Xiaohu
Ge‡
a,
Zhouhong
Ren‡
b,
Yueqiang
Cao
*a,
Xi
Liu
b,
Jing
Zhang
a,
Gang
Qian
a,
Xueqing
Gong
c,
Liwei
Chen
b,
Xinggui
Zhou
a,
Weikang
Yuan
a and
Xuezhi
Duan
*a
aState Key Laboratory of Chemical Engineering, East China University of Science and Technology, 130 Meilong Road, Shanghai 200237, China. E-mail: yqcao@ecust.edu.cn; xzduan@ecust.edu.cn
bSchool of Chemistry and Chemical Engineering, In-situ Center for Physical Sciences, Frontiers Science Center for Transformative Molecules, Shanghai Jiao Tong University, Shanghai 200240, China
cKey Laboratory for Advanced Materials, Centre for Computational Chemistry and Research Institute of Industrial Catalysis, East China University of Science and Technology, 130 Meilong Road, Shanghai 200237, China
First published on 26th May 2022
Tailoring the active sites to promote the formation of the target product is of great importance for selective hydrogenations catalyzed by non-noble metals but remains challenging. Herein, we propose to employ carbon atoms to be incorporated into the Ni3Ga intermetallic with partially isolated Ni sites aiming to enhance the catalytic performances for acetylene semi-hydrogenation. The incorporation of carbon atoms into the lattice of the Ni3Ga intermetallic is achieved by thermal processing of the Ni3Ga intermetallic catalyst in an acetylene atmosphere. The processed catalyst is proven to show the typical Ni3GaC0.5 phase by multiple characterization techniques including atomic-resolution electron microscopy and X-ray absorption spectroscopy. The presence of subsurface carbon in the Ni3GaC0.5 catalyst is experimentally and theoretically demonstrated to synergize with Ga sites for modifying the electronic structures of Ni via obvious hybridization of Ni 3d with Ga 2p and C 2p orbitals. The performance tests show that the Ni3GaC0.5 catalyst delivers high ethylene selectivity, up to ca. 90% at full conversion of acetylene, which outperforms the referred Ni and Ni3Ga catalysts. The excellent selectivity to ethylene is rationalized by theoretical calculations, which point out that the desorption of ethylene from the Ni3GaC0.5 catalyst is kinetically more favourable than its hydrogenation to ethane. In addition, the stability of the Ni3GaC0.5 catalyst is also enhanced against the Ni and Ni3Ga catalysts due to the suppressed formation of C4 products.
Introducing another metal to alloy with Ni is widely employed as a strategy for regulating the Ni active sites via the so-called geometric and electronic effects.1,4,6,8,10–16 Recently, intermetallic catalysts featuring stable structures and long-range ordering atomic arrangement were proposed as promising candidate catalysts for acetylene semi-hydrogenation.11,12,14,17,18 Regulating Ni sites with the guest metal sites to the completely isolated ones in intermetallic structures is an effective approach to suppress the strong σ-adsorption mode while it favors the weak π-adsorption for ethylene, which promotes the ethylene desorption and suppresses its hydrogenation to ethane.8,17,18 However, the adsorption modes for acetylene and ethylene are still σ-adsorption for Ni-/Pd-based intermetallic catalysts with partially isolated Ni/Pd active sites.2,5–8,16–25 These features give rise to unfavorable selectivity to ethylene but relatively higher hydrogenation activity in comparison with the intermetallic catalysts with completely isolated Ni/Pd sites. An interesting challenge that arises is addressing the possibility of further optimizing the adsorption/desorption behaviors of ethylene on such partially isolated active sites toward excellent ethylene selectivity, which could also maintain the relatively higher activity than the completely isolated active sites.
