DOI:
10.1039/C8RA00690C
(Paper)
RSC Adv., 2018,
8, 13898-13909
Environmentally sustainable biogenic fabrication of AuNP decorated-graphitic g-C3N4 nanostructures towards improved photoelectrochemical performances†
Received
23rd January 2018
, Accepted 8th April 2018
First published on 16th April 2018
Abstract
Noble-metal gold (Au) nanoparticles (NPs) anchored/decorated on polymeric graphitic carbon nitride (g-C3N4), as a nanostructure, was fabricated by a simple, single step, and an environmentally friendly synthesis approach using single-strain-developed biofilm as a reducing tool. The well deposited/anchored AuNPs on the sheet-like structure of g-C3N4 exhibited high photoelectrochemical performance under visible-light irradiation. The Au-g-C3N4 nanostructures behaved as a plasmonic material. The nanostructures were analyzed using standard characterization techniques. The effect of AuNPs deposition on the photoelectrochemical performance of the Au-g-C3N4 nanostructures was examined by linear sweep voltammetry (LSV), electrochemical impedance spectroscopy (EIS), incident photon-to-current efficiency (IPCE) and cyclic voltammetry (CV) in the dark and under visible-light irradiation. The optimal charge transfer resistance for Au-g-C3N4 nanostructures (6 mM) recorded at 18.21 ± 1.00 Ω cm−2 and high electron transfer efficiency, as determined by EIS. The improved photoelectrochemical performance of the Au-g-C3N4 nanostructures was attributed to the synergistic effects between the conduction band minimum of g-C3N4 and the plasmonic band of AuNPs, including high optical absorption, uniform distribution, and nanoscale particle size. This simple, biogenic approach opens up new ways of producing photoactive Au-g-C3N4 nanostructures for potential practical applications, such as visible light-induced photonic materials for real device development.
1. Introduction
Green chemistry focuses mainly on the reduction, recycling or removal of toxic and hazardous chemicals in various fabrication processes by finding creative, alternative routes for producing the desired products with a less adverse impact on the environment and human health. Green chemistry is a more eco-friendly green alternative to conventional chemistry practices.1 The development of environmentally friendly methodologies in material synthesis is of great importance to expand their visible light-induced applications in electrochemical analysis.2,3 Currently, noteworthy research efforts have been devoted to the realization of efficient, economical, and green sources for the fabrication of nanoparticles with a well-defined chemical composition, size, and morphology for applications in many cutting-edge technological areas.4–7 Single strain developed biofilms is one of the positive hopes for the fabrication of carbon-based metal nanostructures.8 In general, biofilms form on solid surfaces by different kinds of micro-organism for their mutual benefits. Here, a biofilm was developed using a single strain Shewanella oneidensis, which is an electrochemically active microorganism that can be used to control reactions in a range of fields, such as chemical/biological synthesis and bioremediation.8,9 Nanoparticles of noble metals, such as Au, Ag, Pt, and Pd can strongly absorb visible light from the solar spectrum10,11 owing to their special effect of surface plasmon resonance (SPR), which can be adjusted by varying their size and shape.12–15 The size and shape-dependent optical and electronic properties of metal nanoparticles have made them attractive for interfacial charge transfer in semiconductor–metal nanostructures.14,16,17 Plasmonic AuNPs work as a visible light absorber and a thermal redox active center.18–21 Considering the advantages of AuNPs, it is probable that the photoelectrochemical performance of g-C3N4 can be improved further after the successful anchoring of AuNPs.22 Polymeric graphitic carbon nitride (g-C3N4) with a band gap of 2.7 eV and long range π–π conjugation is a stable allotrope with a stacked two-dimensional structure under ambient conditions.23–25 Compared to its inorganic semiconductor counterparts, g-C3N4 is a sustainable and environmentally friendly organic semiconductor material that consists of carbon and nitrogen, which are among the most abundant elements on Earth. Since Wang et al. first reported that novel molecular photo-based material g-C3N4 nanostructures exhibited photoactivity for H2 production, considerable efforts have been made to synthesize g-C3N4 through the heat treatment of numerous nitrogen-rich organic precursors.26,27 Metal-free π-conjugated g-C3N4 nanostructures have interesting electronic properties as well as high thermal and chemical stability, making them valuable materials for visible light-driven electrochemical analysis.26,28–30
In the present study, a novel, simple and biogenic/green synthesis approach was applied for the fabrication of Au-g-C3N4 nanostructures. The successful anchoring of AuNPs onto the sheet-like structure of g-C3N4 was optimized using HAuCl4 precursor (1 mM, 3 mM, and 6 mM), and it was found that anchoring with up to 6 mM of AuNPs resulted in improved photoelectrochemical performance. The effects of small amounts of AuNPs (1 mM, 3 mM, and 6 mM) anchored successively onto sheet-like structures of g-C3N4 to improve the visible-light absorption performance and separate the photogenerated electron–hole pairs were studied. The as-fabricated nanostructures exhibited improved photocurrent performance under the visible-light irradiation. The photoelectrochemical performance was tested based on the SPR effects of AuNPs, lower band gap energy, low photoluminescence intensity, excellent visible-light absorption, and superior photocurrent generation. The charge transfer properties in the Au-g-C3N4 nanostructures highlight its potential as good quality plasmonic-based electronic material for energy storage and conversion applications for real device fabrication.
2. Experimental section
2.1. Materials
Hydrogen tetrachloroaurate(III) hydrate (HAuCl4·nH2O; n = 3.7) from Kojima Chemicals, Japan. Urea (98.0%), ethyl cellulose, and α-terpineol (C10H18O) were acquired from KANTO Chemical Co., Japan. Sodium acetate (CH3COONa) and sodium sulfate (Na2SO4) were obtained from Duksan Pure Chemicals Co. Ltd., South Korea. Fluorine-doped transparent conducting oxide glass (FTO; F-doped SnO2 glass; 7 Ω sq−1) was acquired from Pilkington, USA. The bacterial culture medium was purchased from Becton Dickinson and Company (NJ, USA). All other chemicals were of analytical grade and used as received. The solutions were prepared from DI water obtained using a PURE ROUP 30 water purification system.
