Rajesh Kumar
Raju
ab
aNational Research Council Canada, Clean Energy Innovation (CEI) Research Centre, Mississauga, Ontario L5K 1B4, UK. E-mail: rajesh.raju@nrc-cnrc.gc.ca; rajesh444@gmail.com
bSchool of Chemistry, University of Birmingham, Birmingham B15 2TT, UK
First published on 25th March 2025
The electrocatalytic reduction of nitrogen (NRR) to ammonia on metal nanoclusters represents a transformative approach to sustainable ammonia synthesis, offering a greener alternative to the highly energy-intensive Haber–Bosch process, which is a significant contributor to global CO2 emissions. By harnessing renewable electricity under ambient conditions, electrocatalytic NRR could dramatically lower the carbon footprint and enable decentralized, on-demand ammonia production. However, the inherent stability of N2 presents a major obstacle to its efficient activation. Metal nanoclusters, with their distinctive electronic and structural characteristics, have emerged as highly promising catalysts to overcome this challenge. This study systematically investigates the NRR catalytic performance of a broad spectrum of d-block and p-block metal nanoclusters. Through the use of Genetic Algorithms (GA) for global minimum structure optimization and comprehensive mechanistic pathway analysis, we uncover key trends in N2 activation, NRR reaction pathways, selectivity, and efficiency across various nanoclusters. Our findings provide critical insights into the design of advanced NRR electrocatalysts, paving the way for more sustainable and efficient technologies for ammonia production.
Electrocatalytic nitrogen reduction reaction (NRR) presents a promising alternative for sustainable ammonia production by utilizing renewable electricity to drive the conversion of N2 to NH3 under ambient conditions.6–9 This approach has the potential not only to reduce the carbon footprint of ammonia production but also to enable decentralized and on-demand synthesis, which could transform the fertilizer industry and related sectors. However, achieving practical and efficient ammonia synthesis through electrocatalytic NRR is challenging due to several formidable obstacles.
One of the main challenges is the activation of the highly stable N2 molecule, which possesses a triple bond with a dissociation energy of 941 kJ mol−1, making it difficult to break.10 Additionally, the NRR competes with the hydrogen evolution reaction (HER), which often dominates under electrochemical conditions, reducing the selectivity and yield of NH3. The low solubility of N2 in aqueous electrolytes and the difficulty of efficient electron transfer to N2 further complicate the process.
Nanoclusters have emerged as a particularly promising class of materials for addressing these challenges in electrocatalytic NRR.11–20 These nanoclusters, characterized by their distinct electronic, optical, magnetic, and chemical properties, offer significant advantages over bulk materials and larger nanoparticles due to their exceptional surface-to-volume ratio and unique electronic structures.21–26 Nanoclusters typically composed of a few to a few hundred metal atoms and are extremely monodispersed small nanoparticles with atomic precision, exhibit a transition from the bulk to molecular regions. The catalytic behavior of nanoclusters can be finely tuned by controlling their size, shape, and composition, providing opportunities to enhance NRR activity and selectivity. Moreover, nanoalloys, or alloy nanoclusters, have garnered significant interest in nanocatalysis, offering catalytic properties that differ markedly from those of pure metal nanoclusters.27–32 The synergistic effects arising from the combination of different metals in nanoalloys can lead to improved N2 activation, stabilization of key intermediates, and suppression of competing reactions like HER.
Studies have shown the efficiency of various nanocluster systems including nanoalloys for NRR.33 Jiang et al. highlighted that low-coordinate atoms in amorphous Ru nanoclusters improve ammonia yield and faradaic efficiency and outperforming their crystalline counterparts.34 Han et al. demonstrated that Ni doping in Ag4Ni2 nanoclusters enhanced performance by suppressing HER and enabling charge reconstruction.35 Ding et al. emphasized the activity of Ru-doped CeO2 nanorods due to oxygen vacancies providing active N2 adsorption sites.36 Tan et al. reported that Mo-decorated Au25 nanoclusters improved catalytic activity for NH3 production.37 Shi et al. showed that optimizing the Pd0.2Cu0.8 alloy composition on graphene boosted NRR performance.38 Ahmed et al. demonstrated synergistic effects of CoFe2O4 clusters on graphene, enhancing ammonia synthesis.39 Suryanto et al. revealed that Ru nanoclusters on 2H-MoS2 suppressed HER and improved NRR selectivity.40 Catalysts such as RhPx nanoparticles41 embedded in N, P dual-doped carbon films and Rh2Sb nanorods42 with rough surfaces have shown significant improvements in NRR. Surface-modified systems like Pd nanoparticles with tannic acid43 and Cu nanoparticles supported on TiO244 with oxygen vacancies have leveraged metal–support interactions for better catalytic activity. High-entropy alloys, such as RuFeCoNiCu45 nanoparticles with small size alongside bimetallic systems like FeWSx@FeWO4,46 and NbTiO4 nanoparticles supported on nitrogen-doped carbon nanorods,47 have also emerged as highly effective catalysts. Additional systems, including ultrafine Rh nanoparticles on CNT,48 Au nanoparticles anchored on a MOF,49 carbon–supported Pt–Rh nanoparticles,50 Ru-based Heusler alloys,51 Au@Cu2−xSe,52 and V2O3/VN53 further highlight the broad potential of nanocluster and alloy catalysts in advancing NRR efficiency through targeted structural and electronic modifications.
Modeling plays a pivotal role in designing and optimizing nanoclusters for nitrogen reduction reaction (NRR), enabling researchers to predict and refine the electronic structure and surface properties of these materials to achieve optimal catalytic performance. While most prior density functional theory (DFT) studies have focused on NRR catalysis over metal surfaces or metal-oxide surfaces, investigations into nanocluster catalysts remain relatively limited.33,54–59 When nanoclusters have been studied, they are often restricted to a specific metal or a small subset of metals.57,60–62 Additionally, many of these studies rely on known crystal surface lattices to model nanoclusters, often overlooking the possibility that the true global minimum (GM) configurations of nanoclusters, including adsorbate-bound ones, may differ significantly from bulk geometries. Given the vast number of possible nanocluster configurations with near-identical energies, accurately identifying the GM for each nanocluster is crucial to properly assess its catalytic behavior.
A significant challenge arises when NRR intermediates or other adsorbates form on the nanocluster surface, as these interactions can dramatically alter the electronic and geometric properties, leading to reorganization or rearrangement of nanocluster moiety. This reconfiguration can shift the nanocluster towards a new, stable minimum, which may drastically impact the overall energetics and reaction pathways. Therefore, determining the correct geometry for both pristine and adsorbate-bound nanoclusters is essential for accurately predicting catalytic performance and optimizing nanoclusters for NRR.
In this study, we introduce a novel approach that combines global minimum structure searching, using genetic algorithms (GA),63–65 with electrochemical studies of NRR on a wide range of metal nanoclusters. The GA-driven search explores the vast configurational space of nanoclusters, allowing us to identify the most stable structures and their corresponding energetics under realistic catalytic conditions. This is particularly critical since the adsorption and interaction of nitrogen intermediates can dramatically alter the structural and electronic properties of nanoclusters, and understanding these changes is essential for accurate predictions of catalytic performance. By coupling GA-based structure optimization with detailed electrochemical analyses of reaction intermediates and pathways, our work provides a comprehensive view of how nanoclusters behave in NRR. This allows for the identification of catalytically favorable nanocluster configurations that were previously overlooked, offering new insights into improving catalytic efficiency in nitrogen fixation reactions.
This study provides a systematic evaluation of size-selected 10-atom nanoclusters for NRR, encompassing all transition metals (d-block) from the 3d, 4d, and 5d series, as well as selected p-block metals, including Al, Ga, In, Tl, Sn, Pb, and Bi. The deliberate inclusion of p-block metals alongside d-block metals introduces a novel dimension to NRR studies. Transition metals are well-recognized for their partially filled d-orbitals, which facilitate the activation of N2 through π-back-donation, while p-block metals, with their unique electronic and geometric properties, offer complementary pathways for stabilizing intermediates and modulating reaction mechanisms. This expanded scope addresses a critical gap in the literature, where studies on nanocluster catalysts are often limited to a few metals or bulk-like configurations.