Considering that introducing another guest metal to the host metal expands the lattice of the host metal, it is of great interest to incorporate light atoms with a small radius into the expanded lattice of intermetallics to tailor the electronic and geometric structures of active sites. For acetylene semi-hydrogenation, light atoms, such as carbon and lithium, located inside the lattice of active metals have been well illustrated to remarkably improve the catalytic performances, especially the selectivity to ethylene.6,26–28 In this work, we propose to employ carbon atoms to be incorporated into the Ni3Ga intermetallic with partially isolated Ni sites aiming to tailor the catalytic performances for acetylene semi-hydrogenation. The Ni3Ga intermetallic catalyst was synthesized using quaternary Ni/Ga/Mg/Al layered double hydroxides (LDHs) as the precursor. The synthesized Ni3Ga catalyst was then processed in an acetylene atmosphere at 300 °C to introduce carbon atoms into the lattice of the Ni3Ga intermetallic. The structural features of the processed catalyst were identified by multiple techniques including atomic-resolution electron microscopy and X-ray absorption spectroscopy, which reveal the formation of the Ni3GaC0.5 phase. The presence of carbon at the interstitial sites of Ni3Ga has been experimentally and theoretically proven to obviously change the electronic properties of Ni sites. Catalytic performance tests show that the Ni3GaC0.5 catalyst exhibits excellent ethylene selectivity up to ca. 90% at 100% acetylene conversion, significantly prevailing over the referred Ni3Ga and Ni catalysts. Density functional theory (DFT) calculations were used to rationalize the origin of enhancement of the subsurface carbon atoms on the Ni3Ga intermetallic for the reaction.
At the conversion of ca. 10%, the carbon differences were both less than 1.0% for the Ni, Ni3Ga and Ni3GaC0.5 catalysts; at the conversion of ca. 90%, the carbon differences were 6.0, 4.5 and 2.0% for Ni, Ni3Ga and Ni3GaC0.5 catalysts, respectively. The higher carbon differences for the Ni and Ni3Ga catalysts suggest that more carbonaceous compounds were formed on the catalysts.
Based on the Ni3Ga catalyst, the subsurface carbon modified Ni3Ga catalyst was synthesized by processing with the C2H2 reactant at 300 °C, in which the phase transformation from Ni3Ga into Ni3GaC0.5 was identified by the time-resolved XRD measurements shown in Fig. 1b. The peak at 43.7° assigned to Ni3Ga(111) shifts gradually to smaller diffraction angles on increasing the processing time during the process, suggesting the incorporation of C atoms into the lattice of Ni3Ga.6,26,37 After processing for 160 min, the XRD pattern in the ESI, Fig. S2† demonstrates the complete formation of the Ni3GaC0.5 phase (JCPDS No. 29-0625), and thus the formed catalyst is denoted as Ni3GaC0.5. A similar process was also carried out for the monometallic Ni catalyst. In contrast, no obvious diffraction peaks corresponding to the Ni3C phase (JCPDS No. 01-7005) were observed from the XRD pattern for the processed Ni catalyst as shown in the ESI, Fig. S3,† indicating the absence of carbon atoms incorporated into the Ni lattice. Instead, the dissociated carbon atoms from acetylene molecules prefer to assemble on the monometallic Ni surface to form carbon nanofibers,6,26 which is also confirmed by the SEM images in the ESI, Fig. S4.† This could be caused by the limited space available for the dissolved carbon atoms at the Ni octahedral site (Fig. S5†), which leads to easier segregation of carbon atoms onto the surface.6
