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Generic approach to access barriers in dehydrogenation reactions

Abstract

The introduction of linear energy correlations, which explicitly relate adsorption energies of reaction intermediates and activation energies in heterogeneous catalysis, has proven to be a key component in the computational search for new and promising catalysts. A simple linear approach to estimate activation energies still requires a significant computational effort. To simplify this process and at the same time incorporate the need for enhanced complexity of reaction intermediates, we generalize a recently proposed approach that evaluates transition state energies based entirely on bond-order conservation arguments. We show that similar variation of the local electronic structure along the reaction coordinate introduces a set of general functions that accurately defines the transition state energy and are transferable to other reactions with similar bonding nature. With such an approach, more complex reaction intermediates can be targeted with an insignificant increase in computational effort and without loss of accuracy.

Introduction

In the last decade, developments in density functional theory (DFT) methods have made it possible to effectively perform computer-based screening studies in the design of heterogeneous catalysts1,2,3,4,5,6,7,8,9,10. The combination of explicit DFT-calculated adsorption energies (i.e., descriptors) and simple modeling methods, which describe effectively and accurately the correlation between these descriptors and complex reaction and activation energies, is an instrumental tool in this approach. Models that are first order in energy, so-called linear scaling methods, have shown to provide sufficient accuracy when evaluating trends in catalytic activity11. However, recently it has been shown that the linearity is closely connected to the intrinsic bond-order of the intermediate, thus suggesting that while accurate for the energy of stable intermediates on a potential energy surface (PES), it will be less accurate in describing the energy of meta-stable intermediates such as transition states12,13. Instead we have introduced a new method, “r-scaling”, which explicitly takes variations in bond-order along the reaction coordinate into account. This directly incorporates structural variations of transition states into the energy correlations and should potentially be more accurate than typical linear approaches, such as Brønsted–Evans–Polanyi-type relations14,15,16,17,18,19. In addition, it also substantially reduces the computational cost when establishing transition state (TS) energy correlations13,20,21.

The r-scaling scheme is built entirely on the bond-order conservation principle, which relies on the hypothesis that any transient structure (defined by the reaction coordinate r) between the initial and final state of an elementary reaction step along the minimum energy reaction pathway obey the following linear relation:

$${E}^{\mathrm{t}}\left( {r,{E}^{\mathrm{d}}} \right) = \gamma\left( r \right) {E}^{\mathrm{d}} + \xi\left( r \right),$$
(1)

where Et (r, Ed) and Ed are the chemisorption energies of a transient intermediate at a specific reaction coordinate r and that of a reaction relevant descriptor species, respectively. The constraints imposed by this hypothesis uniquely define both γ(r) and ξ(r), and the TS energies as a function of Ed can be obtained by maximizing the potential energy Et (r, Ed) given by Eq. (1) along the reaction coordinate.

According to the bond-order conservation principle, the dissociation of a covalent bond on a surface is associated with a relocation of the electrons into the new bonds established between the surface and the fragments of the adsorbate such that the normalized bond order of the fragments is conserved22,23,24,25,26. The electronic details of this process are characterized by the distinct type of bond that is broken and the associated functional forms of γ(r) and ξ(r) in Eq. (1), related to the specific orbitals in the bond and their interaction with the surface. This suggests that the cleavage of chemical bonds exhibiting the same local electronic environment can be grouped into classes. The members in each class expose a similar electron redistribution, and therefore, will share the same functional form of γ(r) and ξ(r).

In this work, we will justify this concept and demonstrate that the functions γ(r) and ξ(r), as defined in Eq. (1), are transferable between reactions within the same class. This allows us to obtain the TS energy-scaling relations for a large number of reactions from a database of template functions of γ(r) and ξ(r) determined accurately for a single element in the class. The functional form for all elements within the class can be easily generated by rescaling the template functions, which requires fewer calculations than establishing the functions for each individual reaction. In the following, we use the dehydrogenation reactions of sp3 hybridized C, N, and O atoms to apply this concept. We show explicitly that when using the functions γ(r) and ξ(r) derived from CH4, NH3*, and H2O* bond activation as our template functions to define each class, we can effectively and accurately derive the TS energy-scaling relations of any other sp3-hybridized C–H, N–H, and O–H dissociation reaction. This not only broadens our understanding of chemical reactions and how the reaction energy evolves, it also significantly speeds up our computational approach.

