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Dynamic Article LinksC<Energy &Environmental Science
Cite this: Energy Environ. Sci., 2012, 5, 6111
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View Online / Journal Homepage / Table of Contents for this issue
Photocatalytic hydrogen evolution with Ni nanoparticles by using2-phenyl-4-(1-naphthyl)quinolinium ion as a photocatalyst†
Yusuke Yamada,a Takamitsu Miyahigashi,a Hiroaki Kotani,a Kei Ohkuboa and Shunichi Fukuzumi*ab
Received 7th November 2011, Accepted 15th December 2011
DOI: 10.1039/c2ee03106j
Photocatalytic hydrogen evolution with 2-phenyl-4-(1-naphthyl)quinolinium ion (QuPh+–NA) as
a photocatalyst and dihydronicotinamide adenine dinucleotide (NADH) as a sacrificial electron donor
has been made possible for the first time by using nickel nanoparticles (NiNPs) as a non-precious metal
catalyst. The hydrogen evolution rate with the most active Ni nanoparticles (hexagonal close-packed
(hcp) structure, 6.6 nm) examined here was 40% of that with commercially available Pt nanoparticles
(2 nm) using the same catalyst weight. The catalytic activity of NiNPs depends not only on their sizes
but also on their crystal phases. The hydrogen-evolution rate normalized by the catalyst weight
increased as the size of NiNPs becomes smaller, with regard to the crystal phase, the hydrogen-
evolution rate of the NiNPs with hcp structure is more than 4 times higher than the rate of the NiNPs
with face-centred cubic (fcc) structure of similar size. NiNPs act as the hydrogen-evolution catalyst
under the pH conditions between 4.5 and 8.0, although the hydrogen-evolution rate at pH > 7.0 was
much lower as compared with the hydrogen-evolution rate at pH 4.5. A kinetic study revealed that the
rate of electron transfer from photogenerated QuPh_–NA to NiNPs was much higher than the rate of
hydrogen evolution, indicating that the rate-determining step may be proton reduction or desorption of
hydrogen.
1. Introduction
Hydrogen is a promising clean fuel for the next generation
without emitting greenhouse gas and other harmful chemicals
aDepartment of Material and Life Science, Division of Advanced Scienceand Biotechnology, Graduate School of Engineering, Osaka University,ALCA, Japan Science and Technology Agency (JST), Suita, Osaka,565-0871, Japan. E-mail: [email protected]; [email protected]; Fax: +81-6-6879-7370; Tel: +81-6-6879-7368bDepartment of Bioinspired Science, EwhaWomans University, Seoul, 120-750, Korea
† Electronic supplementary information (ESI) available: Recyclabilitytest (Fig. S1), hydrogen generation with NiO nanoparticles (Fig. S2),powder XRD pattern of NiNPs (Fig. S3), interaction of fcc- andhcp-NiNPs with a magnet (Fig. S4), catalytic activity test with differentamounts of NiNPs (Fig. S5) and DLS of CuNPs just after preparation(Fig. S6). See DOI: 10.1039/c2ee03106j
Broader context
Photocatalytic hydrogen evolution has been an attractive method
carbon dioxide. A hydrogen-evolution system composed of an org
utilize visible light. However, the metal catalysts usually contain pre
for hydrogen evolution. Replacing platinum with cheap and abunda
that Ni nanoparticles act as efficient catalysts for the photocatalyti
ion as a photocatalyst and NADH as a sacrificial electron donor.
This journal is ª The Royal Society of Chemistry 2012
after burning.1–4 Currently, hydrogen is produced by the steam
reforming of hydrocarbons followed by the high temperature
and low temperature water gas shift reactions and selective CO
oxidation. Thus, CO2, which is regarded as a typical greenhouse
gas, is produced as a byproduct.5 In order to attain hydrogen by
a really clean process, water splitting by using solar energy is the
most desirable method.6–8 Photocatalytic hydrogen evolution
with a photosensitizer, a sacrificial electron donor, an electron
mediator and a hydrogen-evolution catalyst has been studied for
the last few decades to improve the catalytic efficiency.9–28
Although water should be used as an electron source to realize
the water splitting for the solar-energy conversion, it is still very
important to optimize the photocatalytic reactivity of hydrogen
evolution with a sacrificial electron donor. Recently, the effi-
ciency of photocatalytic hydrogen evolution has been improved
by employing electron donor–acceptor linked dyads with
to convert solar energy to chemical energy without emitting
anic photosensitizer and metal catalysts has large potential to
cious metals, typically platinum, because of a low overpotential
nt metals is still a big challenge. Here we report for the first time
c hydrogen evolution with 2-phenyl-4-(1-naphthyl)quinolinium
Energy Environ. Sci., 2012, 5, 6111–6118 | 6111
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a long-lived charge-separated state,29–34 which can inject elec-
trons directly to a hydrogen-evolution catalyst without an elec-
tron mediator upon photoexcitation of the donor–acceptor
linked dyads.35–38
A bottleneck of the photocatalytic hydrogen-evolution system
with heterogeneous catalysts is the demand for a precious metal
such as Pt,9,16 although Fe and Co complexes act as the catalysts
in homogeneous systems39–50 and natural systems utilize non-
precious metals, i.e., Fe and Ni, in the active centres of
hydrogenases.51–57 In heterogeneous systems, Fe nanoparticles
have been employed as a hydrogen-evolution catalyst in the
reaction system with an electron donor–acceptor dyad with long-
lived charge-separated state and NADH as a photocatalyst and
a sacrificial electron donor, respectively.35 However, the catalytic
efficiency is by far lower than that of Pt nanoparticles. On the
other hand, an Ni based catalyst, which is a component metal of
Fe–Ni hydrogenases,51–55 has yet to be examined as a catalyst for
the photocatalytic hydrogen evolution.
