Anjana Tripathi‡
,
Vivianne K. Ocampo-Restrepo‡
,
Jens Nørskov
and
Georg Kastlunger
*
Department of Physics, Technical University of Denmark (DTU), Lyngby, Denmark. E-mail: geokast@dtu.dk
First published on 24th April 2025
Electrochemical water oxidation (OER) is the most important electrode reaction in electrocatalysis, representing the default counter-reaction in the plethora of modern electroreductions. Given this prominent role in the electrochemistry-based green transition, improving its efficiency is of utmost importance. Here, identifying novel catalysts by means of computational screening necessitates clarity on the reaction mechanism as this is used to decide on appropriate activity descriptors. To date, however, the mechanism of OER, even on the most widely used catalyst in acid, IrO2, is still debated, and the debate is fuelled by the consistent appearance of Tafel slopes indicative of a non-electrochemical rate-limiting step. Here, we employ density functional calculations and microkinetic modelling to analyse the mechanism of acidic OER on IrO2(110), with an emphasis on the polarization of reaction intermediates. Introducing this degree of freedom shows that the electrostatic destabilization of surface-bound oxygen atoms with increasingly positive potentials increases the effective potential response of the reaction. Thus, a reaction mechanism through OOH*-formation could be confused with a non-electrochemical rate-limiting step. Furthermore, we highlight that a mechanism limited by the desorption of adsorbed O2 is unlikely, as this step is facile at room temperature, but caution is needed in treating adsorbed O2 in GGA-DFT. By incorporating these elements into our model, we simulate Tafel curves that reproduce the experimental potential response in both the low and high overpotential regions, pointing out that including surface dipole effects is essential for understanding and reproducing experiments.
Sustainability spotlightThe oxygen evolution reaction (OER) plays a critical role in the development of efficient and sustainable energy solutions, particularly in water splitting for hydrogen production. However, the dependence on trial-and-error experiments has made it difficult to find promising electrocatalysts. By applying DFT calculations and microkinetic modeling to OER, we can pinpoint key intermediates, rate-determining steps, and reaction pathways that are central to improving the catalyst performance. This approach can significantly minimize the discrepancy between theory and experiment, making it easier to identify promising materials and conditions that lead to higher efficiency and lower environmental impact. This aligns with the goals of the creation of energy-efficient technologies for renewable energy production where understanding of the OER mechanism offers a promising route for advancing sustainable energy technologies. |
OER requires the transfer of four electrons across the electrode/electrolyte interface and the generation of four protons via the stepwise decomposition of water followed by the formation of an O–O chemical bond, as shown in Scheme 1. In the 1960s, Bockris et al. suggested 14 possible routes for OER on Pt, proposing primary water discharge as the rate-determining step.4 Conversely, on RuO2(110), OER was suggested to occur via the Eley-Rideal (ER) mechanism, with the coupling of surface-bound oxygen with H2O from the solution being reported as the rate-limiting step (RLS).5 In contrast, the Langmuir–Hinshelwood (LH) mechanism (such as by coupling two oxygen atoms on the surface) was deemed energetically less favoured and weakly influenced by the applied potential. Finally, a participation of lattice oxygen in the reaction could also be hypothesized (Mars–Van Krevelen mechanism). Kasian et al. and Scott et al. addressed this possibility by O-isotope labelling of the reacting water and the oxide catalyst, respectively. Both studies concluded that on rutile IrO2, the vast majority of oxygen is formed out of interfacial water.6,7 While lattice oxygen could be a minor contributor in RuO2 and IrO2, it can be important in other materials, such as perovskite (e.g. SrIrO3,8 LaCoO3,9) and Co-based catalysts (e.g. Co3O4).10
Computational analysis of the thermodynamic landscape in OER reveals that the formation of OOH* is the most difficult step for many electrocatalysts including IrO2,11,12 and a further analysis by Dickens et al., including explicit calculations of potential-dependent activation energies confirmed that O–OH bond formation is most likely the RLS in all cases.13 However, the O–O coupling pathway via a LH mechanism, involving a chemical RLS between two oxygen atoms, was suggested in earlier studies due to OER's potential response above ∼1.5 V vs. RHE.14–16 Additionally, S. Kwon et al. concluded that the OER mechanism and RLS depend on the facet and potential of IrO2.17 They concluded that direct oxygen coupling is favourable on the (101)-facet of IrO2, while the other facets follow a mechanism limited by the nucleophilic attack of water.
