Effects of Preparation Conditions on the Efficiency of Visible-Light-Driven Hydrogen Generation Based on Cd_0.25Zn_0.75S Photocatalysts

1. Introduction

Nowadays, the main atmospheric issues arise from the increased consumption of fossil fuels, urging the development of an alternative source of energy to meet the world’s energy demand [1]. Therefore, hydrogen, as a clean and environmentally friendly energy source, was considered to be the most promising candidate, especially after Fujishima and Honda demonstrated photocatalytic hydrogen production by decomposition of water, using semiconductor materials in the early seventies [2,3]. Photocatalytic hydrogen evolution via water splitting remains an important research topic, as indicated by the review of Zhang et al. [4]. The decomposition of H₂S instead of H₂O was widely investigated and shown to be economically and environmentally improved, because it required less energy and resulted in the removal of H₂S, an extremely toxic gas that is mainly produced from the refinery of crude oil and contributes to acid rain [5].

The most common type of photocatalysts previously used were metal oxides [6,7] such as NiO/Ta₂O₅K [8], ZnO/TiO₂ [9], Au/ZnO [10], ZnO/Fe₂O₃ [11]. These materials mostly utilized ultraviolet radiation, which only represents a small part of the solar spectrum. Sulfide-based semiconductors exhibit a better solar response than oxides and have highly negative potential conduction bands suitable for H₂O reduction. Hence, numerous recent studies have focused on the development of these types of photocatalysts. The main sulfide-based catalysts have been reviewed by Zhang and Guo; most of them consist of block d transition metals with d¹⁰ electron configuration, and the most investigated type was CdS or ZnS–CdS [12]. ZnS possesses a highly negative conduction band position, making it possible to achieve a higher efficiency without requiring modification; on the other hand, CdS has a good solar response due to its narrow band gap. The ZnS–CdS composite belongs to the heterojunction photocatalysts which provide an improved separation of the photogenerated electron-hole pairs, resulting higher efficiency [4]. Additionally, the stabilization and immobilization of ZnS–CdS nanoparticles were realized by the application of polyphosphate, gelatin, polyvinyl alcohol [13], or polystyrene [14]. The Fe₂O₃/ZnS–CdS core–shell nanoparticles were prepared for this purpose [15].

A variety of articles have previously reported the excellent photoactivity of the ZnS–CdS semiconductor and how it could be increased by metal modification [16,17,18,19,20,21], however, only few have taken in account the preparation method and the initial parameters and how they may affect the rate of hydrogen production. A simple precipitation of ZnS–CdS from acetate or nitrate salts with Na₂S or TAA (thioacetamide) was applied in most cases with [18,22,23,24] or without further hydrothermal treatment (HTT) [14,15,16,25,26]. In some cases, other sulphide sources were used, such as Na₂S₂O₃ [27], thiourea [28,29,30], cysteine [31] or xanthate [32].

According to Gonzalez-Panzo, I.J. et al. [33], CdS’s precipitation is more favorable at pH > 10 and that of ZnS at pH > 11.5, which suggests that preparing the catalyst with the usual direct precipitation method would lead to a core–shell structure (CdS coated with ZnS), while preparation from ammine complexes could ensure the simultaneous precipitation of ZnS and CdS because the initial pH is increased to approximately 13. Guo and co-workers applied an ethylenediamine complexing agent for the preparation of the ZnS–CdS composites using TAA as a sulphide source [21,34,35]. They achieved considerably high quantum yields by this method. In the present work, a comparison between the conventional preparation method and the synthesis applying ammine complexes was made. The effects of other parameters and conditions such as pH, concentrations, hydrothermal treatment, and the order of the preparation steps (i.e., mixing order) on the structure and the efficiency of the catalyst were also investigated.

2. Results and Discussion

2.1. The Effect of the Mixing Order

In the literature, two different orders for the mixing of the reactants can be found regarding the preparation of the photocatalysts used in this work. Generally, the sulfide reagent was added to the solution containing the metal ions (designated as “normal order”), but in some cases a reverse order was applied [20,36]. Therefore, the effect of the mixing order of the reagents was investigated with regard to the photoactivity of the catalysts.

In this paper, we depicted the rate of hydrogen production (RHP) as a function of the illumination time, but in the bar diagrams, its average calculated for the 200–400 min time range is represented. RHP is provided by μmol H₂ evolved during one hour (i.e., the unit of measurement is μmol/h). The temperature of the collected hydrogen was the same for each experiment (22 °C), we used the same light source and geometrical arrangement for all irradiations in this work. Hence, RHP is linearly proportional to the quantum yield of the hydrogen production.

