Xian-Yang
Zhang
a,
Zhi-Qiang
Wang
*a and
Xue-Qing
Gong
*b
aState Key Laboratory of Green Chemical Engineering and Industrial Catalysis, Centre for Computational Chemistry and Research Institute of Industrial Catalysis, School of Chemistry and Molecular Engineering, East China University of Science and Technology, 130 Meilong Road, Shanghai, 200237, China. E-mail: zhiqiangwang@ecust.edu.cn
bSchool of Chemistry and Chemical Engineering, Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai, 200240, China. E-mail: xqgong@sjtu.edu.cn
First published on 2nd August 2024
ZnO is an important catalytic material for CO/CO2 hydrogenation. In this work, the pristine ZnO(100) and the surfaces with Zn–O dimer vacancies (ZnO(100)–(Zn–O)DiV) and oxygen vacancies are calculated. We find that the hydride (H−) species can be generated via heterolytic H2 dissociation on these surfaces, and that ZnO(100)–(Zn–O)DiV only needs to overcome the energy barrier of ∼0.10 eV. This is because the ZnO system has flexible orbitals for electron storage and release and the low-coordinated Zn3c atoms at the defect sites can form stable Zn–H− covalent bonds with high symmetry. Flexible Zn orbitals also impart the unique feature of activating multiple electrophilic adsorbates simultaneously as excess electrons exist. Moreover, we show that the covalent Zn–H− species can regulate the catalytic activity and selectivity for CO2 hydrogenation by preferentially producing *HCOO intermediates at Zn–O dimer vacancies. These results may help in the design of efficient Zn-based hydrogenation catalysts.
In fact, there have already been many studies about selective hydrogenation reactions on clean ZnO surfaces, which were mainly focused on the activation mechanisms of H2 and CO2.13–15 Wöll and co-workers16 studied the CO2 adsorption and activation on the ZnO(100) surface with infrared reflection absorption spectroscopy (IRRAS) and showed that CO2 can be adsorbed along the [0001] direction and form the carbonate (CO3δ−) species. Ling et al.17 obtained the scanning tunneling microscope (STM) images of the heterolytically dissociated H2 on the ZnO(100) surface under ambient pressure, and the adsorption structure was expected to be beneficial to the stabilization of the formed active H species. Peng and co-workers18 examined the mechanism of H2 activation on ZnO nanorods with and without surface oxygen vacancies by applying 17O nuclear magnetic resonance spectroscopy (NMR), and they found that more hydride species can be produced through homolytic and heterolytic dissociation at the oxygen vacancy sites of the reduced ZnO(100). Theoretically, Tang et al.19 performed systematic on-site Coulomb interaction corrected density functional theory (DFT+U) calculations of the adsorption of CO2 and found that the adsorbed CO2 molecules tend to form linear structures on the polar ZnO facets (such as {0001} and {000}), while the bending structures are produced on the nonpolar ZnO facets (such as {100}, {110} and {111}). Li and co-workers20 calculated the pathways of H2 activation on the pristine ZnO(100) surface, and they determined the heterolytic dissociation of H2 rather than the homolytic one. Furthermore, through DFT calculations, Zhao et al.21 located the complete reaction routes of CO hydrogenation to methanol on the Zn-terminated ZnO(0001) surface and showed that CO would follow the route of being consecutively hydrogenated to formyl (HCO), formaldehyde (H2CO), and methoxy (H3CO) before the formation of methanol. Thus, we can find that the catalytic reactions at ZnO are closely related to its surface structures. However, the relationship between the unique electronic properties of ZnO and the catalytic activities in selective hydrogenation reactions has not been thoroughly investigated.
In this work, the wurtzite ZnO(100) surface, which has a rather low surface energy and exists under real catalytic conditions,9 was constructed for the DFT calculations. Both the pristine and defective surfaces were considered. Specifically, the surface defect structures were confirmed by the calculated p–T phase diagrams.6,11,22 Moreover, their electronic structures were also carefully studied, and the density of states (DOS) calculations showed a shrinkage of the unfilled dsp hybridized orbitals when excess electrons are present on the surfaces; at the same time, no new occupied states appear under the Fermi energy level (EF), indicating a unique strategy of electron storage and release by ZnO. Systematic calculations were then performed to investigate the generation of active H species on these surfaces and their reactivities in the CO2 selective hydrogenation reactions. It was found that the various vacancy defects are beneficial to the stabilization of the hydride species (H−), which can be generated through the heterolytic dissociation of H2. Interestingly, the calculated results also showed that the occurrence of H+ (proton) from heterolytic H2 dissociation on the ZnO(100) surface can be involved in activating the adsorbed H on Zn to the hydride species, and it can also help enhance the adsorption of CO2 as well. This work revealed why the ZnO surface and its defects are favorable for catalyzing hydrogenation reactions as well as the ‘multifunction role’ of surface H in these reactions. It may provide some assistance for the rational design of Zn-based catalysts with high activities and selectivities.