Recent theoretical analyses further suggested that, at high overpotentials on IrO2, the final oxygen desorption step may become thermodynamically unfavourable.18,19 As an alternative to direct O2-desorption from the catalyst surface, recent findings by Binninger et al. suggested that OER on IrO2 may follow the association of two O–O* species, especially at high overpotentials.20 Exner further validated this result21,22 concluding that the *OO–OO* recombination mechanism is crucial and should not be overlooked in future screening studies of OER.
All these deviating mechanistic interpretations need clarification to justify specific catalyst screening strategies. Turning to experiments, one of the strongest mechanistic tools in electrocatalysis for a distinction between the varying pathways is the interpretation of the potential needed to change the current by one order of magnitude, the so-called Tafel slope. From empirical models, such as Butler–Volmer theory in the absence of mass transport limitations,23 the Tafel slope is a consequence of the transfer coefficient α following the relationship:
![]() | (1) |
with referring to the change of current density j with applied potential U and kB, T, and e representing the Boltzmann constant, temperature, and the charge per electron, respectively. Fig. 1 presents a collection of experimental data for OER on IrOx-based catalysts in acid, including both films and nanoparticles (NPs).24–31 Although few data span a broad potential window, for those cases, it is evident that OER exhibits two distinct Tafel slope regions. The potential at which this transition occurs defines the low and high-potential Tafel regions for the data below and above, respectively. The low-potential Tafel region slope is about 40 mV dec−1, representing α ≈ 1.5. However, the more commonly investigated (and commercially more relevant) high-potential region exhibits Tafel slopes of 60–72 mV dec−1 (α between 0.83 and 1) for films and around 50 mV dec−1 for NPs (α ≈ 1.2). Previous theoretical studies successfully reproduced low-potential region behaviours and overestimated values for higher potential ones,13 indicating that there is still a gap in understanding mechanistic details and the origin of the Tafel slope values in the high-potential region.
![]() | ||
Fig. 1 Experimental Tafel plots for OER on IrOx-based catalysts in acidic conditions. Square and circle symbols represent films and nanoparticles (NPs), respectively.24–31 Note that the reported current densities (jtotal) vary in their normalization, making the direct comparison of jtotal unjustified. This does not affect the highlighted Tafel slope values. |
The interaction of intermediate species and transition states with the interfacial field during acidic OER might be the key to solving this conundrum as it adds a degree of freedom to the potential response of the thermodynamic landscape of the reaction. Its relevance is likely, as the intermediate steps involve highly electronegative oxygen species. Electron donation to them upon adsorption creates the formation of distinct surface dipoles, whose interaction with the interfacial field leads to significant electrostatic (de-)stabilization. Further, a variation of this interaction with altering applied potentials leads to contributions to Tafel slopes specific to the surface species and transition states determining the measured current.
The role of such electrostatic effects have recently been experimentally studied by Liang et al., highlighting the role of the interfacial water structure in acidic and alkaline electrolytes on the binding energetics of O* species.31,32 Further, Kelly et al. showed that interfacial field interactions are responsible for selectivity changes within the ORR on noble metal based surfaces like Au(100), Au(111) and Pt(111).33 Both findings emphasize the importance of accounting for interfacial effects on intermediates for mechanistic analyses, which are often overlooked in conventional models.
