The energetics and structure of nickel clusters: Size dependence Charles L. Cleveland and Uzi Landman School of Physics, Georgia Institute of Technology, Atlanta, Georgia 303324430 (Received4 September1990;accepted11 February 1991) The energeticsof nickel clusters over a broad size range are explored within the context of the many-body potentials obtained via the embeddedatom method. Unconstrained local minimum energyconfigurations are found for single crystal clusters consisting of various truncations of the cube or octahedron, with and without ( 110) faces,as well as some monotwinnings of these. We also examine multitwinned structures such as icosahedraand various truncations of the decahedron,such as those of Ino and Marks. Theseclusters range in size from 142 to over 5000 atoms. As in most such previous studies, such as those on Lennard-Jonessystems,we find that icosahedralclusters are favored for the smallest cluster sizesand that Marks’ decahedraare favored for intermediate sizes (all our atomic systemslarger than about 2300 atoms). Of course very large clusters will be single crystal face-centered-cubic(fee) polyhedra: the onset of optimally stable single-crystal nickel clusters is estimatedto occur at 17 000 atoms. We find, via comparisonsto results obtained via atomistic calculations, that simple macroscopicexpressionsusing accuratesurface,strain, and twinning energiescan usefully predict energy differencesbetweendifferent structures even for clusters of much smaller size than expected.These expressionscan be used to assessthe relative energeticmerits of various structural motifs and their dependenceon cluster size. I. INTRODUCTION The structural, electronic, and chemical characteristics of materialsdependon the state (phase) and degree(size) of aggregation.Clusters, i.e., finite aggregatesof up to tens of thousandsof atoms, exhibit unique physical and chemical propertiesand a systematicstudy of the dependenceand evolution of theseproperties with size allows elucidation of the transition from the molecular to condensed matter regimes.‘-4 Such investigationshave becomepossibleover the last two decadesdue to the developmentand proliferation of methods of preparation and characterization of clusters of various elementalmaterials and their compounds,as well as in differing charge states. A particularly complex and intriguing issueis the structure of clustersand the dependenceof structure on size. Difficulties in investigating this question are found on both the experimental and theoretical fronts. On the experimental side, the problem is twofold. First, since cluster systemsare larger than ordinary molecules,but too small to be dealt with as ordinary bulk materials, they are not well suited to exploration of their structure using the traditional approachesof spectroscopyand x-ray diffraction. As a result, structural studiesusingelectron diffraction are the preferredmethod of investigation and have beenapplied with significant success in studies mainly of gas phaseclusters of rare gaseP and molecular clusters.‘.” For metallic clusters, data obtained through electron diffraction experimentsis scarce,but valuable information has beenobtainedvia high-resolution electron microscopy for metal clusters from a few hundred to thousandsof atoms condensedon substrates.“-26 In addition, a scanning tunneling microscope probe has recently beenusedto examinesilver and gold clusters supportedon a graphite surface.27Furthermore, metallic clusters support7376 J. Chem. Phys. 94 (1 I). 1 June 1991 ed on graphite surfaces have also been investigated using extendedx-ray-absorptionfine-structure (EXAFS) and related x-ray techniques.“-” Analysis of this data is complicated, however, by the interaction between the deposited cluster and the substrateand the multitude of cluster sizes presenton the surface.” In the case of structural studies of gas-phaseclusters, analysisof the electron diffraction data is complicated by the clusters’finite size: they do not fill all spaceand so neednot possesstranslational symmetry. Consequently,the analysis reliesto a large extent on comparisonsbetweenthe measured diffraction patterns (i.e., diffraction functions which give the intensity of the scatteredelectron beam as a function of momentum transfer) with the results of model calculations which simulate the experimental data, using prescribedinteratomic interactions and ambient conditions. The analysis of the gas phase data is further complicated by the dependence of the structural characteristics of the system on the generation processand ambient conditions. Furthermore, small clusters (below a few tens of atoms) may undergo a radical structural changeby the addition of a singleatom (or molecule), and for both small and large clusters, a distribution (equilibrium or nonequilibrium dependingon the preparation conditions) of structural isomersmay be found for a given cluster size. The aboveconsiderationsmotivate systematic theoretical studiesof the structure and energeticsof clusters as well asof modesof cluster growth, phasechanges,and isomerization. A principal objective of such structural studies is the determination of size boundaries of energetic stability for various structural forms and the question of the transition from behavior characteristic of a finite system to that of a bulk system with increasingcluster