Results

Application of r-scaling to dehydrogenation reactions

We have studied dehydrogenation reactions of hydrocarbons, ammonia, amine, water, and alcohols, which all contain sp3-hybridized bonds, to illustrate the underlying similarity between specific bond-breaking reactions and how this can be used to address a larger set of reactions at little extra computational cost. The reaction steps examined are listed below. By considering the activation of CH4, NH3*, and H2O* molecules on fcc(211) surfaces as representatives for dehydrogenation reactions of species containing C, N, and O centers, we applied the r-scaling scheme to derive the functional form of γ(r) and ξ(r) for each reaction and identify transient intermediate energies as a function of r and Ed through Eq. (1), as shown in Fig. 1.

$${\mathrm{CH}}_4^\ast + ^\ast \to {\mathrm{CH}}_3^\ast + {\mathrm{H}}^\ast$$
(2)
$${\mathrm{CH}}_3^\ast + ^\ast \to {\mathrm{CH}}_2^\ast + {\mathrm{H}}^\ast$$
(3)
$${\mathrm{CH}}_2^\ast + ^\ast \to {\mathrm{CH}}^\ast + {\mathrm{H}}^\ast$$
(4)
$${\mathrm{CH}}^\ast + ^\ast \to {\mathrm{C}}^\ast + {\mathrm{H}}^\ast$$
(5)
$${\mathrm{CH}}_{\mathrm{3}}{\mathrm{CH}}_{\mathrm{2}}^\ast + ^\ast \to {\mathrm{CH}}_{\mathrm{3}}{\mathrm{CH}}^\ast + {\mathrm{H}}^\ast$$
(6)
$${\mathrm{CH}}_{3}{\mathrm{CH}}_{2}{\mathrm{CH}}_{2}^{\ast} + {}^{\ast} \rightarrow {\mathrm{CH}}_{3}{\mathrm{CH}}_{2}{\mathrm{CH}}^{\ast} + {\mathrm{H}}^{\ast}$$
(7)
$${\mathrm{NH}}_3^\ast + ^\ast \to {\mathrm{NH}}_2^\ast + {\mathrm{H}}^\ast$$
(8)
$${\mathrm{NH}}_2^\ast + ^\ast \to {\mathrm{NH}}^\ast + {\mathrm{H}}^\ast$$
(9)
$${\mathrm{NH}}^\ast + ^\ast \to {\mathrm{N}}^\ast + {\mathrm{H}}^\ast$$
(10)
$${\mathrm{CH}}_3{\mathrm{NH}}^\ast + ^\ast \to {\mathrm{CH}}_3{\mathrm{N}}^\ast + {\mathrm{H}}^\ast$$
(11)
$${\mathrm{H}}_{\mathrm{2}}{\mathrm{O}}^\ast + ^\ast \to {\mathrm{OH}}^\ast + {\mathrm{H}}^\ast$$
(12)
$${\mathrm{OH}}^\ast + ^\ast \to {\mathrm{O}}^\ast + {\mathrm{H}}^\ast$$
(13)
$${\mathrm{CH}}_{\mathrm{3}}{\mathrm{OH}}^\ast + ^\ast \to {\mathrm{CH}}_{\mathrm{3}}{\mathrm{O}}^\ast + {\mathrm{H}}^\ast$$
(14)
$${\mathrm{C}}_{\mathrm{2}}{\mathrm{H}}_{\mathrm{5}}{\mathrm{OH}}^\ast + ^\ast \to {\mathrm{C}}_{\mathrm{2}}{\mathrm{H}}_{\mathrm{5}}{\mathrm{O}}^\ast + {\mathrm{H}}^\ast$$
(15)
$${\mathrm{C}}_{\mathrm{3}}{\mathrm{H}}_{\mathrm{7}}{\mathrm{OH}}^\ast + ^\ast \to {\mathrm{C}}_{\mathrm{3}}{\mathrm{H}}_{\mathrm{7}}{\mathrm{O}}^\ast + {\mathrm{H}}^\ast$$
(16)
Fig. 1
figure1