Two catalysts containing CdS and ZnS in 1:3 molar ratio were prepared. Each of the preparation conditions was the same except for the mixing order of the reagent solutions. The catalyst prepared by the “normal order” (i.e., when the Na₂S solution was added to the solution containing the metal ions) resulted in more than 25% higher RHP compared to that of the one prepared by the reverse order (when the solution of ammine complexes was added to the sulfide solution) (Figure 1). Since there was a significant difference between the two catalysts, the “normal order” was applied for further preparations.

The shape of the rate functions shown in Figure 1a is similar to those obtained for the other catalysts tested. After an initial increase, it shows a slow decrease, then, close to the end of the reaction, it steeply decreases until the sulfide ions are completely consumed. In order to better understand the changes, the rates (RHP values) were also plotted as a function of the sulfide concentration (Figure 1b). The concentration of sulfide was calculated as described in our previous article [37]. Liu and colleagues previously found that RHP displays first-order kinetics regarding the sulfide ions [38]. In the case of the catalysts studied in this work, it can be clearly seen that only at sulfide concentrations of less than 0.01 M (at the end of the reaction) was a direct proportionality between the rate and c(S²⁻) observed. The reaction rate was almost constant during most of the irradiation, as it only slightly decreased, and the slope of this decrease is significantly less than that of the decrease of the sulfide concentration. At this stage, the reaction is diffusion-controlled with pseudo-zero-order kinetics. To interpret this change, it is worth comparing this with the initial increase as well as with the publications describing that the thio functional groups on the surface of CdS and ZnS crystals produced from aqueous media are partially replaced by oxo or hydroxo groups [18,38]. On this basis, it is likely that, in the reaction leading to equilibrium at the initial stage of illumination, the oxo/hydroxo surface function groups will be replaced with sulfide, which will cause an initial increase of the rate. (Notably, at the beginning of the irradiation, the temperature also increases from 25 °C to about 40 °C, but this temperature is reached in less than 1 h, while the increase in the rate often last for 3–4 h.) A slight decrease in the middle stage of the reaction is likely to be a combined effect of several factors. One of the reasons is that sulfide ions must first adsorb onto the catalyst surface to react with the photogenerated hole, but in this process they compete with other ions in the solution. Since the concentration of sulfide decreases in the photoinduced process, while that of thiosulfate increases, the ratio of sulfide concentration to that of other sulfur-containing anions decreases (Figure 1b), which inhibits the adsorption of sulfide ions onto the surface of the catalyst. The re-exchange of surface function groups to hydroxide groups may also result in a reduction in RHP, which is a consequence of a decrease in the sulfide/hydroxide ratio. (When the same catalyst was irradiated several times, it was often found that the initial increasing periods were similar for each illumination cycle, indicating that this change is reversible or rather leads to equilibrium.)

2.2. Photocatalytic Activity of Zn_0.75Cd_0.25S Catalysts

According to several publications [21,29,34,35,39], sulfide catalysts were precipitated from N-based complexes (NH₃ or ethylenediamine). The application of complexes as metal ion sources may decrease the driving force of the precipitation, and can highly influence the process of co-precipitation. Although HTT is another important step in the preparation of the catalyst, its real effect on the photoactivity of ZnS–CdS has not been widely investigated. Therefore, these effects were also investigated in our work.

Three catalysts with different metal ion:NH₃ ratios were prepared. First, no NH₃ was added during the precipitation (Cat-0N). In the second case, a stoichiometric amount of 25% NH₃ solution (1.5 cm³) was added to the metal acetate solution (Cat-1N). In this procedure there was not enough NH₃ to entirely dissolve the Cd(OH)₂ and Zn(OH)₂ precipitates before the addition of Na₂S. In the third case, enough NH₃ solution was added (3.0 cm³) to dissolve all of the hydroxide precipitates (Cat-2N).

The hydrogen production efficiencies were studied on the three catalysts both before (the resulting catalysts are designated with “-0H” extension) and after HTT. The measured RHP values are shown in Figure 2. The catalyst prepared without the addition of ammonia and without HTT displayed a very low catalytic activity (16 μmol/h). This value increased by more than 10 times when the co-precipitation was performed from ammine complexes, no matter whether the stoichiometric amount or excess of ammonia was applied. The results also clearly show that the HTT significantly enhanced the activity of all investigated catalysts, and the best catalytic activity was measured for the sample prepared from the ammine complex, using a stoichiometric amount of ammonia. Its RHP reached 350 μmol/h (19.3 mmol/g/h), which is one of the best published values for such systems, although these rates strongly depend on the light sources and geometrical arrangements.

