The dynamics of nanoscale clusters can be distinct from macroscale behavior described by continuum formalisms. For diffusion of 2D clusters of N atoms in homoepitaxial systems mediated by edge atom hopping, macroscale theory predicts simple monotonic size scaling of the diffusion coefficient, DN ∼ N−β, with β = 3/2. However, modeling for nanoclusters on metal(100) surfaces reveals that slow nucleation-mediated diffusion displaying weak size scaling β < 1 occurs for “perfect” sizes Np = L2 and L(L+1) for integer L = 3,4,… (with unique square or near-square ground state shapes), and also for Np+3, Np+4,…. In contrast, fast facile nucleation-free diffusion displaying strong size scaling β ≈ 2.5 occurs for sizes Np+1 and Np+2. DN versus N oscillates strongly between the slowest branch (for Np+3) and the fastest branch (for Np+1). All branches merge for N = O(102), but macroscale behavior is only achieved for much larger N = O(103). This analysis reveals the unprecedented diversity of behavior on the nanoscale.

Nanoscale dynamics of crystalline clusters,1–4 epitaxial structures,5–7 and even liquid jets8 can differ qualitatively from mesoscale or macroscale behavior described by continuum formalisms. This applies for reshaping of 3D crystalline nanoclusters1–3 and 2D epitaxial nanoclusters.6 Differences occur when linear nanocluster sizes, L, decrease below various characteristic lengths.1–3,9–12 For L < Lk, the characteristic separation between kinks on close-packed step edges, 2D clusters become effectively faceted and reshaping is controlled by inhibited nucleation of new edges.9 Similar anomalies have been discussed for 3D nanoclusters, but here facets can be macroscopic and nucleation of new layers becomes prohibitive above nanoscale.13 Also relevant are characteristic Ehrlich-Schwoebel type lengths associated with additional barriers to round kinks and corners in 2D and to cross step edges and move between facets in 3D.10,14,15 In general, key exponents describing both temporal scaling and size-scaling of relaxation times differ from macroscale theory.1–3,5,6 Note also that reshaping of 2D epitaxial clusters and pits, or 3D clusters and voids in bulk crystals, is equivalent on the macroscale,16 but not on the nanoscale.11,12 The size-dependence of diffusivity of supported metal nanoclusters was also found to deviate from macroscale predictions.17–22 Refined continuum treatments with multiple order parameters might describe such anomalous scaling of diffusion.23 However, the current study reveals a lack of recognition of the full diversity of possible nanoscale dynamics, which undoubtedly cannot be captured even with refined continuum treatments.

To explore this issue, we provide a comprehensive analysis of a canonical model for diffusion of 2D epitaxial clusters on metal(100) surfaces mediated by periphery diffusion.10 Cluster diffusion impacts kinetics of coarsening of arrays of supported nanoclusters via Smoluchowski ripening, i.e., cluster diffusion and coalescence.5,21,24–28 Thus, elucidation of coarsening kinetics has importance for stabilizing functional nanomaterials, e.g., in limiting catalyst degradation. In our stochastic lattice-gas model, clusters of N adatoms on a square lattice of adsorption sites (lattice constant a) interact with just the nearest-neighbor (NN) attractions of strength ϕ > 0. Edge atoms can hop to NN and also to the second NN empty sites, provided that hopping retains at least one NN adatom in the cluster. This preserves cluster connectivity and size. All hop rates have the Arrhenius form h = ν exp[−Eact/(kBT)] for surface temperature T and Boltzmann constant kB. In our simplest model, the activation barrier, Eact, satisfies Eact = Ee + (nNN − 1)ϕ, where nNN denotes the number of in-plane NN adatoms prior to hopping. Thus, Eact = Ee applies for diffusion of isolated edge atoms along close-packed steps and around kinks (or corners), which occurs at rate he = ν exp[−Ee/(kBT)]. For reference, choosing Ee = 0.29 eV and ν = 1012.5 s−1 mimicking Ag/Ag(100) yields he = 107.6 s−1 at 300 K. The above formulation of Eact could be refined to include an additional kink rounding barrier, δ, for second NN hops around kinks, but we concentrate on δ = 0.

