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Electronic Supplementary Information
Plasmonic hot carrier-driven oxygen evolution reaction on Au
nanoparticles/TiO2 nanotube arrays
Song Yi Moona,b, Hee Chan Songb,c, Eun Heui Gwagb,c, Ievgen I. Nedrygailovb,
Changhwan Leeb,c, Jeong Jin Kimb, Won Hui Dohb and Jeong Young Park*,a,b,c
a Department of Chemistry, Korea Advanced Institute of Science and Technology (KAIST),
Daejeon 34141, Republic of Korea b Center for Nanomaterials and Chemical Reactions, Institute for Basic Science (IBS),
Daejeon 34141, Republic of Korea
c Graduate School of EEWS, Korea Advanced Institute of Science and Technology (KAIST),
Daejeon 34141, Republic of Korea
*To whom correspondence should be addressed. E-mail: [email protected]
KEYWORDS: surface plasmon resonance, hot electron, Schottky barrier, oxygen evolution
reaction, solar water splitting, nanostructure
Electronic Supplementary Material (ESI) for Nanoscale.This journal is © The Royal Society of Chemistry 2018
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Figure S1. Au particle size distributions on the titania nanotube arrays (TNAs). Scanning electron
microscopy images and corresponding histograms showing the size distributions of the Au
nanoparticles (NPs) on the surface of the TNAs for (a,b,c) 29 nm Au NPs, (d,e,f) 14.9 nm Au NPs,
and (g,h,i) 4.9 nm Au NPs.
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Figure S2. (a) High-angle annular dark-field scanning transmission electron microscope (HAADF-
STEM) image showing the 5 nm Au NPs@TNAs. (b) High-resolution transmission electron
microscope (HRTEM) image obtained at the interface between the Au NPs and the TiO2. (c)
Energy dispersive spectroscopy (EDS) spectrum of a 5 nm Au NPs@TNAs (2.67 wt%) sample
showing the presence of Au.
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Figure S3. X-ray diffraction (XRD) patterns for the 5 nm Au NPs@TNAs. The XRD pattern for Ti foil
is also shown for reference.
20 30 40 50 60 70 80
5 nmAu NPs@TNAs
TNAsAu
(200
)A(
200)
A(00
4)
A(20
4)
A(21
1)A(
105)
Au(2
20)
A(21
5)Ti
(112
)
Ti(1
03)
Ti(1
10)
Ti(1
02)
Ti(1
01)
Au(1
11)
A(10
3)
A(10
1)
Inte
nsity
(a.u
.)
2 theta (degree)
Ti foil
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Figure S4. Optical properties of the Au NPs@TNAs. (a) UV–vis absorption spectra of the Au
nanoparticles. (b) UV–vis absorption spectra of the 5, 15, and 30 nm Au NPs@TNAs calculated
using the relation %A = 100 − (%T + %R).
%A =100-(%
T + %R
)
400 450 500 550 600 650 7000.0
0.2
0.4
0.6
0.8
1.0
1.2
528nm
524nm
Abso
rban
ce (a
.u.)
Wavelength (nm)
5 nm Au NPs 15 nm Au NPs30 nm Au NPs
520nm
(a) (b)
300 400 500 600 700 8000
20
40
60
80
10030 nm Au NPs@TNAs15 nm Au NPs@TNAs 5 nm Au NPs@TNAs TNAs
Wavelength (nm)Ab
sorp
tion
(%)
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Figure S5. Optical properties of the Au NPs@TNAs. (a) Transmission spectra and (b) UV–vis
absorption spectra of the 5, 15, and 30 nm Au NPs@TNAs.
300 400 500 600 700 8000
20
40
60
80
100
Tran
smiss
ion
(%)
Wavelength (nm)
30 nm Au NPs@TNAs 15 nm Au NPs@TNAs 5 nm Au NPs@TNAs
300 400 500 600 700 8000
20
40
60
80
100
Wavelength (nm)
Refle
ctio
n (%
)
30 nm Au NPs@TNAs 15 nm Au NPs@TNAs 5 nm Au NPs@TNAs
(a) (b)
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Figure S6. TEM characterization with Au loading dependence. TEM images of the 5 nm Au
NPs@TNAs electrode with gold loading between 0.52 and 4.75 wt%.
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Figure S7. Photoelectrochemical performance with the optimum loading amount of Au. (a) Linear
sweep voltammetry of the Au NPs@TNAs electrodes with different gold loading under white light
illumination. (b) Photocurrent density as a function of gold loading for the Au NPs@TNAs
electrodes under white and visible light illumination.