2.3. Diffuse Reflectance Spectra

The HTT of these catalysts caused a change in color from pale to dark yellow. This change is clearly shown by the diffuse reflectance spectra of the catalysts, from which the determinable band-gap (BG) value decreased only slightly, but the absolute value of the reflectance in the visible range significantly increased by the HTT (Figure 3 and

Table 1. The band-gap energies of different catalysts determined from Tauc-representation [40] of KM-functions (Figure S2).

	Band-Gap Energy/eV
Catalyst	Before HTT	After HTT
Cat-0N	2.58 ± 0.03	2.50 ± 0.02
Cat-1N	2.65 ± 0.03	2.60 ± 0.02
Cat-2N	2.65 ± 0.03	2.57 ± 0.02

). A decrease in BG of less than 0.1 eV would only justify an increase in RHP of about 5–10% (see Figure S1), so there must also be some changes in the crystal structure that results in a shift of the conduction band (CB) towards a more negative potential or a decrease in the probability of electron–hole recombination.

The BG and the CB potential of the Cd_0.5Zn_0.5S catalyst prepared from acetate salt and ethylenediamine (en) complexes were determined by electrochemical impedance spectroscopy by Chen et al. [21]. They found only a small difference in BG (2.39 eV and 2.36 eV), but the CB potential values differed significantly. The catalyst they prepared from a complex gave a much higher negative value (−1.06 V) than that produced from acetate salts (−0.91 V). Since the pH of the solution of sacrificial reagent in our system is approx. 13.5, a H₂/H⁺ redox potential of −0.8 V or more negative is required for hydrogen evolution. Although the CB potentials were not measured in this work, according the results discussed above, a possible explanation of the higher RHP values in the case of catalysts prepared from ammine complexes are a result of the more negative Gibbs energy of hydrogen formation. Slower precipitation may result in a deviating crystal structure, the CB potential of which is different.

2.4. XRD Pattern

In order to understand the previously described effects, X-ray diffraction (XRD) measurements were performed on samples dried from suspensions of the catalysts (Figure 4). Freshly prepared ZnS and CdS were used as references. From the diffractograms, it was clearly shown that all the ZnS–CdS samples consisted of only sulfides and did not contain any hydroxides or oxides traces. The investigated catalysts consist of cubic sphalerite and hawleyite. The latter has a crystal structure similar to that of sphalerite. Furthermore, the shifts at different peaks vary, which proves that it originates from the modification of the crystal structure. However, the position of the peaks, mainly the ones belonging to CdS, shifted towards higher 2θ, while those belonging to sphalerite slightly moved towards lower 2θ. This suggests that the Zn²⁺ ions are partly substituted by Cd²⁺ in the hawleyite lattice and the Cd²⁺ ions are slightly replaced by Zn²⁺ in the sphalerite lattice.

The XRD patterns of the catalyst prepared without adding any ammonia show only a slight shift of the peaks of hawleyite and sphalerite towards each other. The hawleyite peaks were shifted more than the sphalerite ones. Nevertheless, the peaks remained well separated. This sample also had the smallest full width at half maximum (FWHM) of the 111 reflection of sphalerite (at around 28.559° 2θ), i.e., the largest crystallite size (CS) according to the Scherrer equation, while the CS of hawleyite was the smallest one for this sample (Figure 5). The results suggest that if precipitation of CdS and ZnS does not occur from ammine complexes, both CdS and ZnS form faster than in the case of the precipitation from ammine complexes. Therefore, the Zn²⁺ ions are only slightly replaced by Cd²⁺ in sphalerite and, in turn, the Cd²⁺ ions by Zn²⁺ in hawleyite. However, the latter phenomenon may be more likely to occur due to the difference between the ionic radii. It is supported by the more perceptible shifts in the case of hawleyite. Increasing the amount of ammonia to the stoichiometric ratio, the 111 reflection of hawleyite (at around 26.552° 2θ) showed a larger shift and its calculated CS was very high. A further increase of the NH₃ content resulted in a smaller CS of hawleyite and its 111 reflection appears only as a small shoulder. Although there was a large error in the determination of CS, a correlation between RHP and CS of hawleyite was observed for the examined catalysts (Figure 5).