While s-block and f-block metals were excluded, this decision was guided by their limited catalytic relevance to NRR. s-block metals, lacking d-orbitals, exhibit weak binding with N2 and intermediates, while f-block metals, though theoretically intriguing, pose challenges due to their complex electronic configurations and limited practical applications in NRR catalysis. Prioritizing d-block and p-block metals allows for a focused evaluation of elements with the highest potential for catalytic activity.
Unlike most previous studies that focus on bulk surfaces or limited subsets of metals, this work systematically evaluates a broad spectrum of metal nanoclusters, uncovering catalytic trends that were previously unexplored. In addition to structural optimization, this study advances the field by performing detailed mechanistic pathway analyses, including adsorption free energies, charge transfer dynamics, and potential-determining steps. The inclusion of linear scaling relationships and descriptor-based analyses provides actionable insights for rational catalyst design, offering a framework for optimizing nanocluster catalysts.
The study also adopts a rigorous computational methodology to ensure the accuracy of results. Global minimum configurations for both pristine and adsorbate-bound nanoclusters were identified using a well-established Genetic Algorithm (GA). This approach overcomes the limitations of previous studies that often rely on assumed geometries derived from bulk surfaces, which may not represent the true energetics of nanocluster systems. By systematically determining the most stable configurations, we provide a robust foundation for analyzing catalytic behavior.
This comprehensive and methodical approach not only highlights the catalytic potential of transition metal nanoclusters but also uncovers the underexplored promise of p-block metal nanoclusters, bridging the gap between conventional and unconventional materials. By identifying periodic trends and offering design principles for nanocluster-based catalysts, this work lays the groundwork for sustainable and efficient ammonia production technologies.
Furthermore, this study extends beyond traditional computational screening by offering experimentally relevant insights into the feasibility of nanocluster-based NRR catalysts. While small nanoclusters are often considered metastable, their stability can be significantly influenced by the choice of ligands, supports, or reaction conditions, which can enhance their practical viability. By systematically evaluating adsorption trends and potential-determining steps across a diverse range of nanoclusters, this work provides a predictive framework that experimentalists can leverage to synthesize and test the most promising candidates. The identification of stable adsorption configurations, coupled with charge transfer analyses, helps pinpoint key factors that govern catalytic efficiency at the nanoscale. These findings not only refine our fundamental understanding of NRR catalysis but also facilitate the rational design of stable, size-selected nanoclusters for real-world electrochemical applications.
The stability of small metal nanoclusters is indeed a critical factor in determining their practical applicability in electrochemical catalysis. It is well established that most small-sized metal clusters, including 10-atom clusters, can exhibit metastability, often requiring inert environments for synthesis and preservation. However, size-selected small nanoclusters have been experimentally demonstrated to behave differently from their bulk or larger counterparts, showing distinct electronic structures, binding affinities, and catalytic behaviors. Such experimental studies validate the importance of investigating nanoclusters at this size scale, as they can exhibit unique catalytic properties that are otherwise absent in larger clusters or bulk materials.
The overall aim of our work is a comprehensive evaluation of different metal nanoclusters to establish systematic trends in NRR activity. By analyzing a diverse range of nanoclusters, including metals from the 3d, 4d, 5d, and p-blocks, this study offers valuable insights into the fundamental structure–activity relationships that govern catalytic performance at the nanoscale. While the absolute stability of pristine 10-atom clusters in realistic electrochemical environments remains an open question, our work serves as a crucial first step in identifying promising candidates that warrant further experimental validation. The trends derived from this study provide a fundamental understanding of how metal composition and nanocluster size influence NRR performance, facilitating the rational design of stable and efficient electrocatalysts. Thus, rather than being a limitation, our approach lays the groundwork for experimentalists to explore the most promising nanoclusters under realistic electrochemical conditions, potentially leading to novel strategies for stabilizing and utilizing these clusters in practical applications.
To locate the global minimum configurations of first-row transition metal (TM) nanoclusters, we employed the GIGA version of the Birmingham Parallel Genetic Algorithm (BPGA)63–65 at the DFT level. The GA process begins by generating a set of random geometries—in this study, 10 initial geometries—which are then relaxed into local minima to form the initial population in the pool. Based on predefined crossover and mutation rates, the GA applies crossover and mutation operations to members of the pool to generate new structures. For the crossover operation, pairs of clusters are selected using a weighted roulette-wheel66 selection method, and mating is performed using a variant of the Deaven and Ho phenotypic cut-and-splice method,67 resulting in a single offspring.
Various mutation operations, such as “move,” “rotate,” “twist,” “partial inversion,” and “rattle,” are applied to randomly selected clusters via roulette-wheel selection. For instance, in skin mutation, 80% of the cluster atoms remain intact while 20% are repositioned randomly around the cluster. In rattle mutation, 40% of the atoms nearest to a randomly chosen atom are moved. Change core mutation alters the core of the cluster, while rotation and twist mutations rotate or twist a percentage of cluster atoms. Partial inversion operation inverts a subset of cluster atoms relative to their geometric center, and tunnel operation relocates the atom farthest from the center to the opposite side of the cluster. The objective of these operations is to maintain diversity within the pool, preventing stagnation after several generations.
We ran the genetic algorithm for a minimum of 400 generations, and in some cases, more than 1500 generations were required. Each generation involved the relaxation of newly generated geometries through crossover or mutation operations. To ensure the robustness of our results, we performed a parallel run for each cluster to confirm that both BPGA runs converged on the same global minimum configuration.
The most stable adsorbate configurations on each nanocluster were determined by optimizing the cluster-adsorbate complexes using the same DFT protocol (PBE functional, DFT-D3 corrections, and higher plane wave cutoff energy). The Bader77 method was employed for charge analysis on these optimized structures. The free energies of the adsorbates were calculated by performing vibrational analysis, assuming the nanoclusters were immobilized on supports. Thermal corrections, including zero-point energy, enthalpy, and entropy corrections, were computed using harmonic vibrational frequencies at 298.15 K with VASPKIT.78 These corrections were added to the DFT electronic energies to obtain the Gibbs free energies of the adsorbates, which are reported as standard values (ΔG0) calculated at 298.15 K.
ΔG[A* + (H+ + e−) → AH*] = μ(AH*) − μ(A*) − [μ(H+) + μ(e−)] |
(H+) + μ(e−) = 0.5μ(H2(g)) − |e|U |
ΔG = ΔG0 + |e|U |
Previous studies have shown that hydrogen bond stabilization introduces a small correction, approximately 0.08 eV per bond.54,81 Consequently, the overall impact on the onset potentials in our calculations is expected to be minimal, with changes likely to be less than 0.1 eV.54,81 Given the negligible effect, and consistent with previous studies, we have chosen not to include these corrections, as they would not significantly influence our results.
Fig. 1 illustrates the global minimum configurations of the nanoclusters, along with selected examples of adsorbate-bound structures. Additionally, Tables S1 and S2 (ESI†) provides detailed bond distances for N–metal and N–N, across all adsorbates. Notably, the N–N bond distance is significantly elongated on early transition metal nanoclusters, ranging from approximately 1.33 Å to 1.35 Å. This elongation serves as a strong indicator of N2 activation on these early TMs, reflecting their high propensity for facilitating the initial nitrogen bond cleavage. Similarly, mid-transition metal nanoclusters, including Ta, Nb, V, W, Tc, Cr, and Mn, exhibit moderate N2 activation, as evidenced by their elongated bond distances in the range of 1.31 Å to 1.20 Å.
In contrast, late transition metal nanoclusters such as Cu, Ag, and Au do not exhibit significant elongation in N–N bond distances. Similar trends are observed for p-block and pseudo-p block metal nanoclusters, suggesting minimal activation of N2 on these metal surfaces. This minimal elongation is indicative of a lower catalytic efficiency for N2 activation on these metal nanoclusters. The distinct variation in N–N bond elongation across different metal categories underscores the varying degrees of N2 activation, which correlates with the electronic properties of the metals studied.
