Lara
Kabalan
a,
Igor
Kowalec
a,
C. Richard A.
Catlow
abc and
Andrew J.
Logsdail
*a
aCardiff Catalysis Institute, School of Chemistry, Cardiff University, Park Place, Cardiff, CF10 3AT, Wales, UK. E-mail: LogsdailA@cardiff.ac.uk
bDepartment of Chemistry, University College London, 20 Gordon Street, London, WC1E 6BT, UK
cUK Catalysis Hub, Research Complex at Harwell, Rutherford Appleton Laboratory, Didcot, OX11 OFA, UK
First published on 22nd June 2021
We report a detailed Density Functional Theory (DFT) based investigation of the structure and stability of bulk and surface structures for the Group 10–12 elements Pd, Cu and Zn, considering the effect of the choice of exchange–correlation density functional and computation parameters. For the initial bulk structures, the lattice parameter and cohesive energy are calculated, which are then augmented by calculation of surface energies and work functions for the lower-index surfaces. Of the 22 density functionals considered, we highlight the mBEEF density functional as providing the best overall agreement with experimental data. The optimal density functional choice is applied to the study of higher index surfaces for the three metals, and Wulff constructions performed for nanoparticles with a radius of 11 nm, commensurate with nanoparticle sizes commonly employed in catalytic chemistry. For Pd and Cu, the low-index (111) facet is dominant in the constructed nanoparticles, covering ∼50% of the surface, with (100) facets covering a further 10 to 25%; however, non-negligible coverage from higher index (332), (332) and (210) facets is also observed for Pd, and (322), (221) and (210) surfaces are observed for Cu. In contrast, only the (0001) and (10−10) facets are observed for Zn. Overall, our results highlight the need for careful validation of computational settings before performing extensive density functional theory investigations of surface properties and nanoparticle structures of metals.
The surface energy can be calculated through the use of interatomic potentials or, as in most recent work, quantum mechanical methods, especially density functional theory (DFT).7–11 Such is the ease and availability of high-throughput density functional theory, Vitos et al. have recently created a database of surface energies computed for the low index surfaces of 60 metals, computed using a full charge density (FCD) approach9 that provides efficient and accurate energetics. In this approach, the Hartree and exchange correlation part of the energy functionals are calculated from the charge density, using LDA or GGA functionals, while the kinetic energy is calculated from the Kohn–Sham kinetic energy, using full potential linear muffin-tin orbitals (LMTO) with the atomic-sphere approximation. The results compare well with other computational investigations that used density functionals (DF) for the surface energy and the work function.9 Cramer et al.12 reviewed the accuracy of GGA, meta-GGA, hybrid, hybrid meta- and range-separated hybrid DFs for the simulation of transition metals, discussing the implications for bulk band structures, structural and spectroscopic properties; and reactivity. Tran et al.10 also published a database of surface energy calculations for 70 elements, with properties calculated employing the GGA approach of Perdew, Burke and Ernzerof (PBE)13 and compared broadly to computation and experiment. Patra et al.14 studied the (111), (110) and (100) surfaces of metals from Groups 8 to 11 of the periodic table (Pd, Pt, Cu, Ag, Ru, Rh, and Au), as well as the main group metal Al, which are all face centered cubic (FCC) metals, using six various DFs: LDA, PBE, PBEsol, SCAN, SCAN+rVV10 and RPA. The investigators concluded that the SCAN functional complemented by non-local van der Waals (vdW) corrections from the revised Vydrov–Van Voorhis 2010 (rVV10) DF, SCAN+rVV10,15 gave the most accurate agreement with experiment for both surface energies and mean work functions.