In this paper, we analyse the possibilities for the reaction mechanism from microkinetic considerations. We show that both the low and high-potential Tafel slopes can be explained by the OOH*-formation mechanism if the interaction of O* and OH* with the interfacial field are accounted for. Further, we will show that the combination of two oxygens from the surface is unlikely as it would lead to negligible current densities that would marginally benefit from an increase in overpotential, and that the desorption of O2* is never rate-limiting but is poorly captured by DFT.
![]() | (2) |
The two derivatives in eqn (2) can formally be further simplified into
![]() | (3) |
![]() | (4) |
α = N‡pe − Npe,RS − βRLS. | (5) |
Interpreting the Tafel slopes in the high overpotential region in Fig. 1 (60–72 mV dec−1) might indicate an RLS whose rate was independent of potential, i.e. βRLS ≈ 0, as it suggests that α is close to an integer value (cf. eqn (1)). Conversely, DFT-based studies suggest that sequential water dissociation is a more feasible pathway.13 Employing such an ER-based mechanism, where OOH* formation is the RLS, it is possible to reproduce the experimental Tafel slope (∼40 mV dec−1) behaviour in the potential region below ∼1.5 V vs. RHE on rutile metal oxides such IrO2, while a Tafel slope of about 120 mV dec−1 is predicted in the higher potential region in disagreement with experiments. Thus, an interpretation based purely on eqn (5) would indicate that the mechanism changes from a proton-coupled electron transfer (PCET)-based RLS at low overpotential (βRLS < 0), to a RLS defined by a potential-independent chemical step (βRLS = 0).
The picture of expected Tafel slopes changes once the system is allowed to deviate from the idealized values. Two deviations can be envisioned; pinning the value of βRLS to −0.5 for PCET steps or zero for formally non-electrochemical steps has no strong justification, where βRLS can, in principle, adopt any value between the effective potential responses of the initial state and final state of the elementary steps.37,38 Further, neglecting the contribution of the polarization of reaction intermediates, γ,34 is a crude approximation. Here, the field response of the RS, γRS, is particularly important, as it will directly influence . While often negligible, particularly the binding of oxygen-containing adsorbates can exhibit a substantial inherent dipole, which changes α into:
α = N‡pe − Npe,RS − βRLS + γRS | (6) |
Note that, analogous to βRLS, we chose the sign of γRS to be consistent with rather than α.
Fig. 2 shows the variations in the Tafel slope, resulting from variations in γRS and βRLS. We highlight the combination of Tafel slopes for RS conditions of a monolayer of OH* (y-axis) and O* (x-axis) defining the RS of the catalyst. The two cases differ in N‡pe − Npe,RS, being 1 and 0 for OH* and O* coverage, respectively. This difference results from the need of OH* to traverse an O*-intermediate to reach the RLS, while O* does not have an equilibrated elementary step preceding the RLS.
Fig. 2a focuses on the mechanism involving O–OH* formation as the RLS. Here, βRLS = −0.5 together with γRLS of both OH* and O* being zero (light turquoise line, γOH − γO = 0) results in the expected combination of 120 and 40 mV dec−1 on the x and y-axes, respectively. While keeping βRLS constant, increasing γOH and γO results in a reduction of their respective Tafel slopes, where e.g. βRLS = −0.5, γO = 0.2 and γOH = 0.1 lead to Tafel slopes of 86 and 38 mV dec−1.
The dependency of the Tafel slopes on γRS in the LH mechanism, shown in Fig. 2b, is even more prominent as its effect is doubled due to the participation of two O*-species in the RLS. Equally, N‡pe − Npe,RS in this case takes the values of 2 and 0, for OH* and O* covered surfaces, respectively. Note that, in this mechanism, βRLS → 0 is likely, making the potential response purely defined by γRS and leading to large Tafel slopes in the high overpotential region.
Overall, Fig. 2 shows that γRS is a central component of the measured potential response and leads to a large variety of possible Tafel slope combinations in OER, independent of the actual mechanism at play.