2.2. Methods
X-Ray diffraction (XRD, PANalytical, X'pert-PRO MPD) was performed using Cu Kα radiation (λ = 0.15405 nm). The diffuse absorbance/reflectance ultraviolet-visible spectra (DRS) of the powder pure g-C3N4 and Au-g-C3N4 nanostructures samples were obtained using an ultraviolet-visible-near infrared (UV-VIS-NIR) double beam spectrophotometer (VARIAN, Cary 5000, USA) equipped with a diffuse reflectance accessory. A given amount of the g-C3N4 and Au-g-C3N4 nanostructure powder was pressed uniformly in the sample holder, which was then placed at the integrating sphere for the absorbance/reflectance measurements. The photoluminescence (PL, Kimon, 1 K, Japan) of the samples was recorded over the scanning range, 300–800 nm, using an excitation wavelength of 325 nm. The BET specific surface area of the samples was measured using a Belsorp II-mini (BEL, Japan Inc.). The microstructure was examined by field emission transmission electron microscopy (FE-TEM, Tecnai G2 F20, FEI, USA) operating at an accelerating voltage of 200 kV. Selected-area electron diffraction (SAED) and high angle annular dark field (HAADF) observations were carried out on the same transmission electron microscope. Quantitative analysis was performed by energy dispersive spectrometry (EDS) attached to the transmission electron microscope. X-ray photoelectron spectroscopy (XPS, ESCALAB 250 XPS System, Thermo Fisher Scientific U.K.) was conducted using the following X-ray source: monochromated Al Kα radiation, hν = 1486.6 eV; X-ray energy, 15 kV; 150 W; spot size, 500 μm; take-off angle, 90; pass energy, 20 eV; BE resolution, 0.6 eV (calibrated using Ag 3d5/2) at the Center for Research Facilities, Yeungnam University, South Korea. XPS fitting was done using “AVANTAGE” software by a Shirley subtraction and the shape of the peaks used for the deconvolution was Gaussian–Lorentzian shapes. The sensitivity factor used for Au 3d5 was 30.5.
Photoelectrochemical analyses, such as linear sweep voltammetry (LSV), electrochemical impedance spectroscopy (EIS), and cyclic voltammetry (CV), were performed using a potentiostat (Versa STAT 3, Princeton Research, USA) comprised of a standard three-electrode system. Ag/AgCl (3 M KCl), a Pt gauge, and FTO glass coated with the pure g-C3N4 and Au-g-C3N4 nanostructures were used as the reference, counter and working photoelectrode, respectively. The experiment LSV and EIS were performed in a 0.2 M sodium sulphate (Na2SO4) solution as the supporting electrolyte at room temperature and CV was performed in a 0.2 M phosphate buffer solution (pH 7; 0.2% PBS). The projection area of the photoelectrode was 1 cm2. The working electrodes were prepared as follows: 100 mg of each sample was mixed thoroughly by adding ethyl cellulose as a binder and α-terpineol as the solvent. The mixture was stirred and heated on a hot plate with a magnetic stirrer until a thick paste was obtained. The paste obtained was then coated on a FTO glass substrate using the doctor-blade method and kept drying overnight under a 60 W lamp; the electrode was later used as a photoelectrode for the photoelectrochemical measurements.
2.3. Development and fabrication of single strain biofilm on carbon foam
Carbon foam was prepared using a melamine sponge (Dae Han Co. Ltd, Korea) as the template.31 The biofilm on the carbon foam was prepared using the procedure reported elsewhere.21,32 Carbon foam (without wet proof, Fuel Cell Earth LLC) with a size of 2.5 × 4.5 cm2 was used as an anode electrode instead of carbon paper. In the anode chamber, Luria Broth (LB) medium was inoculated with overnight cultures of Shewanella oneidensis at a ratio of 1:100. The LB media was purged with N2 gas for 10 min to remove the environmental oxygen and maintain the anaerobic conditions. The fully developed biofilm on the carbon foam was confirmed using a microbial fuel cell by obtaining the appropriate voltage. The living biofilm formed on the carbon foam specimens was used to synthesize the series of Au-g-C3N4 nanostructures.
2.4. Single strain developed biofilm synthesis of Au-g-C3N4 nanostructures (1 mM, 3 mM and 6 mM)
Graphitic g-C3N4 was prepared using a facile single pot method by the modest heating of urea at 550 °C in a muffle furnace for 4 h with a ramping rate of 20 °C min−1 under air flow conditions. The resulting material was then naturally cooled to room temperature, the whitish yellow color powder was extract as a sheet-like structure of pure g-C3N4 (ref. 33 and 34) (Scheme 1).
|
| Scheme 1 Projected schematic model for the biogenic synthesis of the Au-g-C3N4 nanostructures using an environmentally friendly approach. | |
Three setup arrangements of 200 mL of aqueous suspensions of pure g-C3N4 and 1 mM, 3 mM, and 6 mM Au3+ were prepared. The mixture of pure g-C3N4 and HAuCl4 (Au3+ ions) was stirred for 15 min to allow the adsorption of Au3+ ions onto the sheet-like g-C3N4 structure. Subsequently, the optimal amount of sodium acetate (0.2 g) was added individually to the suspension as an electron contributor. The reaction mixtures were sparged with nitrogen (N2) gas for 5 min to sustain an anaerobic environment. The single strain developed biofilm were hung individually in a reaction bottle and the setup was sealed and left for magnetic stirring at 30 °C. The reaction mixture setups were stirred for a further 6 h to complete the reaction. In each case, the initial white color changed to a dark pink color within 30 min, which was the sign of the reduction of Au3+ to Au0. Finally, purple to light purple precipitates were obtained in the 1 mM, 3 mM, and 6 mM HAuCl4 cases, respectively. The reaction mixtures were centrifuged and the powdered Au-g-C3N4 nanostructures were isolated for further characterization and photoelectrochemical studies.