We report herein an efficient photocatalytic hydrogen-evolu-
tion system composed of a donor–acceptor linked dyad,
2-phenyl-4-(1-naphthyl)quinolinium ion (QuPh+–NA), as a pho-
tocatalyst34,38 and NADH as a sacrificial electron donor using Ni
nanoparticles (NiNPs) together with the catalytic activity of
nanoparticles of Fe, Co and Cu. This is the first report to employ
NiNPs as a catalyst for efficient photocatalytic hydrogen
evolution. The whole reaction scheme is depicted in Scheme 1.
The size effects of NiNPs as well as effects of crystal phase on
both the catalytic reactivity for the hydrogen evolution and the
electron injection from QuPh_–NA were also examined in detail
to optimize the catalytic reactivity.
2. Experimental section
All chemicals were obtained from a chemical company and
used without further purification. 1-Octadecene (ODE, 90%),
poly(vinylpyrrolidone) (PVP, Mw ¼ 40 000), cobalt carbonyl
[Co2(CO)8], tri-n-octylphosphine oxide and hexadecylamine were
obtained from Tokyo Chemical Industry Co., Ltd. Pt nano-
particles (2 nm) capped with PVP were supplied by Tanaka
Kikinzoku Kogyo. Nickel acetylacetonate [Ni(acac)2], tri-n-
octylphosphine and oleylamine (70%) were obtained from Sigma-
AldrichCo.LLC.Oleic acid (60%), sodiumborohydride (NaBH4)
and sodium hydroxide were obtained fromWako Pure Chemical
Industries. Copper(II) acetate [Cu(OAc)2] was obtained from
Nacalai Tesque. 2-Phenyl-4-(1-naphthyl)quinolinium perchlo-
rate was synthesized by the reported method.34 Each buffer
solution was prepared by addition of NaOH to an aqueous
solution containing an electrolyte (50mMof phthalate for pH4.5,
Scheme 1 Structure of QuPh+–NA and the overall catalytic cycle for
photocatalytic hydrogen evolution.
6112 | Energy Environ. Sci., 2012, 5, 6111–6118
5.3, 6.0; 50 mM of phosphate for pH 7.0, 8.0 and 25 mM of
carbonate for pH 10). All chemicals were used without further
purification unless otherwise noted. Purified water was provided
by aMilli-Qwater purification system (Millipore, Direct-Q 3UV)
where the electronic conductance was 18.2 MU cm.
2.1. Synthesis of particles
Synthesis of 6.6 nm Ni nanoparticles (NiNPs).58 Ni(acac)2(275 mg, 1.1 mmol), tri-n-octylphosphine (0.50 mL, 1.1 mmol)
and oleic acid (0.50 mL, 2.0 mmol) were dissolved in oleylamine
(7 mL) in a 50 mL three-neck round-bottom flask at room
temperature. The solution was degassed under reduced pressure
for 20 min at 403 K, then heated to 518 K (at 4.8 K min�1) and
kept at this temperature for 30 min under an Ar atmosphere.
After the solution was cooled to room temperature, ethanol was
added to cause flocculation and then the suspension was centri-
fuged (15 000 rpm, 10 min) to separate black precipitates. The
black precipitates were washed three times by dispersion/
precipitation (n-hexane/ethanol) cycles. The final product was
dispersed in n-hexane (5 mL).