The transition states (TSs) of surface reactions were located using a constrained optimization scheme and were verified when (i) all forces on the relaxed atoms vanish and (ii) the total energy is a maximum along the reaction coordinate, but it is a minimum with respect to the rest of the degrees of freedom.32,33
The adsorption energies of different species (X) on the surface (Eads(X)) were calculated with:
Eads(X) = −(EX/slab − Eslab − EX) | (1) |
In addition, we also calculated the formation energies of different defects of ZnO surfaces.34 Firstly, the oxygen vacancy formation energy was calculated as:
(2) |
(3) |
(4) |
(5) |
Notably, the choice for the size of the slab model has been systematically tested by the formation energy of different defects (Fig. S1†), and it was found that the formation energies of the various types of surface defects (OV and (Zn–O)DiV) largely converged with the size above p(4 × 3) (θ = 1/12 ML), which is also in agreement with previous reports.28,29
We also investigated the electronic properties of the pristine and various defect ZnO(100) surfaces by calculating the density of states (DOS) (Fig. 1e–g). The calculated band gap of the pristine ZnO(100) surface was 3.0 eV, which largely agrees with the experimental result (3.3 eV).41 Further analysis of the partial DOS (pDOS) showed that most of the Zn 3d electrons lay deeply below the Fermi energy level (EF), clearly caused by the fully filled orbitals with strong correlations,42 and it also hints at a unique bonding pattern with other species. Besides, from the calculated DOS of the defect surface, we can clearly see that the bonding symmetry change caused by the Zn–O dimer vacancy also has a strong influence on the shape of Zn 3d orbitals (Fig. 1f and S2a†), which are broadened obviously. By contrast, the excess electrons contributed by the O vacancy do shrink the unoccupied dsp hybrid orbital (Fig. S3a†), but they do not change the shape of the Zn orbitals or bring about a new electronic state under EF, indicating a new way of storing electrons that is different from that of some reducible metal oxides,43,44 whose extra electrons would be localized at specific atomic orbitals. In fact, we have also determined that when the 2 electrons resulting from the formation of an oxygen vacancy are forced to be localized at the oxygen vacancy site, the corresponding vacancy formation energy is 0.70 eV higher than that when the 2 electrons are delocalized in the system (Fig. 2c and S3b†); and the pDOS calculation (Fig. S3b†) suggested that these excess electrons would exist within the hybrid orbitals throughout the ZnO bulk, just like the electrons from other atoms. Thus, the Zn orbitals appear to be rather flexible for electron storage.
Firstly, we calculated the adsorption of one H atom at O sites on these surfaces. The calculated results showed that one electron from the H would preferentially transfer to the pristine and different defect ZnO(100) surfaces (Fig. S4†), and the corresponding Bader charges are +0.62, +0.63 and +0.66 |e| for the adsorbed H on the pristine, (Zn–O)DiV and OV surfaces, respectively, indicating that the proton species are formed. The calculated results also showed that the adsorption of the H atom at the O3c site on the ZnO(100)–(Zn–O)DiV surface is exothermic by 1.28 eV. Such a favorable adsorption can be due to the fact that the adsorption location is rather open and the adsorbed H species can form the hydrogen bond with the neighboring O3c (the distance between O3c and H atoms is 2.05 Å, Fig. S4d†). The adsorption of one H atom at the O3c site on the ZnO(100)–OV surface was calculated to be exothermic by 0.71 eV only. This is mainly because the presence of the two excess electrons on the reduced ZnO(100) surface further increases the electron repulsion within the system. Notably, we can also find that the extra electron from an adsorbed H (Fig. S4c, f and i†) barely has any influence on the overall shape of the Zn orbitals of the various ZnO(100) surfaces, which again suggests the flexibility of Zn orbitals in storing electrons.