Despite these detailed computational studies of metal surfaces, there remains a need for a systematic and uniform study of the importance of choice of functional and simulation parameters when modelling both low and high index surfaces of densely packed FCC and HCP metals, as commonly applied to catalytic chemistry, in order to identify how the choice of DF and numerical settings can impact the validity of these simulations. In the context of catalysis, high index surfaces are particularly important as they can exhibit high activity16 when used as catalysts in fuel cells, petrochemical reforming and automotive catalytic converters, due to the higher density of low coordinated sites; and metal catalysts with high-index planes can display enhanced activity relative to close-packed low-index facets such as (111), (110) and (100) planes, such as for Pt.17 High-index facets and high surface-energy nanocrystals also have wider applications such as in drug treatment, sensing and optics,18 stimulating further attention for both simulation and experiment. Quan et al.19 studied high index surfaces for Pd and Pt metals and found that (730) and (411) facets of Pt show improved reactivity towards acid and ethanol oxidation, while the (720) facet offers improved rates for oxygen reduction reaction compared to the low index (100) and (111) surfaces. The Pd(730) facet also shows improved reaction yield when used as a catalyst for electro-oxidation of formic acid and in the Suzuki coupling reaction.20
In this work, we address two key aspects of computational modelling of metal surfaces, namely the choice of simulation settings and functionals, and their use in investigating the properties of high-index surfaces. We present a thorough analysis of the parameters needed for accurate bulk and surface calculations, including for high index surfaces, with specific focus on late-transition FCC (Pd, Cu) and HCP (Zn) metals, representing elements from Group 10, 11 and 12 of the periodic table. In the following section we summarize our methodology; subsequently, results for bulk calculations with 22 exchange–correlation DFs are compared to experimental lattice parameters and cohesive energies, and the best performing DFs are then used to calculate surface energies and work functions for relevant low- and high-index surfaces. We discuss the effect of variation in calculation parameters for surfaces, such as slab thickness, in order to highlight the attention to detail necessary when configuring such simulations. Finally, we present and discuss Wulff constructions of nanoparticles formed with the differing choices of DF, in order to highlight the impact of such approximations.
![]() | (1) |
The surface energy, Esurf, is calculated as a combination of the surface cleavage energy, Ecleav, and the subsequent stabilizing relaxation energy, Erelax, which are obtained as:47
![]() | (2) |
![]() | (3) |
Esurf = Ecleav + Erelax | (4) |
Φ = Vvac − εFermi | (5) |
In order to assemble the results for each DF for collective analysis here, the MPAE is calculated for each XC and material, considering both a0 and Ecoh, with respect to the experiment values:
![]() | (6) |
For all the exchange–correlation DFs considered, the error in Ecoh is generally higher than the error for a0 and c0, especially in the case of Zn. The poor accuracy of Ecoh for Zn has been observed previously by Lejaeghere et al.,52 who highlighted a difference of 20% when using PBE; similar observations are reported by Janthon et al.,53 who reported a difference of 29%. In an attempt to address the discrepancies highlighted, Lejaeghere et al.52 applied zero point and finite temperature phonon corrections to the experimental data; however, these corrections result in only marginal improvements against experiment, thus failing to resolve the significant error. For PBE, the addition of a vdW correction (PBE+TS) provides better agreement between the calculated lattice parameters and experiment; however, the resulting cohesive energies are much greater than experiment, especially for Cu (calculated: 4.14 eV, experiment: 3.49 eV). Similar results are observed for the PBE0 functional with TS included, which highlights the complexity in identifying DFs that can accurately model structure and energetics for multiple systems.
Of the DFs considered, BLYP, B97-D, HCTH-407, B3LYP, R48PBE and RPBE functionals have a high MPAE for Zn (31.23, 30.78, 27.86, 27.26, 21.38, and 19.46% respectively), which contributes strongly to an overall high average MPAE. PBEsol, HSE06, revTPSS and PBEint have an intermediate average MPAE, in the range from 6 to 10%, while PBE, PBE+TS, PBE+MBD-NL, TPSS, SCAN, revSCAN, and mBEEF have an average MPAE of <6%. The lowest average MPAE is obtained for mBEEF, at 2.56%. The accuracy of mBEEF arises from a combination of machine learning with a Bayesian concept to generalize the fitting procedure for a broad range of material properties,40 providing generally accurate cohesive energies and lattice parameters.