Synthesis of 11 nm NiNPs.58 Ni(acac)2 (275 mg, 1.1 mmol) and
tri-n-octylphosphine (1.3 mL, 3.0 mmol) were dissolved in
oleylamine (7 mL) in a 50 mL three-neck round-bottom flask at
room temperature. The solution was degassed under reduced
pressure for 20 min at 403 K, then heated to 523 K (at
4.0 Kmin�1) and kept at this temperature for 30 min under an Ar
atmosphere. After the solution was cooled to room temperature,
ethanol was added to flocculate and then the suspension was
centrifuged (15 000 rpm, 10 min) to separate black precipitates.
The black precipitates were washed three times by dispersion/
precipitation (n-hexane/ethanol) cycles. The final product was
dispersed in n-hexane (5 mL).
Synthesis of 36 nm NiNPs.58 Ni(acac)2 (275 mg, 1.1 mmol) was
dissolved in oleylamine (15 mL) in a 50 mL three-neck round-
bottom flask at room temperature. The solution was degassed
under reduced pressure for 20 min at 403 K, then heated to 543 K
(at 5.2 K min�1) and kept at this temperature for 2 h under an Ar
atmosphere. After the solution was cooled to room temperature,
ethanol was added to flocculate and then the suspension was
centrifuged (15 000 rpm, 10 min) to separate black precipitates.
The black precipitates were washed three times by dispersion/
precipitation (n-hexane/ethanol) cycles. The final product was
dispersed in n-hexane (5 mL).
Synthesis of 210 nm hcp-NiNPs.58 Ni(acac)2 (275 mg,
1.1 mmol) was dissolved in a solution of oleylamine (4 mL) and
octadecene (4 mL) in a 50 mL three-neck round-bottom flask at
room temperature. The solution was degassed under reduced
pressure for 20 min at 403 K, then heated to 543 K (at
5.2 Kmin�1) and kept at this temperature for 30 min under an Ar
atmosphere. After the solution was cooled to room temperature,
ethanol was added to cause flocculation and then the suspension
was centrifuged (15 000 rpm, 10 min) to separate black precipi-
tates. The black precipitates were washed three times by disper-
sion/precipitation (n-hexane/ethanol) cycles. The final product
was dispersed in n-hexane (5 mL).
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Synthesis of Co nanoparticles (CoNPs).59 Co2(CO)8 (540 mg,
1.58 mmol) was dissolved in 1,2-dichlorobenzene (3 mL). The
solution was injected into 1,2-dichlorobenzene (15 mL) con-
taining a mixture of oleic acid (0.20 mL, 0.62 mmol) and tri-n-
octylphosphine oxide (100 mg, 0.26 mmol) in a 50 mL three-neck
round-bottom flask at 455 K and then refluxed for 30 min. After
the solution was cooled to room temperature, ethanol was added
to cause flocculation. Then the suspension was centrifuged
(15 000 rpm, 10 min) to separate black precipitates. The black
precipitates were washed three times by dispersion/precipitation
(n-hexane/ethanol) cycles. The final product was dispersed in
n-hexane (5 mL).
Synthesis of Cu nanoparticles (CuNPs).60 Cu(OAc)2 (60 mg,
0.30 mmol) and PVP (400 mg) were dissolved in water (20 mL) in
a 50 mL three-neck round-bottom flask at room temperature.
Then, an aqueous solution of NaBH4 (11 mg, 0.30 mmol) and
NaOH (12 mg, 0.30 mmol) was injected into the Cu(OAc)2/PVP
aqueous solution and stirred for 15 min under a N2 atmosphere
at room temperature. After the reaction, acetone was added to
cause flocculation and then the suspension was centrifuged
(15 000 rpm, 10 min) to separate black precipitates. The black
precipitates were washed three times by dispersion/precipitation
(acetone/water) cycles. The final product was dispersed in
ethanol (5 mL).
Synthesis of Fe nanoparticles (FeNPs).61 ODE (20 mL) and
oleylamine (0.3 mL) were mixed and degassed by passing Ar gas
at 393 K for 30 min. The temperature was raised to 453 K (at
3.3 K min�1) and Fe(CO)5 (0.7 mL, 5.2 mmol) was slowly added.
The mixture was kept at the temperature for 20 minutes. After
the solution was cooled to room temperature, ethanol was added
to flocculate and then the suspension was centrifuged
(15 000 rpm, 10 min) to separate black precipitates. The black
precipitates were washed three times by dispersion/precipitation
(n-hexane/ethanol) cycles. The final product was dispersed in
n-hexane (5 mL).
Synthesis of 16 nm fcc-NiNPs.62 Ni(acac)2 (200mg, 0.78mmol)
was dissolved in 1,2-dichlorobenzene (5mL) at 373K, andquickly
injected into 1,2-dichlorobenzene (40mL) containing amixture of
hexadecylamine (4.0 g, 17 mmol) and NaBH4 (400 mg, 11 mmol)
at 393 K during vigorous stirring. The resulting mixture was
heated to 453 K and kept at this temperature for 1 h under an Ar
atmosphere. After the solution was cooled to room temperature,
ethanol was added to cause flocculation and then the suspension
was centrifuged (15 000 rpm, 10 min) to separate black precipi-
tates. The black precipitates were washed three times by disper-
sion/precipitation (n-hexane/ethanol) cycles. The final product
was dispersed in n-hexane (5 mL).
