Thana
Maihom
*ab,
Michael
Probst
c and
Jumras
Limtrakul
d
aDivision of Chemistry, Department of Physical and Material Sciences, Faculty of Liberal Arts and Science, Kasetsart University, Kamphaeng Saen Campus, Nakhon Pathom 73140, Thailand. E-mail: faastnm@ku.ac.th
bCenter for Advanced Studies in Nanotechnology for Chemical, Food and Agricultural Industries, Kasetsart University Institute for Advanced Studies, Kasetsart University, Bangkok, 10900, Thailand
cInstitute of Ion Physics and Applied Physics, University of Innsbruck, Innsbruck 6020, Austria
dSchool of Energy Science and Engineering, Vidyasirimedhi Institute of Science and Technology, Rayong 2120, Thailand
First published on 5th February 2026
The selective hydrogenation of acetylene to ethylene is a key reaction for producing polymer-grade ethylene in industrial processes. We study the efficiency of transition metals (Fe, Co, Ni, Cu, and Zn) confined in a chabazite (CHA) zeolite for the selective hydrogenation of acetylene to ethylene using density functional theory (DFT) calculations with the M06-L functional. The proposed reaction mechanism involves H2 dissociation, followed by the formation of an ethenyl intermediate and its subsequent conversion to ethylene. We find that Cu-CHA exhibits the highest catalytic activity among the studied catalysts and shows high selectivity for the hydrogenation of acetylene to ethylene based on the calculated overall reaction barrier and its selectivity parameter. The zeolite frameworks are found to stabilize all the species formed along the reaction pathway, but particularly at the transition states, thereby lowering all the activation barriers. We also find that the zeolite's dipole moment and metal charge are moderately accurate descriptors for predicting the overall activation barrier of the reaction. We use the sure-independence screening and sparsifying operator (SISSO) method to identify optimal nonlinear combinations of DFT-based descriptors,enabling accurate predictions without time-consuming reaction pathway calculations.
Zeolites serve as versatile silica-based supports for metal catalysts. They offer several advantages, including environmental friendliness, reusability, and regenerability, while their nanoporous frameworks impart size- and shape-selective properties. Recently, metals supported on various types of zeolites have emerged as promising catalysts for acetylene hydrogenation to ethylene such as Y-, Beta-, ZSM-12-, and CHA-supported non-noble metal catalysts.12–24 For example, Alhashmi et al.15 reported that single-atom cobalt (Co) supported on a Y zeolite efficiently catalyzed acetylene hydrogenation, achieving an ethylene selectivity of 90% ± 2% for full acetylene conversion and exhibiting a stable performance for over 400 h and a high turnover frequency (TOF). Similarly, an iron (Fe) atom anchored on the same zeolite exhibited an ethylene selectivity of up to 93%, a high TOF and excellent stability for over 600 h.16 Chai et al.20 reported the use of nickel (Ni), one of the first-row transition metals, confined within CHA zeolite frameworks, achieving 100% acetylene conversion with up to 97% selectivity toward ethylene under optimized conditions. Moreover, the introduction of modifiers further enhances the catalytic performance; for example, Sn-modified Ni/ZSM-1219 and alkali metal cation–modified Ni–CHA20 achieved complete acetylene conversion with high ethylene selectivity. These findings motivated us to investigate and compare the activity and selectivity of non-noble transition metals supported on zeolites, along with the influence of zeolite frameworks on acetylene hydrogenation to ethylene, which has not yet been reported.