Model behavior is precisely determined by Kinetic Monte Carlo (KMC) simulation. Our focus is on the cluster diffusion coefficient, DN = lim δt→∞ DN(δt), where DN(δt) = ⟨[δr(δt)]2⟩/(4δt). Here, δr(δt) is the displacement in the cluster center-of-mass (CM) in a time interval δt, and ⟨⟩ denotes an average over a CM trajectory. See Fig. 1. Our model has DN(δt) ∝ a2he so that DN/(a2he) is independent of Ee and ν. Due to backward correlations in the walk of the CM, DN(δt) is not constant but decays to a plateau value for sufficiently long δt > δtc, where ⟨[δr(δtc)]2⟩ ∼ a2. Thus, precise determination of DN from ⟨[δr(δt)]2⟩ for δt ≥ δtc requires a CM trajectory with length, ttot, of at least O(103 δtc). We choose ttot ∼ 35 000δtc. Macroscale theory predicts simple monotonic size scaling of the diffusion coefficient, DN ∼ σPD N−β, with β = 3/2 where the step mobility σPD has Arrhenius energy29 EPD = Ee + ϕ, but we find distinct behavior. Insight beyond KMC simulation comes from analytic treatments. If ΩN denotes the number of distinct configurations of a cluster of size N, then DN follows exactly from analysis of the “acoustic” eigenmode of an ΩN × ΩN matrix encoding allowed transitions between cluster configurations. This matrix is extracted by Fourier transformation of the linear master equations.30,31 However, this analysis is only viable for small N, as ΩN grows rapidly with N. Thus, we instead apply alternative combinatorial analyses.

FIG. 1.

KMC simulation of a cluster CM trajectory with N = 36 (ϕ/kBT ≈ 7.7, he ttot ≈ 4 × 105).

FIG. 1.

KMC simulation of a cluster CM trajectory with N = 36 (ϕ/kBT ≈ 7.7, he ttot ≈ 4 × 105).

Close modal

Prior to presenting KMC results, we characterize nucleation-mediated versus “facile” cluster diffusion for moderate sizes with N ≥ 9. We identify “perfectsizes Np = L2 and L(L+1) with L = 3,4,… for which clusters have unique square or near-square ground state shapes. This uniqueness does not apply for sizes N = L(L + n) with n ≥ 2. For perfect sizes, diffusion is nucleation-mediated in the sense that after an atom is extracted from a corner in the ground state to an edge (raising the energy by ΔE = +ϕ), another atom must quickly detach from a corner or kink to join the first atom before the first atom returns to the corner. Such a pair of atoms is regarded as nucleating a new edge. The most direct pathway to create another perfect configuration with displaced CM shifts atoms from kinks and corners of the opposite edge to complete this new edge. Shifting the second and subsequent atoms from one kink to another does not change the energy after each reattachment, so the system evolves through a series of first excited state configurations with energy ΔE = +ϕ above the perfect configuration. Only when the last (isolated) edge atom is shifted to recover the perfect configuration is the energy lowered by ΔE = −ϕ. See Fig. 2(a). Diffusion of clusters with sizes Np+3, Np+4, etc., is also nucleation-mediated requiring formation of a dimer on an outer edge to facilitate long-range diffusion of the cluster CM. Nucleation-mediated diffusion involves an atom breaking out of a kink (or corner) site with rate hk = ν exp[−(Ee + ϕ)/(kBT)] and aggregating with an isolated edge atom which has low quasi-equilibrium density neq = exp[−βϕ/(kBT)]. Thus, DN ∼ neq hk ∼ exp[−Eeff/(kBT)] with effective barrier9,10,18 Eeff = Ee + 2ϕ.

FIG. 2.

Direct pathway for nucleation-mediated (a) and facile (b) cluster diffusion. Indirect pathway (c) for facile cluster diffusion. All recover the initial configuration with displaced CM. Atoms are denoted by red squares on a gray square grid of surface adsorption sites for the metal(100) surface. X indicates a fixed location on the surface.

FIG. 2.

Direct pathway for nucleation-mediated (a) and facile (b) cluster diffusion. Indirect pathway (c) for facile cluster diffusion. All recover the initial configuration with displaced CM. Atoms are denoted by red squares on a gray square grid of surface adsorption sites for the metal(100) surface. X indicates a fixed location on the surface.