Synthesis of 22 nm fcc-NiNPs.62 Ni(acac)2 (200 mg,
0.78 mmol) was dissolved in 1,2-dichlorobenzene (5 mL) at
373 K, and quickly injected into 1,2-dichlorobenzene (40 mL)
containing a mixture of hexadecylamine (1.5 g, 6.2 mmol), tri-
n-octylphosphine oxide (500 mg, 1.3 mmol) and NaBH4
(150 mg, 4.0 mmol) at 393 K during vigorous stirring. The
resulting mixture was heated to 453 K and kept at this
temperature for 45 min under an Ar atmosphere. After the
This journal is ª The Royal Society of Chemistry 2012
solution was cooled to room temperature, ethanol was added to
cause flocculation and then the suspension was centrifuged
(15 000 rpm, 10 min) to separate black precipitates. The black
precipitates were washed three times by dispersion/precipitation
(n-hexane/ethanol) cycles. The final product was dispersed in
n-hexane (5 mL).
Synthesis of 80 nm fcc-NiNPs.63 Ni(acac)2 (275 mg, 1.1 mmol)
was dissolved in oleylamine (15 mL) in a 50 mL three-neck
round-bottom flask at room temperature. The solution was
degassed under reduced pressure for 20 min at room tempera-
ture, then, heated to 408 K and kept at this temperature for
30 min. Then, the solution was further heated up to 488 K (at
4.7 K min�1) and kept at this temperature for 1 h under an Ar
atmosphere. After the solution was cooled to room temperature,
ethanol was added to cause flocculation and then the suspension
was centrifuged (15 000 rpm, 10 min) to separate black precipi-
tates. The black precipitates were washed three times by disper-
sion/precipitation (n-hexane/ethanol) cycles. The final product
was dispersed in n-hexane (5 mL).
Capping agent exchange with PVP.35 An n-hexane solution
(2.0 mL) containing nanoparticles was mixed with a solution
containing PVP (200 mg) in CHCl3 (8 mL) at 323 K. The solution
was stirred for 9 h to exchange a surfactant. A certain amount of
acetone was added to the solution to cause flocculation and then
the mixture was centrifuged at 15 000 rpm for 10 min. The
collected water-soluble particles were washed three times by
dispersion/precipitation (ethanol/acetone) cycles.
2.2. Photocatalytic hydrogen evolution
Amixed solution (2.0 mL) of an aqueous buffer (pH 4.5, 5.3, 6.0,
7.0, 8.0 or 10) and MeCN [1 : 1 (v/v)] containing QuPh+–NA
(0.44 mM), NADH (1.0 mM) and NiNPs (25 mg) was flushed
with N2 gas. The solution was then irradiated with a Xe lamp
(Ushio Optical, Model X SX-UID 500X AMQ) through a colour
filter glass (Toshiba Glass UV-35) transmitting l > 340 nm at
room temperature. After the solution was stirred for 1 min in the
dark, the gas in the headspace was analyzed using a Shimadzu
GC-14B gas chromatograph (detector, TCD; column tempera-
ture, 50 �C; column, active carbon with 60–80 mesh particle size;
carrier gas, N2) to quantify the evolved hydrogen.
2.3. Kinetic measurements
A mixed solution (2.0 mL) of a deaerated aqueous buffer (pH
4.5, 6.0, 7.0, 8.0 or 10) andMeCN [1 : 1 (v/v)] containing QuPh+–
NA (0.44 mM) and NADH (1.0 mM) was photoirradiated for 1
min with a Xe lamp through a colour filter glass transmitting l >
340 nm. Then, a deaerated aqueous solution containing NiNPs
(25 mg) was added to the photoirradiated solution using
a microsyringe with stirring. Rate constants of electron transfer
from QuPh_–NA (obtained by one-electron reduction of QuPh+–
NA) to the catalyst were determined from the decay of absorp-
tion at 510 nm due to QuPh_–NA, which was monitored using
a Hewlett-Packard 8453 diode-array spectrophotometer with
a quartz cuvette (path length 10 mm) at 298 K.
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2.4. Catalysts characterization
Transmission electron microscope (TEM) images of nano-
particles, which were mounted on a copper microgrid coated
with elastic carbon, were observed by a JEOL JEM 2100 oper-
ating at 200 keV. Powder X-ray diffraction patterns were
recorded by a Rigaku RINT 2000. Incident X-ray radiation was
produced by a Cu X-ray tube, operating at 40 kV and 200 mA
with Cu Ka radiation of 1.54 �A. The scanning rate was 2� min�1
from 20� to 80� in 2q.