Fig. 2 presents our results using the PBE DF to calculate surface energies as function of slab depth. We considered the Pd(111), (100) and (110) facets, and oscillations in the surface energy are observed with varying numbers of layers; the oscillations are most pronounced for sparser k-grid densities of one k-point per (0.039 × 2π) Å−1, with variation of 0.06 J m−2 between 9- and 10-layer slab (111) models. The oscillations decrease with increasing k-grid density, and are reduced across all facets for a k-grid density of one k-point per (0.018 × 2π) Å−1; however, even with a dense k-grid sampling of one k-point per (0.011 × 2π) Å−1, oscillations of 0.01 J m−2 are present for the models of the (110) facet. Structural analysis shows these minor fluctuations are due to the crystallographic cleaving creating a ‘crenulation’, which causes the electronic structure to alternate between even and odd layer numbers, resulting in changes in the electrostatic potentials and therefore the onsite energies.55 An equivalent analysis for Cu(111), (100), and (110) facets, and Zn(0001) and (10−10) facets, shows similar oscillations in the surface energy are reduced when increasing the k-grid density (Fig. S6 and S7, ESI†). Comparing all systems, a slab thickness of seven layers, with a k-grid density of one k-point per (0.018 × 2π) Å−1, is deemed necessary to minimise the QSE in our slab calculations.
DF | Facet | ||||
---|---|---|---|---|---|
(111) | (100) | (110) | (111)/(100) | (111)/(110) | |
a The value were calculated using linear regression for a set of slabs with different thicknesses. | |||||
PBE | 1.36 | 1.54 | 1.60 | 0.86 | 0.85 |
Da silva et al.2 | 1.36 | ||||
Patra et al.14 | 1.36 | 1.79 | 1.61 | 0.76 | 0.84 |
Tran et al.10 | 1.36 | 1.52 | 1.57 | 0.89 | 0.86 |
Singh-Miller et al.48 | 1.31 | 1.49 | 1.55 | 0.88 | 0.84 |
Lin et al.56 | 1.33 | 1.51 | 1.60 | 0.88 | 0.83 |
Janthon et al.57 | 1.25 | ||||
1.27 ± 0.04a | |||||
PBE+TS | 1.52 | 1.64 | 1.74 | 0.92 | 0.87 |
PBE+MBD-NL | 1.64 | 1.72 | 1.80 | 0.95 | 0.91 |
TPSS | 1.67 | 1.82 | 1.95 | 0.92 | 0.86 |
SCAN | 1.67 | 1.80 | 1.88 | 0.92 | 0.89 |
Patra et al.14 | 1.54 | 2.08 | 1.83 | 0.74 | 0.84 |
revSCAN | 1.75 | 1.90 | 1.97 | 0.92 | 0.89 |
mBEEF | 1.32 | 1.50 | 1.58 | 0.88 | 0.83 |
Experiment, Tyson et al.: | |||||
T = 0 K58 | 1.63 | — | — | ||
T = 1828 K3 | 1.74 | — | — |
For all the exchange–correlation DFs considered here, the surface energy of the (111) facet is lower than the (100) and (110) surfaces, agreeing with other theoretical work.10,48 The agreement of our PBE results with previous simulations is good (±0.05 J m−2) with the exception of the investigations of Patra et al.14 who report the (100) surface energy to be greater than (110), contrary to all other studies. The addition of the Tkatchenko–Scheffler vdW correction to PBE (PBE+TS) increases the surface energies for the (111), (100) and (100) facets by 0.16, 0.1 and 0.14 J m−2, respectively, bringing the energies closer to the experimental values. The same increases in surface energy are observed for PBE+MBD-NL, relative to PBE, with increases of 0.28, 0.18 and 0.20 J m−2, for the (111), (100) and (110) surfaces, respectively. For the meta-GGA DFs, TPSS and SCAN give almost identical surface energies for (111) and (100) facets, which are similar to experimental results, whilst the surface energy of the (110) facet is slightly greater with TPSS. revSCAN gives larger surface energies compared to SCAN and is further from the experimental measurements; in contrast, mBEEF gives the lowest surface energies of 1.32, 1.50 and 1.58 J m−2 for the (111), (100) and (110) facets, respectively.