Two precise syntheses were performed to examine the role of the single strain developed biofilm and sodium acetate. Two 5 mM g-C3N4 aqueous suspensions (200 mL) were prepared. In the first controlled synthesis, an aqueous solution containing a 0.2 g sodium acetate and 1 mM HAuCl4 was added. In the second controlled synthesis, only a 3 mM HAuCl4 aqueous solution was added. Both reaction mixtures were sparged with N2 gas for 5 min to sustain the anaerobic environment. The developed biofilm were hung in the second controlled synthesis only. Both systems were sealed and stirred with a magnetic stirrer at 30 °C. No variations were detected, even after 48 h. These long-established reaction steps confirmed that the biofilm and sodium acetate are essential to complete the synthesis of the Au-g-C3N4 nanostructures.
2.5. Photoelectrochemical studies of pure g-C3N4 and Au-g-C3N4 nanostructures as a photoelectrode performance
The photoelectrochemical performance of the pure g-C3N4 and Au-g-C3N4 nanostructures was examined by LSV, EIS and CV under ambient conditions in the dark and under visible light irradiation. The LSV and EIS experiments were performed in 50 mL of an aqueous 0.2 M Na2SO4 solution in the dark and under visible light irradiation at room temperature. The photocurrent response was examined by LSV in the dark and under visible light irradiation at a scan rate of 50 mV s−1 over the applied potential range, −1.0 to 1.0 V. EIS which were conducted using a 400 W lamp under visible light irradiating intensity of 31.0 mW cm2 (3M, USA) with frequencies ranging from 1 to 104 Hz at 0.0 V vs. Ag/AgCl in potentiostatic mode. The CV experiments were conducted in 50 mL of 0.1 M PBS (phosphate buffer solution) in the dark and under visible light irradiation. CV analysis was performed at a scan rate of 50 mV s−1. The incident photon-to-current efficiency (IPCE), used to investigate the photoresponsivity of nanostructures using the xenon lamp with specific wavelength filters to select the required wavelength of light.
3. Results and discussion
3.1. Standard characterization of pure g-C3N4 and Au-g-C3N4 nanostructures
3.1.1. Structural, purity and phase confirmation analysis of pure g-C3N4 and Au-g-C3N4 nanostructures. X-Ray diffraction was performed to explore the crystal structure, phase, and purity of pure g-C3N4, as shown in Fig. 1(a). The XRD pattern of pure g-C3N4 showed two peaks at 13.1° and 27.3° 2θ. The small peak at 13.1° 2θ was assigned to the (100) plane with d = 0.676 nm and the other strong peak at 27.3° 2θ corresponded to d = 0.324 nm due to the long-range interplanar stacking of the aromatic arrangement and it is recognized as the (002) plane of pure g-C3N4 (JCPDSD 87-1526).35 Additionally, the two additional weak diffractions peaks appeared at ∼43° and ∼58° which can be attributed to the planes of graphitic carbon nitride. This outcome from the denser packing or a distortion of the mesopores structure in which every second the arrangement of mesopores sheet is displaced.36 Notably, the mentioned peaks were disappeared in case of 3 mM and 6 mM while small peak appeared in case 1 mM because there was small concentration of Au ions.
|
| Fig. 1 Representative XRD patterns of (a) pure g-C3N4, (b, c and d) 1 mM, 3 mM and 6 mM of Au-g-C3N4 nanostructures. | |
In the case of (1 mM, 3 mM and 6 mM) of AuNPs-decorated g-C3N4 samples, the XRD patterns revealed four separate reflections at 38.1° (111), 44.4° (200), 64.8° (220) and 77.6° (311) for the AuNPs, in addition to the peaks for g-C3N4. The observed reflections were well matched with the AuNPs in the prepared nanostructures corresponding to the reported JCPDS values (04-0784).37 The intensity of the peaks for the AuNPs increased gradually with increasing loading of Au3+ ions onto the sheet-like structure of g-C3N4. The four peaks confirmed the anchoring of AuNPs onto the g-C3N4 surface, which was clearly absent in the pure g-C3N4 sample; no other extra/impurity peaks were found in the as-fabricated samples. The presence of both Au planes and g-C3N4 confirmed the successful formation of the Au-g-C3N4 nanostructures using the green/biogenic synthesis approach.
The mean crystallite size of the g-C3N4 and Au-g-C3N4 nanostructures were calculated using the Scherrer's formula,
|
D = κλ/βcosθ
| (1) |
where
κ is the shape factor and has a typical value of ∼0.9,
λ is the wavelength (Cu Kα = 0.15405 nm),
β is the full width at half maximum of the most intense peak (in radians), and
θ is the main peak of g-C
3N
4, which was observed at 27.43° 2
θ. The calculated crystallite size of bare g-C
3N
4 from the most intense peak at 27.43° 2
θ was 6.6 nm and the calculated crystallite size of the Au-g-C
3N
4 nanostructures from the most intense peak was 12.2, 22.9, and 27.9 nm, respectively. This shows that the crystallite size of the Au-g-C
3N
4 nanostructures increased because of the anchoring of AuNPs on to the g-C
3N
4 sheets compared to pure g-C
3N
4. These increased crystallite values further confirmed the successful fabrication of the Au-g-C
3N
4 nanostructures.
3.1.2. Optical and photoluminescence analysis of pure g-C3N4 and Au-g-C3N4 nanostructures. Fig. 2(a and b) shows the optical absorbance and photoluminescence analysis of the pure g-C3N4 and Au-g-C3N4 nanostructures. The present spectrum showed a high absorbance value in the range, 475–525 nm, because of the SPR band characteristics of the AuNPs, which showed that the AuNPs had been anchored successfully onto the g-C3N4 samples and showed the improved visible light absorption of AuNPs.38,39 In addition to the confinement effect, the interparticle coupling contributes to the SPR broadening of AuNPs decorated g-C3N4 nanostructures as well. It is due to the particle interactions which increase in local field fluctuations, giving rise to an extensive range of photon energies for plasmon resonance to take place.17 From the absorbance spectra in Fig. 2(a), there was a red shift in the absorbance band of the Au-g-C3N4 nanostructures compared to that of pure g-C3N4. The inset in Fig. 2(a) shows that the AuNPs decorated onto g-C3N4, in the 1 mM sample displayed a purple color, which was a clear indication of the successful reduction of Au3+ to Au0 and the fabrication of AuNPs. Fig. S1† presents the typical reflectance spectra from 360–780 nm wavelengths, showing improved reflectance in the case of the Au-g-C3N4 nanostructures, which further confirmed the successful formation of Au-g-C3N4 nanostructures.