To gain a fundamental understanding of the behaviors of zeolites, computational methods, especially those based on density functional theory (DFT) calculations, provide atomistic insights into energetics, electronic structures, and molecular geometries across the potential energy surface, which is information often inaccessible by experimental techniques. They especially enable the identification of active sites, adsorption characteristics and reaction pathways, offering valuable guidance for the rational design of efficient and selective catalysts. Among these quantities, the activation barrier is particularly crucial for elucidating trends in the catalytic performance of zeolite-based systems. Its determination requires locating transition-state structures, which can be computationally demanding.25 Therefore, more cost-effective approaches, particularly those identifying DFT-based descriptors, are valuable for estimating activation barriers. Combinations of descriptors can achieve good predictive accuracy by using the sure independence screening and sparsifying operator (SISSO) method26 if overfitting is carefully avoided. Recently, this approach has been successfully applied not only to predict activation energies but also to estimate transition-state energies for reactions on porous materials, including zeolites and metal–organic frameworks.27–30 To the best of our knowledge, the systematic application of SISSO to acetylene hydrogenation to ethylene over metal sites confined within zeolite frameworks has not previously been reported.
In this work, we investigate the catalytic activity and selectivity of transition metals (Fe, Co, Ni, Cu, and Zn) confined within the CHA zeolite framework for acetylene hydrogenation to ethylene using DFT-based quantum chemical calculations, providing detailed mechanistic and energetic insights. The effects of different metal species on catalytic performance and ethylene selectivity are systematically evaluated. Additionally, several DFT-based descriptors related to the geometric and electronic properties of the zeolites are identified to predict the overall activation barrier. The SISSO method is employed to derive compact nonlinear expressions.
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| Fig. 1 Cluster model of the metal-supported CHA zeolite used in this work. Si, Al, O, C, H and metal atoms are represented in green, pink, red, gray, white, and blue, respectively. | ||
All geometry optimizations of reactants, intermediates, products, and transition states in this work were carried out using the M06-L density functional32 as implemented in Gaussian 16.33 This functional incorporates medium-range dispersion interactions within its parameterization and is well-suited for systems containing transition metals.30 Its robustness and accuracy in describing adsorption and reaction mechanisms on zeolite frameworks have been established in our previous studies.34–41 The def2-SVP basis set was used to describe the C, O, and H atoms, while the Stuttgart–Dresden pseudopotential with a double-ζ basis set was applied for the transition metals. During geometry optimization, both the interacting molecules and the zeolite framework were fully relaxed with only the hydrogen atoms used for cluster termination being fixed. To characterize each stationary point along the reaction pathway, vibrational frequency analyses were conducted on the optimized structures at the same level of theory. These calculations also provide thermodynamic properties. They were evaluated at 453.15 K, corresponding to experimental studies on acetylene hydrogenation over zeolites.20 The Gibbs free energy (G) is evaluated according to eqn (1), as follows:
| G = Eel + Gcorr | (1) |
| Gcorr = Etot + kBT − TStot | (2) |
| ΔG = Gcomplex − Gprobe – GCHA | (3) |
We further discuss the reaction mechanism and the energetic trends of acetylene hydrogenation to ethylene on M-CHA (M = Zn, Cu, Ni, Co, or Fe). The reaction proceeds in three main steps: (i) hydrogen molecule dissociation, (ii) the formation of a surface ethenyl intermediate, and (iii) ethylene formation, as shown in Fig. 2.20 The relative free energy profile is given in Table 1, and the corresponding Gibbs free energy barriers (ΔG#) are illustrated in Fig. 3. The optimized structures for the reaction on M-CHA are displayed in Fig. S1–S5 of the SI.
