments on Re-diiminecomplexes,[26] this new species can be assigned as [Re]−-[NiFe2] formed through reductive quenching of [Re]*-[NiFe2] by NEt3. On a longer time scale (100–10 000
ns) [Re]−-[NiFe2] decays (τ = 3100
± 100 ns, Figure e, red dots), and the remaining bands associated with the [Re] center
recover. Concomitantly the ν(CO) bands of the [NiFe2] unit are bleached (Figure e, black circles), and bands associated with the formation
of [Re]-[NiFe2]− grow in at 1970, 1926,
and 1889 cm–1 (Figure d). Thus, electron transfer involving [Re]−-[NiFe2] occurs to form [Re]-[NiFe2]− via a reductive quenching pathway from the 3MLCT of the photosensitizing unit. The growth of [Re]-[NiFe2]− (100–10 000 ns) is biexponential
(Figure e, green dots);
a possible consequence of its formation from [Re]−-[NiFe2] and from the decomposition of the oxidized electron
donor (•NEt3+). This process
has been observed previously for similarRe-diiminecomplexes following
reductive quenching by NEt3 or TEOA.[12a,27] We have also observed similar behavior in photolysis experiments
involving [ReCl(CO)3(bpy)] and [NiFe2] in a
solution of CH3CNcontaining NEt3.[12a] In this example decomposition of NEt3resulted in the reduction of [NiFe2] to [NiFe2]−. Once formed, [Re]-[NiFe2]− remains stable on the time scale of this experiment (up to 70 μs).
Figure 8
FTIR and
nanosecond-TRIR spectra of [Re]-[NiFe2] in a solution of
CH3CN containing NEt3 (2 M). (a) FTIR ground
state spectrum. nanosecond-TRIR difference spectra taken (b) 2 ns,
(c) 50 ns, and (d) 50 μs after flash photolysis at 355 nm. (e)
TRIR kinetic traces for the decay of the 3MLCT excited
state, [Re]*-[NiFe2] (blue); the growth and decay of [Re]−-[NiFe2] (red dots), the growth of [Re]-[NiFe2]− (green), the regeneration of the [Re]
center (black ●), and the loss of the [NiFe2] center
(black ○). The solid black line is a monoexponential best fit
of the data.
FTIR and
nanosecond-TRIR spectra of [Re]-[NiFe2] in a solution of
CH3CNcontaining NEt3 (2 M). (a) FTIR ground
state spectrum. nanosecond-TRIR difference spectra taken (b) 2 ns,
(c) 50 ns, and (d) 50 μs after flash photolysis at 355 nm. (e)
TRIR kinetic traces for the decay of the 3MLCT excited
state, [Re]*-[NiFe2] (blue); the growth and decay of [Re]−-[NiFe2] (red dots), the growth of [Re]-[NiFe2]− (green), the regeneration of the [Re]
center (black ●), and the loss of the [NiFe2] center
(black ○). The solid black line is a monoexponential best fit
of the data.