Direct comparison for each Pd surface facet with experiment is not straightforward, as experimental surface energies are averaged over the various crystal facets (1.63 J m−2 at 0 K, and 1.74 J m−2 at the 1828 K3,58); however, broad comparison of each DF with experiment can be made. Comparing our average results for each DF with experiment leads to the conclusions, firstly, that PBE and mBEEF underestimate the surface energies of Pd by a small amount (averages of 1.50 and 1.46 J m−2, respectively); secondly, that PBE+TS and PBE+MBD-NL compare well with experiment (averages of 1.63 and 1.72 J m−2, respectively); and finally, that all other DFs overestimate the surface energy of Pd.
The ratio of surface energies is an alternative metric of DF accuracy. Such ratios are important as they determine the equilibrium nanoparticle shape and the dominant facets; for instance, the smaller the ratio of (111)/(100) surface energies, the more the (111) facet dominates the nanoparticle surface. Recently, Chen et al.59 reported experimental measurements for Pd of 0.77 ± 0.02 for the (111)/(100) surface energy ratio, obtaining the equilibrium nanoparticle shape by annealing at 450 °C. From our calculations, closest agreement with experiment is for the PBE (0.86) and mBEEF (0.88) DFs; all other approaches predict a ratio >0.92. We also present in Table 2 the calculated (111)/(110) ratio for Pd, and note that the trends are inconsistent compared to the (111)/(100) ratio, with the lowest ratio obtained with mBEEF (0.83) and the highest with PBE+MBD-NL (0.91).
The surface energies calculated for Cu(111), (100) and (110) facets are reported in Table 3, where they are compared with previous computational and experimental work. It is noted for Cu that Tyson et al. report experimental surface energies at T = 0 K of 1.79 J m−2 and then 1.57 J m−2 at the melting temperature (T = 1357 K), i.e. a decrease in the surface energy with increasing temperature, in contrast to results for Pd (Table 2).
DF | Facet | ||||
---|---|---|---|---|---|
(111) | (100) | (110) | (111)/(100) | (111)/(100) | |
a The value were calculated using linear regression for a set of slabs with different thicknesses. | |||||
PBE | 1.37 | 1.51 | 1.58 | 0.91 | 0.87 |
Da silva2et al. | 1.41 | ||||
Da silva60et al. | 1.32 | 1.48 | 1.59 | 0.76 | 0.83 |
Patra et al.14 | 1.36 | 1.79 | 1.61 | 0.91 | 0.84 |
Tran et al.10 | 1.34 | 1.47 | 1.56 | 0.90 | 0.86 |
Janthon et al.57 | 1.31 | ||||
1.30 ± 0.11a | |||||
PBE+TS | 2.57 | 2.72 | 2.77 | 0.94 | 0.93 |
PBE+MBD-NL | 1.80 | 1.93 | 1.99 | 0.93 | 0.90 |
TPSS | 1.60 | 1.77 | 1.93 | 0.90 | 0.83 |
SCAN | 1.58 | 1.78 | 1.90 | 0.93 | 0.83 |
Patra et al.14 | 1.49 | 1.71 | 1.84 | 0.87 | 0.80 |
revSCAN | 1.75 | 1.93 | 2.02 | 0.90 | 0.67 |
mBEEF | 1.43 | 1.56 | 1.63 | 0.92 | 0.88 |
Experiment, Tyson et al.: | |||||
T = 0 K58 | 1.79 | — | — | ||
T = 1357 K3 | 1.57 | — | — |
For the GGA functionals, again PBE provides low surface energies, with 1.37, 1.51 and 1.58 J m−2 for the (111), (100) and (110) facets; these are marginally below the experimental values, also. Inclusion of van der Waals correlation corrections, using the TS approach (PBE+TS), results in seemingly poor agreement with experiment, as the surface energies increase dramatically to 2.57, 2.72 and 2.77 J m−2 for the (111), (100) and (110) facets, respectively. For the meta-GGA DFs, SCAN and TPSS again give very similar results, as observed for Pd; mBEEF also gives relatively low surface energies, compared to contemporary meta-GGA methods, of 1.43, 1.56 and 1.63 J m−2 for (111), (100) and (110) facets, respectively; these are again similar to the PBE results. As a consequence, the average surface energy for the three facets obtained by PBE (1.49 J m−2) and mBEEF (1.54 J m−2) are similar, again being lower than the experimental results, while TPSS and SCAN give results closer to experiment. The average result for PBE+TS (2.68 J m−2) is anomalously large compared to experiment, and further investigation is warranted to understand the cause of this result.