Framework for the r-scaling scheme. ac Linear energy-scaling relations of transient structures at fixed bond lengths r ranging from 1.2 to 2.2 Å for CH4, NH3*, and H2O* activation on nine transition-metal (211) surfaces, respectively. The fits are obtained from linear regression of the calculated points (Supplementary Figures 13). Here we define \(E^{\mathrm{d}} = E_{\mathrm{ads}}{\mathrm{(A)}_{\mathrm{A = C,N,O}} = E_{\mathrm{A@surf}}-E_{\mathrm{surf}}-E_{\mathrm{A(g)}}}\) and \(E^{\mathrm{t}} = E_{\mathrm{rel}}{({\mathrm{AH}}_{x{\mathrm{ -1}}}{\mathrm{ -H}})}_{\mathrm{A = C,N,O}} = E_{\mathrm{AH}_{x{\mathrm{ -1}}}{\mathrm{-H@surf}}}-{E}_{{\mathrm{surf}}}-{E}_{{\mathrm{AH}}_{\mathrm{x}}{\mathrm{(g)}}}\), where EA@surf and \(E_{{\mathrm{AH}}_x{\mathrm{-H@surf}}}\) are the total energies of the adsorbed surface structures. Esurf is the total energy of the surface, EA(g) the gas-phase energies of C, N, and O, and \(E_{{\mathrm{AH}}_x(\rm {g})}\) the gas-phase energy of CH4, NH3, and H2O. The parameter x has the value 4, 3, and 2 for C, N, and O, respectively. df Fitted curves of slope γ and intercept ξ for the lines in ac as functions of r (see Methods, and Supplementary Table 1). gi PESs for CH4, NH3*, and H2O* activation, respectively. jl The TS energy-scaling relations as obtained from the r-scaling scheme together with explicit DFT-calculated energies for CH4, NH3*, and H2O* activation, respectively. All the TS structures are shown in the Supplementary Figures 46

For all transient structures with fixed bond lengths ranging from 1.2 to 2.2 Å, the slope and intercept of the scaling of chemisorption energies (i.e., Et as a function of Ed) changes uniformly as the bond is splitting (Fig. 1a–c). The observed increase in the slope stems from the bond-order conservation and is a manifestation of the increasing surface-adsorbate bond order as the R–H bond is breaking20,21. The surface corresponding to Ed = 0 in Fig. 1g–i identifies the intercept ξ, which can be interpreted as the potential energy of the reaction proceeding on a non-interacting surface. On the basis of the linear relations in Eq. (1), the monotonically increasing functions γ(r) and ξ(r) can be fitted as shown in Fig. 1d–f and the 2D PES for the three reactions shown in Fig. 1g–i can be derived from Eq. (1). The first order saddle points on the 2D PES (blue lines) define the TS energies, which are obtained by maximizing Eq. (1) along the reaction coordinate r:

$${E}_{{\mathrm{ts}}}\left( {{E}_{{\mathrm{ads}}}\left( {\mathrm{A}} \right)} \right)_{{\mathrm{A = C,N,O}}} = {\rm {max}}_r[\gamma \left( r \right) {E}_{{\mathrm{ads}}}\left( {\mathrm{A}} \right) + \xi\left( r \right)].$$
(17)

Equation (17) defines the mapping of these saddle-point energies into a set of functions depending only on a single descriptor (Eads(A))A=C,N,O. These functions represent the TS energy-scaling relations (solid black lines in Fig. 1g–i). When compared with the actual calculated TS energies, we find a mean absolute error (MAE) of 0.07, 0.09, and 0.08 eV for the activation of CH4, NH3*, and H2O*, respectively, as shown in Fig. 1j–l. Using the r-scaling scheme, TS scaling relations of all the dehydrogenation reactions can be derived as shown in Supplementary Figure 7.