Time-Resolved Infrared
Studies on [Re]/[NiFe2]
A previous picosecond-TRIR
investigation of [NiFe2] in CH3CN has shown
that a short-lived transient (τ = 90 ps) is formed following
photolysis with characteristic bands shifted to lower wavenumber,
namely, [NiFe2]* (see above). The presence of NEt3 did not affect the lifetime or band positions of [NiFe2]*, and no direct interaction between [NiFe2]*, [ReCl(CO)3(bpy)], or the 3MLCT excited state of [ReCl(CO)3(bpy)] was observed on these time scales.[12a] Therefore, to simplify the analysis of the spectra in this
study, solutionscontaining [NiFe2] at time delays of less
than 2 ns after excitation are not reported.Figure S6a shows the ground-state FTIR spectrum of [Re]/[NiFe2] with three bands associated with [ReCl(CO)3(CH3-bpy-COOCH3)] (2023, 1919, and 1901 cm–1) and three with [NiFe2] (2035, 1995, and 1955 cm–1). The nanosecond-TRIR spectrum recorded 2 ns after
the photolysis of a solution of [Re]/[NiFe2] (both at 1
mM) in CH3CN is shown in Figure S6b. Depletion of the parent [ReCl(CO)3(CH3-bpy-COOCH3)] bands are observed with the formation of
a species at 2067, 1997, and 1959 cm–1 characteristic
of the production of a Re-diimine 3MLCT excited state ([ReCl(CO)3(CH3-bpy-COOCH3)]*). [ReCl(CO)3(CH3-bpy-COOCH3)]* decays back
to the ground state (τ = 22 ± 1 ns) as the parent bleaches
for [ReCl(CO)3(CH3-bpy-COOCH3)] recover and the rate of decay is similar to the 3MLCT
emission (τ = 25 ± 0.5 ns) measured above using luminescence
spectroscopy. The CO bands corresponding to [NiFe2]− were not observed, which suggests that electron transfer
from [ReCl(CO)3(CH3-bpy-COOCH3)]*
to [NiFe2] does not occur to an extent that can be monitored
in these experiments.Figure S7 shows
the nanosecond-TRIR spectra recorded following photolysis (λ
= 355 nm) of [ReCl(CO)3(CH3-bpy-COOCH3)] (0.5 mM) in a solution of CH3CNcontaining NEt3 (1 M). Bands characteristic of [ReCl(CO)3(CH3-bpy-COOCH3)]* are observed to form 4 ns after
excitation (Figure S7b). [ReCl(CO)3(CH3-bpy-COOCH3)]* (τ =
10 ± 2 ns) is reductively quenched by NEt3 to form
[ReCl(CO)3(CH3-bpy-COOCH3)]− (43%) with bands at 2000, 1891, and 1894 cm–1, while the remaining 57% decays back to the ground state. The rise
in [ReCl(CO)3(CH3-bpy-COOCH3)]− is observed as two processes over two different
time scales (Figure S7d, red dots). The
first phase (0–70 ns), which occurs on a similar time scale
to the decay of the 3MLCT excited stated, is associated
with the reductive quenching process described above involving [ReCl(CO)3(CH3-bpy-COOCH3)] and NEt3. The second phase (70–1000 ns) can be explained by considering
the decomposition of the oxidized electron donor •NEt3+, which
may result in the reduction of a second equivalent of [ReCl(CO)3(CH3-bpy-COOCH3)] as was observed
previously for the reduction of [Re]-[NiFe2].[Re]/[NiFe2] (1 mM) was investigated in a solution of CH3CNcontaining NEt3 (2 M). [ReCl(CO)3(CH3-bpy-COOCH3)]* is observable 2 ns after photolysis
as a transient in the spectrum (Figure S8b). This 3MLCT excited state decays (τ = 10 ±
2 ns, Figure S8e, blue dots) to the ground
state (57%) and through reductive quenching by NEt3 (43%)
to form [ReCl(CO)3(CH3-bpy-COOCH3)]− (Figure S8c). Over
greater time scales (50–1500 ns), the CO bands associated with
[ReCl(CO)3(CH3-bpy-COOCH3)]− are lost (τ = 250 ± 10 ns, Figure S8e, red dots) as this species reduces
[NiFe2] to [NiFe2]− to generate
a spectrum with bands at 1969, 1921, and 1896 cm–1 (Figure S8d). [NiFe2]− remains stable for the time scale of the experiment
(70 μs).The most noticeable difference in the excited-state
electron transfer mechanisms in [Re]-[NiFe2] and [Re]/[NiFe2] is the lifetime of the reduced photosensitizer. The monoexponential
decay of [ReCl(CO)3(CH3-bpy-COOCH3)]− (τ = 250 ± 10 ns, Figure S8e, red dots) is significantly shorter
than that measured for [Re]−-[NiFe2]
(τ = 3100 ± 100 ns, Figure e, red dots) under similarconditions. This faster
rate for [Re]/[NiFe2] was investigated further by the determination
of the rate constants of the electron transfer processes in both [Re]-[NiFe2] and [Re]/[NiFe2].