Previous measurement of the ratios for (111)/(100) surface energies for Cu facets are absent from the current literature; in the present work, the ratio of (111) to (100) surface energies is calculated to range from 0.88 (PBEsol) to 0.94 (PBE+TS). The (111)/(110) ratio has a similar range, from 0.82 to 0.94.
Table 4 reports the surface energies calculated for the (0001) and (10−10) facets of HCP Zn, together with computational work by Tran et al.10 and the experimental data of Tyson et al.3,58
The Zn surface energies presented in Table 4 span a wide range of energies. revSCAN and PBEsol give the lowest surface energies for the (0001) facet, of just 0.06 J m−2 and 0.14 J m−2 respectively, while PBE+TS gives the highest value of 0.92 J m−2. All other DFs give surface energies for the (0001) facet between 0.24 J m−2 to 0.50 J m−2, seemingly well below the experimental results; the results obtained for the PBE DF are noted, however, to be in excellent agreement with the previous computations of Tran et al.10
The surface energies calculated for the (10−10) facet are much larger than the (0001) facet, with the lowest value obtained for PBE (0.99 J m−2) and a maximum for PBE+TS (1.73 J m−2). Interestingly, the (10−10) surface energy calculated here with PBE is much larger than that reported by Tran et al.,10 which we attribute to differences in nearest neighbour distances; in their work, the nearest neighbor separations are smaller than the experimental values. Overall, the surface energies of the (0001) facet are much lower than the (10−10) facet, though values calculated for the latter are noticeably closer to the experimental results.
We conclude our study of Zn by tentatively calculating a ratio of (0001)/(10−10) facet energies for each DF. The span of ratios is large, with the smallest ratio observed for revSCAN (0.03), and the largest ratios observed being 0.40 and 0.53, with PBE+MBD-NL and PBE+TS, respectively. We note that the (0001)/(10−10) ratio is potentially misleading when the surface energy of (0001) is computed as being very low, such as for revSCAN, and future studies will further investigate the causes of these observations.
Values of the work function (Φ) for Pd, as calculated with each considered DF, are presented in Table 5. For all the DFs considered, the work functions decrease in line with surface energies, such that Φ (111) > Φ (100) > Φ (110). For the (111) facet, the best match between calculation and experiment was obtained with TPSS, with a difference of 1.10%; the greatest difference was 4.96% with PBE+MBD-NL and mBEEF, which both under-estimate Φ (5.17 eV). For the (100) facet, SCAN and TPSS match well with experiment, with a difference of 1.51%, while the largest difference is for mBEEF (5.85%). The similarity between TPSS and SCAN for electronic properties is interesting, given their similarity also for energetics in Tables 2–4. Finally, for the (110) facet, PBE and mBEEF agree accurately with experiment, while SCAN gives the largest difference (7.50%).