Comparing the XRD pattern of hydrothermally treated and not treated catalysts, no visible change could be observed in the position of the peaks, but their FWHMs were decreased, i.e., the crystallite sizes increased, during the treatment. These changes suggest that the HTT favors the substitution of Cd²⁺ and Zn²⁺ ions for each other.

2.5. Equilibrium Calculations

Some equilibrium calculations were performed in order to evaluate the driving force during the preparation of the Cat-0N, Cat-1N, and Cat-2N catalysts. The driving force of the precipitation (Δμ) is the difference between the chemical potential of the reactants just mixed and that of the resulting suspension. This could be estimated from the supersaturation (S), which is equal to the ratio of the initial (c) and the equilibrium free metal ion concentration (c*) [41].

$$\mathsf{\Delta }\mu =\mathrm{R}T\ln S=\mathrm{R}T\left(\ln c-\ln c^{*}\right)$$

(1)

The initial free metal ion concentration (c) could be calculated from the stability constants of the ammine and hydroxo complexes and the protonation constants of ammonia and acetate ion (

Table 2. Overall stability constants used for the calculation of the initial free metal ion concentrations [42,43].

n	NH4+	HAc	[Cd(NH3)n]2+	[Zn(NH3)n]2+	[Zn(OH)n]2−n
1	9.25	4.73	2.51	2.32	6.31
2	-	-	4.47	4.61	11.19
3	-	-	5.77	6.97	14.31
4	-	-	6.56	9.36	17.7

). The calculations were performed with a self-developed program using the Newton-Raphson method. The calculated free metal ion concentrations are indicated in Figure 6 by thin solid and dashed lines for the excess (T_NH3 = 3 M) or stoichiometric amount of ammonia (T_NH3 = 1.5 M), respectively. The orange and grey colors indicate the values for cadmium (II) and zinc (II) ions, respectively.

Equilibrium metal ion concentrations (c*) at a given pH can be determined from the total concentration of sulfide ion in the solution (T_S), the formation constants of CdS and ZnS (lgK_s,CdS = 26.1 and lgK_s,ZnS = 22.9 [44]) and the protonation constants of sulfide ion (lgK₁ = 17.4 and lgK₂ = 7.05 [45]).

$$c^{*}=\frac{1+K_1\left[H^{+}\right]+K_1{K}_2{\left[H^{+}\right]}^2}{T_S{K}_s}$$

(2)

Two different c^* values have been calculated from two different total sulfide concentrations. The first was obtained assuming that all the added sulfides were still in dissolved form (T_S = 0.22 M). The second one is for the state after the precipitation, when only the excess of the sulfide ion remains in solution (T_S = 0.02 M). The former one is indicated by a thick solid line and the latter one by a thick dashed line in Figure 6.

Since the driving force of precipitation is proportional to (lnc − lnc*), the vertical distance between the lgc and lgc* curves will also be proportional to the initial driving force, which was indicated by the thick vertical lines in Figure 6. The arrows indicate the real initial and end points before and after the addition of the sulfide reagent. In this figure, a higher lying curve represents a more stable species of a given metal ion.

The pH of the solution of cadmium acetate and zinc acetate was about 6.0, which increased to about 9 after the addition of a stoichiometric amount of Na₂S, while the pH reached 12 with the application of 10% excess of sulfide reagent. If the precipitation was started from the solution containing stoichiometric amount or excess of ammonia, the initial pH was 9.6 or 10.5, which increased up to 12. Realizing the precipitation from complexes, the precipitation driving forces decreased in both cases, but this decrease was more enhanced for the formation of ZnS (

Table 3. The initial pH of the solution of metal complexes before addition of Na₂S reagent, and the initial supersaturation (c/c*) at the beginning of precipitation.

Catalyst	Cat-0N	Cat-1N	Cat-2N
pH	6.0	9.6	10.5
lgSZnS	8.9	5.5	3.9
lgSCdS	11.7	10.9	9.4

). The lower driving force could cause a slower rate of precipitation, allowing the Cd²⁺ and Zn²⁺ ions to substitute each other, which is consistent with the peak shifts shown in XRD. The highest RHP of catalyst Cat-1N suggests that the undissolved Zn(OH)₂ particles influence the precipitation into a favorable direction.