|
| Fig. 2 (a) UV-Vis absorbance spectra, and (b) photoluminescence spectra of pure g-C3N4 and Au-g-C3N4 nanostructures. | |
Fig. 2(b) shows the photoluminescence (PL) spectra of the pure g-C3N4 and Au-g-C3N4 nanostructures. These spectra are very helpful for examining the migration, transfer of charge carriers, and separation and recombination processes of the photogenerated electron–hole pairs.13,18 The PL intensity is exceedingly reliant on the electron–hole pair recombination processes. The PL intensity is dependent on electron–hole pair recombination processes. The as-fabricated pure g-C3N4 and Au-g-C3N4 nanostructures materials showed only one type of PL intensity in the recorded spectra. The broad luminescence peak at 455 nm was assigned to the band–band PL phenomenon with a light energy approximately equal to the band gap energy of the g-C3N4 and Au-g-C3N4 nanostructures for the photoelectrode performance.13,40 As the PL intensity is inversely related to the charge recombination between the photogenerated electron–hole pairs, the anchoring/decoration of the AuNPs onto the sheet-like structure of g-C3N4 could prevent charge recombination between the opposite charge carriers, leading to improved photoelectrochemical performance.40,41 The overall PL studies of the Au-g-C3N4 nanostructures clearly showed higher charge transfer ability, which could be responsible for the improved photoelectrochemical performance. On the other hand, the inset in Fig. 2(b) shows that there is no shift in the emission wavelength of 455 nm. In addition, two emission centers were observed in the shorter excitation wavelength (436.0 nm and 458.8 nm) which was in contrast to that observed for longer excitation wavelengths. The PL intensity decreased gradually with increasing wavelength as the corresponding excitation energy is reduced in the case of (1 mM to 6 mM) of Au-g-C3N4 nanostructures.
3.1.3. High resolution transmission electron microscopy (HR-TEM) image of pure g-C3N4 and Au-g-C3N4 nanostructures. The surface structures, morphology, and particle size of the as-fabricated samples Au-g-C3N4 nanostructures were investigated by TEM and HR-TEM. As shown in Fig. 3(a), the particles with a dark color can be assigned to AuNPs and the sheet like gray color area was assigned to the sheet-like structure of g-C3N4. The as-synthesized Au-g-C3N4 nanostructures displayed a sheet like morphology with a few layered structures. The sheets consisted mainly of graphitic planes with a conjugated aromatic system.13 The flat surface of the g-C3N4 sheet acts as a visible-light absorber. The TEM images (a, b and c) show that the number of AuNPs increases with increasing concentration of the Au precursor. The SAED pattern of the nanostructure showed a series of bright concentric rings, suggesting that the as-fabricated sample is polycrystalline in nature (inset of Fig. 3(a–c)).
|
| Fig. 3 (a, b and c) TEM images of the 1 mM, 3 mM, and 6 mM of Au-g-C3N4 nanostructures shows the uniform presence of AuNPs onto g-C3N4 (the inset shows the SAED crystal ring pattern); (d) HR-TEM image showing the interface between the AuNPs and g-C3N4, lattice fringes of AuNPs onto the g-C3N4; (e, f and g), showing elemental mapping of C (yellow color), N (green color), and Au (metallic gold color); (h) shows the elemental composition of the Au-g-C3N4 nanostructures. | |
The mean diameter of the AuNPs was in the range, 12–15 nm, and the nanoparticles were clearly attached to the surface and edges of the g-C3N4 sheet. Fig. 3(d) clearly showed the interfacial interaction of AuNPs with the sheet-like structure of g-C3N4, which also covered the intact surface area of the sheet uniformly. The lattice fringes of the Au 0.23 nm (111) plane for metallic Au indicated the crystalline behavior of the samples, which further confirmed the presence of the AuNPs and the good interaction at the interface of the g-C3N4 sheet. The elemental mapping presented in Fig. 3(e, f and g) shows C (yellow), N (green), and Au (metallic gold), which provides strong evidence for the existence of carbon, nitrogen, and AuNPs anchored successfully onto the sheet-like structure of g-C3N4. Fig. 3(h) shows the elemental composition of the Au-g-C3N4 nanostructures without any other elemental peak. Fig. S2(a–d)† presents HR-TEM images of the Au-g-C3N4 nanostructures. The average particle size distribution graph of Fig. S3(a–c)† screening the average particle size is ranging between 12–15 nm.