Close modal

For “facilesizes Np+1 and Np+2, edge nucleation is not necessary. For Np+1, an isolated edge adatom on a perfect core (a “special” ground state configuration) can readily diffuse around the cluster. For Np+2, a NN pair of edge atoms or edge dimers on a perfect core (a ground state) can dissociate and reform on another edge. Neither process results in a net change of energy. After the isolated edge atom or dimer is transferred to a new edge, atoms can be transferred from the opposite edge of the core to complete the edge to which the isolated adatom or dimer was moved. This again leaves an isolated adatom or dimer on the edge of a displaced perfect core. Shifting of atoms from one kink to another does not change the energy after reattachment, and in this case the system evolves through a set of configurations iso-energetic with the initial ground state configuration. See Fig. 2(b). Facile diffusion just involves breaking atoms out of kink sites and subsequent edge diffusion so that Eeff = Ee + ϕ.

In addition to the above direct pathways for long-range diffusion, there are numerous less efficient indirect pathways with atoms removed from multiple corners. Here, the cluster wanders through a large phase space of configurations iso-energetic with the first excited state for perfect sizes or with the ground state for facile sizes. See Fig. 2(c). However, for long-range diffusion, most of these eroded corners must be rebuilt as the cluster must repeatedly pass through the unique ground state for perfect sizes and the “special” ground state for facile sizes (unless accessing higher excited states).

Next, we present an overview of KMC results illustrating various regimes and branches of DN behavior for ϕ = 0.24 eV and δ = 0 at 300 K. See Fig. 3. Small sizes N = 4-8 all have the form Np+1 or Np+2 and exhibit facile diffusion with high DN. (Even higher DN values for N = 2 or 3 where Eeff = Ee are not shown.) For moderate sizes, N = 9 to O(102), for clarity we just show four distinct branches: facile Np+1, facile Np+2, perfect Np, and slow Np+3. Key features are as follows: (i) initially high values and rapid decay of DN ∼ N−βf for facile sizes Np+1 with large βf ≈ 2.6 up to N ∼ 100 (see the supplementary material) and similarly high DN but less regular decay for facile sizes Np+2; (ii) lowest values of DN for sizes Np+3 (not Np) with slow decay DN ∼ N−βs, where βs ≈ 0.53 for N ∼ 67-200; (iii) very weak size-dependence of DN for perfect sizes up to Np ≈ 81; also perfect and Np+3 branches merge for small N = 12; (iv) intermingling of DN for perfect Np with facile branches for Nmingle ≈ 81 (dashed yellow arrow in Fig. 3), and subsequent transition to a rapid decrease of DN for perfect sizes; (v) near-merging of all branches for N ≈ Nmerge ≈ 250 (solid brown arrow in Fig. 3). For larger sizes N > Nmerge, if we write DN ∼ N−βeff, the effective exponent slowly varies from βeff ≈ 0.75 for N just above Nmerge, to βeff ≈ 1.12 for N from 500 to 1000, and to β = 1.5 (the macroscopic value) for N → ∞. Here, the kink separation is Lk = ½ exp[½ϕ/(kBT)] ≈ 52, and the asymptotic regime N >> (Lk)2 ≈ 2700 is not achieved in our simulations.

FIG. 3.

DN versus N for ϕ = 0.24 eV and δ = 0 at 300 K. Inset: Strong oscillations with maxima (at Np+1) and minima (at Np+3).

FIG. 3.

DN versus N for ϕ = 0.24 eV and δ = 0 at 300 K. Inset: Strong oscillations with maxima (at Np+1) and minima (at Np+3).

Close modal

We have also assessed behavior for ϕ = 0.20 eV at 300 K. All the features for ϕ = 0.24 eV are preserved qualitatively, but now βf ≈ 2.3 up to N ∼ 100, βs ≈ 0.84 for N ∼ 67-200, Nmingle ≈ 49, Nmerge ≈ 150, with βeff ≈ 1.06 just above Nmerge, βeff ≈ 1.33 for N from 500 to 1000, and βeff ≈ 1.48 for N from 2000 to 3600. Here Lk = 24 consistent with achieving asymptotic scaling N >> (Lk)2 ≈ 570.