In our previous work on CO2 reduction using first-row transition metal (TM) nanoclusters, we identified 3 to 10 global minimum (GM) configurations for Sc–Cu nanoclusters.82 Additionally, we conducted a detailed comparison of the GM structures and low-lying geometric configurations obtained from the Basin-Hopping Particle Swarm Genetic Algorithm (BPGA) method with those reported in the literature.83–104 In Our analysis revealed that different computational methods and variations in DFT settings can sometimes lead to different GM configurations due to differences in convergence criteria and energy landscapes. However, despite these variations, all studies consistently identified the same set of geometric configurations within the low-energy nanocluster regime. While the relative energetic ordering of these configurations may change across different methods, the low-lying isomers remain energetically competitive and are likely to coexist under realistic conditions.
Given the close energetic proximity of these low-energy isomers, we extended our analysis beyond the global minimum configurations to ensure a comprehensive evaluation of adsorbate binding. To ensure a thorough assessment of adsorbate binding on nanoclusters, we extended our analysis beyond the global minimum configurations by incorporating ten low-energy isomers, as their energy differences from the global minimum were often minimal. Given the competitive stability of these low-lying isomers, we conducted an extensive search to determine the most energetically favorable binding sites. This involved exploring all possible unsymmetrical edges, metal atom sites, and diverse binding modes and orientations of the adsorbates. By systematically evaluating cluster-adsorbate interactions across a wider range of configurations, we enhanced the accuracy of identifying the most stable adsorbate binding sites. This approach provides a more comprehensive understanding of the active sites that influence catalytic performance, ensuring that structural variations among low-energy isomers are accounted for in our analysis.
In the 4d block, yttrium (Y) and zirconium (Zr) stand out with strong negative adsorption free energies of −3.49 eV and −3.44 eV, respectively. The adsorption energies of other 4d transition metal nanoclusters vary from weak to moderate, with technetium (Tc), ruthenium (Ru), rhodium (Rh), and palladium (Pd) exhibiting moderate adsorption free energies ranging from −0.83 eV to −0.59 eV. Niobium (Nb) and molybdenum (Mo) show mildly favorable adsorption energies of −0.29 eV and −0.13 eV, respectively. In contrast, silver (Ag) and cadmium (Cd) exhibit positive adsorption free energies, indicating weaker interactions with N2. Cadmium, despite being a 4d metal, mirrors the p-block behaviour seen in zinc, with a positive adsorption energy that suggests less effective N2 adsorption.
Among the 5d transition metals, hafnium (Hf) exhibits the most negative adsorption free energy at −3.54 eV, indicating a highly favorable interaction with N2. Tungsten (W) also shows strong adsorption, with a free energy of −1.37 eV, the most negative among the mid-transition metals in the 5d series. Other 5d metals, including rhenium (Re), osmium (Os), tantalum (Ta), iridium (Ir), and platinum (Pt), display moderate adsorption free energies in the range of −0.86 eV to −0.32 eV. Gold (Au) and mercury (Hg), however, exhibit slightly positive adsorption energies, indicating weaker adsorption characteristics. It is noteworthy that lanthanum (La), a 5d metal, was not included in this analysis.
The p-block metal nanoclusters, including aluminum (Al), gallium (Ga), indium (In), thallium (Tl), tin (Sn), lead (Pb), and bismuth (Bi), predominantly exhibit positive adsorption free energies for N2, reflecting very weak or unfavorable adsorption. This trend underscores the lesser suitability of these metals for N2 adsorption applications compared to transition metals, which generally exhibit negative adsorption free energies.
Overall, the analysis reveals that early transition metal nanoclusters, particularly those with d1 and d2 electronic configurations, exhibit significantly larger negative adsorption free energies, indicating strong N2 adsorption potential. In contrast, mid- and late-transition metal nanoclusters show weaker to moderate N2 adsorption characteristics. Metals with a completely filled d-shell configuration (d10), such as Zn, Cd, and Hg, do not exhibit favorable adsorption free energies, as evidenced by their positive values. These metals, although traditionally considered transition metals, exhibit adsorption behaviors more akin to p-block metals and are therefore classified as “pseudo-p-block” metals in this context. This analysis highlights the critical role of electronic configuration and metal selection in optimizing N2 adsorption or activation for catalytic applications.
Here after to make our studies across various d and p-block metal nanoclusters, we use the following classifications:
(a) Early transition metals: TM with d1 and d2 configurations (Sc, Ti, Y, Zr, Hf)
(b) Mid transition metals: TM with d3 to d7 configurations (V, Cr, Mn, Fe, Co, Nb, Mo, Tc, Ru, Rh, Ta, W, Re, Os, and Ir)
(c) Late transition metals: TM with d8 to d9 configurations (Ni, Cu, Pd, Ag, Pt and Au)
(d) Pseudo P-block metals: d10 configurations (Zn, Cd, and Hg)
(e) P-Block metals. (Al, Ga, In, Tl, Sn, Pb, and Bi)
In contrast, the associative mechanism is more favorable under mild electrochemical nitrogen reduction reaction (NRR) conditions, as it bypasses the need for NN bond dissociation, thereby avoiding the high energy demand associated with N2 bond cleavage. The reaction proceeds via six proton-coupled electron transfer (PCET) steps, making it particularly feasible for electrochemical systems. Given these conditions, we excluded both the dissociative mechanism and the enzymatic pathway, which typically involves the side-on binding of N2, as seen in biological nitrogenases or extended metal surfaces. Nanoclusters, with their limited surface area and distinct structural properties, do not accommodate such configurations. Instead, we meticulously explored every potential binding site and orientation for N2 on nanoclusters, ensuring we captured the most stable arrangement that supports the associative mechanism.
The associative mechanism is further categorized into:
• Associative alternating pathway: hydrogenation occurs alternately on both nitrogen atoms, resulting in the sequential release of two ammonia molecules.
• Associative distal pathway: hydrogenation occurs primarily on one nitrogen atom before the second, leading to the sequential release of two ammonia molecules.
The NRR associative pathways involve key intermediates such as *NNH, *NHNH, *NNH2, *NHNH2, *NH2NH2, *N, *NH, and *NH2. The following section provides a detailed analysis of the energetics associated with each PCET step across these intermediates.
Our study focuses predominantly on the associative mechanism, encompassing both the distal and alternating pathways. In addition, we explore mixed-type pathways, including the distal-alternating (I) and (II) pathways, as well as the alternating-distal (I) pathway. These mixed-type pathways, which are typically underexplored in previous studies of NRR over heterogeneous catalysts, offer novel insights into the NRR mechanism.
Path I: * + N2 → NNH* → NNH2* → N* → NH* → NH2* → * Distal |
Path II: * + N2 → NNH* → NNH2* → NHNH2* → NH* → NH2* → * Distal-alternative mixed I |
Path III: * + N2 → NNH* → NNH2* → NHNH2* → NH2NH2* → NH2* → * Distal-alternative mixed II |
Path IV: * + N2 → NNH* → NHNH* → NHNH2* → NH* → NH2* → * Alternative-distal mixed (I) |
Path V: * + N2 → NNH* → NHNH* → NHNH2* → NH2NH2* → NH2* → * Alternative |
In this study, we have not explicitly considered the enzymatic mechanism for NRR. While both the associative alternative and enzymatic mechanisms follow the same stepwise hydrogenation pathway, they primarily differ in how N2 binds to the catalyst. The associative alternative mechanism typically involves end-on binding, whereas the enzymatic mechanism features side-on binding on well-defined active sites. However, due to the structural diversity of nanoclusters and the absence of a uniform metal arrangement as in metal or metal oxide surfaces, it is challenging to distinctly classify N2 adsorption as strictly end-on or side-on.