2.6. SEM, TEM, and EDS Measurements

The SEM images of the catalysts measured with an energy dispersive detector clearly indicate their compositional inhomogeneity (Figure 7). All pictures show a darker (rich in ZnS) bulk with lighter (CdS-rich) spots. The Zn:Cd atomic ratios calculated by the EDS analysis were summarized in

Table 4. The Zn:Cd atomic ratios of the investigated catalysts calculated from the EDS analyses of different areas: A: average values regarding the whole area shown in the SEM pictures, B: the average of some lighter spots, and C: the average of a darker area.

Catalyst	Whole Average (A)	Lighter Spots (B)	Darker Area (C)
Cat-0N-0H	3.09	2.0	4.3
Cat-0N	3.14	2.5	3.4
Cat-1N-0H	3.10	1.3	3.6
Cat-1N	2.95	1.4	3.1
Cat-2N-0H	3.09	0.9	3.4
Cat-2N	3.02	1.3	3.1

. The average atomic ratio for the whole photographed area were very close to the expected 3.0 value for all catalysts investigated. The catalyst prepared without the addition of ammonia had a higher Zn:Cd ratio in the ZnS–rich bulk, and the number of CdS-rich particles were also higher than that for the other catalysts. Although the error of the calculated ratio is about 0.3–0.5, there is no doubt that the HTT enriches the CdS-rich particles in ZnS and the ZnS-rich particles in CdS, i.e., the sample becomes more homogeneous during the heat treatment. These results are in good agreement with the conclusions based on the XRD measurements and confirm the idea that Cd²⁺ and Zn²⁺ ions can substitute one other in the crystal lattice during HTT. In the case of the Cat-0N catalyst, the high initial chemical driving force could lead to the formation of numerous CdS cores, which caused the formation of many small CdS-rich particles.

For the morphological study of the catalysts prepared from solutions of different ammonia contents, STEM measurements were carried out, the result of which are shown in Figure 8. Higher ammonia concentrations applied during preparation unambiguously decreased the particle size. In the case of the catalyst prepared in the absence of ammonia, the size of the particles was in the region of about 10–40 nm (Figure 8a), and the shape of the particles were not elongated, i.e., nearly spherical. These results are in accordance with the XRD data (see Section 2.4), which showed the highest crystallite size in sphalerite. The large particle size may be one of the factors that decreased photocatalytic performance. Using ammonia, nanorods (or rather elongated nanoparticles) were formed with a typical diameter of 5–10 nm, and a length of 20–30 nm (Figure 8b). The particles prepared at the highest ammonia concentration were the smallest in size, 5–10 nm (Figure 8c).

In order to understand the structural changes during HTT, a TEM analysis was performed before and after HTT for the Cat-1N sample (Figure 9). The two pairs of bright-field (Figure 9A,C) and HRTEM images (Figure 9E,G) show the differences in crystal sizes between the two samples; smaller crystals occur in Cat-1N-0H (Figure 9A,E), whereas larger crystals are typical in the HTT sample (Figure 9C,G). According to the calculation of the crystal-size distribution (Figure S3), the typical size ranges are 3–12 nm and 5–26 nm, and the average sizes are around 5 nm and 12 nm in the Cat-1N-0H and Cat-1N samples, respectively. The crystal morphologies are similar in the two samples (axis ratios shown in Figure S3), and nearly isometric and slightly elongated shapes also occur in both samples. The crystal size difference is also recognizable in the electron diffraction patterns (Figure 9B,D), with broad diffraction rings produced by the Cat-1N-0H sample and sharp rings by the heat-treated sample, indicating smaller and larger average crystal sizes, respectively. These results are in agreement with the sizes obtained from XRD, likely due to the aging (Ostwald ripening) process during the treatment. The diffraction rings of both samples occur at the same d-values, close to the typical strong reflections of sphalerite.

The compositional inhomogeneity of crystallites expected on the basis of SEM/EDS images is less obvious. The STEM EDS Zn (blue) and Cd (yellow) elemental maps were measured on the same areas as the HRTEM images (Figure 9E,G) and illustrate the inhomogeneity of the chemical compositions, as also indicated by the compositions calculated from the marked areas. For both catalysts, the Zn:Cd ratio varied over a wide range. Compared to the theoretical Zn:Cd ratio of 3:1, significant deviations in both directions were observed, but neither pure CdS, nor pure ZnS were detected in the STEM-EDS element maps. The nanocrystals with the highest Cd content had Zn:Cd ratios of around 1 (Figure 9J,L), whereas the most Zn-rich nanocrystals had at least 6–10% Cd content (Figure 9I,K). The elemental distribution within a given crystallite appeared to be uniform. Thus, a STEM-EDS analysis suggested that the catalyst is composed of crystallites with homogeneous but variable compositions corresponding to a Cd_xZn_(1-x)S solid solution. This result is consistent with the peak shifts observed in XRD measurements.