High resolution transmission electron microscopy (HRTEM) and high angle annular dark-field scanning transmission electron microscopy (HAADF-STEM) were further performed to reveal the detailed microstructural features of the synthesized Ni, Ni3Ga and Ni3GaC0.5 catalysts. Fig. S6†, 2a and b display the typical HRTEM images with the corresponding fast Fourier transform (FFT) patterns of Ni, Ni3Ga and Ni3Ga0.5, respectively. The interplanar spacing of lattice fringes in the ESI, Fig. S6† is determined to be 0.204 nm, which is ascribed to the interplanar spacing of the Ni(111) plane. Similarly, the averaged spacing of lattice fringes in the HRTEM image of the Ni3Ga catalyst is measured to be around 0.206 nm, agreeing well with the interplanar spacing of the Ni3Ga(111) plane. In contrast, the interlayer lattice spacing is determined to be 0.212 nm for the Ni3GaC0.5 catalyst, which is assigned to the (111) plane of the Ni3GaC0.5 phase (JCPDS No. 29-0625). Clearly, the lattice of the Ni3GaC0.5 catalyst is expanded as compared to that of the Ni3Ga catalyst, demonstrating the presence of C atoms located in the Ni3Ga crystal lattice. Moreover, no carbonaceous carbon is observed on the Ni3GaC0.5 particle, indicating that the expanded lattice of Ni3Ga (Fig. S5†) as compared to that of Ni is more favorable for stabilizing carbon atoms at the larger octahedral site.6 Furthermore, the Ni, Ni3Ga and Ni3GaC0.5 nanoparticles are uniformly distributed on the catalysts, as shown in the HAADF-STEM images (Fig. S7†, 2c and d), and the measured average nanoparticle sizes of Ni, Ni3Ga and Ni3GaC0.5 are 12.3, 11.9 and 12.1 nm, respectively. These similar particle sizes enable one to unravel the synergetic effects of surface Ga and subsurface C atoms on Ni active sites by excluding the particle size effects on acetylene hydrogenation. The energy dispersive X-ray spectroscopy (EDS) line-scanning within a single nanoparticle for the Ni3Ga catalyst shows that Ni and Ga elements are uniformly distributed over the particle (Fig. 2e), which is consistent with the EDS mapping analysis in the ESI, Fig. S8.† For the Ni3GaC0.5 catalyst, as seen in the EDS line-scanning in Fig. 2f, the Ni, Ga and C elements are also homogeneously distributed over the entire Ni3GaC0.5 nanoparticle, agreeing well with the EDS mapping analysis in the ESI, Fig. S9.† These results indicate the successful fabrication of Ni3Ga and Ni3GaC0.5 structures. Similarly, the EDS line-scanning and mapping analysis for the monometallic Ni catalyst shown in the ESI, Fig. S10 and S11† demonstrate the uniform spatial distribution of Ni element and the absence of Ga and C elements.
The atomic-scale structures of the Ni3Ga and Ni3GaC0.5 catalysts were further revealed by AC-HAADF-STEM techniques. The typical AC-HAADF-STEM image of the Ni3Ga catalyst in Fig. 2g displays the well-defined arrangement of Ni and Ga atoms in a rhombic periodic arrangement throughout the whole nanoparticle. As shown in Fig. 2h, the line intensity profile along with the red arrow marked in Fig. 2g illustrates that the lattice spacing along this direction is 0.205 nm, close to that of the (111) plane of the Pmm Ni3Ga intermetallic phase. In addition, the atomic arrangement predicted by the crystal structural models along with the [20] zone axis, which is determined by the FFT pattern (Fig. 2i) for the region marked by the yellow rectangle in Fig. 2g, is in good agreement with that experimentally observed by AC-HAADF-STEM in Fig. 2j. The AC-HAADF-STEM image of the Ni3GaC0.5 catalyst in Fig. 2k shows the well-defined ordered atomic arrangement with clear lattice fringes. The integrated pixel intensity profile (Fig. 2l) taken from the red arrow marked in Fig. 2k reveals that the average spacing of the lattice fringe is 0.211 nm, which is assigned to the Ni3GaC0.5(111) plane. Furthermore, the predicted atomic distribution of Ni3GaC0.5 along with the [20] zone axis determined by the corresponding FFT pattern (Fig. 2m) for the yellow rectangle region in Fig. 2k matches well with the observed one in Fig. 2n. These results unequivocally show the atomically ordered structure of intermetallic Ni3Ga and that of the carbon doped one (i.e., Ni3GaC0.5).