In addition, we also calculated the adsorption of one H atom at Zn sites on these surfaces. The results showed that the H species, as a radical, is barely adsorbed at the Zn site on the ZnO(100) surface since the adsorption is endothermic by 1.48 eV (Fig. 2a and d). By contrast, the H adsorbed on the ZnO(100)–OV surface can actually form three H–Zn bonds at the OV site, and it turns into a hydride species (Fig. 2c, the corresponding Bader charge is −0.42 |e|) with the exothermic adsorption energy of 0.10 eV. This result is largely consistent with the findings that the hydride species can form on some reduced metal oxide surfaces such as CeO2.39,45 For the adsorption of a single H atom at the Zn site on the ZnO(100)–(Zn–O)DiV surface, the hydride, rather than a H radical, is also formed (Fig. 2b, the calculated Bader charge is −0.40 |e|), though this process is endothermic by 0.35 eV. In this case, the adsorbed H species would interact with the two Zn3c (Fig. 2e). Notably, the electronic analysis suggested that the hydrides on both the OV and (Zn–O)DiV surfaces occur via the covalent bonds contributed by the s electron from H and the multiple symmetric d electrons from Zn, in particular dx2−y2 (Fig. 2e and f), and the energy levels of the as-formed covalent Zn–H bonds at ZnO(100)–(Zn–O)DiV and ZnO(100)–(Zn–O)OV are far below EF.
The calculated results showed that the homolytic dissociation of H2 to form two O–H species at O sites on the pristine, Zn–O dimer vacancies and oxygen vacancies of the ZnO(100) surfaces needs to overcome the energy barriers of 1.48 eV, 0.70 eV and 1.52 eV (Fig. 3a and S6b, e and h†), respectively, and they are exothermic by 0.64 eV, 1.57 eV and 0.98 eV (Fig. 3a, c, f and i), respectively. Our results also showed that the homolytic H2 dissociation can produce two Zn–H species at adjacent Zn3c sites on the ZnO(100), ZnO(100)–(Zn–O)DiV and ZnO(100)–OV surfaces, and the corresponding electronic analyses indicated that they are 2Zn–H˙, Zn–H˙ and Zn–H−, and OV–H− and Zn–H− species, respectively. Moreover, these processes need to overcome energy barriers as high as 2.81 eV, 2.38 eV and 1.43 eV, respectively (Fig. 3a and S6c, f and i†), and the calculated reaction energies also indicated that these processes are energetically unfavorable.
On the other hand, according to our calculated results, the heterolytic H2 dissociation on the different ZnO surfaces (ZnO(100), ZnO(100)–(Zn–O)DiV and ZnO(100)–OV surfaces) can readily occur to form the Zn–H− and O–H species, which only need to overcome the small energy barriers of 0.45 eV, 0.10 eV and 0.45 eV (Fig. 3a and S6a, d and g†), respectively, and the corresponding processes are exothermic by 0.53 eV, 1.51 eV and 0.77 eV, which are consistent with those reported in previous experimental and theoretical studies.20,48,49 The stabilities could be attributed to the structural features of the transition states of the heterolytic H2 dissociations: the characteristic [H–O–Zn–H] four-membered ring at ZnO(100), the [H–O–Zn–O–Zn–H] hexatomic ring at ZnO(100)–(Zn–O)DiV and a double [H–O–Zn–O–Zn–H] hexatomic ring at ZnO(100)–OV.
From the above results, we can find that H2 can be activated more readily through heterolytic dissociation rather than homolytic cleavage on the different ZnO surfaces, which is also consistent with the previously reported results on some other metal oxides.18,20,50 Specifically, among the different ZnO(100) surfaces, the (Zn–O)DiV surface is the most active one for the heterolytic H2 dissociation. This is because the low-coordinated O species around the ZnV site on the ZnO(100)–(Zn–O)DiV surface are rather active for the transformation of the adsorbed H into stable protons, while the OV site on the (Zn–O)DiV surface can help produce the stable hydrides that interact with the surface through covalent Zn–H bonds. We also performed the density-functional perturbation theory (DFPT) calculations51,52 of the O–H and Zn–H species produced by the heterolytic H2 dissociation on the ZnO(100) and ZnO(100)–(Zn–O)DiV surfaces, and obtained the corresponding simulated infrared (IR) spectra (3550 (O–H) and 1773 (Zn–H) cm−1 for pristine ZnO(100); 3345 (O–H) and 1522 (Zn–H) cm−1 for ZnO(100)–(Zn–O)DiV; see Fig. S7†). The wavenumber differences for the species on the pristine and (Zn–O)DiV surfaces are due to their different structures, i.e. on the (Zn–O)DiV surface, the O–H species can also form a hydrogen bond with the neighboring lattice O, and the hydride actually bonds with two Zn sites. These calculated wavenumbers are largely consistent with the reported experimental results that the pristine ZnO(100) surface gives rise to 3490 (O–H) and 1710 (Zn–H) cm−1 and the ZnO(100)–(Zn–O)DiV gives rise to 3400 (O–H) and 1475 (Zn–H) cm−1.48,53,54
Besides, to further understand the energy barrier and product stability of heterolytic H2 dissociation on the different surfaces, we also calculated the partial DOS of the H species in the transition and final states of these processes (Fig. 4, S8 and S9†). The results indicated that the Zn–H ionic bonds occur in the transition states on the ZnO(100) and ZnO(100)–OV surfaces (Fig. 4a). Moreover, the structural properties of the Zn–H bonds in the transition states (Fig. S8†) also showed that only a single asymmetric Zn–H bond forms on the pristine and OV surfaces, while the double symmetric Zn–H bond occurs on the (Zn–O)DiV surface. Accordingly, higher energy barriers were obtained on the pristine and OV surfaces (0.45 eV) compared with that on the (Zn–O)DiV surface (0.10 eV). Interestingly, stable covalent Zn–H bonds with relatively low energy levels can be formed on the defect surfaces, while Zn–H ionic bonds with relatively high energy levels were formed on the pristine ZnO(100) surface, leading to the different stabilities of the hydride species on the three surfaces.