The structures of the two boxed crystals in Figure 9E,G (see the magnified inserts F and H) contain a series of stacking faults. Such defects occur in both samples but are more common in the hydrothermally treated one. Similar planar defects were also described in detail by Liu [35] and Chen et al. [21]. White arrows in Figure 9F,H clearly show twin boundaries in sphalerite, resulting in ABCABCBACBA-type sequences of the close-packed layers, with the bold letter indicating a layer in a hcp stacking environment (as in wurtzite). In addition, stacking faults with ABCABCBCABC-type stacking sequences also occur, resulting in disordered structures between those of sphalerite and wurtzite (a common example is provided by the elongated nanocrystal in Figure 9H).

2.7. The Effect of the pH of Preparation on the ZnS–CdS Photoactivity

Three catalysts were prepared similarly to Cat-2N, but the initial pH was adjusted to 10.0, 11.0, or 12.0 through the addition of perchloric acid (2 M) after the formation of ammine complexes. The following procedure was identical with that applied for the other hydrothermally treated catalysts. The designation of the catalysts obtained were: Cat-2N-pH10, Cat-2N-pH11 and Cat-2N-pH12, corresponding to the initial pH applied for the preparation. The RHP was measured, and the results are depicted in Figure 10. Increasing the pH of the preparation in the presence of NH₄OH did not cause any remarkable changes in the evolution rate of hydrogen. This rate remained almost constant (~260 μmol/h) until the sulfide was depleted. This independence implies that, unlike the conventional preparation method, preparing the catalyst from ammine complexes confers the catalyst with high stability without the need of pH adjustment.

2.8. Stability of ZnS-CdS Catalysts

The reusability of the ZnS–CdS catalysts with the highest RHP values was also studied in order to check their stability (Figure 11). The ZnS–CdS catalysts prepared with the stoichiometric amount and an excess of NH₄OH were re-illuminated for three cycles of 16 h each. The ZnS–CdS catalyst prepared with an excess of NH₄OH exhibited an appropriate stability, and only a small decrease in the RHP was observed after three illuminations (from 270 μmol/h to 240 μmol/h). The catalyst prepared with the stoichiometric amount of NH₄OH appeared to be more stable than the previous one. Moreover, it demonstrated a small increase during the second and third illuminations (≈390 μmol/h), but the RHP in this case began decreasing after approximately 9 h, unlike the catalyst prepared with an excess of NH₄OH that showed a constant rate even after 13 h.

2.9. Quantum Yields

The quantum yields and the IPCEs (Incident-Photon-to-Current-Efficiency) were determined for the Cat-2N catalyst by three different light sources. The IPCEs and the quantum yields (QY) were calculated according to the following equations:

$$\mathrm{IPCE}=\frac{{2\times \mathrm{number}\mathrm{of}\mathrm{produced}\mathrm{H}}_2}{\mathrm{number}\mathrm{of}\mathrm{incident}\mathrm{photons}}$$

(3)

$$\mathrm{QY}=\frac{{2\times \mathrm{number}\mathrm{of}\mathrm{produced}\mathrm{H}}_2}{\mathrm{number}\mathrm{of}\mathrm{absorbed}\mathrm{photons}}$$

(4)

The number of incident photons were determined as described in the experimental part and in the Supplementary Materials, and the results are summarized in

Table 5. Measured data for the calculation of IPCE and QY for the Cat-2N catalyst illuminated by different light sources, and the resulting IPCE and QY values.

		Light Sources
	UV-LED	Hg-Xe	Vis-LED
nphotons/t (mmol/h)	12.06	11.25	27.75
RHP (mmol H2/h)	0.551	0.384	0.261
RHP (mmol H2/g/h)	30.6	21.3	14.5
IPCE	9.14%	6.82%	1.88%
Ratio of abs. photons	99.8%	85.0%	47.3%
QY	9.16%	8.02%	3.98%

. The number of absorbed photons for opaque solids is difficult to calculate. Although it might be estimated from the DRS spectra, in this case the geometrical arrangement and the thickness of the catalyst layer were different, hence it was evaluated from the band gap. The number of the absorbed photons was calculated by supposing that all photons of higher energy than the band gap were absorbed. Of course, the value obtained in this way was higher than the actual value. In the case of illumination with the 380 nm LED, almost all photons were absorbed and the calculated IPCE and the QY were almost the same (9.2%). The IPCEs for the Hg-Xe lamp and for the visible LED were 6.8% and 1.9%, respectively.