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| Fig. 2 Reaction mechanism for the acetylene hydrogenation to ethylene on M-CHA. Si, Al, O, C, H and metal atoms are represented in green, pink, red, gray, white, and blue, respectively. | ||
| Species | Relative Gibbs free energy (kcal mol−1) | ||||
|---|---|---|---|---|---|
| Fe-CHA | Co-CHA | Ni-CHA | Cu-CHA | Zn-CHA | |
| Ads | 10.4 | 3.2 | 3.3 | 6.7 | 5.1 |
| TS1 | 32.7 | 24.6 | 17.7 | 18.7 | 21.0 |
| Int1 | 33.1 | 25.0 | 18.1 | 16.6 | 13.2 |
| Int1-Ace | 30.3 | 23.4 | 14.8 | 13.4 | 16.9 |
| TS2 | 40.1 | 35.9 | 25.0 | 22.7 | 43.0 |
| Int2 | −3.0 | −11.0 | −16.7 | −20.1 | −19.1 |
| TS3 | −1.5 | −7.8 | −13.5 | −14.6 | −13.5 |
| Prod | −42.4 | −49.1 | −49.6 | −39.6 | −46.3 |
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| Fig. 3 Gibbs free energy barrier for the acetylene hydrogenation to ethylene on M-CHA calculated at 453.15 K. | ||
The reaction starts with H2 binding to the metal site (Ads) in a symmetric configuration, with identical H⋯M distances. Upon adsorption, the H2 molecule becomes more positive, while the positive charge on the metal site decreases relative to the isolated zeolite systems, indicating electron transfer from H2 to the zeolite active site. This charge transfer leads to elongation of the H–H bond from 0.75 to 0.76–0.78 Å. In line with this minor geometrical change, the adsorption free energy of H2 adsorption is endothermic at 453.15 K for all the systems (see Table 1). The adsorbed H2 then dissociates via the transition state (TS1), in which the H–H bond is cleaved and the two hydrogen atoms are simultaneously transferred to the metal site and the oxygen atom (O1) of the zeolite, as illustrated in Fig. 2. In this state, the H–H bond distance is elongated, while the M⋯H and O1⋯H distances are shortened, indicating bond formation. The dissociation of H2 proceeds via heterolytic cleavage. This is shown by the NBO partial charge analysis, where H1 gains a negative partial charge while H2 acquires a positive one. The activation barriers for this step (Ea1), relative to the energy of the isolated molecule, increase as follows: Cu-CHA (12.0 kcal mol−1) < Ni-CHA (14.4 kcal mol−1) < Zn-CHA (15.9 kcal mol−1) < Co-CHA (21.4 kcal mol−1) < Fe-CHA (22.3 kcal mol−1), as shown in Fig. 3. These activation energies are in the same range as those previously reported45 for H–H activation on metal alkoxide MOFs. The value obtained for Ni-CHA is also consistent with previous theoretical studies.20 The lower barrier observed for Cu-CHA can be ascribed to its shorter H–H bond distance in the TS1 structure, which facilitates earlier bond activation, and thus stabilizes the transition state. The NBO charge analysis also shows that the hydride species in TS1 of Cu-CHA is less negative than the ones associated with the other metals (see Table S1). This stems from a larger donation of electron density from the H2 σ-bonding orbital into the vacant orbitals of Cu, which contributes to the lower activation barrier. The transition state subsequently leads to the formation of a metal-bound hydride and a proton bound to the zeolite oxygen atom (Int1).
An acetylene molecule diffuses and adsorbs on the metal-bound hydride site (Int1-Ace) with calculated relative energies, referenced to the isolated reactants, ranging from 13.4 to 30.3 kcal mol−1 (see Table 1). Acetylene is then hydrogenated to form the ethenyl intermediate via the TS2 transition state. The M–H1 bond breaks, transferring H1 to the C1 carbon of acetylene, while a new bond forms between C2 and metal. TS2 is considered a four-center transition state, formed through the breaking of the M–H1 bond and the formation of the C1–H1 and M–C2 bonds. The activation barriers (Ea2) relative to the co-adsorption complex are 9.8, 12.5, 10.2, 9.3, and 26.1 kcal mol−1 for Fe-, Co-, Ni-, Cu-, and Zn-CHA, respectively (see Fig. 3). Next, the ethenyl intermediate (Int2) is formed at the active site of M-CHA. This species has been experimentally observed at 453 K on the Ni-CHA zeolite.20 As revealed by the NBO charge analysis (see Table S1), the lower activation barrier for Cu-CHA originates from the smaller positive charge on the Cu center in Int1-Ace compared to the other metals. This causes a weaker electrostatic interaction with the hydride species and a lower activation barrier for M–H bond cleavage. The complexation energies for the formation of this intermediate are exothermic in all the systems (−3.0 to −20.1 kcal mol−1), as shown in Fig. 3.