The corresponding Bader charge and spin charge density difference analyses (Fig. 3b–j) also supported that the heterolytic H2 dissociation on the various surfaces indeed produced a hydride and a hydroxyl species. The calculated Bader charges of the formed H+ and H− species are +0.66 |e| and −0.40 |e| at ZnO(100), +0.69 |e| and −0.38 |e| at ZnO(100)–(Zn–O)DiV, and +0.75 |e| and −0.42 |e| at ZnO(100)–OV. Interestingly, one can notice that the value of the calculated charge of H+ is approximately two times that of H− on the different ZnO(100) surfaces. This suggested that only some part of the charge contributed by the H during H2 dissociation is used to activate another H to form the hydride species, while the other part of the charge might be transferred to the ZnO(100) surface (Table S2†). This is very different from some other metal oxides (e.g., MgO and CeO2), on which the calculated Bader charges of the H+ and H− species generated through heterolytic H2 dissociation are approximately equal.45,55
For this unusual phenomenon, the calculated DOS (Fig. S8†) of the products of heterolytic H2 dissociation showed that the shapes of the Zn orbitals are almost unchanged, which is consistent with the situations of single H adsorption at surface O explored earlier on. In fact, the hydrides from these heterolytically dissociated H2 molecules can be recognized to evolve from the H adsorbing immediately following the H+ formation at the surface O site, in which case the electrons are released after storage. Therefore, it can also be concluded that the Zn orbitals are indeed quite flexible since they largely maintain the same shape during electron storage/release.
Finally, we further investigated if the transferred charge from the adsorbed H can be involved in the generation of multiple hydrides on the ZnO(100)–(Zn–O)DiV surface (Fig. 5). The calculated results showed that, together with the surface H+, two hydride species can indeed occur, and their corresponding Bader charges are −0.36 |e| and −0.31 |e| (Fig. 5a). However, the charge contributed by one adsorbed H species cannot be used to activate more adsorbed H to the hydride species (e.g., the corresponding Bader charges of the three co-adsorbed H species are −0.36, −0.29 and 0.00 |e|, respectively, forming only two hydride species; Fig. 5b). Thus, we can expect that the charge released by the formation of a proton may perform dual functions for the simultaneous activation of two electrophilic adsorbates (e.g., CO2δ− and hydride).
Next, we calculated the further adsorption of H2 and found that it is generally rather weak on the pristine and different defect ZnO(100) surfaces with the pre-adsorbed CO2 (the corresponding adsorption energies are close to 0 eV; see Fig. 6a and S11†). The adsorbed H2 then undergoes heterolytic dissociation to produce one hydride and one proton species with the barriers of 0.49 eV, 0.30 eV and 0.42 eV on the pristine and defect ZnO(100) surfaces, and the corresponding processes are exothermic by 0.53 eV, 1.69 eV and 0.77 eV. Interestingly, we also found that the adsorption energies of CO2 were enhanced by 0.18 eV and 0.06 eV on the pristine and (Zn–O)DiV surfaces, respectively, following the heterolytic dissociation of the H2, in comparison with the CO2 adsorbed alone. This is consistent with our findings above that the charges provided by the H that turns into a proton have ‘dual functions’ in activating multiple adsorbates.