To estimate the magnitude of γRS, in Fig. 3 we show the DFT-predicted response of the differential formation free energy of the relevant intermediates of OER to an applied homogeneous electric field perpendicular to the electrode surface at a full background coverage of OH* (Fig. 3a) and O* (Fig. 3b) on the CUS sites of IrO2(110) (see ESI Section 1† for Computational details). Analogous results for the field dependence of the change of surface phases by means of average formation free energies are shown in ESI Section 3,† with nearly identical values.
We found that, in the vicinity of the potential of zero charge (PZC) of the electrode, O*, OH*, and O2* are destabilized by negative field strengths, corresponding to more anodic conditions, while H2O* and OOH* are stabilized. This varying behaviour results from the varying surface dipole changes upon adsorption, Δμ, and, thus, γ, as summarized in Fig. 3c. We provide the framework to define γ from the change in surface dipole Δμ and polarizability Δη in ESI Section 4.†
γO is generally enhanced relative to γOH, which can be attributed to its binding motif in a top site on the IrO2(110) CUS, forming a distinct dipole perpendicular to the catalyst surface.39 Conversely, OH* tends to form a hydrogen bond network with the hydrogen pointing parallel to the surface, reducing its overall dipole perpendicular to the surface.
We now show how γ, and particularly its relative differences influence phase stabilities. Fig. 4a shows the calculated Pourbaix diagrams for IrO2(110) including interfacial field effects (see ESI Section 5† for calculation details). In agreement with previous results,32 we identified that IrO2(110) is covered by OH* on the IrO2(110) CUS when ramping up the potential to 1.52 V vs. RHE, where it transitions into a monolayer of O*. We also identified that the deprotonation of the bridge-O (Ob) is likely responsible for the capacitive peaks in cyclovoltammetry (CV) appearing at intermediate positive RHE potential, as reported in ref. 26 for single-crystal IrO2(110). This phenomenon has also been documented in amorphous IrOx and rutile IrO2 in acid.31,32
![]() | ||
Fig. 4 Surface phase diagram for different coverage conditions on the pristine IrO2(110) surface at the full coverage limit with field effects (a). Potential vs. RHE where full OH* coverage transitions to full O* coverage at different pH when no field effect is included (white circles), when a field effect is included (solid black circles) and from experimental data (black triangles)26 (b). *IrCUS represents empty IrCUS sites and Ob an oxygen bridge. |
The field response of the varying surface phases has a minor effect on the transition from OH*- to O*-covered IrO2(110) CUS sites when compared to the case without the inclusion of the field effect shown in ESI Sections 6 & 7.† Conversely, OH* formation on IrO2(110) CUS shifts by ∼−0.7 V. This behavior is a consequence of our choice of PZC in the field response model, which we chose based on the calculated value for the bare IrO2 surface (see Fig. S2†). As the OH*- to O*-covered IrO2(110) CUS-transition happens close to the PZC, the field is small and thus has little influence on it. We note that the PZC does influence the specific transition potential, but its change with potential, our central benchmark, is less affected.