Following the formation of the ethenyl intermediate, the reaction proceeds through its hydrogenation, resulting in the formation of ethylene. The transition state of this step, as shown in Fig. 2 (TS3), involves the concerted cleavage of the O1–H2 bond and formation of the H2–C2 bond, resulting in an increased O1–H2 distance and a decreased H2⋯C2 distance. The activation barriers (Ea3) in this step are low, ranging from 1.5 kcal mol−1 for Fe-CHA to 5.6 kcal mol−1 for Zn-CHA. This indicates that ethenyl can be easily converted to the ethylene product. The lower activation barrier for Fe-CHA can be attributed to the less negative charge on the Fe center in TS3 (see Table S1). Thus, proton release is facilitated and the energy barrier is lowered. Subsequently, the ethylene product (Prod) adsorbs on the Ni active site through its π bond, with a complexation energy ranging from −39.6 to −49.6 kcal mol−1 relative to the isolated molecule. Finally, the desorption of the product from the M-CHA surface requires 3.9, 10.6, 11.1, 1.1, and 7.8 kcal mol−1 for Fe-, Co-, Ni-, Cu-, and Zn-CHA, respectively.
| ΔG#overall = GTS2 − GAds |
The ΔG#overall values are 29.7, 32.7, 21.8, 16.0, and 37.9 kcal mol−1 for Fe-, Co-, Ni-, Cu-, and Zn-CHA, respectively (see Fig. 4). The lower overall activation barrier for Cu-CHA is associated with the higher energetic stability of TS2 (see Table 1). This enhanced stability of TS2 for Cu-CHA is directly linked to the negligible charge accumulation on the ethenyl intermediate, which remains close to neutral (see Table S1). The minimized internal electrostatic repulsion results in the lowest transition-state energy among the studied metal centers.
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| Fig. 4 Overall Gibbs free energy barrier (ΔG#overall) and selectivity parameter (ΔΔG) for the acetylene hydrogenation to ethylene on M-CHA calculated at 453.15 K. | ||
To check the importance of dispersion effects, we compared the M06-L results with those obtained using M06-L-D3, a model that explicitly includes dispersion terms, for ΔG#overall. The results show that the trends in ΔG#overall across the metal series remain unchanged (Table S2). This indicates that the inclusion of dispersion corrections is not crucial for our conclusions.
We further validated the computational methodology employed in this work by benchmarking the M06-L functional against another commonly used functional, B3LYP combined with both Grimme's D3 dispersion correction and the D3(BJ) damping scheme, and by comparing results obtained with the def2-SVP and def2-TZVP basis sets (see Tables S2 and S3), respectively. In all cases, the ΔG#overall values exhibit the same trends as found with M06-L, identifying Cu-CHA as the most favorable candidate. Therefore, we believe that M06-L in combination with the chosen level of theory provides a reliable description of the systems studied.