By systematically exploring adsorption at metal–metal edges and metal binding sites, we identified the most favorable binding configurations without imposing a predefined mechanistic constraint. Our study considered all possible adsorption configurations for N2 on nanoclusters, including both end-on and side-on orientations. Since both mechanisms share similar reduction steps, the enzymatic mechanism was not explicitly examined but was inherently included in our analysis. However, our approach inherently captures all possible binding orientations relevant to nanocluster catalysis.
Our findings indicate that nanoclusters composed of early transition metals from the 3d, 4d, and 5d series—specifically scandium (Sc), titanium (Ti), yttrium (Y), zirconium (Zr), and hafnium (Hf)—exhibit significantly more favorable adsorption free energies for NNH*, typically around −3.0 eV. This suggests that these nanoclusters form stable, exergonic NNH* adsorbates on their surfaces. Conversely, nanoclusters made from mid to late transition metals tend to show weaker adsorption affinities, as evidenced by relatively lower or even positive adsorption free energies.
Among the mid to late transition metals, only a select few—namely vanadium (V) and manganese (Mn) from the 3d series, technetium (Tc) from the 4d series, and tantalum (Ta), tungsten (W), rhenium (Re), and osmium (Os) from the 5d series—exhibit modest but favourable negative adsorption free energies ranging from −0.9 eV to −0.3 eV. Notably, late transition metals such as copper (Cu), gold (Au), and silver (Ag) display significantly positive adsorption free energies, indicating a much weaker propensity for NNH* adsorption.
Additionally, nanoclusters composed of p-block metals with the exception of aluminium (Al) and pseudo p-block metals, namely zinc (Zn), cadmium (Cd), and mercury (Hg), exhibit significantly larger positive adsorption free energies for NNH* (>1.7 eV), indicating their limited effectiveness in facilitating NNH* formation during the nitrogen reduction reaction (NRR). In contrast, aluminium (Al) does not conform to this trend, displaying a small negative free energy (−0.10 eV), suggesting a slight advantage in promoting NNH* formation compared to its p-block counterparts.
Interestingly, the adsorption free energies for NNH* are consistently lower than those for N2* adsorption across the nanoclusters studied. Fig. 3(a) highlights the differences in adsorption free energies between N2* and NNH*, serving as an indicator of the relative stabilities of these intermediates on nanocluster surfaces. For instance, the adsorption free energies for N2* on Sc and Ti are −3.88 eV and −3.43 eV, respectively, which decrease to −3.16 eV and −2.85 eV for NNH*. Only three metal nanoclusters—manganese (Mn), iron (Fe), and aluminum (Al)—exhibit a higher preference for NNH* adsorption compared to N2* adsorption. These observations suggest that early transition metal nanoclusters, particularly those of Sc, Ti, Y, Zr, and Hf, may serve as promising catalysts for N2 activation and subsequent NNH* formation.
Among the mid-transition metals, several nanoclusters from the 5d series—specifically tantalum (Ta), tungsten (W), rhenium (Re), and osmium (Os), and tantalum (Ta) —exhibit favorable negative adsorption free energies for NHNH*, ranging from −1.12 eV to −0.56 eV. Additionally, nanoclusters composed of vanadium (V), chromium (Cr), and manganese (Mn) from the 3d transition metal block; and technetium (Tc) from the 4d transition metal block; and aluminium (Al) from the p-block also demonstrate favorable adsorption free energies for NHNH*, with values between −0.47 eV and −0.21 eV.
For NNH2* adsorption, a similar pattern is observed with minor variations. Nanoclusters of V, Cr, and Mn from the 3d block; Nb, and Tc from the 4d block; and Ta, W, Re, and Os from the 5d block, as well as Al from the p-block, exhibit negative adsorption free energies. Notably, Mn, Re, Tc and W show strong adsorption free energy values ranging from −1.14 eV to −0.74 eV, while all other metal nanoclusters display adsorption free energies above −0.36 eV. We have observed that, with the single exception of aluminum, all other p-block and pseudo p-block metals display large positive adsorption free energies for both NHNH* and NNH2* adsorbates.
The feasibility of forming intermediates during the NRR critically depends on the free energy changes associated with each electrochemical step. Fig. 4 presents the free energy changes for the formation of NNH2* and NHNH* from NNH*, where negative values denote exergonic (thermodynamically favorable) processes and positive values denote endergonic (thermodynamically unfavorable) processes.
Early TMs exhibit significantly larger endergonic free energy changes for the electrochemical step NNH* → NHNH*, attributed to the strong stabilization of the NNH* intermediate, which impedes further conversion to NHNH*. In contrast, several metal nanoclusters from mid- and late-TMs, as well as p-block and pseudo-p-block metals, display favorable exergonic free energy changes, with moderate values ranging from −0.7 eV to −0.3 eV. Additionally, other metal nanoclusters exhibit relatively small exergonic to mildly endergonic free energy changes (−0.3 eV to +0.13 eV), indicating a near-thermoneutral to slightly unfavorable process.
For the NNH* → NNH2* step, only a limited number of metal nanoclusters—specifically those of Cr, Ga, In, Ir, and Mn—show favorable exergonic free energy changes, ranging from −0.75 eV to −0.23 eV. In contrast, most other metal nanoclusters, excluding early transition metals, exhibit mild exergonic to moderate endergonic free energy changes for this step, indicating a less favorable or unfavorable thermodynamic process. Early transition metals once again stand out, with significantly larger endergonic free energy changes, further emphasizing the difficulty of forming the NNH2* intermediate on these surfaces from NNH*.
To elucidate this preference for the formation of NHNH* or NNH2* from NNH*, we plotted the relative stability of the two intermediates, NNH2* and NHNH*, on the nanoclusters by calculating the difference in their adsorption free energies. The analysis, depicted in Fig. 3(b), indicates an overall preference for the formation of NHNH* over NNH2* on most nanoclusters. However, the relatively small differences in preference values (less than 0.2 eV) for most metal nanoclusters suggest that both intermediates are feasible to form at relatively low potentials. Interestingly, Mn and Tc, are the only metal nanoclusters that show a greater preference for the formation of NNH2* over NHNH* and Re exhibit mild preference.
Overall, these observed trends emphasize the critical role of metal selection in optimizing the NRR pathway, particularly in the context of stabilizing or destabilizing key intermediates such as NNH*, NHNH*, and NNH2*. The findings highlight the challenges associated with early transition metals in progressing beyond the NNH* intermediate due to the high energy barriers linked with the formation of subsequent intermediates. The exergonicity observed for p-block and pseudo-p-block metals primarily arises from the transition between two endergonic states, where the final state has a relatively lower energy.
Aside from early transition metal nanoclusters, only a few exhibit favorable negative adsorption free energies for NHNH2*. These include chromium (Cr) and manganese (Mn) from the 3d block, technetium (Tc) and ruthenium (Ru) from the 4d block, and tantalum (Ta), tungsten (W), rhenium (Re), osmium (Os), and iridium (Ir) from the 5d block. Among these, Mn, Tc, W, Re, and Os show favorable adsorption free energy values ranging from −0.78 eV to −0.41 eV. All p-block metal nanoclusters, with the exception of aluminum, exhibit significantly larger unfavorable positive adsorption free energies, ranging from 1.15 eV to 2.0 eV. In contrast, aluminum shows a much smaller positive adsorption free energy of 0.13 eV.
In general, the adsorption free energies for N* are significantly more negative for most d-block metal nanoclusters, with the exception of late transition metals (TMs). All p-block metals, except aluminum (Al), along with pseudo p-block metals and late TMs such as Cu, Ag, Pt, and Au, exhibit unfavorable positive adsorption energies for N*. Notably, the adsorption free energies for N* intermediates are similar to those observed for N2*. Mid-transition metals display more negative adsorption free energies for N*, ranging from −2.1 eV to −0.3 eV across the 3d, 4d, and 5d blocks. Specifically, W, Tc, Mn, Cr, Ta, V and Nb show values between −2.1 eV and −1.5 eV, while Re, Al, and Os have values between −1.50 eV and −0.90 eV. Furthermore, adsorption free energies tend to decrease across the periodic table, especially after the d5 configuration, where they become positive or nearly zero. Among the p-block metals, aluminum is notable for its favorable adsorption energy of −1.33 eV for N*.