3. Results and discussion
3.1. Photocatalytic hydrogen evolution with catalytic
nanoparticles
Catalytic nanoparticles were prepared by reduction of metal ion
sources followed by reported methods with some modifications.
Ni nanoparticles (NiNPs) were prepared by the reduction of
Ni(acac)2 complex in oleylamine at high temperature in the
presence or absence of tri-n-octylphosphine and oleic acid. Cu
nanoparticles (CuNPs) were obtained by Cu(OAc)2 reduction by
NaBH4 in the presence of PVP at room temperature. Fe nano-
particles (FeNPs) and Co nanoparticles (CoNPs) were prepared
from corresponding carbonyl complexes by thermal decompo-
sition (see the Experimental section). The obtained Co, Cu and
Fe nanoparticles were characterized by TEM and dynamic laser
scattering (DLS) as displayed in Fig. 1. The TEM images and
DLS data for NiNPs are shown in Fig. 4a (vide infra). The
diameters of NiNPs, CuNPs, FeNPs and CoNPs were 6.6 �1.6 nm, 200 � 100 nm, 16 � 5.0 nm and 4.5 � 2.0 nm,
Fig. 1 TEM images and particles size distributions determined by
dynamic laser scattering (DLS) of (a) CoNPs, (b) CuNPs and (c) FeNPs.
6114 | Energy Environ. Sci., 2012, 5, 6111–6118
respectively.64 The capping agents of the NiNPs, FeNPs and
CoNPs were exchanged to PVP before catalysis measurements in
order to increase the dispersity to an aqueous solution.
Fig. 2 shows the time courses of photocatalytic hydrogen
evolution under photoirradiation (l > 340 nm) of a mixed
solution [MeCN/buffer (pH 4.5) ¼ 1/1 (v/v)] containing NADH,
QuPh+–NA and metal nanoparticles (MNPs, M ¼ Ni, Cu, Fe or
Co) as a sacrificial electron donor, a photocatalyst and
hydrogen-evolution catalysts, respectively. Commercially avail-
able Pt nanoparticles (PtNPs, 2 nm) were also employed as
a hydrogen-evolution catalyst for a reference. No hydrogen
evolution was observed from the mixed solution in the dark. The
photoirradiation (l > 340 nm) of the solution resulted in
hydrogen evolution. Among the nanoparticles used here, only
NiNPs (Fig. 2, red closed square) and PtNPs (blue diamond)
provided the evolution of the stoichiometric amount of hydrogen
(2.0 mmol) in a certain reaction time. The hydrogen-evolution
rates with PtNPs and NiNPs were 28 mmol h�1 and 11 mmol h�1,
respectively. The catalytic reactivity of NiNPs was maintained
for the repetitive use for three times as shown in Fig. S1 in the
ESI†. CuNPs and FeNPs also acted as catalysts for hydrogen
evolution, however, their catalytic reactivity was rather modest
compared with NiNPs. No hydrogen evolution was observed
with CoNPs. Under atmospheric conditions, Ni metal might be
oxidized to form nickel oxide. The catalytic activity of NiO
nanoparticles was investigated in the photocatalytic hydrogen
evolution under the same conditions described above. As indi-
cated in Fig. S2†, only 10% of the stoichiometric amount of
hydrogen was evolved for the first reaction cycle. When the NiO
catalyst was used repeatedly, the catalytic activity was gradually
improved, because NiO was probably reduced to Ni metal under
the reaction conditions. Thus, we focused on examining the
catalytic reactivity of NiNPs depending on the particle sizes and
crystal phases including the kinetic measurements.
3.2. Electron transfer from QuPh_–NA to NiNPs
Rates of electron transfer from QuPh_–NA to NiNPs in a mixed
solution of a phthalate buffer (pH 4.5) and MeCN [1 : 1 (v/v)]
were determined by UV-vis spectral change to compare the
results with the corresponding rates of hydrogen evolution
Fig. 2 Time courses of hydrogen evolution under photoirradiation (l >
340 nm) of a deaerated mixed solution (2 mL) of a phthalate buffer
(pH 4.5) and MeCN [1 : 1 (v/v)] containing QuPh+–NA (0.44 mM),
NADH (1.0 mM) and various catalysts [12.5 mg L�1, closed square,
NiNPs (6.6 nm); open square, CuNPs; closed circle, FeNPs; open circle,
CoNPs and closed diamond, PtNPs (2 nm)] at 298 K.