In addition to the catalytic activity, the selectivity for ethylene formation represents a crucial factor in acetylene hydrogenation. As reported previously, ethylene desorption from the catalyst surface is generally favored over its further hydrogenation.46,47 The latter requires the dissociation of an additional H2 molecule as the initial step for hydrogenating the ethylene formed in the primary reaction. Consequently, high selectivity towards ethylene formation is achieved when the free energy barrier for ethylene desorption is lower than that for a subsequent H2 dissociation step, leading to ethylene over-hydrogenation. The difference between these two barriers has been used as selectivity parameter in previous studies on selective acetylene hydrogenation on metal–alkoxide MOFs.38 Accordingly, eqn (4) defines this difference between two relative free energies:
| ΔΔG = ΔGover – ΔGdes | (4) |
Concerning the issue of ethylene selectivity discussed above, we explicitly investigated the possible over-hydrogenation of ethylene to ethane on all the studied zeolites. This process proceeds via two consecutive hydrogenation steps: firstly, hydrogenation of ethylene to form the ethyl intermediate, followed by a second hydrogenation step leading to ethane formation (see Fig. S7). The relative free energies are reported in Table S4. The calculated overall free-energy barriers for the hydrogenation of ethylene to ethane, defined as the free-energy difference between the co-adsorbed ethylene and the H2 state (Int3; rate-determining intermediate) and the transition state for ethyl formation (TS5; rate-determining transition state) are 45.1, 43.3, 31.0, 16.1, and 50.7 kcal mol−1 for Fe-, Co-, Ni-, Cu-, and Zn-CHA, respectively. These barriers are higher than those associated with the initial acetylene hydrogenation to ethylene and also exceed the free energy barriers for ethylene desorption reported above. These results indicate that once formed, ethylene preferentially desorbs from the catalyst surface rather than undergoing further hydrogenation to ethane. This kinetic preference supports the notion of high selectivity toward ethylene formation in these systems.
To reveal the influence of the zeolite framework, we carried out single-point calculations on the 42T geometries using a reduced 12T cluster model of M-CHA, which preserves only the D6R structure (see Fig. S8). The relative energies of the systems along the reaction coordinate are summarized in Table S1. We observed a strong linear correlation between the relative energies calculated from the 42T and 12T clusters, as indicated by the coefficients of determination (R2) ranging from 0.928 to 0.979, demonstrating that both models follow the same trend. Nevertheless, the relative energies obtained from the 42T cluster model are consistently lower than those from the 12T cluster, particularly for the reaction intermediates and transition states. The energy differences fall in the ranges of 6.3–15.7 kcal mol−1 for Fe-CHA, 0.9–11.0 kcal mol−1 for Co-CHA, 2.4–13.6 kcal mol−1 for Ni-CHA, 0.3–15.9 kcal mol−1 for Cu-CHA and 4.6–14.7 kcal mol−1 for Zn-CHA, as summarized in Table S5. These results reflect the stabilizing effect of the extended zeolite framework. Fig. 5 shows the result of the linear fit between the ΔG#overall from the large and the small cluster models. The R2 value of this regression is 0.929. The trends in ΔG#overall are the same for all the metal systems when the 12T model is used. However, the ΔG#overall values for the 12T cluster are consistently higher by 11.5–14.3 kcal mol−1 than those from the 42T cluster for all the zeolites (see Table S5). This indicates that the extended zeolite framework stabilizes the species formed along the reaction coordinates and reduces the overall barrier, thereby enhancing the activity of the metal active site.
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| Fig. 5 Linear scaling relationship between the overall activation barriers obtained from the 12T and 42T models. | ||
To ensure that the 42T cluster model used in this work is converged with respect to cluster size, single-point calculations of ΔG#overall were performed at the same level of theory on extended 78T cluster models based on the structures optimized with the 42T model (see Fig. S9). The ΔG#overall values of all the systems using the 42T model are nearly identical to those obtained with the 78T model, and more importantly, the trends of ΔG#overall across the metal series remain unchanged (see Table S6). These results indicate that the practical 42T cluster model is sufficiently large to accurately represent the interactions between the adsorbates and the zeolite framework.