The γ(r) function in Eq. (1) reflects the intrinsic variation in the bond-order between the surface and the reactant and therefore, it changes independently of the orientation of the catalyst surface. In contrast, the function ξ(r) in Eq. (1) has a very strong dependence on the surface orientation, and therefore needs to be determined specifically for a certain reaction coordinate. However, when bond-breaking processes involve a specific bonding network along a well-defined reaction coordinate, such as sp3-hybridized bonds (e.g., CH4, *CH3, *CH2, and *CH), these processes will form a class of reactions where all members share similar functional forms of γ(r) and ξ(r). As a result, each reaction in the class will experience similar electron redistribution along the reaction coordinate as reflected in the comparison of molecular orbital and projected densities of states for C1 dehydrogenation reactions shown in Fig. 2a and b. In the following, we justify that through a simple rescaling, the functions γ(r) and ξ(r) can be transferred between bond dissociation reactions belonging to the same class. The corresponding PES can then be found through Eq. (1) and the TS energies can be derived from Eq. (17).

Fig. 2
figure2

Bonding features and electronic state analysis of C1 species. a sp3-hybridized bonding feature of CH4 in the gas phase, CH3 adsorbed on the top site, CH2 on the bridge site and CH on the hollow site. b Projected density of states (PDOS) of the H atom in the transient structures of CH3–H, CH2–H, CH–H, and C–H on Ru(211) surface with r fixed at 1.5 Å

Once the members of a specific class have been identified, a successful rescaling of the functions γ(r) and ξ(r) within the class depends on only two conditions: (1) that the template functions γ i (r) and ξ i (r) derived explicitly for a single element i in the class are accurately established and (2) that the initial and final values of the functions for other members j ≠ i are determined. Rescaling the template functions according to the initial and final points of the jth member, allows us to generate the complete set of functions for all j, as illustrated in Fig. 3. In the following, we show how the transfer scheme can be applied to a class of reactions involving C–H bond splitting. The activation of CH4 is used to establish the set of template functions γ(r) and ξ(r) from which new functions are generated to describe the activation of CH3*, CH2*, and CH*. The domain for any set of the continuous functions γ(r) and ξ(r) is reduced to a generalized reaction coordinate involving only the bond distance, which in this work ranges from 1.2 to 2.2 Å. The functional values at r = 1.2 and 2.2 Å will be obtained from the linear relations described by Eq. (1) using only two metal surfaces as shown in Fig. 4a and b. The two metals are chosen, based on the established scaling relations for the equilibrium initial and final state structures of the elementary reaction step, such that the smallest energy-averaged root-mean-square error (σavg) is achieved (see Methods)21. For CH3*, CH2*, and CH* activation, the two metals with the smallest σavg are {Ag,Ru}, {Ag,Ru}, and {Au,Rh}, respectively. Figure 4a and b shows the relations for CH3*, CH2*, and CH* as established using the two metal surfaces for C–H bond lengths fixed at r = 1.2 and 2.2 Å, respectively. The obtained values for slopes γ and intercepts ξ are seen to be very close to those obtained from linear relations fitted using all nine metal surfaces (Table 1) and these values are used as rescaling parameters to perform the transfer process as shown in Fig. 4c and d. TS energies for CH3*, CH2*, and CH* activation can now be obtained using Eq. (17). The whole process is detailed in the Methods section.