The relative stabilities of NHNH2* and N*, determined from the difference in their adsorption free energies as shown in Fig. 3(c), demonstrate a clear thermodynamic preference for N* over NHNH2*. This implies that when there is competition between the formation of NHNH2* and N* from a common precursor such as NNH2*, N* is preferentially formed. Interestingly, a few metal nanoclusters, including Cu, Zn, Ag, Cd, Au, and Hg, exhibit greater stabilization for NHNH2* compared to N*, although both intermediates display unfavorable positive adsorption free energies.
The electrochemical step favoring the formation of N* from NNH2* (as shown in Fig. 5a) is strongly exergonic across most nanoclusters, with the notable exceptions of Ag, Au, and Hg. The exergonicity of these free energy changes generally decreases as one progresses from early to mid to late transition metals. In contrast, the formation of NHNH2* from NNH2* or NHNH* (Fig. 5c and e) is typically endergonic or only mildly exergonic on most d-block nanoclusters.
For the NNH2* → NHNH2* step, only a limited number of metal nanoclusters exhibit favorable exergonic free energy changes. Excluding early TMs, which show significantly larger endergonic free energy changes for this step, mid- and late transition metals such as Ag, Cu, Os, Rh, Ru, Co, Pd, Au, Pt, and Ir display favorable exergonic free energy changes, ranging from −0.7 eV to −0.2 eV. Additionally, p-block and pseudo-p-block metal nanoclusters also demonstrate favorable exergonic free energy changes. A similar trend is observed for the electrochemical step NHNH* → NHNH2*, where the process is predominantly endergonic on most nanoclusters. However, favorable exergonic free energy changes occur on select nanoclusters, particularly mid- and late transition metals such as Cu, Ru, Ag, Mn, and Co, with values ranging from −0.3 eV to −0.2 eV. P-Block and pseudo p-block metals also exhibit favorable adsorption free energies. Furthermore, the NHNH*→ NHNH2* step is generally more endergonic compared to NNH2* → NHNH2*, correlating with the higher thermodynamic stability of NHNH* relative to NNH2*, as previously discussed. A general trend from unfavorable endergonic free energy changes to favorable exergonic free energy changes is observed as one moves from early to late transition metals for these two electrochemical steps.
Moreover, late transition metals, as well as p-block and pseudo p-block metals, exhibit exergonic free energy changes for the electrochemical step leading to the formation of NHNH2* from either NNH2* or NHNH*. However, caution is warranted, as these cases represent a transition from a more endergonic to a less endergonic thermodynamic state. For instance, the adsorption free energy of NNH2* on a Pb nanocluster is 2.56 eV, while that for NHNH2* is 2.00 eV, indicating an exergonic step with the release of 0.56 eV.
It is crucial to recognize that the feasibility of forming N* intermediates is highly dependent on the preceding reaction pathways, particularly whether NNH2* or NHNH* is formed from NNH* in the second electrochemical step. If NNH2* is formed, it leads exclusively to the formation of N* through a highly exergonic step on all nanoclusters. Conversely, if NHNH* is formed in the second electrochemical step, the third electrochemical step must overcome more endergonic free energy changes to form NHNH2*.
In contrast, NH2NH2* generally exhibits unfavorable positive adsorption free energy values on all nanoclusters as shown in Fig. 2(g), with the exceptions of Mn and Rh, which show small favorable adsorption free energies of −0.10 eV and −0.19 eV, respectively. This suggests that the hydrogenation of NHNH2* on the non-terminal nitrogen atom is a highly disfavored electrochemical step. Consequently, if NHNH2* is formed in the third electrochemical step, it predominantly leads to the formation of NH* on most nanoclusters. The relative preference for NH* over NH2NH2* is clearly illustrated in Fig. 3(d), which depicts the relative stability of these two intermediates on most nanoclusters, calculated from the difference in their free energy values.
Fig. 5(b), (d) and (f) present the free energy changes associated with the three electrochemical steps: N* → NH*, NHNH2*→ NH*, and NHNH2* → NH2NH2*. The N* → NH* step is generally exergonic on most nanoclusters, with a few exceptions where moderate endergonic free energies are observed, particularly among early TMs. Typically, the free energy change for the N* → NH* transition shifts from endergonic in early TMs to mild to moderately large exergonic values in mid- and late TMs. Furthermore, this step is highly exergonic for p-block and pseudo p-block metals.
The electrochemical step NHNH2* → NH* exhibits significantly large exergonic free energy changes across all nanoclusters, driven by the transition from the less stable NHNH2* to the more thermodynamically stable NH* species. This step is highly exergonic for early transition metals (TMs) but decreases as one moves toward late TMs, with exergonic free energy changes ranging from −2.44 eV to −0.49 eV; the only exception is Hg, which shows a small endergonic free energy change of 0.23 eV.
Conversely, the NHNH2* → NH2NH2* step is predominantly endergonic, with only a few exceptions among p-block and pseudo-p block metals, which exhibit unfavorable adsorption free energies for both NHNH2* and NH2NH2*. Late transition metals such as Au, Ag, and Pt display relatively higher favorable exergonic free energy changes of −0.82 eV, −0.61 eV, and −0.34 eV, respectively, while the mid-transition metal Rh nanocluster shows a favorable exergonic free energy of −0.50 eV.
The transition from NH* to NH2* (Fig. 6a) is generally characterized by favorable exergonic free energy changes except on early transition metal nanoclusters. Mid-transition metal nanocluster, with few exceptions, exhibit moderate exergonicity, while late transition metals display larger exergonic free energy changes for the NH* → NH2* electrochemical step. The trend is evident, with early TMs showing higher endergonicity, and as one moves from early to late TMs, the free energy changes shift from endergonic to increasingly exergonic.
![]() | ||
Fig. 6 Free energy changes (ΔG, eV) in the fifth electrochemical step (a) NH* → NH2* and (b) NH2NH2* → NH2*. |
Conversely, the NH2NH2* → NH2* step (Fig. 6b) is associated with significantly larger exergonic free energy changes, primarily due to the transformation of the highly endergonic NH2NH2* adsorbate into the highly stable NH2* adsorbate on all nanoclusters. In this case, the trend is reversed, with early TMs exhibiting larger exergonic free energy changes, and the exergonicity decreasing as we move from early to late TMs. The exergonicity of this step falls within the range of −2.97 eV to −0.85 eV.
We have further conducted a comprehensive examination of five distinct electrochemical pathways (I to V) involved in the NRR mechanism. Table 1 provides a comprehensive analysis of the NRR mechanisms across various metal nanoclusters, identifying the lowest potential pathways along with their corresponding rate-limiting potentials (RLP) in Volts (V) and rate-limiting step. Fig. 8(a) illustrates the RLP for different nanoclusters, revealing clear trends in RLP.