DF | Facet | ||
---|---|---|---|
(111) | (100) | (110) | |
PBE | 5.19 (−4.60) | 5.02 (−5.28) | 4.80 (0.00) |
Da Silva et al.2 | 5.64 | ||
Patra et al.14 | 5.32 | 5.12 | 4.95 |
Tran et al.10 | 5.20 | 5.13 | 4.62 |
Singh-Miller et al.48 | 5.25 | 5.11 | 4.87 |
PBE+TS | 5.24 (−3.67) | 5.04 (−4.91) | 4.85 (+1.04) |
PBE+MBD-NL | 5.17 (−4.96) | 5.04 (−4.91) | 4.77 (−0.62) |
TPSS | 5.50 (+1.10) | 5.38 (+1.51) | 5.11 (+6.46) |
SCAN | 5.51 (+1.29) | 5.38 (+1.51) | 5.16 (+7.50) |
Patra et al.14 | 5.39 | 5.19 | 5.04 |
RevSCAN | 5.42 (0.37) | 5.03 (−5.09) | 4.82 (+0.42) |
mBEEF | 5.17 (−4.96) | 4.99 (−5.85) | 4.80 (0.00) |
Derry et al.62 | 5.67 ± 0.12 | 5.48 ± 0.23 | 5.07 ± 0.2 |
Fisher et al.61 | 5.44 ± 0.03 | — | — |
Küppers et al.64 | — | 5.3 | — |
Gay et al.63 | — | — | 4.8 |
The work function data for Cu are presented in Table 6 compared with other computational and experimental work. For the (111) facet, SCAN predicts a value of Φ that is very close to experiment (4.89 for 4.94 eV,65 respectively) with an difference of 1.01%, followed by mBEEF with a difference of 2.23%, while PBE+MBD-NL give a large difference (4.71 eV, 4.66%). For the (100) facet, TPSS gives the value of 4.59 eV reported experimentally,66 with mBEEF also performing well (4.53 eV, 1.31%) while a larger deviation was obtained with PBE (4.44 eV, 3.27%). For the (110) facet, the calculated Φ using TPSS is in good agreement with experiment (4.50 eV for 4.45 eV, respectively)62 with a difference of 1.12%, followed by PBE and mBEEF [4.35 eV (2.25%) and 4.33 eV (2.69%), respectively], while RevSCAN predicts a low Φ of 4.18 eV, giving the largest difference (6.06%).
DF | Facet | ||
---|---|---|---|
(111) | (100) | (110) | |
PBE | 4.72 (−4.45) | 4.44 (−3.27) | 4.35 (−2.25) |
Patra et al.14 | 4.78 | 4.42 | 4.38 |
Tran et al.10 | 4.88 | 4.47 | 4.19 |
Wang et al.67 | 4.71 | 4.50 | 4.27 |
PBE+TS | 4.76 (−3.64) | 4.50 (−1.96) | 4.28 (−3.82) |
PBE+MBD-NL | 4.71 (−4.66) | 4.45 (−3.05) | 4.23 (−4.94) |
TPSS | 4.75 (−3.85) | 4.59 (0.00) | 4.50 (+1.12) |
SCAN | 4.89 (−1.01) | 4.55 (−0.87) | 4.30 (−3.37) |
Patra et al.14 | 4.98 | 4.43 | 4.48 |
revSCAN | 4.85 (−1.82) | 4.52 (−1.52) | 4.18 (−6.06) |
mBEEF | 4.83 (−2.23) | 4.53 (−1.31) | 4.33 (−2.69) |
Rowe et al.65 | 4.94 ± 0.03 | — | — |
Gartland et al.66 | — | 4.59 ± 0.03 | — |
Derry et al.62 | — | — | 4.45 |
For Zn, the work functions of the (0001) and (10−10) surface facets are given in Table 7. mBEEF provides the closest agreement with experiment for the (0001) facet, with a difference of 0.72%, while PBE+TS gives the largest difference (−6.02%). An experimental work function for the (10−10) facet is unavailable for comparison with the computed values; however, it is interesting to note for the computed results that the work function is greater for this facet than the more stable (0001) facet, which is in contrast to the FCC metals, where the less stable surfaces have smaller work functions.
Fig. 3 summarises the observations in this section, presenting the percentage differences between calculated and experimental work functions for each element with each DF. All DFs have provided errors below 7% for the three elements, which is in the same order of the MPAE presented in Fig. 1. As discussed, PBE gives the best agreement for Pd; TPSS and SCAN give the best agreement for Cu; and mBEEF gives the best agreement for Zn. An average MPAE (i.e. mean of means) with respect to experiment has been proposed for the three considered elements: for this metric, mBEEF gives the lowest average difference of 1.94%.