Fig. 3
figure3

Functional rescaling according to shifted initial and final state values. Objective function f j (r) is generated from rescaling template function f i (r) by f j (r) = f j (rinit) + (a × [f i (r) − f i (rinit)])/b, in which a = f j (rfinal)−f j (rinit) and b = f i (rfinal)−f i (rinit)

Fig. 4
figure4

Determination of the initial and final values of γ(r) and ξ(r) functions and transfer of γ(r) and ξ(r) functions. a, b The scaling relations for transient structures in the CH3*, CH2*, and CH* activation on (211) surfaces with bond lengths fixed at r = 1.2 and 2.2 Å, which are established using the selected two metal surfaces. Eads of C* on the threefold hollow site is used as the descriptor for CH4, CH3*, and CH2* activation. As CH* prefers the fourfold hollow site, considering the implicit adsorption behavior of carbon species on the fourfold site in which the Eads is non-linearly related to that on the three(or less)-fold site11, the Eads of C* on the fourfold hollow site is used as the descriptor for CH* activation to achieve a better accuracy. c, d The transfer of γ(r) and ξ(r) functions of CH4 activation to CH3*, CH2*, and CH* activation according to the slope and intercept values at r = 1.2 and 2.2 Å as obtained in a, b, e.g., for CH3* activation, γ(1.2) = 0.33, ξ(1.2) = −0.72, γ(2.2) = 0.73, ξ(2.2) = 2.52

Table 1 γ and ξ values derived using two or all nine metal surfaces

Discussion

The general scheme and the electronic structure similarities of the bonds formed between the catalyst surface and the reactants allow us to expand upon the three reaction classes defined by the functions obtained from CH4, NH3*, and H2O* activation. In principle, all reactants R–H, where R is any residue forming an sp3-hybridized bond with hydrogen through C, N, or O should fall in one of the three classes defined above, e.g., activation of CH3*, CH2*, CH*, CH3CH2*, and CH3CH2CH2* belong to the same class as CH4 activation, NH2*, NH*, and CH3NH* to the same class as NH3* activation, and OH*, CH3OH*, C2H5OH*, and C3H7OH* to the same class as H2O* activation. Using the transfer scheme, we established the γ(r) and ξ(r) functions for all the members of each class and subsequently extrapolated the TS energy-scaling relations of all the considered dehydrogenation reactions from Eq. (17) (Supplementary Figure 8). In Fig. 5, a comparison is shown between the transition state energies obtained using this simple model and the energies obtained using a constrained optimization in DFT based on either the fixed bond-length method or the Nudged–Elastic–Band (NEB) approach27,28. Our comparison shows an overall MAE of only 0.12 eV using CH4, NH3*, and H2O* activation on (211) surfaces to obtain the template functions for each class. Using alternative members to establish the template functions, the overall MAE ranges from 0.11 to 0.17 eV. It is noteworthy to mention that our model provides a much cheaper route for obtaining TS energies, since only four constrained calculations are required to secure the necessary information for a specific reaction belonging to a class with pre-established template γ(r) and ξ(r) functions. In contrast to traditional NEB methods, where TS energies are computed for every reaction step and catalyst surface, our model classifies reactions and applies a transfer scheme to effortlessly derive the TS energies thus significantly reducing the associated computational cost.

Fig. 5
figure5

The accuracy of our transfer model. Calculated TS energies are compared with the predictions from our model based on the transfer of template γ(r) and ξ(r) functions for classes of dehydrogenation reactions involving species with sp3-hybridized C–H, N–H, or O–H bonds. The γ(r) and ξ(r) functions of CH4, NH3*, and H2O* activation on fcc(211) surfaces are used as the templates for each class, respectively. Data of TS energy calculations are shown in the Supplementary Tables 222

In summary, the functions γ(r) and ξ(r) are shown to depend only on the electronic nature of the activated bonds irrespective of the surface type or residual groups. Using three series of dehydrogenation reactions involving sp-hybridized C, N, and O on three low index metal surfaces: (100), (111), and (211), we have shown that the derived functions γ(r) and ξ(r) define three unique classes of reactions and that they can be transferred easily between bond-breaking reactions belonging to the same class. Only four constrained calculations are required to apply the transfer scheme for a given reaction step, allowing access to the full PES from which TS energies along the reaction coordinate can be derived. Moving forward, this enables us to build databases of bond specific γ(r) and ξ(r) functions for a well-defined set of surface reaction classes and then employ the transfer scheme to obtain relevant kinetic parameters. This approach introduces a significant reduction in the computational cost of calculating transition state energies. A simple estimation shows a factor of ~36 in the reduction of cpu time compared to traditional NEB methods, resulting in significant savings in power consumption as well as time spent by scientific personnel (Methods). This expansion of scaling methods to include the description of reaction transients increases the efficiency in the computation of kinetic parameters without loss of accuracy and primarily it enables an even faster screening of catalyst materials.