Metal | Path preference (rank 1 to 5) | RL step | RLP (in V) | ||||||
---|---|---|---|---|---|---|---|---|---|
1 | 2 | 3 | 4 | 5 | NRR | HER | (NRR-HER) | ||
Sc | IV | V | I | II | III | NH2* → NH3(g) + * | 1.55 | 0.97 | 0.58 |
Ti | IV | V | I | II | III | NH2* → NH3(g) + * | 1.48 | 0.90 | 0.58 |
V | IV | V | I | II | III | NH2* → NH3(g) + * | 0.63 | 0.13 | 0.51 |
Cr | I | II | III | IV | V | NH2* → NH3(g) + * | 0.89 | 0.36 | 0.53 |
Mn | I | II | III | IV | V | NH2* → NH3(g) + * | 0.94 | 1.24 | −0.29 |
Fe | IV | V | I | II | III | NH2* → NH3(g) + * | 1.02 | 0.46 | 0.55 |
Co | IV | V | I | II | III | NH2* → NH3(g) + * | 1.06 | 0.46 | 0.61 |
Ni | IV | V | I | II | III | * + N2* → NNH* | 0.56 | 0.20 | 0.36 |
Cu | IV | V | II | III | I | * + N2* → NNH* | 1.33 | 0.03 | 1.30 |
Zn | IV | V | II | III | I | * + N2* → NNH* | 2.15 | 0.36 | 1.79 |
Y | IV | V | I | II | III | NH2* → NH3(g) + * | 1.70 | 1.02 | 0.68 |
Zr | IV | V | I | II | III | NH2* → NH3(g) + * | 1.33 | 0.89 | 0.44 |
Nb | IV | V | I | II | III | NNH2* → NHNH2* | 0.48 | 0.20 | 0.28 |
Mo | IV | V | I | II | III | NH2* → NH3(g) + * | 0.83 | 0.27 | 0.56 |
Tc | I | II | III | IV | V | NH2* → NH3(g) + * | 1.28 | 0.90 | 0.38 |
Ru | IV | V | II | III | I | NH2* → NH3(g) + * | 0.85 | 0.59 | 0.26 |
Rh | IV | V | I | II | III | NH2* → NH3(g) + * | 0.23 | 0.32 | −0.09 |
Pd | IV | V | I | II | III | NH2* → NH3(g) + * | 0.31 | 0.46 | −0.16 |
Ag | IV | V | II | III | I | * + N2* → NNH* | 2.07 | 0.40 | 1.67 |
Cd | IV | V | II | III | I | * + N2* → NNH* | 2.19 | 0.80 | 1.38 |
Hf | IV | V | I | II | III | NNH* → NHNH* | 1.40 | 0.83 | 0.58 |
Ta | IV | V | I | II | III | NH2* → NH3(g) + * | 0.97 | 0.18 | 0.80 |
W | IV | V | I | II | III | NH2* → NH3(g) + * | 1.72 | 0.95 | 0.77 |
Re | I | II | III | IV | V | NH2* → NH3(g) + * | 1.38 | 0.26 | 1.12 |
Os | IV | V | I | II | III | NH2* → NH3(g) + * | 1.26 | 0.70 | 0.56 |
Ir | IV | V | I | II | III | NH2* → NH3(g) + * | 0.70 | 0.66 | 0.04 |
Pt | IV | V | I | II | III | * + N2* → NNH* | 0.70 | 0.12 | 0.58 |
Au | IV | V | II | III | I | * + N2* → NNH* | 1.80 | 0.06 | 1.74 |
Hg | V | IV | III | II | I | * + N2* → NNH* | 2.18 | 1.69 | 0.49 |
Al | IV | V | I | II | III | NH2* → NH3(g) + * | 1.04 | 0.21 | 0.83 |
Ga | IV | V | I | II | III | * + N2* → NNH* | 1.69 | 0.13 | 1.57 |
In | IV | V | I | II | III | * + N2* → NNH* | 1.92 | 0.48 | 1.44 |
Tl | IV | V | I | II | III | * + N2* → NNH* | 1.93 | 0.40 | 1.53 |
Sn | IV | V | I | II | III | * + N2* → NNH* | 2.37 | 0.88 | 1.49 |
Pb | IV | V | I | II | III | * + N2* → NNH* | 2.28 | 0.82 | 1.46 |
Bi | IV | V | I | II | III | * + N2* → NNH* | 2.36 | 0.55 | 1.81 |
![]() | ||
Fig. 8 Rate-limiting potentials (RLP) for (a) the nitrogen reduction reaction (NRR) and (b) the hydrogen evolution reaction (HER) in volts (V). |
With few exceptions—such as Cr, Mn, Tc, Re, and Hg—all metal nanoclusters predominantly favor the alternative-distal mixed pathway (Path IV) as their most preferred mechanism, with the alternative pathway (Path V) following closely as the second choice. The distal pathways are generally less favored, typically ranking from third to fifth, with the predominant order for distal mechanism being Path I < Path II < Path III. This trend suggests a general preference for the reaction pathway involving the NHNH* intermediate. However, Cr, Mn, Tc, and Re diverge from this pattern by favoring Path I, which follows the distal mechanism, indicating a distinct catalytic behavior for these metals. Hg stands out as the only metal preferring the alternative mechanism (Path V), although it exhibits unfavorable adsorption energies across all species, making this metal less effective for catalysis.
The nitrogen reduction reaction (NRR) on metal and metal oxide surfaces typically considers the distal and alternating pathways. However, for nanoclusters, we have identified that the alternative-distal mixed pathway (Path IV: * + N2 → NNH* → NHNH* → NHNH2* → NH* → NH2* → *) is the preferred mechanism. This finding emphasizes the need to account for mixed pathways, which are often overlooked in favor of the more conventional distal (Path I) and alternating (Path V) pathways in NRR studies.
In terms of the rate-limiting steps (RLP), early and mid-transition metals, including Al from the p-block, predominantly experience their rate-limiting step during the sixth electrochemical step, NH2* → NH3(g) + *. This step is crucial as it involves the regeneration of the nanocluster surface by removing the NH2* adsorbate, which is vital for the continuation of the catalytic cycle.
On the other hand, late transition metals and p-block metals (excluding Al) and pseudo-P block metals exhibit a shift in their rate-limiting step to the first hydrogenation step, * + N2* → NNH*, indicating a complete reversal from the last step to the first. This suggests that for these metals, the initial activation of nitrogen and its conversion to NNH* is the most energetically challenging step, thus setting the pace for the entire reaction process.
There are notable exceptions to these general trends. For example, niobium (Nb), among the mid-transition metals, displays a unique reaction limiting potential (RLP) during the NNH2* → NHNH2* step. Similarly, hafnium (Hf), an early transition metal, shows its RLP during the NNH* → NHNH* transition, suggesting that this specific step is particularly challenging for Hf nanoclusters.
Overall, the analysis reveals that the preference for reaction pathways and rate-limiting steps in the NRR is significantly influenced by the type of metal and its position in the periodic table. Early and mid-transition metals, along with Al, tend to have their catalytic efficiency dictated by the final nanocluster regeneration step, while late transition metals and most p-block metals focus on the initial nitrogen activation step. The exceptions observed in Nb and Hf highlight the diversity in catalytic behavior across different metals, emphasizing the need for tailored approaches when designing nanocluster catalysts for efficient NRR. This nuanced understanding of pathway preferences and rate-limiting steps provides valuable insights that can drive the development of next-generation catalysts for sustainable ammonia production.
Fig. 9 highlights the efficiency of various metal nanoclusters for the nitrogen reduction reaction (NRR) by displaying their rate-limiting potential (RLP) values in ascending order. Rhodium (Rh) stands out with the lowest RLP of 0.23 V, indicating its superior catalytic efficiency for NRR, as it requires the least potential to drive the rate-limiting step. Following closely, palladium (Pd) and niobium (Nb) also demonstrate high efficiency with RLP values of 0.31 V and 0.48 V, respectively, suggesting that these metals are also highly effective catalysts for NRR.
In addition to these top performers, a group of metal nanoclusters, including nickel (Ni), vanadium (V), platinum (Pt), iridium (Ir), molybdenum (Mo), ruthenium (Ru), chromium (Cr), manganese (Mn), tantalum (Ta), iron (Fe), aluminium (Al) and cobalt (Co) all exhibit RLP values around or below 1.0 V. This range of values suggests that these metals are relatively efficient for NRR, as they require a moderate potential to overcome the rate-limiting step. Their lower RLPs indicate a balance between the energy required to drive the reaction and the stability of the intermediate species involved, making them viable candidates for NRR catalysis.