Differences in γ of the two phases involved in the transition are expressed as pH-dependence on the RHE potential scale,34 which allows us to directly benchmark our determined values against experimental observations. In Fig. 4b, we benchmarked the potential where the RS changes from a monolayer of OH* to a monolayer of O* on the CUS of IrO2 against experimental validations from Kuo et al., who studied the transition between the two phases based on the appearance of oxidation/reduction waves in CVs.26 The fingerprint CVs of IrO2(110) were recorded in a wide pH range, exhibiting a non-Nernstian shift in the peak position of two phase transitions between 0.8 and 1.6 V vs. RHE. Based on Fig. 4a, we can attribute the two waves to the electrochemical desorption of H* from the Ob sites (0.87 V vs. RHE) and the transition from OH* to O* (1.52 V vs. RHE) on IrO2(110) CUS. With increasing pH, the experimental peak positions shifted in the negative direction against the RHE potential scale, which allows us to directly probe the γO with respect to γOH. The experimental behaviour is in line with the results from our calculations including the calculated γi, with . This proves the qualitative behavior that O* is destabilized by increasingly anodic potentials more than OH*, strongly indicating that γO may substantially influence on the Tafel slopes in the high overpotential region. Spin polarized results for the same are shown in Fig. S3.†
After having identified the relevant surface phases at reaction conditions and estimating γOH and γO, we now show how both these aspects influence experimental OER observations. For this, Fig. 5 shows the calculated free energy diagram at pH zero for all the intermediates involved in the (a) ER and (b) LH pathways. The effective changes of the free energy of each state with U at constant pH, , are explicitly given. For clarity, only the energetics on an O*-covered surface are shown, while corresponding energetics with a full OH* coverage as the RS are shown in Fig. S6,† and the qualitative picture is equal in both cases. The direct link to experimental observations is made in the corresponding lower panels (c and d) of Fig. 5 resulting from a microkinetic model (see section 8 in ESI† for more detail).
Starting from an empty IrO2(110) CUS-site, the adsorption of water to form H2O* does not involve a proton–electron pair (Npe,*H2O = 0). However, H2O* is considerably stabilized by increasing the potential, and when calculating γH2O at 1.23, 1.43, and 1.63 vs. RHE the average value is γH2O = −0.29, defining its whole potential response. Next, one proton–electron pair is produced for reaching OH* (Npe,*OH = 1). Combined with γOH, the effective potential response of OH* formation resulted in −0.98 eV/V. Subsequently, to produce O*, two proton–electron pairs are created with respect to the empty site (Npe,*O = 2). However, the considerable γO partially counters the purely Nernstian potential response leading to an effective . O* is followed by the RLS in both considered reaction mechanisms. For the ER mechanism shown in panel (a), we used the activation energy and βO–OH = −0.58 as determined in our previous work.13 Here, Dickens et al. calculated the activation energy for the formation of OOH* on oxides and investigated its dependence on the applied potential (See ESI Section 8† for further details).
as no extra proton or OH− are involved for reaching the transition state under acidic conditions. After crossing the RLS barrier in the ER mechanism, OOH* is reached, which, in contrast to O* and OH*, is stabilized by an increase in the negative field (more positive potential), resulting in an enhanced potential response compared to the field free case (i.e. αOOH* − αO* = 1.71).
Finally, O2* results from the deprotonation of OOH*, which exhibits a net potential response of −3.93 eV/V. Note that we did not use the bare DFT calculated formation free energy of O2* in the free energy diagram in Fig. 5, as it is overstabilized by the applied GGA-DFT methodology. Instead, we used a value benchmarked by employing the Redhead analysis of experimental temperature-programmed profiles (TPD) of O2 desorption from IrO2(110).40–42 We describe the process of determining the energy in more detail in ESI Section 9† and will discuss the need for this correction for a correct mechanistic analysis in the discussion of the microkinetic results below.
For the definition of α in the ER mechanism (αER), we can invoke eqn (6), hence simply calculating the potential response difference between the RLS transition state (−2.58 eV/V) and the RS, i.e. −0.98 eV/V and −1.80 eV/V at low and high overpotentials, respectively. Thus, the predicted αER values are 1.6 and 0.78. In the LH mechanism, shown in Fig. 5b, 2O* species act as the reactants of the RLS. Thus, the energy landscape is altered involving two adsorbates throughout up to the RLS. Analogously, the potential response of each step before the RLS is doubled as well. As the RLS represents a formally non-electrochemical step in this mechanism, the potential response between 2O* and O2(g) only varies by 0.4 eV/V, purely defined by the quenching of γO upon desorption. Thus, αLH calculated from Fig. 5b results in 2.04 and 0.4 for the low and high overpotential regions, respectively.