For bulk materials, mBEEF and PBE+MBD-NL provide the lowest differences relative to experiment, of 2.55 and 2.78% in the MPAE respectively; when considering surface energies, the differences between computation and experiment are on average larger, and the DFs that performed well for bulk were worse performing: mBEEF (and PBE) generally underestimate the surface energies, while PBE+MBD-NL (plus revSCAN and PBE+TS) overestimate. As well as the absolute energies being a metric of accuracy, one can also consider the relative surface energies as representing accurately the energetic ordering of surfaces for a given element: considering the ratio of the (111)/(100) surface energies for Pd, and comparing to the experimental results of Chen et al.,59 PBE and mBEEF are noted as agreeing better with experiment, with all other DFs giving values closer to unity.
For electronic work functions, SCAN and TPSS give (similar) results with good agreement to experiment for the Pd(111) and (100) facets, with SCAN also performing well for the Cu(111) facet and TPSS best performing for the Cu(100) and Cu(110) facet. For the other Pd facet, (110), mBEEF performs well, and similarly is closest to experiment for the Zn work function. When we average the deviations in calculated work functions from experiment, across all the density functionals, as shown in Fig. 3, we note that all DFs selected for surface calculations provide errors below 5% on average, which is in the same order of the average MPAE presented in Fig. 1. Overall, it is clear that mBEEF provides the lowest mean error for bulk and surface calculations, and therefore we highlight mBEEF as the most accurate options for general application to the different metals considered, and potentially for more complex systems such as alloys.
In order to ensure accuracy for the Wulff construction process, additional high index (332), (322), (211) and (221) facets were cleaved from the crystal bulk for Pd and Cu, and the stabilities evaluated; for Zn, Tran et al.10 have shown that (0001) and (10−10) are significantly lower in energy than all other surfaces and so other high index facets were not considered here. Some high index surfaces offer comparable stability to the low index surface facets, and thus are observed in the outcomes of the Wulff construction. For Pd, the order of stability of all facets is (111) > (100) > (332) > (210) > (322); for Cu, a slight difference is noted with both the (111) and (100) facets more stable (i.e. lower in energy) than the (322) > (332) > (221) > (110) > (210) facets. The work functions were also calculated for the high index facets (ESI,† Table S5), and in general are inversely related to the surface energy for these FCC metals, though not strictly: the Pd and Cu(221) facets give the smallest value of Φ, with the (110) and (210) facets providing the next smallest values.
The structures predicted by the Wulff construction for a 5000 atoms nanoparticle of Pd, Cu and Zn are given in Fig. 4. The morphology predicted for all three species is in good agreement with other computational work by Tran et al.10 and Lin et al.56 The surface coverage of each facet type, presented in Table 8, shows that the (111) facet is most prevalent for Pd (48.83%), followed by the (100) facet (18.80%). The high index (332) and (210) facets cover 18.30% and 6.96%, respectively. Whilst not the highest in surface energy, we note that the (110) facet is not present, in agreement with the Wulff construction provided by Tran et al.10
![]() | ||
Fig. 4 The crystal morphology calculated by Wulff construction for (a) Pd, (b) Cu and (c) Zn nanoparticles of 5000 atoms. |
Facet | Surface energy | Surface coverage | Surface energy | Surface coverage |
---|---|---|---|---|
Pd | Cu | |||
(111) | 1.32 (1.36) | 48.83 (48.81) | 1.43 (1.37) | 47.83 (57.32) |
(100) | 1.50 (1.54) | 18.80 (9.29) | 1.56 (1.51) | 23.91 (25.84) |
(110) | 1.58 (1.60) | 0.00 (0.00) | 1.63 (1.58) | 8.10 (6.97) |
(332) | 1.41 (1.45) | 18.30 (19.59) | 1.57 (1.50) | 0.00 (0.00) |
(322) | 1.45 (1.50) | 7.11 (4.19) | 1.55 (1.51) | 10.47 (0.02) |
(221) | 1.49 (1.51) | 0.00 (1.26) | 1.58 (1.53) | 6.73 (6.72) |
(210) | 1.59 (1.63) | 6.96 (7.53) | 1.70 (1.66) | 2.95 (2.94) |
Facet | Surface energy | Surface coverage |
---|---|---|
Zn | ||
(0001) | 0.24 (0.32) | 71.02 (60.24) |
(10−10) | 1.17 (0.97) | 28.98 (39.75) |
To provide a demonstration of the impact that DF choices have on nanoparticle structure, and the consequences for investigations of reactivity we also, as noted, computed the Wulff construction considering the surface energies calculated with the widely used PBE approach; the outcomes show that the Pd(100) facet has a 10% higher surface coverage with mBEEF. The (210) facet was absent in the Wulff construction using mBEEF while it represents 1.26% using PBE. Such information is critical in understanding the behaviour of Pd nanoparticles toward catalytic reaction: Zhang et al.72 have compared the reactivity of (111) and (100) facets toward CO2 reaction and concluded, by comparing the activation energies of the two facets, that the (100) is more reactive than the (111). Having the (100) facet more abundant in the nanoparticle as obtained from the mBEEF Wulff construction would result in a more reactive nanoparticle. No experimental proof of the existence of (210) facet for Pd has been found in current literature.