Nanosecond-TRIR experiments
have shown that the reduction of the [NiFe2] center in
[Re]-[NiFe2] can be achieved via the photochemical formation
of [Re]−-[NiFe2] and subsequent electron
transfer to generate [Re]-[NiFe2]−. We
performed concentration-dependent studies to determine the mechanism
of this electron transfer process in [Re]-[NiFe2] and [Re]/[NiFe2]. For [Re]/[NiFe2] only intermolecular electron
transfer is possible (eq ) with the observed rate constant expected to exhibit pseudo-first-order
kinetics and to be dependent on [NiFe2] concentration.
However, in the case of [Re]-[NiFe2], both intra- and intermolecular
electron transfer processes are feasible (eqs and 3). Therefore,
concentration-dependent analysis of the observed rate constant for
electron transfer should be able to distinguish between the two mechanisms.
The observed rate constant can be calculated from the reciprocal of
the lifetime of either [Re]−-[NiFe2]
or [ReCl(CO)3(CH3-bpy-COOCH3)]−.To
quantify the rate of electron transfer in [Re]/[NiFe2]
the concentrations of all components were keptconstant (0.5 mM [ReCl(CO)3(CH3-bpy-COOCH3)]; 1 or 2 M NEt3) except for the concentration of [NiFe2], which
was varied between 0.34 and 1.00 mM. The lifetime dependence of [ReCl(CO)3(CH3-bpy-COOCH3)]− on the concentration of [NiFe2] is shown in Table S2 with the pseudo-first-order rate plot
in Figure a. Since
[NiFe2] is in excess, its concentration remains almost
constant, and so the observed pseudo-first-order rate constant can
be used to calculate the second-order rate constant for electron transfer, kinter = 3.8 ± 0.5 × 109 M–1 s–1. This is in a similar
range to the value reported for electron transfer between [ReCl(CO)3(bpy)]− and [NiFe2], kinter = 6.7 × 109 M–1 s–1.[12a]
Figure 9
Variation of the observed
electron transfer rate constants with catalyst concentration. (a)
[Re]/[NiFe2] in a solution of CH3CN containing
NEt3, linear fitting (solid line) gives kinter = 3.8 ± 0.5 × 109 M–1 s–1 (gradient). (b) [Re]-[NiFe2] in
a solution of NEt3 and CH3CN, linear fitting
(solid line) gives kinter = 5.9 ±
0.7 × 108 M–1 s–1 (gradient) and kintra = 1.5 ± 0.1
× 105 s–1 (x = 0 intercept). Dashed
lines are extensions of the linear fits.
In a
similar experiment, the concentration of [Re]-[NiFe2] was
varied between 0 and 0.3 mM (Figure b and Table S2). This concentration
range was selected to reduce the overall absorbance at the excitation
wavelength (355 nm). A similar trend to that for [Re]/[NiFe2] is observed: as the concentration of [Re]-[NiFe2] is
increased the observed electron transfer rate constant also increases.
However, it is not directly proportional to the concentration of [Re]-[NiFe2] and does not pass close to the origin (Figure b). This could suggest that
intra- and intermolecular pathways operate in this
system. Thus, assuming that these two processes are the only significant
processes occurring following photolysis, then the gradient of the
linear fit provides an estimate of the intermolecular electron transfer
rate constant, kinter = 5.9 ± 0.7
× 108 M–1 s–1.