The rate-limiting potential (RLP) serves as a key descriptor for evaluating the catalytic efficiency of different nitrogen reduction reaction (NRR) catalysts. However, direct comparisons between different catalyst systems—such as nanoclusters, single-atom catalysts (SACs), double-atom catalysts (DACs), core–shell nanoalloys, and size-selected clusters—are challenging due to fundamental differences in their electronic structures, coordination environments, and stabilization mechanisms.105–115
For instance, Fe single-atom catalysts on TiO2(001) exhibit an RLP of 1.27 V, which is slightly higher than the Fe nanocluster (1.02 V) studied here.105 This suggests that Fe nanoclusters may exhibit improved catalytic performance in some cases, but SACs on oxide supports can provide enhanced stability and selectivity. Similarly, Yang et al. reported an RLP of 0.58 V for Ni13/TiO2(101), which is remarkably close to our reported 0.56 V for free-standing Ni10 nanoclusters, indicating that larger Ni clusters behave similarly in supported and unsupported environments.109 However, for small nanoclusters (Ni4/TiO2), Yang et al. observed a much lower RLP of 0.33 V, demonstrating that reducing cluster size can significantly alter catalytic behavior.
Beyond size effects, composition plays a crucial role in tuning the RLP. Chen et al. screened a large number of three-metal clusters embedded in a two-dimensional metal nitride (W2N3) with a nitrogen vacancy and found that the VNiCu cluster exhibits a wide range of RLP values from 0.37 V to 1.43 V, depending on the specific metal composition.108 This demonstrates that size-selected clusters and multi-metallic compositions introduce strong variations in NRR activity, making general comparisons difficult. A similar trend was observed by Li et al., who predicted that Fe&Ni@Mo2CS2 diatomic catalysts exhibit exceptional NRR performance, with an RLP as low as 0.48 V.115 Their study attributed this to the efficient combination of Fe in a high-spin state and Ni in a low-spin state, which facilitates nitrogen activation and ammonia desorption. Das et al. investigated core–shell iron nanoalloy catalysts M15@Fe50, where M = Co, Ni, Cu and reported varying RLP values of 0.33 V (Co@Fe), 0.94 V (Ni@Fe), and 0.27 V (Cu@Fe).113 Interestingly, our reported RLP for Ni10 nanoclusters closely matches the value for Ni15@Fe50, suggesting that in certain cases, isolated nanoclusters and core–shell systems may exhibit similar trends.
Perhaps the most striking deviation arises when comparing nanoclusters with double-atom catalysts (DACs). Rasool et al. reported extremely low RLP values of −0.56 V, −0.58 V, and −0.53 V for Fe2, Co2, and W2 DACs, impregnated in a tetracyanoquinodimethane-based monolayer respectively.110 These values differ significantly from our reported RLP values for 10-atom clusters of the same metals. This suggests that DACs and nanocluster-based catalysts do not behave similarly, as the presence of additional metal atoms in nanoclusters leads to different electronic environments, coordination effects, and reaction mechanisms compared to DACs.
Our findings, in conjunction with recently reported RLP values, highlight that direct comparisons between different catalyst systems must be approached with caution. Nanoclusters, single-atom catalysts, double-atom catalysts, core–shell alloys, and multi-metal nanoalloys all exhibit distinct electronic properties and stabilization mechanisms, leading to substantial variations in RLP values. While trends can be drawn within a specific class of catalysts, one-to-one comparisons across different catalyst architectures can be misleading. Future studies should focus on systematically correlating catalyst size, composition, and support effects to better understand the design principles governing NRR efficiency across various catalytic architectures.
Fig. 7(b) depicts the free energy changes for H* desorption across different nanoclusters, and Fig. 8(b) displays the rate-limiting potentials (RLP) for the hydrogen evolution reaction (HER). The desorption step is observed to be endergonic on most nanoclusters, with the exception of p-block metals (excluding Al), pseudo-p-block metals, and Ag. Based on the values of RLP(NRR)–RLP(HER) presented in Table 1, where a negative value indicates a stronger selectivity towards NRR over HER, certain metals exhibit promising performance. Specifically, Mn (−0.29 eV), Pd (−0.16 eV), and Rh (−0.09 eV) show a clear preference for NRR, suggesting that these metals are more selective for nitrogen reduction under the studied conditions. In contrast, Ir (0.0428) demonstrates a slight preference for HER, but the minimal difference between NRR and HER activity suggests it could potentially be optimized for NRR. Other metals such as Ru (0.26 eV) and Nb (0.28 eV) show a moderate preference for HER, with small but positive values indicating a more competitive balance between the two reactions. However, the remaining metals exhibit a much stronger inclination towards HER, with values greater than 0.35 eV, indicating significant challenges in using these metals for NRR. These insights are critical for guiding the design and selection of electrocatalysts aimed at improving the selectivity and efficiency of NRR in future studies.
Our analysis reveals that a strong correlation between residual charges on adsorbates and their respective adsorption free energies is not universally observed. The most pronounced correlation is seen with the N2* adsorbate (R = −0.87), followed by NNH* (R = −0.77), whereas NH2NH2* shows no significant correlation. These negative correlations suggest that increased electron density, indicative of greater electron transfer from the nanocluster to the adsorbate, generally results in greater stabilization of the adsorbate, reflected in more negative adsorption free energy values.
The plots demonstrate a significant electron transfer from the nanocluster moiety to the adsorbate, particularly for early TMs, which show notably larger adsorption free energies. For example, the residual electron densities on the N2* adsorbate are approximately 1.9e− on Sc and 1.7e− on Ti nanoclusters, indicating substantial electron transfer from the cluster to the adsorbate, with roughly 1e− transferred to each nitrogen atom.
Further examination reveals that early TMs consistently exhibit high electron density on the adsorbates, correlating with stronger adsorption energies. This suggests that early TMs effectively facilitate charge transfer to the adsorbates, thereby stabilizing them more robustly. As we progress from early to late TMs, there is a noticeable decline in both the residual charge on the adsorbates and the adsorption energies, indicating a reduced ability of the metal clusters to donate electrons to the adsorbates, resulting in weaker adsorption.
When we narrow our analysis to early, mid, and late transition metals (excluding p-block and pseudo-p-block metals), as shown in Fig. S2 (ESI†), the correlation coefficients improve for all adsorbates, ranging from −0.80 to −0.86, with the exceptions of NH2* (R = −0.66), NHNH2* (R = −0.63), and NH2NH2* (R = 0.09). This indicates that the inclusion of p- and pseudo p-block metals reduces the observed correlation between adsorption free energies and residual charges on adsorbates.
Interestingly, p-block and pseudo p-block metals generally display moderate to large residual charges on adsorbates across most nanoclusters, except for the N2* and NH2NH2* intermediates. Notably, N2* does not exhibit adsorption on most p-block and pseudo-p block metal nanoclusters, with the exception of Al, where a bond with N2* is formed, as reflected in a Bader charge density of 0.41e−.
Despite the moderate to large electron transfer observed for adsorbates on p-block and pseudo-p block metals, the adsorption free energies are generally unfavorable. For instance, NNH* on Ga, In, and Tl nanoclusters shows residual charges of 0.98e−, 0.85e−, and 0.63e−, respectively, yet the adsorption free energies remain positive and unfavorable, with values of 1.69 eV, 1.91 eV, and 1.93 eV, respectively. Aluminum shows a significantly larger electron density transfer to NNH* (2.22e−), but the adsorption energy is only slightly favorable at −0.10 eV. Similar observations hold true for other intermediates. This suggests that for p-block and pseudo-p block metals, there is no clear correlation between residual charges and adsorption free energies.
In the global minimum configurations, the HOMO–LUMO gap increases for the first 10 metal nanoclusters in the order of Ru < Mn < Ir < Cr < W < Pd < Y < Rh < Ti < Co, with values ranging from 0.02 eV to 0.15 eV. However, the free energy change for the first electrochemical step leading to the formation of NNH* from the global minimum configuration (* + N2* → NNH*) exhibits both exergonic and endergonic values, ranging from −2.90 eV to 0.36 eV. This suggests that there is no direct relationship between the HOMO–LUMO gap and the exergonicity or endergonicity associated with each electrochemical step. Similar observations hold true for other adsorbates.