To unravel the electronic interaction between Ni, Ga and C, XPS analysis was employed to identify the electronic structures of Ni, Ni3Ga and Ni3GaC0.5 catalysts. The satellite peaks at the binding energy of 861.9 eV seen in the Ni 2p XPS spectrum of the monometallic Ni catalyst are ascribed to multielectron excitation (Fig. 3a).38 Besides, the two peaks centred at binding energies of 852.9 and 855.7 eV are attributed to Ni0 and Ni2+ species, respectively. In contrast, the Ni 2p peaks of the Ni3Ga catalyst shift towards lower binding energy by 0.51 eV compared with those of the Ni catalyst, revealing the visible electron transfer from Ga to Ni in the Ni3Ga intermetallic structure due to the higher electronegativity of Ni (1.91) than that of Ga (1.81).8 Notably, the Ni 2p peaks of the Ni3GaC0.5 catalyst show an evident shift to higher binding energy by 0.46 eV as compared with those of the Ni3Ga catalyst. Meanwhile, the binding energy of the Ga 2p XPS spectrum of the Ni3GaC0.5 catalyst is close to that of the Ni3Ga catalyst in Fig. 3b, which implies that the electrons are transferred from Ni atoms to C ones after introducing C atoms into the lattice of the intermetallic Ni3Ga. It should be noted that the presence of the Ni2+ and Ga3+ species is reasonably related to the re-oxidation of the sample during the ex situ tests.5,8 The normalized X-ray absorption near-edge structure (XANES) spectrum at the Ni K-edge was further employed to reveal the electronic structures of the Ni, Ni3Ga and Ni3GaC0.5 catalysts. As shown in Fig. 3c, the energy of the adsorption edge of the Ni3GaC0.5 catalyst shifts to higher position compared with that of the Ni3Ga catalyst. This demonstrates the electron-deficient character of the Ni atoms in the Ni3GaC0.5 catalyst due to the considerable electron transfer from Ni atoms to the adjacent C atoms,8,11,12,15 which is in good accordance with the XPS analyses. Furthermore, the extended X-ray absorption fine structure (EXAFS) spectrum of the Ni3GaC0.5 catalyst shows an obvious scattering peak at 1.7 Å,26 which is assigned to the formation of Ni–C coordination in Fig. 3d. Besides, the Ni–Ni (Ga) scattering peak at 2.1 Å of Ni3GaC0.5 shifts slightly to a longer radial distance than those of the Ni and Ni3Ga catalysts. The EXAFS oscillations at the K edge of these Ni catalysts in the ESI, Fig. S12† reveal that the Ni3GaC0.5 catalyst displays shorter periods and smaller amplitudes than the Ni3Ga and Ni catalysts, demonstrating the longer coordination distance of Ni–Ni (Ga) and lower coordination environment in the Ni3GaC0.5 catalyst.39–42 Wavelet transform (WT) analyses of the Ni EXAFS oscillations were further carried out to confirm the formation of Ni–C coordination in the Ni3GaC0.5 catalyst (Fig. 3e). The WT-EXAFS contour plots of these catalysts exhibit a maximum at around 8.1 Å−1 contributed by the Ni–Ni (Ga) coordination. Moreover, the WT-EXAFS contour plot of the Ni3GaC0.5 catalyst shows a maximum at around 4.5 Å−1, which is ascribed to the contribution of the Ni–C coordination. The curve fitting results of all three Ni-based catalysts are shown in the ESI, Fig. S13–S15 and Table S1,† which also reveal the presence of Ni–C coordination in the Ni3GaC0.5 catalyst.
The electronic structures of Ni3Ga and Ni3GaC0.5 catalysts were then studied by DFT calculations. Based on the Wulff construction crystals for Ni, Ni3Ga and Ni3GaC0.5 in the ESI, Fig. S16,† the thermodynamically stable and mostly exposed surfaces, i.e., Ni(111), Ni3Ga(111) and Ni3GaC0.5(111) surfaces, were selected for the model calculations. The configurations of these surfaces are schematically shown in the ESI, Fig. S17.† Bader charge density difference analyses on the Ni3Ga(111) and Ni3GaC0.5(111) surfaces were employed to reveal the changes in the electronic structure after doping C atoms into the lattice of Ni3Ga. Fig. 4a and S18† exhibit distinct charge transfer from Ni atoms to the C atoms underneath these Ni atoms, which is well consistent with the above XPS and XANES analyses. As further revealed by the density of states (DOS) profiles (Fig. 4b), the d-band of Ni atoms overlaps with the p-bands of Ga and C atoms in Ni3GaC0.5, suggesting obvious hybridization of Ni 3d with Ga 2p and C 2p orbitals, especially the hybridization of Ni 3d with Ga 2p orbitals. The hybridizations result in clear electron transfer from Ga atoms to Ni ones and then from Ni atoms to C ones. Moreover, the d-band centre of Ni on the Ni3GaC0.5(111) surface downshifts toward lower energy compared with those on the Ni(111) and Ni3Ga(111) surfaces. These indicate that the introduction of C atoms into the Ni3Ga lattice could effectively weaken the interaction between ethylene and Ni active sites and thus favour the desorption against its hydrogenation. Thus, the acetylene semi-hydrogenation would be enhanced on the Ni3GaC0.5 catalyst due to the synergistic modifications of Ga and subsurface C onto the Ni active sites.