A comparison of the simulated polarization curves in Fig. 5c and d reveals that the ER mechanism aligns much more closely with experimental data both in terms of Tafel slopes and absolute current densities, which approach at 1 mA cm−2 at ∼1.6 V. Conversely, the LH mechanism, exhibits negligible reaction rates throughout the potential range because of the huge thermodynamic barrier connected to the formation of O2 from two O* species.
As expected, αER directly translates into the Tafel slope estimates of 37 mV dec−1 and 77 mV dec−1 for the low and high overpotential regions, respectively, under O* coverage (see Fig. 5c). Note that this result is only obtained when the O2* to O2(g) energy value is set to ∼0.31 eV, as fitted from the TPD analysis shown in Fig. S7,† as O–OH* formation remains the RLS within the simulated potential range. Specifically, including the field effect for O2* shows that this species destabilizes at oxidative potentials, weakening its interaction with the surface compared with pure TPD-derived data, then when the potential increases, the O2* to O2(g) value is even smaller than 0.31 eV. However, this picture changes when using the desorption energy predicted by GGA-DFT (∼0.81 eV). As the activation energy for O–OH* formation is potential-dependent, it decreases as the potential increases. At a certain potential, it becomes smaller than the desorption energy of O2*, as predicted by GGA-DFT, making the latter the apparent RLS. This shift alters the Tafel curve behaviour, resulting in a near complete loss of potential response, in strict disagreement with experiments.
In contrast to the ER reaction path, the simulated LH mechanism exhibited Tafel slopes of 29 and 150 mV dec−1 (see Fig. 5d), which also disagrees with the measurements shown in Fig. 1. A degree of rate control analysis (cf. Fig. S8 & S9 in ESI†) for this mechanism shows that the chemical O–O coupling step and the energy of O2* do not influence the overall rate of the reaction, as O2(g) defines the highest barrier to the product starting from the RS.
Note that we have chosen constant values of CH (i.e. 25 μF cm−2) and Upzc (1.5 V vs. SHE) in our model. These choices directly affect the quantitative values of the Tafel slopes and the potentials of surface phase changes. Therefore, we also probed the sensitivity of simulated Tafel plots to variations of CH (Fig. S10†) and Upzc (Fig. S11 and S12†). The results show that the trends in Tafel slopes are mostly unaffected by the choice of parameters. That is, while the low overpotential region (*OH-covered surface) is virtually unaffected by the interfacial field, the high overpotential region (*O-covered surface) shows a substantial field response, leading to reduced Tafel slopes compared to the case without the field effects.
While in the present study, we focussed only on the most stable (110)-surface of IrO2, we are confident that analogous characteristic field interactions are present on other facets. Further, the stronger binding of *O on less coordinated surface sites likely even reduces the probability of the LH mechanism. However, specific evaluations on other facets would be needed to confirm these hypotheses.
Overall, our analysis shows that while the proximity of experimental Tafel slopes to the characteristic value of 60 mV dec−1 might make it tempting to assign a chemical RLS. This can be equally well explained by the combined potential response of the RLS and RS in a PCET-limited step, as is the case for the ER mechanism. Conversely, the LH mechanism would never have a value approaching 60 mV dec−1, as it would formally (from purely Nernstian behaviour) only exhibit Tafel slopes of ∼30 mV dec−1 or infinity. However, including γO leads to non-zero potential responses, which still deviate strongly from the experimentally observed values.
This a priori unintuitive Tafel behaviour likely extends beyond IrO2(110), both in terms of alternative surface facets and other rutile oxides. To account for the behaviour, a further simplified model directly applicable in large scale screening studies can be applied: conventional DFT calculations for the relevant reaction intermediates directly provide μ from the ground state charge density (mostly given in the output of DFT codes) and the work function as an estimate for Upzc. Utilizing them allows a first order estimate of relevant γ values without the need for field dependent (or even more sophisticated) calculations.
Footnotes |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d5su00080g |
‡ These authors contributed equally to this work. |
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