3.1.4. XPS of pure g-C3N4 and Au-g-C3N4 nanostructures. XPS is a surface-specific characterization tool that can be used to confirm the chemical environment and elemental oxidation state. XPS was carried out on the pure g-C3N4 and Au-g-C3N4 nanostructures in the region, 0–1000 eV (Fig. 4). Consequently, XPS was used to determine the formal oxidation state of all the elements present in the pure g-C3N4 and Au-g-C3N4 (1 mM, 3 mM, and 6 mM). Fig. 4(a) displayed the elemental composition of pure g-C3N4, in which two major peaks were assigned to C and N and a small peak for oxygen at ∼531 eV, which might be some hydroxyl groups (–OH) attached to the surface of g-C3N4. No impurity peak was observed.42 The survey scan spectrum (Fig. 4(b)) of Au-g-C3N4 confirmed the presence of an Au peak at ∼84 eV along with C and N, which verified the successful attachment of AuNPs onto the sheet-like structure of g-C3N4.41
|
| Fig. 4 (a and b) XPS survey scan spectra of pure g-C3N4 and Au-g-C3N4 nanostructures, (c, d and e) fitted spectra of C 1s, N 1s and Au 4f, and, (f) combined spectra of pure g-C3N4 and Au-g-C3N4 nanostructures. | |
The C 1s peaks were observed at 285 eV and 288.3 eV (Fig. 4(c)),42 which were assigned to the sp2-hybridized carbon atom and the carbon atom bonded to three nitrogen atoms –C(N3) of g-C3N4, respectively. The broad fitted peak of N 1s was observed at 398.5 eV (Fig. 4(d)),43 which were assigned to the nitrogen atom bonded to two carbon atoms (C–N–C) and the other small fitted peaks were attributed to nitrogen atoms bonded to the environment of three carbon atoms N–(C3) and to N–H bonding, respectively.43 The fitted spectrum of Au 4f (Fig. 4(e)) showed two peaks at 84.19 eV and 87.87 eV, which originated from the Au 4f7/2 and 4f5/2 electrons of the metallic behavior of gold.41,44 Therefore, the Au3+ ions were reduced to the Au0 oxidation state on the sheet like surface of g-C3N4.45,46 Fig. 4(f) shows the combined C 1s spectrum of pure g-C3N4 and Au-g-C3N4 nanostructure. In case of AuNPs, the peak intensity is decreased (Fig. 4(f)) with the little shift in the binding energy. Therefore, its mainly related to a change of oxidation state of the element, here the shifting of binding energy relates to the changes of Au3+ to Au0 oxidation state. This analysis was supported by XRD, XPS, BET, and HR-TEM studies.
3.1.5. Brunauer–Emmett–Teller, specific surface area analysis of the pure g-C3N4 and Au-g-C3N4 nanostructures. N2-BET (Nitrogen Adsorption Brunauer–Emmett–Teller) was performed to detect the changes in the specific surface area of the as-fabricated samples. The measured specific surface areas of the pure g-C3N4 and Au-g-C3N4 nanostructures (1 mM, 3 mM, and 6 mM) were 31.0116 ± 0.3652 m2 g−1, 31.9655 ± 0.1336 m2 g−1, 34.9131 ± 0.3450 m2 g−1, and 41.1593 ± 0.4697 m2 g−1, respectively. In Fig. 5, the surface area of Au-g-C3N4 (6 mM) increased with increasing amount of precursor, which was much higher than that of pure g-C3N4. The higher specific surface area provides larger spaces to accommodate more charge storage and expose more active sites for the photochemical reaction. These results suggest that the visible light photoelectrochemical performance of the Au-g-C3N4 nanostructures could be improved greatly due to the higher specific surface area.
|
| Fig. 5 Nitrogen adsorption–desorption isotherm of the pure g-C3N4 and Au-g-C3N4 nanostructures. | |
The nitrogen adsorption–desorption isotherm of pure g-C3N4 displays a hysteresis loop, suggesting the existence of mesopores.42 The AuNPs-loaded g-C3N4 exhibited much higher specific surface areas that of pure g-C3N4 (Table 1). The 6 mM AuNPs decorated g-C3N4 had a specific surface area of up to 41.15 m2 g−1. This shows that the optimal amount of AuNPs decorated g-C3N4 could provide more adsorption sites and photochemical reaction sites to improve the photoelectrochemical performance.
Table 1 Specific surface area measured from BET analysis of the pure-g-C3N4 and Au-g-C3N4 nanostructures
Sample name |
BET surface area (m2 g−1) |
Pure g-C3N4 |
31.0116 ± 0.3652 |
Au-g-C3N4 (1 mM) |
31.9655 ± 0.1336 |
Au-g-C3N4 (3 mM) |
34.9131 ± 0.3450 |
Au-g-C3N4 (6 mM) |
41.1593 ± 0.4697 |
4. Photoelectrochemical studies
4.1. Photoelectrochemical studies of pure g-C3N4 and Au-g-C3N4 nanostructures using LSV, EIS and CV measurements
Studies of the photoelectric behavior of pure g-C3N4 and Au-g-C3N4 nanostructures as a photoelectrode were performed using a standard three-electrode system. The measurements were taken under ambient conditions in the dark and under visible light irradiation in a 50 mL, a 0.2 M aqueous Na2SO4 solution as an electrolyte at room temperature. LSV and EIS were first performed in the dark and then under visible light irradiation (λ ≥ 400 nm) at a scan rate of 50 mV s−1 over the applied potential range, (−1 to 1 V).41 LSV is a voltammetry process, where the current at a working electrode is measured while the potential between the working electrode and reference electrode is swept linearly with time. LSV was performed in the dark and under visible light irradiation to provide evidence of the visible light-induced performance. The Au-g-C3N4 nanostructures (1–6 mM) displayed an enhanced photocurrent compared to pure g-C3N4 (Fig. 6(a)). The results in Fig. 6(a) showed that the photocurrent density depends basically on AuNPs deposition onto the sheet-like structure of g-C3N4. The current density increased significantly with increasing amount of AuNPs deposition. This higher increment in photocurrent density can be explained by the improved visible light absorption behavior of the material. The photocurrent depends largely on the number of photogenerated electrons; a higher number of electrons generated will improve the photocurrent density.43,47 The large number of electrons amassed in the conduction band of g-C3N4 resulted in a higher amount of photocurrent generation.43,44,48
|
| Fig. 6 Visible light-induced photoelectrochemical performance (a) LSV, (b) EIS Nyquist plot of the pure g-C3N4 and Au-g-C3N4 as a photoelectrode in the dark and under visible light irradiation, and (c) equivalent circuit from the Nyquist plots. | |
The interfacial charge transfer rate is essential for improving the photoelectrode performance. Electrochemical impedance spectroscopy (EIS) was performed in the dark and under visible light irradiation to understand the charge separation process and transport properties of pure g-C3N4 and Au-g-C3N4 as a photoelectrode material, as shown in Fig. 6(b). In general, the complex impedance plot is normally presented as Z′/ohm vs. −Z′′/ohm, which initiates from the resistance and capacitance component of the electrochemical cell. A representative Nyquist plot includes one or more semicircular arcs with the diameter along the Z′/ohm axis.41 The semicircular arcs observed in the high and low frequency regions correspond to an electron transfer process, and its diameter represents the electron transfer or charge transfer resistance. In the present graph, a half circle arc with a reduced diameter for the Au-g-C3N4 was obtained compared to pure g-C3N4, which clearly reveals a rapid electron-transfer process in the case of the Au-g-C3N4 nanostructures under visible light irradiation. Generally, the small radius of the arc in the EIS spectra indicated lower electron transfer resistance at the surface of the photoelectrode, which is usually associated with the faster interfacial charge transfer. The concentration was increased from 1 mM to 6 mM under visible light irradiation; the EIS spectrum displayed a smaller arc radius of Au-g-C3N4. The performance of the as-fabricated nanostructure was better than that of pure g-C3N4.