For Cu, the most prominent facet is again the (111), with a descending order of surface coverage thus: (111) > (100) > (332) > (110) > (221) and (210). In contrast to Pd, the (322) facet was not observed. Tran et al.10 obtained a similar result for the absence of the (322) facet, though did predict the presence of (331), (311) and (310) facets. Again, we computed a Wulff construction with the PBE DF for comparison and identify notable differences in the surface coverages when changing the DF: for mBEEF, the (111) surface coverage is 10% lower than when using PBE, and for mBEEF the (322) facet has a 10% coverage whereas is essentially absent in the PBE model; such differences could be significant when designing nanocatalysts based on DFT calculations, thus demonstrating the impact of DF choice.
For Zn, a simple hexagonal closed packed morphology is formed by the two main (0001) and (10−10) facets, covering 71.02% and 28.98% of the surface, respectively, while with PBE this coverage is 64.24% and 39.75%, respectively. The Zn results are in close agreement with the TEM presented by Mai et al.,73 as well as the theoretical work of Tran et al.10
The selected density functionals were further used to study low-index surfaces. To remove the presence of quantum size effects, a minimum model thickness of 7 atomic layers perpendicular to the surface plane were necessary, as well as a dense k-grid of one k-point per (0.018 × 2π) Å−1. The surface energies obtained agree reasonably with experiment. It is noted that vdW corrections considered on PBE calculations, namely PBE+TS and PBE+MBD-NL, increase the surface energy of all three elements, with particularly poor outcomes for Cu surfaces with PBE+TS. By considering the computed absolute and relative surface energies, work functions, and previously highlighted bulk observables, and comparing to a range of experimental data, mBEEF is concluded as offering the greatest accuracy of the bulk and surface properties of these metals.
The significance of the choice of density functional is demonstrated by a comparison of nanoparticles formed using Wulff construction with mBEEF and PBE computed surface energies, showing surface coverage differences of some facets of up to 10%. Despite PBE providing relatively good agreement with experiment for bulk and surface energies, the differences observed between mBEEF and PBE when calculating Wulff structures, coupled with weaknesses of PBE in adsorption chemistry,40 highlight that careful density functional choices should be made when studying surface reactivity or catalytic processes. The observations provide a sound basis for the use of mBEEF, together with the k-point and layer thickness settings discussed above, for future computational studies of surfaces of these metals and their alloys. Whilst it is reasonable to assume mBEEF may be appropriate for studying structure and energetics of other materials given its derivation with emphasis on bulk and surface properties, further work is necessary to investigate the generality of our observations towards all transition metals and the composite materials they may form.
Footnote |
† Electronic supplementary information (ESI) available: The accompanying supporting information is available at DOI: 10.1039/d1cp01602d and includes: figures of the FCC(111), (100) and (110) surfaces, and the HCP(0001) and (10−10) surfaces; graphs of Cu and Zn surface energies as a function of slab thickness; tables of the element specific deviations in lattice parameters and cohesive energy when considering each separate exchange–correlation DF, and also exchange–correlation averaged values; and surface energies and work functions for high-index facets as calculated with mBEEF. The structures from this study have been uploaded to the NOMAD repository (DOI: http://10.17172/NOMAD/2021.05.21-1). The raw data from which all energetic results were derived is available to access at DOI: 10.17035/d.2021.0133038780. |
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