Next, to provide fundamental insight into DN behavior, we exploit instructive combinational analysis of cluster configurations and also apply first-passage concepts:

Fast decay of DNfor facile cases. For facile Np+1 clusters, we find scaling of DN ∼ N−βf exhibits exponents βf ≈ 2.3-2.6 far exceeding any identified previously for 2D cluster diffusion. We attribute this behavior to the feature that the cluster can wander between a large number of iso-energetic ground state configurations, ΩN(0) ∼ Nα, with α ≈ 2.8 for N = O(102). Most configurations are far removed from the special configuration with one edge atom on a perfect core through which the cluster must pass for long-range diffusion. If ⟨tN⟩ denotes the first-passage time for the walk through configuration space to return to the special configuration, one expects that DN ∝ 1/⟨tN⟩. Analysis for random walks in any dimension suggest that32 ⟨tN⟩ ∝ ΩN(0) so that DN ∼ 1/ΩN(0) implying that βf ≈ α.

Intermingling of DNfor perfect and facile branches. The distinction between perfect and other sizes of clusters is predicated by the former primarily existing in square or near-square ground state shapes. However, the number of configurations, ΩNp(1), corresponding to first excited states with energy ΔE = +ϕ above the ground state increases strongly with Np, e.g., ΩNp(1) = 1140, 2472, 5152, 10 352, 20 208,… for Np = 36, 49, 64, 81, 100,…, respectively. Perfect sized clusters have a significant probability of being in the 1st excited state when17 ΩNp(1) ≈ exp[ϕ/(kBT)] = 2208 (10 764) for ϕ = 0.20 (0.24) eV at 300 K corresponding to Np ≈ 49 (81). This roughly matches the size where perfect and facile branches intermingle (dashed yellow arrow in Fig. 3 for ϕ = 0.24 eV).

Behavior for perfect sizes. When N is not too large, diffusion is largely controlled by the nucleation step, which depends weakly on N and not so much on the subsequent transfer of atoms to complete the new edge. This explains the weak dependence of DNp on Np. The property that DNp for larger Np = L2 actually exceeds that for smaller Np = L(L − 1) reflects the feature that nucleation for perfect rectangular shapes is slightly more likely to occur on the longer side which increases the chance that subsequent nucleation will return the cluster to its original configuration.

Variation of DNwithin each cycle. DN varies quasi-periodically within each cycle between consecutive perfect sizes. The local minimum always occurs for size N = Np+3. Nucleation-mediated diffusion corresponds to sizes N = Np+n with n = 3, 4, …, n*, where n* corresponds to the next largest perfect size (e.g., n* = 4 for Np = 7 × 7 and Np+n* = 7 × 8). DN increases smoothly with N = Np+n in this range from a minimum for n = 3 to a maximum for n = n*. A relevant observation is that the degeneracy of the ground state decreases strongly with n from a maximum for n = 3 to a minimum of 1 or 2 for n = n*. These degenerate states include multiple atoms shifted from various corners of the cluster and thus multiple kinks which trap atoms. This makes it more difficult to efficiently nucleate a new outer edge (as the lifetime of isolated atoms is reduced) and also to transfer atoms to complete that new outer edge (which is required for long-range diffusion). Consequently, DNp+n unexpectedly increases with n. A local maximum within each cycle in DN occurs for the facile case N = Np+1 (or n = n* + 1).

“Oscillations” were observed in previous simulation studies,17,33 but limited analysis can provide misimpressions, e.g., that perfect sizes Np = L2 diffuse slowest. Note that DN values for n = n* (perfect sizes) can be quite close to those for the local maximum for facile n = n* + 1 and especially n = n* + 2. Thus, one might question the assignment of nucleation-mediated versus facile. However, an Arrhenius-type plot of DN does show clearly the distinction between Eeff for these classes. See Fig. 4.

FIG. 4.

Arrhenius analysis of diffusivity for facile (Np+1, Np+2) and nucleation-mediated (Np+n for n = 3, 4, …, n*) sizes with Np = 56 and n* = 8. Here we fix T = 300 K and vary ϕ over an experimentally relevant range (versus traditionally fixing ϕ and varying T).

FIG. 4.

Arrhenius analysis of diffusivity for facile (Np+1, Np+2) and nucleation-mediated (Np+n for n = 3, 4, …, n*) sizes with Np = 56 and n* = 8. Here we fix T = 300 K and vary ϕ over an experimentally relevant range (versus traditionally fixing ϕ and varying T).