Methods

DFT calculations

DFT calculations are performed using the plane-wave-based PWSCF (Quantum-ESPRESSO) code and the Atomic Simulation Environment (ASE)29. The ultrasoft Vanderbilt pseudopotential method with BEEF exchange-correlation functional is adopted30,31,32,33. A cutoff energy of 500 eV for the wavefunctions is used. The fcc(211), fcc(111), and fcc(100) surfaces of nine transition metals including Cu, Ni, Ag, Pd, Re, Rh, Ru, Pt, and Au are chosen as catalysts for the dehydrogenation reactions. The (211) slabs are built with 4 atomic layers in the [111] direction in rectangular 1 × 3 supercells with the bottom three [111] layers fixed during structural optimizations. The (111) and (100) slabs are built with four atomic layers with the bottom two layers fixed during structural optimizations using hexagonal 3 × 3 and rectangular 2 × 2 supercells, respectively. The Monkhorst–Pack scheme is used for sampling the Brillouin zone34 and k-point grids of 4 × 2 × 1, 4 × 4 × 1 and 4 × 4 × 1 are selected for (211), (111), and (100) slabs, respectively. The vacuum thickness is set to more than 10 Å in all slab calculations and the dipole correction is applied to decouple the interaction between slabs. During structural relaxations, the residual force between atoms is converged to a value below 0.02 eV/Å.

TS energies for the dehydrogenation reactions are calculated using the fixed bond-length (FBL) method as implemented in ASE. All TS structures show a single imaginary frequency thus identifying it as a first order saddle-point. The fixed bond-length calculations range from 1.2 to 2.2 Å with increments of 0.1 Å, which is accurate enough to cover transition states of any dehydrogenation reaction. TS’s with a bond-length shorter than 1.2 Å are close to the initial state, and in these cases the reaction is treated as if it has no barrier. TS energy calculations for all reactions (2–16) are performed on fcc(211) surfaces and for reactions (3), (6), and (7) calculations have also been performed on fcc(111) and fcc(100) surfaces.

Fitting procedure

In the r-scaling scheme, fitting of the slope γ(r) and the intercept ξ(r) is done applying the scipy.optmize.minimize method using a fifth-order polynomial. The functions are constrained to be monotonically increasing.

$$\gamma\left( r \right) = a_0 + a_1r + a_2r^2 + a_3r^3 + a_4r^4 + a_5r^5,$$
(18)
$$\xi \left( r \right) = b_0 + b_1r + b_2r^2 + b_3r^3 + b_4r^4 + b_5r^5.$$
(19)

Choosing the two metal surfaces

Established linear scaling relations for the initial and final state equilibrium structures for a given reaction have been used for selecting the two transition-metal surfaces. Selection of a metal surface is partly determined by the root-mean square error (σ) of the linear regressions of the initial and final state:

$$\sigma = \sqrt {(R_{{\mathrm{IS}}}^2 + R_{{\mathrm{FS}}}^2)/2},$$
(20)

where RIS and RFS are the metal-specific absolute residuals of the initial and final state linear regression, respectively. The energy span of the descriptor is also a significant factor. To ensure that the metals chosen reflect both the reactive as well as the noble surfaces, we define an energy-averaged root-mean square error of two metals (m1 and m2) as:

$$\sigma _{{\mathrm{avg}}} = \frac{{\sigma _{{\mathrm{m}}_{\mathrm{1}}}{\mathrm{ + }}\sigma _{{\mathrm{m}}_{\mathrm{2}}}}}{{|{\mathrm{E}}_{{\mathrm{ads}}}^{{\mathrm{m}}_{\mathrm{2}}}{\mathrm{(A) - }}E_{{\mathrm{ads}}}^{{\mathrm{m}}_{\mathrm{1}}}{\mathrm{(A)|}}}}.$$
(21)

The choice of two transition-metal surfaces that minimizes Eq. (21) is finally used for building the scaling relations of transient structures with bond-length fixed at r = 1.2 and 2.2 Å. More details about the method selecting the two metals can be found in ref. 21.