We next considered two possible routes for CO2 activation, i.e. direct dissociation of CO2 and direct hydrogenation of CO2. The results indicated that the direct CO2 dissociation into co-adsorbed *CO and *O on the ZnO(100), ZnO(100)–(Zn–O)DiV and ZnO(100)–Ov surfaces requires endothermic energies of 5.09 eV, 5.04 eV and 4.78 eV (Fig. S12†), respectively, and such high energy demands suggested that direct CO2 dissociation is unfavorable. In the route of direct hydrogenation of CO2, two possible pathways were then tested (Fig. 6 and S13–S15†). The first is the so-called COOH (carboxyl) pathway, in which the H+ or H− binds with the Oδ− of the adsorbed CO2 to form a *COOH species; the second is the so-called HCOO (formate) pathway, in which the H+ or H− reacts with the Cδ+ of the adsorbed CO2 to produce a *HCOO species. According to our calculated results, the processes with the H+ attacking the adsorbed CO2 to form the *HCOO species need to overcome enormously large energy barriers of 4.29 eV, 2.76 eV and 6.42 eV on the ZnO(100), ZnO(100)–Ov and ZnO(100)–(Zn–O)DiV surfaces, respectively, and they are also highly endothermic (4.13 eV, 1.92 eV and 4.13 eV, respectively; Fig. S13a, e and i, and S14a, e and i†). When the H+ species attacks the Oδ− of the adsorbed CO2 to generate a *COOH species (Fig. S13c, g, and k, and S14c, g and k†), it also needs to overcome very large energy barriers (4.25 eV, 1.43 eV and 4.06 eV on the ZnO(100), ZnO(100)–Ov and ZnO(100)–(Zn–O)DiV surfaces, respectively) and these processes are highly endothermic (1.05 eV, 1.02 eV and 1.34 eV). Interestingly, for the processes with the H− species as the active H species to react with CO2, both the carboxylate and formate pathways can occur quite easily. For the pathway for the hydride species to attack the Cδ+ of the adsorbed CO2 to form the *HCOO species, the energy barriers are 2.26 eV, 1.39 eV and 1.46 eV on the pristine and the two defect ZnO(100) surfaces and they are exothermic by 0.53 eV and endothermic by 0.01 eV and 0.09 eV, respectively. At the same time, the reactions between H− and the Oδ− of the adsorbed CO2 (the COOH pathway) need to overcome the energy barriers of 2.42 eV, 1.40 eV and 1.71 eV, while they are endothermic by 0.09 eV, 0.05 eV and 0.67 eV.
In addition, we also calculated the subsequent hydrogenation reaction steps in both the HCOO-to-methanol pathway and the COOH-to-methanol pathway (Fig. S16–19†) on the ZnO(100)–(ZnO)DiV surface. The results indicated that the HCOO-to-methanol pathway is more favorable than the COOH-to-methanol pathway in the formation of *H2CO species, where the maximum endothermic step (*HCOO + *H− → *HCOOH, ΔE = 0.78 eV) of the HCOO-to-methanol pathway is lower than that of the COOH-to-methanol pathway (*CO + *OH + *H+ → *CO + H2O(g), ΔE = 1.29 eV) (Fig. S16 and S18†). After the formation of the *H2CO species, the H2 dissociation into H+ and H− species releases an exothermic energy of 0.56 eV, while the formation of *H3CO is exothermic by 1.67 eV. The subsequent step of H2 adsorption and dissociation is exothermic by 0.18 eV, and the formation of *CH3OH species is highly exothermic by 1.89 eV. Therefore, it can be concluded that the *HCOO species is more readily formed and more stable during the CO2 hydrogenation to methanol reaction, and we believe that the *HCOO intermediate species is the most abundant reactive intermediate (MARI) in the CO2 hydrogenation reaction, which is consistent with other reports.58,59
From the above results, one can surely expect that the CO2 hydrogenation with the H− species on the ZnO(100)–(Zn–O)DiV surface is more likely to follow the HCOO pathway, which may lead to the formation of CH3OH as the main product,60 and this stoichiometric surface with (Zn–O)DiV defects is more active than the reduced one with OV defects. This result is consistent with those reported recently by Ling et al.17 Moreover, the simulated infrared spectra (calculated by the DFPT method51,52) of formate (1355 and 1515 cm−1, Fig. S20†) are also consistent with the reported experimental results61,62 (1370 and 1595 cm−1). In general, we can learn from the calculated results in the current work that defects on the ZnO(100) surface are key to its improved catalytic activities in H2 activation and CO2 hydrogenation, and the Zn–O dimer vacancy appears even more active than the usual O vacancy.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d4sc04344h |
This journal is © The Royal Society of Chemistry 2024 |