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Supplementary information for
Sustained, photocatalytic CO2 reduction to CH4 in a continuous flow reactor
by earth-abundant materials: Reduced titania-Cu2O Z-Scheme
heterostructures
Shahzad Ali a,b, Junho Lee a, Hwapyong Kim a, Yunju Hwang a, Abdul Razzaq b, Jin-Woo Jung c, Chang-Hee Cho c and Su-Il In a,d,*
a Department of Energy Science & Engineering, DGIST, 333 Techno Jungang daero,
Hyeonpung-eup, Dalseong-gun, Daegu 42988, Republic of Korea
b Department of Chemical Engineering, COMSATS University Islamabad, Lahore Campus, 1.5
KM Defense Road, Off Raiwind Road, Lahore 54000, Pakistan
c Department of Emerging Materials Science, DGIST, 333 Techno Jungang daero, Hyeonpung-
eup, Dalseong-gun, Daegu 42988, Republic of Korea
d Linde + Robinson Laboratories, California Institute of Technology, Pasadena, CA 91125, USA
*Email: [email protected]
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Fig. S1 Schematic illustration for the synthesis of RT-Cux samples (x = 0.25, 0.50, 0.60, 0.75, 0.90 and 1.00 wt. % of Cu).
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Fig. S2 XRD patterns for P25, RT and various RT-Cux samples.
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Fig. S3 (a) TEM image of overall scan for RT-Cu0.75 sample and elemental mapping of (b) Ti, (c) O, and (d) Cu within the sample.
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Fig. S4 Raman spectra of P25 and RT, with inset showing raman shift.
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Fig. S5 (a) Tauc’s plot for Band gap estimation of P25, RT and RT-Cux samples, and VB-XPS of (b) P25, (c) RT and (d) Cu2O.
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Fig. S6 XPS survey scan for (a) RT-Cu0.75 and, (b) O 1s spectra for P25 and RT.
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Coumarin dye test:[1]
Coumarin dye test aimed to detect hydroxyl radicals (•OH) was performed by mixing 50 mg of
the photocatalyst with 50 ml (2 x 10-4 M) aqueous solution of coumarin dye (Sigma Aldrich,
95% ). The resultant mixture was stirred vigorously under dark for 30 min and then illuminated
under 1 sun conditions over a period of 1 h. After that the mixture was centrifuged and 4 ml of
supernatant was further analyzed by PL spectroscopy.
Fig. S7 PL spectra for RT, and RT-Cu0.75 originating from coumarin dye test
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Fig. S8 Different control tests for photocatalytic CO2 reaction.
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Table S1 Time resolved PL decay parameter for P25, RT and RT-Cu0.75.
τ1 (ns) A1 τ2 (ns) A2 τavg (ns)
P25 0.448 289.8 3.738 118.65 1.40
RT 0.3864 196.9 3.104 93.5 1.26
RT-Cu0.75 0.2742 110 2.586 45.99 0.96
I(t) = A 1 exp (‧ ‧ -tτ1
¿+A 2 exp (‧ ‧ -tτ 2
¿ (S1)
τ avg = A 1 ‧ τ1 + A 2 ‧τ 2 (S2) A⁖ 1 +A2 = 1
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Calculations of Yield:
For a 100 ppm CH4 standard in He the yield can be calculated as,
CH 4 yield in ppm = Peak area of the CH 4 from tested samplePeak area of the standard CH 4
× 100 (S3)
CH 4 yield in µmole = [ CH4 yield in ppm ] × [ moles of the gaseous mixture containing CH4 ]
The yield in ppm can be written as,
CH 4 yield in ppm = µ mole of CH4 moles of gaseous mixture
moles of gaseous mixture = Volume of gaseous mixture ( L )Molar volume ( L mol‧ -1)
Assuming all molecules are ideal gases, at 298 K (25 ) temperature (T) and operating pressure℃
(P) of 1 atm,
Molar volume (L mol‧ -1) = R‧TP
= 0.08206 atm L mol‧ ‧ -1 K‧ -1 × 298 K1 atm
Molar volume (L mol‧ -1) = 24.45 L mol‧ -1
As one cycle is prolonged over 30 min and flow rate is set to 1.0 ml min‧ -1, thus over the course
of one cycle,
Volume of gaseous mixture ( L) = 0.030 L
Thus, in one cycle
moles of gaseous mixture = 0.030 L24.45 L mol‧ -1
= 0.0012 mol
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Thus, CH4 yield in ppm, as calculated in equation (S3), will be converted to µmole of CH4 if
multiplied by “0.0012 mol” and yield in ppm will be converted to nmole of CH4 if multiplied
with factor of “1.2”.