0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.40.0
0.5
1.0
1.5
2.0
Curre
nt d
ensit
y (m
A/cm
2 )
Potential (V vs RHE)
TNAs Au NPs@TNAs (0.52 wt%) Au NPs@TNAs (1.29 wt%) Au NPs@TNAs (2.67 wt%) Au NPs@TNAs (4.75 wt%)
(a) (b)
0 1 2 3 4 5
0.5
1.0
1.5
2.0
2.5
3.0
Phot
ocur
rent
den
sity
(mA/
cm2 )
Under white light Under visible light
0
50
100
150
200
Amount of Au loading (wt%)
Pho
tocu
rrent
den
sity
(μA/
cm2 )
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Calculation of Decay Lifetime. The decay lifetime can be calculated by fitting the V–t curves to a
biexponential function () = + / + / and the harmonic mean of the
lifetime (τm) is obtained by = ()/( + ) . Finally, the total lifetimes estimated by log(2
x τm) of the bare TNAs, 30 nm Au NPs@TNAs, 15 nm Au NPs@TNAs, and 5 nm Au NPs@TNAs are
0.68, 0.63, 0.49, and 0.27 s, respectively.
Figure S8. Photovoltage–time spectra collected for (a) bare TNAs and (b) 30nm Au NPs@TNAs,
(c) 15nm Au NPs@TNAs, and (d) 5nm Au NPs@TNAs.
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Figure S9. Calculation of the Schottky barrier height. Fitting of the experimental current–voltage
curves to the thermionic emission equation for (a) 40 nm Au NPs@TNAs and (b) 76 nm Au
NPs@TNAs.
(a) (b)
0.0 0.5 1.0 1.5 2.00
10
20
30
Current Fitting Line
Curre
nt (p
A)
Tip Bias (V)0.0 0.5 1.0 1.5 2.0
0
5
10
15
20
Current Fitting Line
Curre
nt (p
A)Tip Bias (V)
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Figure S10. Ultraviolet photoelectron spectroscopy (UPS) spectra. (a) Valence band edges from
the Au NPs@TNAs. (b) Secondary electron emission spectra observed for 130 eV photons incident
on the Au NPs@TNAs.
7 6 5 4 3 2 1 0 -1
Inte
nsity
(a.u
.)
VBm= 3.23 eV
Binding energy (eV)
TNAs
30 nm Au NPs@TNAs
15 nm Au NPs@TNAs
5nm Au NPs@TNAs
VBm= 3.16 eV
VBm= 3.03 eV
VBm= 2.94 eV
48.6 48.8 49.0 49.2 49.4 49.6
Inte
nsity
(a.u
.)
Binding Energy (eV)
5 nm Au@TNAs15 nm Au@TNAs30nm Au@TNAs TNAs
hλ= 130 eVBias = -5.0 V
(a)
(b)
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Finite-Difference Time-Domain (FDTD) Simulation. The FDTD simulation model was based on
TEM images (Figure S2). All the simulations were carried out in three spatial dimensions that are
periodic in the x- and y-directions and the perfectly matched layer (PML) was used in the z-
direction. The incident light was a plane wave at 537 nm, which is the wavelength of the strongest
LSPR excitation.
Figure S11. Electric field distribution formed at the Au NPs@TNAs. The gold nanoparticle sizes
are (a) 5, (b) 15, and (c) 30 nm. The field images are a cross-section of the Au NPs@TNAs and are
output from the FDTD simulation.
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Table S1. Atomic weight percentage of Au in the EDX and XPS spectra.
Au wt % on TiO2 30 nm Au NPs @TNAs
15 nm Au NPs @TNAs
5 nm Au NPs @TNAs
EDX - Au (L) % 12.095±0.40 3.761±0.14 1.294±0.25
XPS - Au (4f) % 14.863±0.85 4.367±0.43 1.49±0.16 (Amount of Au loading was analyzed at several different spots in the sample)
Table S2. Parameters obtained from fitting the thermionic emission equation to current–voltage
(I–V) curves measured on the plasmonic Au NPs@TNAs.
Au NPs diameter (nm)
SBH (φb) Ideal factor (η)
20 0.565 eV 11.9 23 0.52 eV 12 25 0.579 eV 9.2 31 0.571 eV 7.5 35 0.577 eV 7.8 40 0.593 eV 6.32 49 0.64 eV 5.07 58 0.70 eV 4.3 60 0.715 eV 3.7 70 0.73 eV 3.8 75 0.76 eV 2.5