This journal is ª The Royal Society of Chemistry 2012
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determined by gas chromatography. This is the first example to
observe the electron-transfer rate from a radical species to NiNPs
compared with the hydrogen-evolution rate. An aliquot (2.0 mL)
of QuPh+–NA (0.44 mM) was photoirradiated in the presence of
NADH (1.0 mM) for several minutes to generate QuPh_–NA.
Then, a small portion of an aqueous solution containing NiNPs
(12.5 mg L�1) was added to the mixed solution containing QuPh_–
NA to initiate the hydrogen evolution. Fig. 3 depicts the time
profiles of UV-vis absorption change at 510 nm (blue circles) and
those of the amount of evolved hydrogen quantified by gas
chromatography (red circles) for NiNPs. The total amount of
evolved hydrogen was 0.4 mmol, which corresponds to 80% of the
stoichiometric amount of hydrogen predicted from the absorp-
tion change due to QuPh_–NA. As shown in Fig. 3, the decay of
QuPh_–NA due to electron transfer from QuPh_–NA to NiNPs is
completed within 30 s (blue lines), whereas hydrogen evolution
lasts for a longer period (red line, ca. 500 s). These results indicate
that the rate-determining step is not electron transfer from
QuPh_–NA to NiNPs but the hydrogen evolution step, which
includes the proton reduction, hydrogen association and
hydrogen desorption.
Fig. 4 TEM images and particles size distributions determined by
dynamic laser scattering of hcp-NiNPs with sizes of (a) 6.6 nm, (b) 11 nm,
(c) 36 nm and (d) 210 nm.
3.3. Size effects of NiNPs on the photocatalytic hydrogen
evolution
TEM images and dynamic laser scattering (DLS) of NiNPs with
different sizes are displayed in Fig. 4. The size-controlled NiNPs
were prepared by thermal decomposition of Ni(acac)2 in oleyl-
amine with oleic acid, tri-n-octylphosphine or octadecene at the
temperature higher than 523 K (see the Experimental section).
The sizes determined for NiNPs were 6.6 � 1.6 nm (Fig. 4a),
11 � 2 nm (Fig. 4b), 36 � 12 nm (Fig. 4c) and 210 � 80 nm
(Fig. 4d). The TEM images indicated that no shape-controlled
particles were obtained. The powder X-ray diffraction patterns
of smaller NiNPs (6.6 nm and 11 nm) were very broad,
however, those of larger NiNPs (36 nm and 210 nm) indicated
that the crystal phase of these NiNPs is mainly a hexagonal
close-packed (hcp) structure (Fig. S3 in the ESI†). More obvi-
ously, these particles were not attracted to a magnet as shown in
Fig. S4 in the ESI†.
Fig. 3 Decay time profile of absorption at 510 nm due to QuPh_–NA in
electron transfer from QuPh_–NA to NiNPs (12.5 mg L�1) (solid line) and
corresponding time profile of hydrogen evolution (broken line) in mixed
solutions of a phthalate buffer (pH 4.5) and MeCN [1 : 1 (v/v)]. QuPh_–
NA was produced by photoirradiation of QuPh+–NA (0.44 mM) in the
presence of NADH (1.0 mM).
This journal is ª The Royal Society of Chemistry 2012
The photocatalytic hydrogen evolution was conducted under
photoirradiation of a mixed solution (2.0 mL) of a deaerated
buffer (pH 4.5) and MeCN [1 : 1 (v/v)] containing QuPh+–NA
(0.44 mM), NADH (1.0 mM) and NiNPs (12.5 mg L�1) with
different sizes (6.6–210 nm).When smaller NiNPs with the size of
6.6 nm or 11 nm were employed as hydrogen-evolution catalysts,
nearly a stoichiometric amount of hydrogen was evolved (closed
and open circles in Fig. 5a), although the amount of evolved
hydrogen was �80% of the stoichiometric amount in the case of
NiNPs with the size of 36 nm (closed square in Fig. 5a) and only
50% with the size of 210 nm. The hydrogen-evolution rates (VH2)
Fig. 5 (a) Time courses of hydrogen evolution under photoirradiation
(l > 340 nm) of mixed solutions of deaerated phthalate buffer (pH 4.5)
and MeCN [1 : 1 (v/v)] containing NADH (1.0 mM), QuPh+–NA
(0.44 mM), and NiNPs with different sizes (12.5 mg L�1) at 298 K. (b)
Plots of hydrogen-evolution rates normalized by weight concentration of
NiNPs vs. the size of NiNPs.
Energy Environ. Sci., 2012, 5, 6111–6118 | 6115
Fig. 7 Dynamic laser scattering (DLS) of fcc-NiNPs with different sizes.
(a) 16 � 4.0 nm, (b) 22 � 6.0 nm and (c) 80 � 20 nm. (d) Powder X-ray
diffraction patterns obtained from NiNPs with different sizes.