Calculations of AQY:
For RT-Cu0.75 [2]:
Primary product: CH4
Product yield = 77 nmol‧g-1‧h-1
Apparent Light input (H) = 1000 W‧m-2 (100 W xenon solar simulator (Oriel, LCS-100)
with an AM 1.5 filter)
Area of reactor under irradiation (A) = 0.00049 m2
Band gap (Eg) = 2.72 eV
The calculations to find the electrons, participated in photocatalytic reaction, are as follow
number of reacted electrons = [ Production rate of CH4 ] ×[electrons required per mole of CH 4 formation]× NA
As we know from balanced chemical equation, CO2 + 8H+ + 8e- → CH4 + 2H2O, 8 electrons are
consumed per mole of CH4 formed, therefore
number of reacted electrons = [77×10- 9 mol g‧ -1 h‧ -1 ]× [ 8 ] × 6.022× 1023 mol -1
number of reacted electrons = 3.71×1017 g-1 h‧ -1
Basis for calculations = 1 g
number of reacted electrons = 3.71×1017 h -1
The number of photons incident upon photocatalyst is calculated by
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number of incident photons = light absorbed by the photocatalystaverage energy of the photon
× t
Light absorbed by the photocatalyst and average energy of photon is calculated as
light absorbed by the photocatalyst = H × A = 1000 W m‧ -2 × 0.00049 m2 = 0.49 W
average energy of the photon = hcλ
Where, h is Planck’s constant (6.626x10-34 J s), c is speed of light (3x10‧ 8 m s‧ -1) and λ is the
average wavelength for the photocatalyst's absorption range.
For finding λ we calculated λmax from the band gap by the formula:
λmax = hcEg
= (6.626×10-34 J∙s ) × (3× 108 m s‧ -1 )2.72 eV
× 1 eV1.6× 10-19 J
× 109 nm m‧ -1 = 45 5 nm
Therefore, the average wavelength would be
λ = λmin + λmax
2 = 250 + 45 5
2 = 352.5 nm
The average photon energy is then computed to be
average photon energy = ( 6.626×10-34 ) × (3×108 )352.5× 10-9 m
= 5.63×10 -19 J
number of incident photons = 2.92 W5.63×10 -19 J
× 3600 s h‧ -1
number of incident photons = 3.13× 1021 h -1
AQY computation:
AQY (% ) = number of reacted electronsnumber of incident photons
× 100%
AQY (% ) = 3.71× 1017
3.13× 1021 × 100% = 0.012%
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Joule to joule computation:[3]
For calculating joule to joule efficiency, we computed the amount of the energy content
harvested after methane production,
Energy the methane possess = 810000 J mol‧ -1
Output energy as a methane formatio n = 77× 10-9 mol g‧ -1 h‧ -1 × 6 h × 0.04 g × 810000 J mol‧ -1
Output energy as a methane formation = 0.015 J
Input energy absorbed by photocatalyst = 0.49 J s‧ -1 × 21600 s = 10584 J
Joule to joule efficiency (%) = Output energy as a methane formationInput energy absorbed by photocatalyst
× 100%
Joule to joule efficiency (%) = 0.015 J10584 J
× 100% = 0.00014%
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Table S2 Photocatalytic CH4 yield from CO2 reduction employing P25, RT and RT-Cux samples
with corresponding A.Q.Y and joule to joule efficiency.
Sample Name CH4 Yield ( nmol g‧ −1 h‧ −1) Joule to Joule Efficiency AQY (%)
P25 0 - -
RT 7.3 0.13 x 10-4 0.001
RT-Cu0.25 12.6 0.23 x 10-4 0.002
RT-Cu0.50 36.9 0.68 x 10-4 0.006
RT-Cu0.60 52.4 0.96 x 10-4 0.008
RT-Cu0.75 77.0 1.41 x 10-4 0.012
RT-Cu0.90 52.9 0.97 x 10-4 0.008
RT-Cu1.00 28.1 0.52 x 10-4 0.004
RTs-Cu0.75 32.9 0.60 x 10-4 0.005
RTh-Cu0.75 18.9 0.35x 10-4 0.003
P25-Cu0.75 15.3 0.28 x 10-4 0.003
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Table S3 Comparison of the photocatalytic activities for the Cu based photocatalysts reported in
literature.