The positive intercept of this line at 0 M [Re]-[NiFe2]
(Figure b) suggests
that intramolecular electron transfer also occurs, the first-order
rate constant of which can be estimated at kintra = 1.5 ± 0.1 × 105 s–1. It must be noted that this simplification of the electron transfer
mechanism does not include any potential effects resulting from the
decomposition of the electron donor, NEt3.Variation of the observed
electron transfer rate constants with catalyst concentration. (a)
[Re]/[NiFe2] in a solution of CH3CNcontaining
NEt3, linear fitting (solid line) gives kinter = 3.8 ± 0.5 × 109 M–1 s–1 (gradient). (b) [Re]-[NiFe2] in
a solution of NEt3 and CH3CN, linear fitting
(solid line) gives kinter = 5.9 ±
0.7 × 108 M–1 s–1 (gradient) and kintra = 1.5 ± 0.1
× 105 s–1 (x = 0 intercept). Dashed
lines are extensions of the linearfits.
To assess the stability of [Re]-[NiFe2] and [Re]/[NiFe2] during continued photolysis, the FTIR spectrum was monitored
following irradiation using white light from a light-emitting diode
(LED; λ < 420 nm cutoff filter). Figure b shows the FTIR spectrum taken ca. 5 s
after 1 min of photolysis of [Re]-[NiFe2], and the bands
originating from [Re]-[NiFe2]− (1970,
1926, and 1889 cm–1) are observed with an associated
loss in the bands from the [NiFe2] unit. In addition, bands
at 1938 and 1909 cm–1 develop, and by comparison
with our previous studies on [NiFe2] in CH3CN,[12a] these can be assigned as originating from the
formation of a second isomer of [Re]-[NiFe2]−, where the two of the terminal carbonyl bands of the [NiFe2] unit bridge across the two Fe atoms. Depletion of the parent bands
of the [Re] center is also evident and a broad positive feature is
observed at 2013 cm–1, which is in a similarregion
to related products reported following chemical reduction of [ReCl(CO)3(bpy)]. These include [ReCl(CO)3(bpy)]− (1998, 1880, and 1866 cm–1, in CH3CN),
[Re(CH3CN)(CO)3(bpy)]• (2017
and 1902(br) cm–1, in CH3CN), and [Re(CO)3(bpy)]2 (1990, 1952, 1886, and 1863 cm–1 in tetrahydrofuran);[28] however, the precise
origin of the band in our experiment could not be determined. The
apparent loss of bands associated with the [Re] center upon photolysis,
without the clear formation of a new species, suggests that decomposition
of the [Re] diiminecenter has occurred to yield products that are
not clearly observable in this region of the IR spectrum.
Figure 10
FTIR spectra of [Re]-[NiFe2] before and after
steady-state photolysis in a solution of CH3CN containing
NEt3 (1 M). (a) Ground-state FTIR spectrum. (b) FTIR difference
spectrum taken ca. 5 s after 1 min photolysis. In situ photolysis
was performed using an LED white light source and a λ < 420
nm cutoff filter.
A
similar spectral profile was observed for [Re]/[NiFe2]
after 1 min of photolysis. Almost complete depletion of the bands
originating from both [ReCl(CO)3(CH3-bpy-COOCH3)] and [NiFe2] can been seen with the formation
of both isomers of [NiFe2]− (Figure S9). This apparent decomposition of the
photosensitizer in [Re]/[NiFe2] was not observed when [ReCl(CO)3(bpy)] was used in place of [ReCl(CO)3(CH3-bpy-COOCH3)].[12a] In
this example no apparent loss in the bands of [ReCl(CO)3(bpy)] could be observed after 30 s of photolysis under similarconditions.
Thus, it appears that functionalizing the bipyridine ligand in [Re]-[NiFe2] and [ReCl(CO)3(CH3-bpy-COOCH3)] reduces the stability of the photosensitizer when compared
to [ReCl(CO)3(bpy)], on continuous photolysis in reducing
conditions.FTIR spectra of [Re]-[NiFe2] before and after
steady-state photolysis in a solution of CH3CNcontaining
NEt3 (1 M). (a) Ground-state FTIR spectrum. (b) FTIR difference
spectrum taken ca. 5 s after 1 min photolysis. In situ photolysis
was performed using an LED white light source and a λ < 420
nm cutoff filter.