The catalytic performance of the fabricated Ni3GaC0.5 catalyst was evaluated for acetylene semi-hydrogenation in excess ethylene in comparison with those of the Ni and Ni3Ga catalysts. Fig. 5a, b, S19 and S20† show the conversion of acetylene as well as the selectivity to ethylene, ethane and C4 products on the Ni, Ni3Ga and Ni3GaC0.5 catalysts, respectively. The Ni catalyst exhibits significant over-hydrogenation and coupling performance for acetylene and thus leads to obvious formation of ethane and C4 products (Fig. S19 and S20†), respectively. Notably, the negative ethylene selectivity on the Ni catalyst indicates the hydrogenation of ethylene contained in the reactant mixture. In contrast, the over-hydrogenation and coupling processes are suppressed on the Ni3Ga intermetallic, due to the partial isolation of Ni sites by Ga and electronic interaction between Ni and Ga.8 However, the performance on the Ni3Ga catalyst is not good enough for acetylene semi-hydrogenation. Further incorporation of C atoms in Ni3Ga forming the Ni3GaC0.5 catalyst results in much higher selectivity to the target ethylene product compared to Ni and Ni3Ga catalysts in the temperature range from 20 to 130 °C, probably due to the favoured desorption of ethylene as predicted by the DOS analysis. In addition, the over-hydrogenation of acetylene to ethane and the coupling to C4 products are remarkably suppressed on the Ni3GaC0.5 catalyst (Fig. S19 and S20†). As clearly shown in Fig. 5c, the Ni3GaC0.5 catalyst exhibits an extraordinary ethylene selectivity of 89.1% even at full acetylene conversion, with only 6.6% of ethane selectivity and 4.3% of C4 selectivity. However, the Ni and Ni3Ga catalysts exhibit much lower ethylene selectivity of 46.7% and 65.1% at the full conversion of acetylene, respectively. Moreover, the selectivities to C4 products on the Ni and Ni3Ga catalysts are 15.2% and 10.2%, significantly higher than that on the Ni3GaC0.5 catalyst. Thus, the catalytic performance of the Ni3GaC0.5 catalyst is more promising than those of the Ni and Ni3Ga catalysts as well as previously reported Ni-based catalysts (Table 1).