Based on the EIS data (Fig. 6(b)), an equivalent circuit (Fig. 6(c)) fitted by the Zsimp Win 3.20d program with fine accuracy was obtained. Basically the equivalent circuit is used to analyze the measured impedance data. As shown in the circuitry, Rct and Cdl represent the charge transfer resistance and double layer capacitance, and L describes the diffusion behavior at low frequencies, respectively. Table 2 shows the EIS fitting data obtained from the fitting of the equivalent circuits and the experimental values obtained from the impedance data. The fitting values of Rct for Au-g-C3N4 nanostructures decrease from 1 mM to 6 mM. The higher concentration of AuNPs exhibit the small Rct value which was much lower than that of pure-g-C3N4, which clearly suggested that the charge-transfer resistance is significantly reduced by anchoring of AuNPs onto sheet like structure of g-C3N4. The Cdl values displayed the opposite tendency as that of Rct values. The low Rct and high Cdl values indicate high electron transfer efficiency which further supports the improved photoelectrochemical performance of Au-g-C3N4 nanostructures.
Table 2 Fitting circuit values from equivalent circuit to analyze the Nyquist plots
Sample |
Rct (Ω cm−2) |
Cdl × 108 (F cm−2) |
Pure-g-C3N4 |
21.82 ± 1.12 |
1.39 ± 0.14 |
Au-g-C3N4 (1 mM) |
21.42 ± 0.96 |
2.01 ± 0.19 |
Au-g-C3N4 (3 mM) |
19.26 ± 0.89 |
2.16 ± 0.21 |
Au-g-C3N4 (6 mM) |
18.21 ± 1.00 |
2.49 ± 0.29 |
The cyclic voltammogram (Fig. 7) of pure g-C3N4 and Au-g-C3N4 nanostructures were obtained in the dark and under visible light irradiation at a scan rate of 0.05 mV s−1. The CV plot of the Au-g-C3N4 nanostructures showed an improved positive and negative sweep, indicating their pseudo capacitive nature. The peak current of the Au-g-C3N4 nanostructures from 1 mM to 6 mM increased linearly in the dark and under visible light irradiation with a positive shift of the cathodic peak and a negative shift of the anodic peak.41,45 The improved anodic and cathodic peak verified the amended current transfer ability of the Au-g-C3N4 nanostructures under visible light irradiation, which also reveals better capacitive performance of the as-fabricated nanostructures. Consequently, the improved capacitive performance of the Au-g-C3N4 nanostructures can be attributed to its improved charge loading ability and the synergistic effect of AuNPs and g-C3N4 under visible light irradiation.46,49,50
|
| Fig. 7 Cyclic voltammetry profile of pure g-C3N4 and Au-g-C3N4 nanostructures in a 0.2 M phosphate buffer (pH = 7) solution at 25 °C at a scan rate of 0.05 mV s−1. | |
4.2. Incident photon-to-current conversion efficiency (IPCE) test
To investigate the photoresponse of pure-g-C3N4 and Au-g-C3N4 (1–6 mM) nanostructures, IPCE measurements at 1.2 eV vs. Ag/AgCl as the reference electrode are presented in Fig. 8. The IPCE can be expressed as follows:51,52 |
| (2) |
where λ, φ and Ip denote the wavelength of the incident light (nm), the irradiation power (mW cm−2), and the photocurrent density (A cm−2) measured at the corresponding wavelength, respectively.
|
| Fig. 8 IPCE graph for pure-g-C3N4 and Au-g-C3N4 (1–6 mM) nanostructures at 1.2 eV vs. Ag/AgCl in 0.2 M Na2SO4. | |
Fig. 8 of IPCE tests shows a visible light response in case of higher Au-g-C3N4 nanostructures. The absorption threshold of g-C3N4 is approximately 460 nm, with a lower IPCE value. Anchoring of AuNPs onto sheet like structure of g-C3N4 results in substantial enhancement of the IPCE values for Au-g-C3N4 nanostructures (1–6 mM) as follows: 14.6%, 10.5%, and 7.4% under visible light irradiation respectively. In addition, the small hump appeared in the visible region which is caused primarily by the SPR effect of AuNPs. While in the case of bare g-C3N4, the IPCE performance was very less (2.2%) without any hump in visible region as compared to Au-g-C3N4 which further confirms the role of AuNPs with spatial effect of SPR. This result indicates the anchored AuNPs shows SPR effect which helps to improve the photoelectrochemical performance of nanostructures.
The progressive visible light-induced photoelectrochemical performance using Au-g-C3N4 nanostructures confirmed the successful anchoring of AuNPs onto the sheet-like structure of g-C3N4. The improved photocurrent performance revealed the interfacial interaction and charge transfer between the AuNPs and g-C3N4, which could explain the enhanced photoelectrochemical performance of the Au-g-C3N4 nanostructures.