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normalized by the weight concentrations of NiNPs were plotted
against the size of NiNPs in Fig. 5b. The smallest NiNPs with the
size of 6.6 nm exhibited the highest VH2 of 1.1 mmol h�1 mg L�1.
This result is quite reasonable, because smaller NiNPs have
a higher specific surface area per weight.
The rate constants (ket) of electron transfer from QuPh_–NA to
NiNPs with different sizes were determined from the slopes of the
linear plots of kobs vs. the weight concentration of NiNPs in
Fig. 6a where kobs is the pseudo-first-order rate constant deter-
mined from the first-order plots. A mixed solution (2.0 mL) of
a phthalate buffer and MeCN [1 : 1 (v/v)] containing QuPh+–NA
(0.44 mM) was photoirradiated in the presence of NADH
(1.0 mM) to generate QuPh_–NA until no significant absorption
change was observed. Then, a small portion of an aqueous
solution containing NiNPs was added to the solution containing
QuPh_–NA to initiate the electron transfer to NiNPs. Larger ketvalue was achieved at smaller NiNPs with the size of 11 nm as
shown in Fig. 6b. Although the electron transfer is much faster
than hydrogen evolution as shown in Fig. 3, the slower electron
transfer from QuPh_–NA to NiNPs with large particles may be
a disadvantage for hydrogen evolution.
3.4. Effects of crystal phase of NiNPs
Two different types of crystal phases have been reported for
NiNPs, which are hexagonal close-packed (hcp) and face-centred
cubic (fcc) structures. The fcc-Ni nanoparticles with three
different sizes were prepared by the reported method. Fig. 7a–c
show the particles size distributions of fcc-NiNPs determined by
DLS. The sizes of fcc-NiNPs were 16 � 4.0 nm, 22 � 6.0 nm and
80 � 20 nm. The crystal phase of these fcc-NiNPs was confirmed
by the X-ray diffraction patterns as indicated in Fig. 7d. The
three characteristic peaks appeared at 44.5�, 51.9� and 76.5� areoriginated from the diffractions from (111), (200) and (220)
planes, respectively.65
Photocatalytic hydrogen evolution with fcc-NiNPs as
a hydrogen-evolution catalyst was investigated by photo-
irradiation of mixed solution of phthalate buffer (pH 4.5) and
MeCN containing NADH (1.0 mM) and QuPh+–NA (0.44 mM).
Fig. 8 shows the time courses of hydrogen evolution with fcc-
NiNPs (12.5 mg L�1) at 298 K. The fastest hydrogen evolution
was observed with fcc-NiNPs (16 nm) and the slowest hydrogen
Fig. 6 (a) Plots of the pseudo first-order rate constants (kobs) of electron
transfer from QuPh_–NA to NiNPs vs. weight concentrations of NiNPs at
298 K. (b) Size dependence of the rate constants (ket) of electron transfer
from QuPh_–NA to NiNPs with various sizes determined from the slopes
of the plots in (a).
6116 | Energy Environ. Sci., 2012, 5, 6111–6118
evolution was attained with fcc-NiNPs (80 nm). This result is
quite reasonable, because the specific surface area increases at
smaller particles. Even at smallest particles, the hydrogen yield
was lower than 40% of the stoichiometric amount. The
hydrogen-evolution rates with fcc-NiNPs normalized by the
weight concentrations (black circles) are compared with NiNPs,
mainly composed of hcp structure (red circles) in Fig. 8b. The
hydrogen-evolution rate with hcp-NiNPs (11 nm) was 4.8 times
higher than that with fcc-NiNPs (16 nm).
Ni nanoparticles are often used as hydrogen-production
catalysts for steam reforming of hydrocarbons.66 The catalytic
activity of Ni catalysts has been reported as highly dependent on
their surface structures.67 Certain step sites are considerably
more reactive than close-packed facets. For steam reforming of
glycerol, high product selectivity to hydrogen has been reported
on hcp-NiNPs compared with fcc-NiNPs.67 Additionally,
intrinsic activity of hcp-Ni is much higher than fcc-Ni in propene
hydrogenation.68 The fcc-Ni structure is thermally stable and
Fig. 8 (a) Time courses of hydrogen evolution under photoirradiation
(l > 340 nm) of mixed solutions of deaerated phthalate buffer (pH 4.5)
and MeCN [1 : 1 (v/v)] containing NADH (1.0 mM), QuPh+–NA
(0.44 mM), and fccNiNPs with different sizes (12.5 mg L�1) at 298 K. (b)
Plots of hydrogen-evolution rates with different structures of NiNPs
(circle, hcp; square, fcc) vs. the sizes of NiNPs.