Although the QY should be independent of the light source, our calculations resulted in lower QYs for these two light sources. Considering the shape of the Kubelka-Munk function of the catalyst, it can be seen that it increases from the band gap (2.57 eV) up to about 3.0 eV (Figure 12). When calculating the number of the absorbed photons, it was assumed that all photons in this range were absorbed, although the absorption increased from 0 to ~100% (see also the dashed lines in Figure 12). The relative intensity of the visible LED shows that all the emitted photons of this LED which have a higher energy than the BG fall into this range, so it is likely that only around 40% of the photons were absorbed in this range. In the case of the Hg-Xe lamp, there was only one peak in the growing region of the Kubelka-Munk function, hence, the difference between the calculated and the real absorbed fractions is lower (by only about 10%). The RHP values obtained with the three light sources are shown in Figure 13.

Since the geometric arrangements of all illumination experiments in this work were the same, the ratios of the RHPs to the QYs are equal (see in Figure S5). Based on this relationship, the QY of the most efficient Cat-1N catalyst was calculated to be 11.5% (see in Table S1).

Even if our goal was to study the effects of various conditions of the catalyst preparation on the efficiency of the photocatalytic hydrogen generation and not to reach a quantum yield approaching or exceeding the best quantum yields so far published, a comparison is worth making. The QY values obtained by similar systems for visible-light-driven hydrogen production are in the 1–62% range [16,17,18,23,30,35,39,46,47,48,49,50]. The order of magnitude of the best QY reached in our work corresponds to this range. Considering that the conditions of the photocatalysis were not optimized, e.g., no stirring was applied, and no precious co-catalyst was used, and the fraction of the toxic cadmium was rather low, this value may be promising for practical utilization.

3. Materials and Methods

3.1. Materials

Zinc and cadmium acetate dihydrate (Zn(CH₃COO)₂⋅2H₂O and Cd(CH₃COO)₂⋅2H₂O) and sodium thiosulfate pentahydrate (Na₂S₂O₃⋅5H₂O) were purchased from Reanal, and sodium sulfide nonahydrate >98% (Na₂S⋅9H₂O) from Acros Organics. The water applied was cleaned by a Millipore Elix equipment (Millipore S.A.S., Molsheim, France) completed with a Milli-Q 50 purification system (Millipore S.A., Molsheim, France). The solutions containing sulfide/sulfite were prepared in advance using argon bubbled Milli-Q water and kept in the freezer for further experiments.

3.2. Photocatalyst Preparation

The typical preparation method of ZnS–CdS catalyst was as follows: 1 mmol cadmium acetate dihydrate and 3 mmol zinc acetate dihydrate were dissolved in 10 mL Milli-Q water, 0, 1.5 mL or 3.0 mL of 25% ammonia solution was added, and the mixture was stirred for 5 min. 4.4 mmol (10% excess) of Na₂S⋅9H₂O was dissolved in 10 mL Milli-Q water which was de-aerated by bubbling argon gas for 20 min. This Na₂S solution was added to the solution containing the metal ions under vigorous stirring. The suspension was stirred for 10 min, and then poured into the 50 mL Teflon lined autoclave and treated at 170 °C for 3 h. After decantation, the yellowish ZnS–CdS precipitate was washed twice with Milli-Q water and centrifuged. The catalyst was then stored in water-suspension. In the case of pH-dependent investigation, the initial pH of the solution of metal-ammine complexes was set with 2M perchloric acid (pH = 10, 11, 12).

3.3. Characterization

The crystallite size and phase composition was determined by an X-ray diffraction measurement (Philips PW3710, Cu Kα radiation, 50 kV and 40 mA). Data collections were carried out with X’Pert Data Collector software (2.0e, PANalytical B.V., Almelo, The Netherlands, 2010) The full width at half-maximum (FWHM) values of the individual reflections were determined by the profile fitting treatment of the X’Pert High Score Plus software (2.2.5, PANalytical B.V., Almelo, The Netherlands, 2009). The peak broadening caused by the samples was explained by the presence of very small crystallites. The broadening of the 111 reflections of hawleyite and sphalerite (measured breadth minus the instrumental breadth) was used to calculate the average crystallite size through the well-established Scherrer equation [51]. The FWHM of the 100 reflection of the ZnO (heated at 1000 °C) was employed as the instrumental breadth. The 01–075-0581, 00-005-0566, 00-006-0314, and 00-036-1450 Powder Diffraction File (PDF) of ICDD (International Centre for Diffraction Data) of hawleyite, sphalerite, greenockite, and wurtzite, respectively, were used to identify phases.