Catalysts | Acetylene conversion (%) | Temperature (°C) | Reaction time (h) | Ethylene selectivity (%) | Ethylene selectivitya (%) | Reactants |
---|---|---|---|---|---|---|
a Ethylene selectivity at acetylene conversion higher than 90%. | ||||||
Ni/SiO2 (ref. 43) | 40 | 180 | 36 | 50 | — | C2H2 + H2 |
Ni/SiO2–Al2O3 (ref. 44) | <8 | 175 | 3 | 70–80 | — | C2H2 + H2 |
NiGa/MgAl2O4 (ref. 8) | 93 | 190 | 24 | 78 | 78 | C2H2 + C2H4 + H2 |
Ni3Ga10 | 92 | 200 | 24 | 77 | 77 | C2H2 + C2H4 + H2 |
Ni3GaC0.5 (this work) | 100 | 110 | 36 | 90 | 90 | C2H2 + C2H4 + H2 |
Ni10In/SiO2 (ref. 43) | 100 | 180 | 36 | 60 | 60 | C2H2 + H2 |
AgNi0.125/SiO2 (ref. 45) | 90.4 | 160 | — | 31.4 | 31.4 | C2H2 + C2H4 + H2 |
Ni5Zn21 (ref. 46) | 75 | 160 | 12 | 50 | 50 | C2H2 + C2H4 + H2 |
NiZn2/MgAl2O4 (ref. 47) | 75 | 120 | — | 60 | 50 | C2H2 + H2 |
Pre-NiCu/MMO4 | 60 | 150 | 20 | — | 70 | C2H2 + C2H4 + H2 |
Cu2.75Ni0.25Fe48 | 100 | 250 | 5 | 75 | 75 | C2H2 + C2H4 + H2 |
Ni3Sn2 (ref. 10) | 76 | 200 | 24 | 80 | 80 | C2H2 + C2H4 + H2 |
Ni3ZnC0.7/C49 | 100 | 165 | 10 | 85 | 85 | C2H2 + H2 |
Ni1MoS/Al2O3 (ref. 25) | 100 | 120 | 16 | 90 | 90 | C2H2 + C2H4 + H2 |
Ni1/g-C3N4 (ref. 1) | 30 | 260 | 50 | 85 | 85 | C2H2 + C2H4 + H2 |
Ni1Cu2/g-C3N4 (ref. 1) | 100 | 160 | 350 | 90 | 90 | C2H2 + C2H4 + H2 |
The differences in the selectivity to C4 products on these catalysts indicate the different stabilities of the Ni, Ni3Ga and Ni3GaC0.5 catalysts. Therefore, stability tests were further carried out for the Ni, Ni3Ga and Ni3GaC0.5 catalysts in the presence of excess ethylene. As shown in Fig. 5d, e, S21 and S22,† the conversions of acetylene on the Ni and Ni3Ga catalysts decrease gradually with time on stream, showing poor catalytic stability. This could be ascribed to the accumulation of green oil on the catalysts due to the coupling of acetylene. Moreover, the selectivities to ethylene on the Ni and Ni3Ga catalysts also decrease slightly with the time on stream while those to ethane and C4 products increase slightly, which implies that the deposition of green oil is unfavourable for the semi-hydrogenation. Differently, the acetylene conversion on the Ni3GaC0.5 catalyst remains steady at 91.3% through the 36 hour stability test, and the selectivity toward ethylene could be maintained at 90.1% without legible decline, which are both superior to the Ni and Ni3Ga catalysts. All the above results unambiguously demonstrate that the Ni3GaC0.5 catalyst exhibits superior performance for the acetylene semi-hydrogenation.
The difference in the stabilities of Ni, Ni3Ga and Ni3GaC0.5 catalysts is explored by the thermogravimetric-differential thermal analysis (TG-DTG) and pyrolysis gas chromatography-mass spectrometer (GC-MS) measurements. As shown in Fig. 6a, the weight loss of the spent Ni3GaC0.5 catalyst (about 2.6 wt%), attributed to the oxidative decomposition of green oil, is lower than those of the spent Ni and Ni3Ga catalysts. Besides, in the DTG curves, the main peak clearly observed for the spent Ni3GaC0.5 catalyst shifts toward lower temperature in comparison with those of the Ni and Ni3Ga catalysts, which indicates that the small amount of hydrocarbons accumulated on the spent Ni3GaC0.5 catalyst are lighter than those on the Ni and Ni3Ga catalysts.4,5,8
The main composition of green oil formed on the used Ni, Ni3Ga and Ni3GaC0.5 catalysts is determined by pyrolysis GC-MS and shown in Fig. 6b. The result of pyrolysis GC-MS analysis of a standard sample completely mixed with various chain hydrocarbons is also included to identify the components in the green oil. The main intensities of peaks observed on the spent Ni and Ni3Ga catalysts are much stronger than those for the used Ni3GaC0.5 catalyst, indicating that more considerable green oil was accumulated on the Ni and Ni3Ga catalysts than on the Ni3GaC0.5 catalyst. More importantly, it can be obviously seen from Fig. 6c that the green oil accumulated on Ni and Ni3Ga catalysts contains more heavy hydrocarbons than those on the Ni3GaC0.5 catalyst, which is also revealed by the statistical average carbon number of the components contained in the green oil for the used Ni, Ni3Ga and Ni3GaC0.5 catalysts. These clearly reveal that the formation of green oil on the Ni3GaC0.5 catalyst is restrained as compared to those on the Ni and Ni3Ga catalysts.