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hcp-Ni structure is known as a metastable structure.66 The
superior catalysis of hcp-NiNPs can be ascribed to the loose
packing of hcp structure. Thus, the hcp-NiNPs are more active
catalysts for the photocatalytic hydrogen evolution than the fcc-
NiNPs.
Fig. 10 (a) Plots of the pseudo-first-order rate constants (kobs) for
electron transfer from QuPh_–NA vs. weight concentrations of NiNPs at
298 K. Time courses of hydrogen evolution with different weights of
NiNPs are indicated in Fig. S5†. (b) pHDependence of the rate constants
(ket) for electron transfer from QuPh_–NA to NiNPs determined from
slopes of the plots in (a).
3.5. Photocatalytic hydrogen evolution with NiNPs under
various pH conditions
The photocatalytic hydrogen-evolution experiments were per-
formed with a mixture of an aqueous buffer and MeCN [1 : 1
(v/v)] containing QuPh+–NA (0.44 mM), NADH (1.0 mM) and
NiNPs (12.5 mg L�1) under various pH conditions. Fig. 9a shows
the amount of evolved hydrogen as a function of photo-
irradiation time under the conditions of pH 4.5, 5.3, 6.0, 7.0, 8.0
and 10. When the pH of the buffer was as low as 4.5, the stoi-
chiometric amount (2.0 mmol) of hydrogen was evolved,
however, the amount of hydrogen evolved decreased with
increasing the pH. Fig. 9b plots the hydrogen-evolution rates
normalized by the weight concentration of the NiNPs against pH
values of the buffer solution. Although the concentration of
proton in the buffer solution decreases logarithmically by
increasing pH, the hydrogen-evolution rate moderately
decreased. For example, proton concentration decreases to 1/30
when pH changes from 4.5 to 6.0, whilst the hydrogen-evolution
rate at pH 6.0 maintained 1/3 of that at pH 4.5. These results also
indicate that Ni nanoparticles can catalyze H2 evolution with
little overpotential when provided with electrons of energy near
the H+/H2 couple. The standard potential for NAD+ to NADH
at pH 0 is�0.11 V vs.NHE, and this couple exhibits a 29 mV per
pH unit dependence. Thus, at pH 4, the reduction of H+ with
NADH is essentially thermoneutral and it becomes endergonic
as the pH is increased.
Fig. 10a shows the plots of the pseudo-first-order rate
constants (kobs) for electron transfer from QuPh_–NA against
weight concentrations of NiNPs at 298 K under various pH
conditions. Fig. 10b indicates the rate constant of electron
transfer from QuPh_–NA to NiNPs determined from the slope of
Fig. 10a in logarithmic scale. The small pH dependence of ketindicates that the electron-transfer process is not coupled with
proton.
Fig. 9 (a) Time courses of hydrogen evolution under photoirradiation
(l > 340 nm) of deaerated mixed solutions (2 mL) of aqueous buffers with
various pH values and MeCN [1 : 1 (v/v)] containing QuPh+–NA
(0.44 mM), NADH (1.0 mM), and NiNPs (12.5 mg L�1) at 298 K. (b)
The pH dependences of hydrogen-evolution rates (VH2) of NiNPs
(12.5 mg L�1).
This journal is ª The Royal Society of Chemistry 2012
4. Conclusions
We have revealed for the first time that Ni (non-precious metal)
nanoparticles act as an efficient catalyst for the photocatalytic
hydrogen evolution with 2-phenyl-4-(1-naphthyl)quinolinium
ion as a photocatalyst and NADH as a sacrificial electron donor.
Among metal nanoparticles (NPs) of Ni, Fe, Co and Cu, which
were examined as hydrogen-evolution catalysts in the photo-
catalytic hydrogen-evolution system, NiNPs (hcp, 6.6 nm)
exhibited the highest catalytic activity to provide the stoichio-
metric amount of hydrogen evolution. The catalytic reactivity of
NiNPs depends on both their sizes and also crystal phases. The
smaller size and hexagonal close-packed (hcp) surface are merited
for the high specific surface area and loose-packed structure
compared with the face centred cubic (fcc) structure, respectively,
leading to the high catalytic reactivity of hydrogen evolution.
Acknowledgements
This work was supported by Grants-in-Aid (20108010 and
23750014) and a Global COE Program, ‘‘The Global Education
and Research Centre for Bio-Environmental Chemistry’’, from
the Ministry of Education, Culture, Sports, Science and Tech-
nology, Japan and NRF/MEST of Korea through the WCU
(R31-2008-000-10010-0) and GRL (2010-00353) Programs. We
sincerely acknowledge the Research Centre for Ultra-Precision
Science & Technology, Osaka University, for TEM
measurements.
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