The morphology of the catalysts were studied by Schottky-field emission scanning electron microscope (FEI/Thermo Fisher Scientific, Waltham, MA, USA, model Apreo S) under high vacuum conditions using scanning-transmission electron imaging (STEM) mode. The energy-dispersive-spectroscopy (EDS) studies were performed by an EDAX Ametek (Mahwah, NI, USA) apparatus equipped with an Octane Elect Plus detector. Specord S600 spectrofluorometer (Analytic Jena GmbH, Jena, Germany) equipped with integrating sphere was used to measure the diffuse reflectance spectra and deduce the band-gap energy with the Kubelka-Munk function.

Samples for transmission electron microscopy (TEM) were prepared by depositing a drop of diluted aqueous suspension of the original samples on copper TEM grids that were covered by continuous carbon amorphous support film. TEM analyses were performed using a Talos F200X G2 instrument (Thermo Fisher Scientific), operated at 200 kV accelerating voltage, equipped with a field-emission gun and a four-detector Super-X energy-dispersive X-ray spectrometer (Termo Fisher Scientific), and capable of working in both conventional TEM and scanning transmission (STEM) modes. In our study, TEM bright-field images, HRTEM images and STEM high-angle annular dark-field (HAADF) images were collected to visualize the crystal size and the morphology of the particles and HRTEM images, and electron diffraction patterns were used to study the structural properties. To characterize the size and the morphologies of the nanocrystals before and after HTT, around 100-100 particles were analyzed in both of the samples Cat-1N-0H and Cat-1N in the following way: Two dimensions (the longest and the perpendicular to the longest diameters) were measured on all particles with properly visible edges on each of the analyzed images (typically separated or slightly overlapping particles). To reach the required 100-100 particles, 5 and 6 HRTEM images were analyzed, resulting in 103 and 108 particles for the Cat-1N-0H and Cat-1N samples, respectively. STEM-EDS elemental mapping was applied to measure and visualize the chemical composition and inhomogeneities.

3.4. Photochemical Experiments

The photochemical experiments were performed under the conditions described by Fodor et al. [37], in a double-necked reactor of 40 cm³ volume (14 mm height, 60 mm diameter). The total volume of all sacrificial solution was 30 cm³ and they contained 0.13 M Na₂S, 0,18 M Na₂SO₃ and 18 mg of catalyst (0.6 g/dm³). Before illumination, all samples were de-aerated by argon bubbling for 10 min. Two 7 W 6000 K Optonica visible LEDs were used as the light source. The intensity of light sources (i.e., the amount of incident photons per unit volume per unit time) was determined by trioxalato-ferrate (III) actinometer. A detailed evaluation for this determination is described in the Supplementary Materials.

The evolved hydrogen was bubbled into a vessel filled with 1 mM NaOH solution and its volume was calculated from the mass of the displaced NaOH solution. Mass data were collected every minute using a Kern PCB balance (Kern & Sohn GmbH, Balingen, Germany) connected to a PC. In all cases, illuminations were performed until the end of the reactions. Importantly, the reaction mixture was not stirred during the irradiation. The amount of evolved hydrogen was equal to the initial amount of Na₂S in all case.

4. Conclusions

In this work, ZnS-CdS composites were prepared in various ways, for visible-light-driven photocatalytic hydrogen generation in an aqueous system containing sulfide ions. The effect of their preparation conditions on the rate of hydrogen evolution was investigated. Our results unambiguously indicated that both the HTT of the catalysts and application of ammonia (as a ligand) during precipitation increased the photocatalytic efficiency. Notably, metal deposition on the catalyst particles was not required for promising photoactivity. Besides, the efficiency of these catalysts was independent of the pH applied for their preparation within the range of 10–12. This type of catalyst proved to be stable, i.e., its efficiency hardly changed during several re-uses. Additionally, the reaction mixture was not stirred during the irradiation, hence, this system is promising from the viewpoint of practical utilization.