Photo catalyst
Composition of Photocatalyst and Synthesis Method
Light Source, Reaction Conditions
Product Yield
Cu/TiO2
[4]1% Cu/TiO2 Precipitation-calcination and then H2 pretreatment
Continuous mode, catalyst weight 50 mg, moist CO2 at flow of 2 ml min‧ -1 for 6.5 hLight Source: 150 W solar simulatorLight intensity: 90 mW cm‧ -2
Room temperatureStability not reported
CH4 4.0 μmol g‧ −1
CO 25 μmol g‧ −1
Cu2O/ TiO2
[5]0.03 wt.% Cu/TiO2
Sol–gelBatch mode in liquid water for1.5 hStability not reported
CH4 36 nmol g‧ −1
Cu/TiO2 [6] 1.2% Cu/TiO2
Thermal hydrolysisTiO2-coated optical fiberCO2 and H2O feed mixture with partial pressure of 1.19 and 0.03 bar, respectively, at 75 °C and wavelength of 365 nm
CH4 5.2-5.5 μmol g‧ −1
CuO/TiO2
Cu2O/TiO2
Hollow Microspheres [7]
One-pot template-free
Batch reactor10 mgHg UV lamp (40 W; 254 nm; lightintensity at the location of the catalyst: 20 mW cm‧ −2
CH4 2.1μmol g‧ −1 h‧ −1
CO 14.5 μmol g‧ −1 h‧ −1
H2 2.8 μmol g‧ −1 h‧ −1
Cu/TiO2 [8] 1% Cu/TiO2
Impregnation method
Batch reactor210 min450 W Xe lampUnder UV-vis light irradiationStability not reported
CH4 4.4 μmol g‧ −1
CO 25 μmol g‧ −1
Cu2O−TiO2
[9]5.0 wt.% of Cu pre-cursorSolvothermal process
Batch reactor, catalyst weight 30 mg, 20 °C and light source is Xe arc lamp λ ≥ 305 nm. Testing for 4 cycles (1 h each)
CO 2.11 μmol g‧ −1 h‧ −1
Silica supported
0.5% Cu/TiO2–SiO2
one-pot sol–gel Continuous mode with light source of Xe arc lamp
CH4 10 μmol g‧ −1 h‧ −1
CO 60 μmol g‧ −1 h‧ −1
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Cu/TiO2 [10] method 2.4 mW cm‧ -2 for 250 nm < λ < 400 nmStability not reported
CuxO−TiO2
[11]Thermal decomposition and calcination
Batch reactorStability not reported
CH4 221.63 ppm g‧ −1
·h−1
Cu/TiO2 [12] 3.0 wt.% Cu/TiO2 Continuous mode at 100 °C with light source of 200 W Hg reflector lamp 150 mW‧cm-2, λ = 254 nm.Stability not reported
CH4 4.20 μmol g‧ −1 h‧ −1
CO 763 μmol g‧ −1 h‧ −1
CuO−TiO2
[13] -
300 W Xe lamp (AM 1.5 filter), 100 mW cm−2
100 mgStability not reported
CH4 26.2 ppm g−1 h‧ −1
Cu/mTiO2
(mesoporus)
[14]
solvothermal
Batch mode, catalyst weight 20 mg, moist pure CO2 at 25 °C for 24 h300 W Xe lamp (AM 1.5 filter), 0.8 mW cm−2
Stability for 5 cycles (10 h), also it decreased after 2nd
cycle
CH4 4.5 μmol g‧ −1 h‧ −1
CO 1.0 μmol g‧ −1 h‧ −1
H2 0.75 μmol g‧ −1 h‧ −1
RT/Cu2O
(This work)
0.75 wt.% of CuCombination of thermochemical reduction and photodeposition
CO2 (moist) 1000 ppm in He at flow rate of 1.2 ml‧min−1, 40 mg catalystAt ambient temperaturefor 6 h irradiation in continuous flow reactor with 100WXe solar simulator with an AM 1.5 filter;100 m W cm‧ -2
Stability 42 h
CH4 77 nmol g‧ −1 h‧ −1
17
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