Close modal

Weak variation of DNversus N for N = Np+3. While the high ground state degeneracy for facile sizes Np+1 produces rapid decay of DN versus N, this is not the case for N = Np+3. Why? The fundamental difference is that long-range diffusion of clusters for sizes Np+3 does not require repeatedly passing through a single special configuration, unlike for Np+1.

Merging of branches and post-merging behavior. Near-merging of all branches of diffusivity, and in particular of facile Np+1 and slow Np+3 branches, occurs for N ≈ Nmerge. Here, we argue that the distinctive nature of Np+3 clusters (relative to Np+1) is lost when the ratio of the number of 1st excited states ΩNp+3(1) to the number of ground states ΩNp+3(0) satisfies ΩNp+3(1)/ΩNp+3(0) ≈ exp[ϕ/(kBT)]. We find that ΩNp+3(1)/ΩNp+3(0) ≈ 2565, 7002, and 11 116 for Np = 196, 324, and 400, respectively, which implies that merging should occur for Nmerge ≈ 400 for ϕ = 0.24 eV. This estimate is above Nmerge ≈ 250 (solid brown arrow in Fig. 3) cited earlier. However, closer examination of data (see the supplementary material) reveals that DN values for Np+3 and Np+1 branches actually slightly cross at N ≈ 250 and more properly merge at N ≈ 400. After merging, the effective scaling exponent, βeff, describing the size-dependence of diffusivity is well below the asymptotic value of β = 1.5 from continuum theory. However, our simulations for ϕ = 0.20 eV indicate that βeff increases with N to approach β = 1.5 for N above ∼6(Lk)2.

In summary, KMC simulation of a model for diffusion of 2D epitaxial clusters reveals an extraordinary diversity of behavior with multiple distinct branches in the nanoscale size regime. We elucidate this behavior by exploiting combinatorial analysis. Surprisingly, perfect “closed shell” sizes are not the slowest, a feature plausibly extending to 3D supported clusters.7 Experimentally observed anomalous scaling5,22 corresponds to behavior in the merged regime where the scaling exponent varies continuously towards the asymptotic value. Additional analysis (see the supplementary material) for non-zero kink rounding barrier, δ > 0, reveals that behavior for δ = 0 is preserved qualitatively, although βeff is lower.

See supplementary material for simulation results for size-scaling of DN for facile clusters, merging of facile and also branches, and behavior for non-zero kink rounding barrier.

K.C.L. and J.W.E. were supported for this work by NSF Grant No. CHE-1507223. They developed theoretical interpretations of the data and performed detailed KMC analysis. D.-J.L. was supported by the USDOE, Office of Science, Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and Biological Sciences, and his work was performed at Ames Laboratory which is operated by Iowa State University for the USDOE under Contract No. DE-AC02-07CH11358. He performed the exploratory KMC simulations revealing diverse behavior together with preliminary analysis.