H2 Production
Studies
We investigated the use of [Re]-[NiFe2] and [Re]/[NiFe2] for photoinduced H2 production
using both NEt3 and TEOA as sacrificial electron donors.
[ReCl(CO)3(bpy)] has been used previously as a photosensitizer
for photocatalyticH2 production from [NiFe2] with a TON of 55 under optimal conditions.[12a] Using similarconditions, [Re]-[NiFe2] (0.1
mM) was investigated in a solution of CH3CNcontaining
TEOA (1 M) and [HTEOA][BF4] (0.1 M) as a proton source.
Only a trace amount of H2could be detected from this system,
with a TON of ca. 1 based on [Re]-[NiFe2] as the catalytic
moiety. Replacing TEOA with NEt3 had a negative effect
on the total amount of H2 evolved. In a solution containing
[Re]/[NiFe2] (both at 0.1 mM), TEOA (1 M), and [HTEOA][BF4] (0.1 M) in CH3CN, again only a trace amount of
H2 was evolved. Thus, from FTIR and H2 production
studies it appears that when either [Re]-[NiFe2] or [Re]/[NiFe2] are used for H2 production, rapid decomposition
of the esterified photosensitizer occurs, resulting in an almost complete
loss in catalytic activity toward H2 production.
Conclusions
We have investigated a linked dyad, [Re]-[NiFe2] (Figure ), designed for photoinduced
electron transfer and proton reduction. Following flash photolysis,
picosecond-TRIR and nanosecond-TRIR spectroscopies have monitored
the reduction of the [NiFe2] catalytic moiety in [Re]-[NiFe2] and probed the mechanisms of electron transfer. Excitation
of the [Re] center results in the population of the 3MLCT
excited state, [Re]*-[NiFe2]. Reductive quenching of [Re]*-[NiFe2] by NEt3 forms [Re]−-[NiFe2], which subsequently undergoes electron transfer to the [NiFe2] center to form [Re]-[NiFe2]−. The mechanisms of this electron transfer step were probed by concentration-dependent
studies and suggest that both intra- and intermolecular electron transfer
processes are involved (kinter = 5.9 ±
0.7 × 108 M–1 s–1, kintra = 1.5 ± 0.1 × 105 s–1). As expected, in the analogous bimolecular
system ([Re]/[NiFe2]), only intermolecular electron transfer
could be observed (kinter = 3.8 ±
0.5 × 109 M–1 s–1). One of the key advantages for directly linking the photosensitizer
and catalyst is to increase the rate of electron transfer. However,
in this study the overall observed rate of electron transfer is significantly
slower in [Re]-[NiFe2] than in [Re]/[NiFe2].
During continuous photolysis, rapid decomposition of the photosensitizing
unit in both [Re]-[NiFe2] and [Re]/[NiFe2] can
be observed using FTIR spectroscopy. This may, in part, help to explain
the poor activity of this dyad and the bimolecular system toward H2 evolution in acidic media. In the ester-linked dyad probed
in this study, linking the catalytic and photosensitizing moieties
appears to be detrimental to both the electron transfer rate and the
chemical stability of the system on continuous photolysis. However,
careful consideration in the development of future systems can overcome
these problems so that the benefits of linked dyads can be exploited.
Authors: Gregory M Greetham; Pierre Burgos; Qian Cao; Ian P Clark; Peter S Codd; Richard C Farrow; Michael W George; Moschos Kogimtzis; Pavel Matousek; Anthony W Parker; Mark R Pollard; David A Robinson; Zhi-Jun Xin; Michael Towrie Journal: Appl Spectrosc Date: 2010-12 Impact factor: 2.388
Authors: A M Kluwer; R Kapre; F Hartl; M Lutz; A L Spek; A M Brouwer; P W N M van Leeuwen; J N H Reek Journal: Proc Natl Acad Sci U S A Date: 2009-01-21 Impact factor: 11.205