A broader analysis reveals that p-block metals (e.g., Al, Ga, In, and Tl) and pseudo-p block metals (Zn, Cd, and Hg) generally tend to exhibit significantly larger HOMO–LUMO gaps compared to most transition metals, suggesting that these nanoclusters are generally more chemically stable and less reactive. In contrast, transition metals, particularly those from the early and mid-transition series (e.g., Ti, Cr, Fe, and Ni), tend to display smaller HOMO–LUMO gaps, which correlates with higher chemical reactivity and catalytic potential. Late transition metals, including Cu, Ag, and Au, exhibit relatively larger HOMO–LUMO gaps, indicating lower catalytic activity. Furthermore, metals with a d3 configuration, such as Ti, Nb, and Ta, show larger HOMO–LUMO gaps for many adsorbates compared to other early or mid-transition metals within the 3d, 4d, and 5d blocks, respectively. Similarly, late transition metals with a d9 configuration, such as Cu, Ag, and Au, generally display larger HOMO–LUMO gaps. These observations suggest that no clear trend can be established between adsorption free energies and HOMO–LUMO gap values.
![]() | ||
Fig. 11 Heatmap illustrating the correlation between the adsorption free energies (ΔG) of various intermediates in the nitrogen reduction reaction (NRR). |
![]() | ||
Fig. 12 Correlation plot showing the relationship between the adsorption free energies (ΔG) of NH* and other adsorbates in the nitrogen reduction reaction (NRR). |
A key observation from the heatmap is the strong linear scaling relationships among many of the intermediates involved in the NRR patways. For instance, the correlations between intermediates such as N*, NH*, NH2*, NNH*, NHNH*, NNH2*, and NHNH2* are notably high, with coefficients ranging from 0.87 to 0.98. Except for a single case involving the correlation between NH2* and NNH*, where the coefficient is slightly lower, all other values exceed 0.90. This consistency indicates that catalysts that favorably bind one of these intermediates are likely to similarly favor the binding of others, following a predictable linear trend. These strong correlations imply that the adsorption energies of these species are governed by similar surface interactions and electronic factors, making the optimization of catalysts more straightforward when focusing on these intermediates.
In contrast, the intermediate NH2NH2* exhibits weaker correlations with other species, indicating that its adsorption energy does not scale as predictably with other NRR intermediates. This deviation suggests that NH2NH2* may involve more complex interactions with the catalytic surface, likely due to a different electronic environment or distinct binding modes. One possible reason for this deviation is that NH2NH2* has a fully saturated bonding pattern, which differs significantly from other intermediates that typically have at least one bonding site open for further coordination. This unique bonding configuration may result in distinct adsorption behavior, necessitating specialized considerations in catalyst design.
The adsorption free energies of N2* do not correlate well with the intermediates involved in the NRR mechanism (see Fig. S5, ESI†). Although N2* exhibits a stronger correlation with NNH* (0.91), it shows only moderate correlations with intermediates such as N*, NH*, NHNH*, and NNH2*, with coefficients ranging from 0.80 to 0.85. Additionally, N2* displays even weaker correlations with NH2* (0.66), NHNH2* (0.71) and NH2NH2* (0.47). These weaker correlations indicate that the binding of N2* is not a reliable descriptor for the NRR mechanism, as it may be influenced by different surface characteristics or adsorption sites compared to those affecting the binding of other intermediates. Therefore, it is more effective to include intermediates directly involved in the NRR mechanism as descriptors when optimizing nanocluster surfaces for enhanced NRR performance.
– Adsorption free energies for nearly all NRR intermediates exhibit significantly larger negative values for early transition metals (TMs), which progressively decrease from early TMs to mid and late TMs.
– Early TMs show strong favorable adsorption for most NRR intermediates, except for NH2NH2*, which remains unstable. Mid TMs exhibit mild to moderately favorable adsorption free energies, with some exceptions displaying mildly unfavorable positive free energies. Late TMs generally show unfavorable positive or only slightly favorable negative adsorption free energies for most intermediates.
– P-Block and pseudo-p block metals exhibit highly unfavorable positive adsorption energies, limiting their catalytic efficacy. However, aluminum (Al) exhibits electrochemical behavior that somewhat resembles early TMs in several key electrochemical steps, making it a unique p-block metal in this regard.
– NH2NH2* is identified as the least stable intermediate, with unfavorable adsorption free energies on nearly all nanoclusters, except for manganese (Mn) and rhodium (Rh).
– In the second electrochemical step, the formation of NHNH* from NNH* is favored over NNH2*, while in the third step, N* is preferred over NHNH2*, and in the fourth step, NH* is more stable than NH2NH2*.
– The alternative-distal mixed pathway (Path IV) is identified as the preferred mechanism for nanoclusters in the NRR, emphasizing the need to consider mixed pathways, often overlooked in favor of conventional distal and alternating pathways in electrochemical NRR studies.
– Rhodium (Rh) demonstrates the highest catalytic efficiency, with the lowest rate-limiting potential (RLP) of 0.23 V. Palladium (Pd) and niobium (Nb) also show high efficiency, with RLP values of 0.31 V and 0.48 V, respectively. Several other metals, including nickel (Ni), vanadium (V), platinum (Pt), iridium (Ir), molybdenum (Mo), and manganese (Mn), exhibit RLP values around or below 1.0 V, indicating moderate efficiency.
– Manganese (Mn), palladium (Pd), and rhodium (Rh) show moderate selectivity for nitrogen reduction over the competing hydrogen evolution reaction (HER), making them promising candidates for efficient NRR catalysis.
– Strong linear scaling relationships were identified among key NRR intermediates, such as N*, NH*, NH2*, NNH*, NHNH*, and NNH2*, indicating that stabilizing one intermediate often stabilizes others, aiding in catalyst optimization.
– Charge analysis reveals that a strong correlation between the residual charges on adsorbates and their respective adsorption free energies is not consistently observed.
– No clear correlation was found between the HOMO–LUMO gaps of nanocluster surfaces and the adsorption free energies of NRR intermediates, suggesting that other factors contribute to catalytic behavior.
Overall, this study provides valuable insights into the catalytic performance of d- and p-block metal nanoclusters for the nitrogen reduction reaction, offering guidance for future catalyst design and optimization efforts in sustainable ammonia production.
This study focuses exclusively on 10-atom nanoclusters, and the findings are not directly scalable to significantly larger nanoclusters due to quantum size effects, which can substantially alter electronic and catalytic properties. However, these results are particularly relevant for size-selected nanoclusters, where precise control over cluster size allows for targeted catalytic performance. While our findings provide valuable insights into nitrogen reduction on small nanoclusters, we acknowledge that larger clusters may exhibit different trends. Future studies should explore the impact of cluster size scaling to better understand how catalytic behavior evolves with increasing cluster size. This study provides significant fundamental insights into the trends in NRR performance across different nanoclusters, depending on whether they belong to 3d, 4d, 5d, or p-block metals, thereby facilitating the strategic design of stable and efficient electrocatalysts, particularly for size-selected small nanocluster-based electrocatalysis applications.
Footnote |
† Electronic supplementary information (ESI) available: The ESI includes several figures and tables providing detailed insights into the nitrogen reduction reaction (NRR) on various metal nanoclusters. Fig. S1 presents residual Bader charges for different NRR adsorbates across 3d, 4d, 5d, and p-block metals, Fig. S2 illustrates the correlation between adsorption free energies (ΔG) and residual Bader charges for these adsorbates, excluding p-block and pseudo-p-block metals. Fig. S3 reports the HOMO–LUMO gaps for NRR adsorbates, and Fig. S4 and S5 show correlation plots for the adsorption free energies of N* and N2* with other intermediates. Table S1 summarizes the bond distances between nitrogen and metal atoms in the global minimum configurations of nanoclusters, reporting the shortest bond when two nitrogen atoms are involved in bonding and Table S2 provides N–N bond distances in adsorbates. Table S3 presents adsorption free energies (ΔG) for various NRR intermediates. Table S4 lists residual Bader charge values, and Table S5 reports spin multiplicities for intermediates and global minimum configurations. Table S6 details the HOMO–LUMO gaps, and Table S7 outlines the thermodynamic free energy changes for different electrochemical steps in the NRR. See DOI: https://doi.org/10.1039/d5cp00046g |
This journal is © the Owner Societies 2025 |