5. Proposed electron transfer mechanism of Au-g-C3N4 nanostructures under visible-light irradiation
Generally, in case of a semiconducting material, visible-light irradiation plays a significant role in the excitation of electrons from the valence band (VB) to the conduction band (CB). In presence of visible-light irradiation (λ ≥ 400 nm) g-C3N4 nanostructures excited and electrons (e−) from the VB transfer to the CB, leaving the holes (h+) in the VB, thereby forming the electron–hole pairs.21,53–57 The photogenerated electrons can rapidly transfer the AuNPs due to their intimate interfacial contact between g-C3N4 and AuNPs, resulting in a significantly improved lifetime of the photogenerated electron–hole charge carrier.41,56
Fig. 9 shows a schematic diagram of the probable procedure for the charge separation in Au-g-C3N4nanostructures under visible-light irradiation. As shown in Fig. 9 visible-light irradiation was focused on the as-prepared electrode on FTO glass, which was dipped in the electrolyte solution. The electrolyte solution acts as a donor or acceptor to contribute or receive electrons from the electrodes. The Au-g-C3N4 nanostructures sample showed higher photocurrent performance (1–6 mM) because of its tuned optical properties compared to the bare g-C3N4. The counter and reference electrode measure the photocurrent with the help of the electrolyte solution and finally we recorded the improved performance of photocurrent form Au-g-C3N4 nanostructures.
|
| Fig. 9 Proposed schematic charge transfer mechanism for the photocurrent performance over the visible light-induced Au-g-C3N4 nanostructures as a photoelectrode. | |
6. Conclusions
This paper reported a facile, green, and competent approach for the fabrication of Au-g-C3N4nanostructures with spherical and uniform sized AuNPs with a high surface area (41.1593 m2 g−1) and improved photoelectrochemical performance. A single strain developed biofilm was used as a tool to reduce Au3+ to Au0 and Au-g-C3N4 nanostructures (1 mM, 3 mM and 6 mM) were fabricated. The anchoring of AuNPs onto the sheet-like structure of g-C3N4 produced promising photoelectrode material for real photonic devices. The boosted photoelectrochemical performance of Au-g-C3N4 nanostructures compared to that of pure g-C3N4 were explained based on the strong visible-light absorption, superior photocurrent generation, surface plasmon effect of AuNPs, and lower photoluminescence intensity. The spherical shape, size and uniform dispersion of the AuNPs over the g-C3N4 sheet were valuable for increasing the photocurrent performance. These findings were attributed mainly to the higher visible-light absorption by AuNPs ensuring the formation of a large number of photogenerated electron–hole pairs. This large number of exciton was transferred immediately through the polar-semiconductor–noble-metal interface to the-sheet like structure of g-C3N4, which inhibited the charge recombination process and increased the photocurrent performance.
Conflicts of interest
The authors declare no competing financial interests.
Acknowledgements
This study was supported by Priority Research Centers Program (Grant No. 2014R1A6A1031189) through the National Research Foundation of Korea (NRF) funded by the Ministry of Education.
References
- P. T. Anastas and J. B. Zimmerman, Environ. Sci. Technol., 2003, 94A–101A CrossRef.
- P. T. Anastas and J. C. Warner, Green chemistry: theory and practice, Oxford university press, 2000 Search PubMed.
- P. T. Anastas and T. C. Williamson, Green chemistry: frontiers in benign chemical syntheses and processes, Oxford University Press, USA, 1998 Search PubMed.
- M. M. Khan, J. Lee and M. H. Cho, Int. J. Hydrogen Energy, 2013, 38, 5243–5250 CrossRef CAS.
- M. M. Khan, S. A. Ansari, M. I. Amal, J. Lee and M. H. Cho, Nanoscale, 2013, 5, 4427–4435 RSC.
- S. A. Ansari, M. M. Khan, M. O. Ansari, S. Kalathil, J. Lee and M. H. Cho, RSC Adv., 2014, 4, 16782–16791 RSC.
- L. Wang, C. Wang, X. Hu, H. Xue and H. Pang, Chem.–Asian J., 2016, 11, 3305–3328 CrossRef CAS PubMed.
- X. Z. Li, B. Hauer and B. Rosche, Appl. Microbiol. Biotechnol., 2007, 76, 1255–1262 CrossRef CAS PubMed.
- S. Andersson, G. Kuttuva Rajarao, C. J. Land and G. Dalhammar, FEMS Microbiol. Lett., 2008, 283, 83–90 CrossRef CAS PubMed.
- S.-i. Naya, A. Inoue and H. Tada, J. Am. Chem. Soc., 2010, 132, 6292–6293 CrossRef CAS PubMed.
- Z. Yu and S. S. Chuang, Appl. Catal., B, 2008, 83, 277–285 CrossRef CAS.
- Y. Yang, J. Wen, J. Wei, R. Xiong, J. Shi and C. Pan, ACS Appl. Mater. Interfaces, 2013, 5, 6201–6207 CAS.
- S. Martha, A. Nashim and K. Parida, J. Mater. Chem. A, 2013, 1, 7816–7824 CAS.
- S. Sarina, E. R. Waclawik and H. Zhu, Green Chem., 2013, 15, 1814–1833 RSC.
- V. Amendola, R. Pilot, M. Frasconi, O. M. Maragò and M. A. Iatì, J. Phys.: Condens. Matter, 2017, 29, 203002–203050 CrossRef PubMed.
- S. K. Ghosh and T. Pal, Chem. Rev., 2007, 107, 4797–4862 CrossRef CAS PubMed.
- K.-H. Chen, Y.-C. Pu, K.-D. Chang, Y.-F. Liang, C.-M. Liu, J.-W. Yeh, H.-C. Shih and Y.-J. Hsu, J. Phys. Chem. C, 2012, 116, 19039–19045 CAS.
- P. Wang, B. Huang, Y. Dai and M.-H. Whangbo, Phys. Chem. Chem. Phys., 2012, 14, 9813–9825 RSC.
- M. Careem and A. Arof, Materials Today: Proceedings, 2016, 3, S73–S79 CrossRef.
- Y.-C. Pu, G. Wang, K.-D. Chang, Y. Ling, Y.-K. Lin, B. C. Fitzmorris, C.-M. Liu, X. Lu, Y. Tong and J. Z. Zhang, Nano Lett., 2013, 13, 3817–3823 CrossRef CAS PubMed.
- M. M. Khan, S. A. Ansari, M. E. Khan, M. O. Ansari, B.-K. Min and M. H. Cho, New J. Chem., 2015, 39, 2758–2766 RSC.