Steps of transfer scheme for obtaining TS energy relations

  1. (1)

    Obtain the γ(r) and ξ(r) functions for a single reaction in a class using a global or simplified r-scaling scheme21. These functions will be used as the template functions for the reaction class.

  2. (2)

    For a given reaction in the class, calculate adsorption energies (Erel) of the initial state and final state on a sufficiently large number of metal surfaces and build the linear relations of Erel vs. descriptor for the two states, from which two metal surfaces are determined as detailed above. Note that the initial and final state structures in this step are the equilibrium structures, not those with bond-length fixed at 1.2 and 2.2 Å.

  3. (3)

    Calculate the adsorption energies (Erel) on the two metal surfaces determined in step (2) of two transient structures with bond-length fixed at 1.2 and 2.2 Å, respectively (four calculations total disregarding the clean surfaces and gas-phase calculations). Then build the linear relations of Erel vs. descriptor for the two transient structures using just two points for each (Fig. 4a, b) and obtain the values of γ(1.2), ξ(1.2), γ(2.2), and ξ(2.2) from the linear relations.

  4. (4)

    Rescale the template functions γ(r) and ξ(r) functions as shown in Fig. 3.

  5. (5)

    Build the TS energy-scaling relation for the reaction according to Eq. (17).

NEB versus r-scaling comparison

To establish the transition state scaling relation for a specific reaction using nine catalyst surfaces, the NEB method requires:

$${\mathrm{8}}\,{\mathrm{images}}\,\left( {{\mathrm{per}}\,{\mathrm{NEB}}} \right)\,{\mathrm{ \times }}\,{\mathrm{9}}\,{\mathrm{surfaces}}\,{\mathrm{ \times }}\,{N}_{{\mathrm{core}}} = {\mathrm{72}}\,{N}_{{\mathrm{core}}}{\mathrm{.}}$$
(22)

The r-scaling method needs:

$${\mathrm{2}}\,{\mathrm{images}}\,{\mathrm{ \times }}\,{\mathrm{2}}\,{\mathrm{surfaces}}\,{\mathrm{ \times }}\,{N}_{{\mathrm{core}}}{\mathrm{ = 4}}\,{N}_{{\mathrm{core}}}{\mathrm{,}}$$
(23)

where Ncore is the number of cpu-cores used per image or structure. Considering that NEB calculations take longer time to converge, we shall assume that NEB calculations take a factor of two more time than the constrained minimization calculations used in the r-scaling method. The difference in the number of cores used is (2×72Ncore)/4Ncore = 36, in favor of r-scaling. Thus r-scaling introduces a substantial reduction in cpu time, which renders it a highly efficient and accurate method for estimating TS energies.

Data availability

Part of the data sets generated and analysed during the current study are included in the Supplementary Information file and others are available in the “figshare” repository, https://doi.org/10.6084/m9.figshare.5601622.v2.

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Acknowledgements

We acknowledge support from the U.S. Department of Energy, Office of Basic Energy Sciences, to the SUNCAT Center for Interface Science and Catalysis at SLAC National Accelerator Laboratory and Stanford University.

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L.Y. conducted all DFT calculations for the N–H and O–H bonds dissociation reactions and processed and analyzed data. L.V. conducted all DFT calculations for C–H bond dissociation reactions. F.A.-P. conceived the calculations and analyzed results. All the authors interpreted the structures and contributed to the preparation of the manuscript.

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Correspondence to Frank Abild-Pedersen.

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Yu, L., Vilella, L. & Abild-Pedersen, F. Generic approach to access barriers in dehydrogenation reactions. Commun Chem 1, 2 (2018). https://doi.org/10.1038/s42004-017-0001-z

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