DFT calculations were performed to gain more mechanistic insights into the boosted acetylene semi-hydrogenation on the Ni3GaC0.5 catalyst with the incorporation of C atoms in the lattice. As shown in Fig. 7a and Tables S2, S3,† the adsorption of C2H2 and C2H4 on the Ni3GaC0.5(111) surface is energetically favourable through the di-σ configurations with moderate adsorption free energies of −1.71 and −0.69 eV, respectively. In contrast, the adsorption free energies of acetylene and ethylene increase in the order of Ni3GaC0.5(111) < Ni3Ga(111) < Ni(111) (Tables S2–S7†), which is in good accordance with the predictions of the DOS analyses. The calculated free energy barriers of the initial two hydrogenation steps from C2H2 to C2H4 over the Ni3GaC0.5(111) surface are 0.66 and 0.36 eV with exothermic energies of 0.76 and 0.81 eV, respectively, indicating the decent hydrogenation activity of acetylene. The effective energy barrier (Geffa) is employed to further compare the differences in the hydrogenation activities on Ni, Ni3Ga and Ni3GaC0.5, and the lower Geffa indicates higher activity.50,51 More details on the calculation of Geffa are presented in the ESI, Fig. S23–S26 and Table S10.† The values of Geffa on the Ni(111), Ni3Ga(111) and Ni3GaC0.5(111) surfaces are 1.19, 1.35 and 1.67 eV, respectively, which suggest that the hydrogenation activity decreases in the order Ni > Ni3Ga > Ni3GaC0.5. The kinetics studies on these catalysts also reveal that the apparent activation energy for acetylene hydrogenation on the Ni, Ni3Ga and Ni3GaC0.5 catalysts also increases in the order Ni < Ni3Ga < Ni3GaC0.5 (Fig. S27†), which is in good accordance with the DFT results. The free energy barrier for further hydrogenation of the formed C2H4 species to C2H5 on the Ni3GaC0.5 (111) surface is calculated to be 1.18 eV, which is obviously higher than the desorption free energy of C2H4 (i.e., 0.69 eV). This energetics comparison demonstrates that the formed C2H4 species prefers to desorb from the surface rather than to be hydrogenated,8,17 highlighting the excellent selectivity to ethylene. Similar results are also seen on the sub-stable Ni3GaC0.5(200) surface, on which the free energy barrier for further hydrogenation of the formed C2H4 species to C2H5 is clearly higher than that for ethylene desorption (Fig. S30, Tables S9 and S11†).
For comparison, the hydrogenation of acetylene over the Ni(111) and Ni3Ga(111) surfaces was also investigated. As seen in Fig. 7b, the free energy barriers for the conversion of C2H2 to C2H4via two-step hydrogenations on the Ni3Ga(111) surface are 0.90 and 0.64 eV with exothermic energies of 0.51 and 0.57 eV, respectively. Notably, the free energy barrier for the hydrogenation of the formed C2H4 species is 0.55 eV, much lower than its desorption free energy, which reveals that ethylene on the Ni3Ga(111) surface is prone to hydrogenation to the undesired ethane before desorption. On the sub-stable Ni3Ga(200) surface, the hydrogenation of ethylene is also demonstrated to be more favorable than the desorption of ethylene (Fig. S29, Tables S8 and S11†). As shown in the ESI, Fig. S28,† similar results are also seen with the Ni(111) surface, on which the free energy barrier for the hydrogenation of C2H4 (i.e., 0.42 eV) is clearly lower than the desorption free energy (i.e., 0.82 eV). These results are well consistent with the remarkably lower selectivity to ethylene on the Ni and Ni3Ga catalysts than on the Ni3GaC0.5 catalyst (Fig. 5b).
Footnotes |
† Electronic supplementary information (ESI) available. See https://doi.org/10.1039/d2ta02216h |
‡ These authors contributed equally to this work. |
This journal is © The Royal Society of Chemistry 2022 |