The R2 and root-mean-square errors (RMSE) for the linear correlations between the descriptors and ΔG#overall are presented in Table S7. A reasonably strong linear relationship is observed for Di and ρ, with R2 values of 0.718 and 0.817 and corresponding RMSEs of 5.3 and 4.3 kcal mol−1, respectively. ΔG#overall decreases with decreasing metal charge and increasing dipole moment. These linear relationships for predicting ΔG#overall are:
| ΔG#overall = −12.065 × Di + 69.712 kcal mol−1 | (5) |
| ΔG#overall = 72.799 × ρ + 2.213 kcal mol−1 | (6) |
The predictive power of these simple regression models remains moderate, as reflected by the R2 and RMSE values reported above. To enhance it, we employ the SISSO method and generate more complex descriptors by screening a large set of candidates formed from combinations of primary descriptors through various mathematical expressions. In this work, 8 primary descriptors, as outlined above, are used as inputs. These descriptors are expanded by applying various mathematical operators (+, −, ×, ÷, exp, exp−, −1, 2, 3, √, and | |) to generate nonlinear expressions forming the candidate descriptor space. Due to the limited size of the dataset, all 10 data points were used for model training, which is a common and accepted practice in SISSO applications involving small datasets. Within the SISSO framework, the Sure Independence Screening (SIS) procedure is first applied to rank candidate descriptors according to their correlation with the target property, ΔG#overall. Subsequently, the sparsifying operator based on L0 regularization is used to identify the most relevant low-dimensional descriptors. The descriptor dimensionality (D) is limited to 3, with a maximum of 3 operations per term, resulting in a total of 3 model levels.
Table 2 lists the comprehensive mathematical equations derived for each model complexity. Fig. 6 shows a comparison between the ΔG#overall values from DFT and those predicted by SISSO, including the corresponding R2 and RMSE for the trained models. The increase in the coefficient of determination, R2, from 0.938 for the 1D model to 0.975 and 0.997 for the 2D and 3D models, respectively, shows that the reproduction of the energetic trends improves progressively. The corresponding RMSE values decrease from 2.5 to 1.6 and 0.5 kcal mol−1, reflecting a substantial reduction in the errors in predicting ΔG#overall for the higher-dimensional models. The robustness of these predictive models is validated to prevent overfitting using the leave-one-group-out cross validation (LOOCV) procedure.48 The R2 and RMSE values are used to evaluate the overall cross-validation performance. The high R2 values obtained (0.938–0.997) together with low RMSEs (0.1–1.0 kcal mol−1) indicate that the SISSO models for predicting ΔG#overall are robust and not prone to overfitting. It should be noted that the SISSO analysis in this work is based on a limited but chemically consistent dataset comprising five transition-metal-exchanged CHA zeolites described by two cluster models. SISSO has been shown to be effective in small-data regimes for descriptor discovery.49 Nevertheless, expanding the dataset to include additional metals and different zeolite topologies would be beneficial for assessing both predictive power and descriptor transferability. These extensions will be the focus of future work.
We can try to rationalize the physical meaning of the nonlinear descriptors selected by the SISSO algorithm for describing the overall activation free energy. The 1D descriptor captures the dominant contribution to the activation barrier by combining the average metal–oxygen bond distance (BM–O) with the dipole moment (Di) and the HOMO energy (EH). The inverse cubic dependence on BM–O highlights the dominant role of the metal–oxygen interaction strength in governing the overall activation barrier, whereby shorter BM–O distances tend to correspond to lower barriers. This geometric contribution is further modulated by the Di/EH term, which reflects the influence of electronic polarization and donor ability of the metal-exchanged CHA zeolites. In particular, a higher dipole moment is associated with a reduced activation barrier. Overall, the 1D descriptor containing three basis properties captures the leading geometric–electronic control of the reaction barrier and provides a physically transparent baseline model for describing the catalytic activity trend.
The 2D descriptor extends the 1D model by adding an additive term that contains the Mulliken charge of the metal center (ρ), coupled with the mismatch between BM–O and Di effects. This additional term accounts for local charge redistribution at the active site, indicating that the activation barrier is not determined solely by the bond strength but is also sensitive to the degree of charge accumulation and polarization around the metal center. The improved performance of the 2D model demonstrates the importance of simultaneously considering geometric structure and electronic charge effects.
The 3D descriptor further includes higher-order electronic properties, including the LUMO energy (EL), global hardness (η), and electrophilicity index (ω), together with charge ρ. The inclusion of these electronic terms further improves the prediction accuracy by approximately the same amount as going from the one- to the two-dimensional expression.
Supplementary information (SI) is available. See DOI: https://doi.org/10.1039/d5cp04172d.
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