1.
N.
Combe
,
P.
Jensen
, and
A.
Pimpinelli
,
Phys. Rev. Lett.
85
,
110
(
2000
).
2.
T. H.
Lim
,
D.
McCarthy
,
S. C.
Hendy
,
K. J.
Stevens
,
S. A.
Brown
, and
R. D.
Tilley
,
ACS Nano
3
,
3809
(
2009
).
3.
D. N.
McCarthy
and
S. A.
Brown
,
Phys. Rev. B
80
,
064107
(
2009
).
4.
V.
Gorshkov
,
V.
Kuzmenko
, and
V.
Privman
,
CrystEngComm
15
,
7177
(
2013
).
5.
W. W.
Pai
,
A. K.
Swan
,
Z.
Zhang
, and
J. F.
Wendelken
,
Phys. Rev. Lett.
79
,
3210
(
1997
).
6.
C. R.
Stoldt
,
A. M.
Cadilhe
,
C. J.
Jenks
,
J.-M.
Wen
,
J. W.
Evans
, and
P. A.
Thiel
,
Phys. Rev. Lett.
81
,
2950
(
1998
).
7.
L.
Li
,
P. N.
Plessow
,
M.
Rieger
,
S.
Sauer
,
R. S.
Sánchez-Carrera
,
A.
Schaefer
, and
F.
Abild-Pedersen
,
J. Phys. Chem. C
121
,
4261
(
2017
).
8.
M.
Moseler
and
U.
Landman
,
Science
289
,
1165
(
2000
).
9.
P.
Jensen
,
N.
Combe
,
H.
Larralde
,
J. L.
Barrat
,
C.
Misbah
, and
A.
Pimpinelli
,
Eur. Phys. J. B
11
,
497
(
1999
).
10.
D.-J.
Liu
and
J. W.
Evans
,
Phys. Rev. B
66
,
165407
(
2002
).
11.
J. L.
Iguain
and
L. J.
Lewis
,
Phys. Rev. B
68
,
195407
(
2003
).
12.
Y.
Han
,
C. R.
Stoldt
,
P. A.
Thiel
, and
J. W.
Evans
,
J. Phys. Chem. C
120
,
21617
(
2016
).
13.
W. W.
Mullins
and
G. S.
Rohrer
,
J. Am. Ceram. Soc.
83
,
214
(
2000
).
14.
B. W.
Sheldon
and
J.
Rankin
,
J. Am. Ceram. Soc.
85
,
683
(
2002
).
15.
M. G.
Lagally
and
Z. Y.
Zhang
,
Nature
417
,
907
(
2002
).
16.
W. W.
Pai
,
J. F.
Wendelken
,
C. R.
Stoldt
,
P. A.
Thiel
,
J. W.
Evans
, and
D.-J.
Liu
,
Phys. Rev. Lett.
86
,
3088
(
2001
).
17.
J.
Heinonen
,
I.
Koponen
,
J.
Merikoski
, and
T.
Ala-Nissila
,
Phys. Rev. Lett.
82
,
2733
(
1999
).
18.
G.
Mills
,
T. R.
Mattsson
,
L.
Mollnitz
, and
H.
Metiu
,
J. Chem. Phys.
111
,
8639
(
1999
).
19.
S. V.
Khare
,
N. C.
Bartelt
, and
T. L.
Einstein
,
Phys. Rev. Lett.
75
,
2148
(
1995
).
20.
S. V.
Khare
and
T. L.
Einstein
,
Phys. Rev. B
57
,
4782
(
1998
).
21.
P. A.
Thiel
,
M.
Shen
,
D.-J.
Liu
, and
J. W.
Evans
,
J. Phys. Chem. C
113
,
5047
(
2009
).
22.
X.
Ge
and
K.
Morgenstern
,
Phys. Rev. B
85
,
045417
(
2012
).
23.
O.
Pierre-Louis
,
Phys. Rev. Lett.
87
,
106104
(
2001
).
24.
K.
Morgenstern
,
Physica Status Solidi B
242
,
773
(
2005
).
25.
T. W.
Hansen
,
A. T.
DeLaRiva
,
S. R.
Challa
, and
A. K.
Datye
,
Acc. Chem. Res.
46
,
1720
(
2013
).
26.
T.
Gerber
,
J.
Knudsen
,
P.
Stratmann
,
K.
Schulte
,
J. N.
Andersen
, and
T.
Michely
,
ACS Nano
7
,
2020
(
2013
).
27.
Y.
Fukamori
,
M.
Konig
,
B.
Yoon
,
B.
Wang
,
F.
Esch
,
U.
Heiz
, and
U.
Landman
,
ChemCatChem
5
,
3330
(
2013
).
28.
M.
Jiao
,
W.
Song
,
H.-J.
Qian
,
Y.
Wang
,
Z.
Wu
,
S.
Irle
, and
K.
Morokuma
,
Nanoscale
8
,
3067
(
2016
).
29.
J.
Krug
,
H. T.
Dobbs
, and
S.
Majaniemi
,
Z. Phys. B: Condens. Matter
97
,
281
(
1995
).
30.
J. R.
Sanchez
and
J. W.
Evans
,
Phys. Rev. B
59
,
3224
(
1999
).
31.
U. M.
Titulaer
and
J. M.
Deutsch
,
J. Chem. Phys.
77
,
472
(
1982
).
32.
E. W.
Montroll
and
G. H.
Weiss
,
J. Math. Phys.
6
,
167
(
1965
).
33.
K. A.
Fichthorn
and
S.
Pal
,
Bull. Am. Phys. Soc.
43
,
850
(
1998
).

Supplementary Material