- R. Matsumoto, S. Yamada and H. Yonemura, Mol. Cryst. Liq. Cryst., 2014, 598, 86–91 CrossRef CAS.
- X. Wang, K. Maeda, A. Thomas, K. Takanabe, G. Xin, J. M. Carlsson, K. Domen and M. Antonietti, Nat. Mater., 2009, 8, 76–80 CrossRef CAS PubMed.
- Y. Zheng, J. Liu, J. Liang, M. Jaroniec and S. Z. Qiao, Energy Environ. Sci., 2012, 5, 6717–6731 CAS.
- F. Goettmann, A. Thomas and M. Antonietti, Angew. Chem., Int. Ed., 2007, 46, 2717–2720 CrossRef CAS PubMed.
- J. Liu, T. Zhang, Z. Wang, G. Dawson and W. Chen, J. Mater. Chem., 2011, 21, 14398–14401 RSC.
- L. J. Brennan, F. Purcell-Milton, A. S. Salmeron, H. Zhang, A. O. Govorov, A. V. Fedorov and Y. K. Gun'ko, Nanoscale Res. Lett., 2015, 10, 38–50 CrossRef PubMed.
- F. Dong, Y. Sun, L. Wu, M. Fu and Z. Wu, Catal. Sci. Technol., 2012, 2, 1332–1335 CAS.
- J.-M. Li, H.-Y. Cheng, Y.-H. Chiu and Y.-J. Hsu, Nanoscale, 2016, 8, 15720–15729 RSC.
- Y.-H. Chiu, K.-D. Chang and Y.-J. Hsu, J. Mater. Chem. A, 2018, 6, 4286–4296 CAS.
- T. H. Han, S. Y. Sawant, S.-J. Hwang and M. H. Cho, RSC Adv., 2016, 6, 25799–25807 RSC.
- M. E. Khan, M. M. Khan and M. H. Cho, RSC Adv., 2015, 5, 26897–26904 RSC.
- M. E. Khan, M. M. Khan and M. H. Cho, New J. Chem., 2015, 39, 8121–8129 RSC.
- K. Saravanakumar, R. Karthik, S.-M. Chen, J. V. Kumar, K. Prakash and V. Muthuraj, J. Colloid Interface Sci., 2017, 15, 514–526 CrossRef PubMed.
- L. Ge, C. Han and J. Liu, J. Mater. Chem., 2012, 22, 11843–11850 RSC.
- Y.-P. Zhu, T.-Z. Ren and Z.-Y. Yuan, ACS Appl. Mater. Interfaces, 2015, 7, 16850–16856 CAS.
- J. Song, L. Xu, R. Xing, Q. Li, C. Zhou, D. Liu and H. Song, Sci. Rep., 2014, 4, 7515–7522 CrossRef CAS PubMed.
- J. Li, C.-y. Liu and Y. Liu, J. Mater. Chem., 2012, 22, 8426–8430 RSC.
- Y. H. Lee, L. Polavarapu, N. Gao, P. Yuan and Q.-H. Xu, Langmuir, 2011, 28, 321–326 CrossRef PubMed.
- M. E. Khan, M. M. Khan and M. H. Cho, Sci. Rep., 2017, 7, 5928–5945 CrossRef PubMed.
- M. E. Khan, M. M. Khan and M. H. Cho, J. Colloid Interface Sci., 2016, 482, 221–232 CrossRef CAS PubMed.
- D. Zheng, C. Pang, Y. Liu and X. Wang, Chem. Commun., 2015, 51, 9706–9709 RSC.
- K. Parida, S. Martha, D. Das and N. Biswal, J. Mater. Chem., 2010, 20, 7144–7149 RSC.
- A. Corma and H. Garcia, Chem. Soc. Rev., 2008, 37, 2096–2126 RSC.
- M. E. Khan, M. M. Khan and M. H. Cho, RSC Adv., 2016, 6, 20824–20833 RSC.
- Y. Hou, Z. Wen, S. Cui, X. Guo and J. Chen, Adv. Mater., 2013, 25, 6291–6297 CrossRef CAS PubMed.
- P. D. Long, D. T. Chien, N. T. Trung, N. S. Hieu, L. H. Chi, V. Van Cat and V. D. Lam, J. Electron. Mater., 2017, 46, 4448–4454 CrossRef CAS.
- N. Chander, P. Singh, A. Khan, V. Dutta and V. K. Komarala, Thin Solid Films, 2014, 568, 74–80 CrossRef CAS.
- J. Zeng, T. Song, M. Lv, T. Wang, J. Qin and H. Zeng, RSC Adv., 2016, 6, 54964–54975 RSC.
- M. E. Khan, M. M. Khan, B.-K. Min and M. H. Cho, Sci. Rep., 2018, 8, 1723–1735 CrossRef PubMed.
- W. Zhao, L. Xie, M. Zhang, Z. Ai, H. Xi, Y. Li, Q. Shi and J. Chen, Int. J. Hydrogen Energy, 2016, 41, 6277–6287 CrossRef CAS.
- W. Zhao, Z. Ai, X. Zhu, M. Zhang, Q. Shi and J. Dai, Int. J. Hydrogen Energy, 2014, 39, 7705–7712 CrossRef CAS.
- M. E. Khan, M. M. Khan and M. H. Cho, J. Phys. Chem. Solids, 2017, 104, 233–242 CrossRef CAS.
- N. C. Jeong, C. Prasittichai and J. T. Hupp, Langmuir, 2011, 27, 14609–14614 CrossRef CAS PubMed.
- T. Akiyama, M. Nakada, K. Sugawa and S. Yamada, Macromol. Symp., 2008, 270, 171–176 CrossRef CAS.
- Y. Pu and J. Zhang, Austin Journal of Nanomedicine & Nanotechnology, 2014, 2, 1030–1034 Search PubMed.
- T. Akiyama, A. Masuhara, Y. Matsuda, T. Arakawa, T. Munaoka, T. Onodera, H. Oikawa and S. Yamada, Jpn. J. Appl. Phys., 2011, 50, 04DH15 CrossRef.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c8ra00690c |
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