size. Ideally, we would seekanswersto the abovequestionsfor all cluster sizesand 0021-9606/91 /‘I 17376-21$03.00 @I 1991 American Institute of Physics Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters for a range of temperatures. However, the plethora of possible structures and the isomerizations between them make such studies rather prohibitive. Instead, as severalresearchers previously have done, we limit ourselvesin this study to consideration of a number of structures whose selection is motivated by energetic and morphological considerations, as well as guided by accumulated past experience. As a further simplification, the energetic optimization of the structures is performed at zero temperature and thus neglects entropic effects. Nevertheless, such studies are relevant for developing understanding and establishing a conceptual framework which could guide a rational approach to thesecomplex structural issues,as well as aiding in the analysis of experimental data. In addition, obtaining the structural (and underlying energetic) trends, via minimization of the clusters’energiesusing a conjugate gradient technique, permits us to assesscritically the validity of formulas which we derive on the basis of macroscopic arguments for the energies of various structural motifs. Our results demonstrate the remarkable adequacy for many cluster types of such “macroscopic” expressions,provided the input energies (such as crystal plane dependentsurface energies,twinning energies,and strain energiesassociatedwith particular deformations) are known. The majority of experimental’-” and theoretica18*33-45 investigations to date on the structure of clusters have been on rare-gas clusters produced in supersonic beams during gas expansion. In such experiments, clusters can obtain stable structures (for eachcluster size) sincethey are formed at high temperatures and thus may anneal effectively.46Using electron diffraction data and analysis via molecular dynamics simulations employing Lennard-Jones(LJ) pair interactions, thesestudies have establishedthe presenceof icosahedral structures for small rare gas clusters (RGCs) containing 40-800 atoms. Much bigger argon clusters ( 104-10’atoms) exhibit a crystalline face-centered-cubic (fee) structure containing twin boundariesET4’ (which are detected by extra reflections in the diffraction patterns). However, the structural evolution of rare gas clusters in the intermediate regime is somewhat elusive. All theoretical studies of the energeticsand structure of RGCs employed pair interactions (mostly LJ potentials). The most complete study of these systemsis the recent one by Raoult et al.* These authors conclude on the basis of a relaxation method,48and using LJ potentials, that for clusters with less than 1600 atoms, the most stable structures belong to the icosahedral sequence,while for larger clusters the decahedra1sequenceis energetically more stable. Additionally, they found that although monotwinned fee models have a slightly lower energy than crystalline fee polyhedra, they are not expectedto becomethe structurally stable form for RGCs containing lessthan - IO5atoms. Theoretical investigations of the energetics and structure of metal clusters are complicated by the complex nature of bonding and cohesionin metals. While for very small clusters (mainly of alkali metals and aluminum) rigorous quantum chemical calculations haveprovided valuable structural information,49v5ofor larger clusters one must resort to approximate descriptions of the interatomic interactions. Such 7377 atomistic studiesemploying various levels of approximation havebeenperformed5’-55for clusters containing up to - 100 atoms. Another approach in the investigation of the structure of metal particles, which has been used for a rather long time ,22*5c6’ is founded on macroscopicconceptsrather than atomistic structural optimization. This approach is basedon the Wulff construction56’57which determines the equilibrium macroscopicmorphology of the crystallite (seeSec.III) and on the theory of elasticity which allows estimatesof the elastic strain energyfor a given structure.58The first systematic study employing the above principles was that of InoS8 who calculated the free energy of multiply twinned particles and compared it to that of an fee crystal of the samevolume using as input to the calculation macroscopic quantities characteristic of the material, such as cohesive, surface, twin-boundary, and elastic strain energies.In addition, the adhesive energy of interaction between the metal particle and the substrate support was included. The sequenceof structures obtained from Ino’s calculations is as follows: for metal particles smaller than a critical value ( - 100 w in diameter for gold), structures basedon the icosahedronare the most stable. For larger clusters, the optimal structures are truncated octahedra (these are semiregular polyhedra of 14 faces,sometimescalled tetrakaidecahedra,or TKDs). In addition, it was concluded that the decahedra, specifically those called Ino’s decahedra (seeSec.IV), are not structurally preferred at any size. A modified Wulff construction was introduced by Marks” to include twin boundaries. Motivated by experimental observations,” this modified construction allows for reentrant faces at the twin boundaries of the decahedron, thus decreasing its surface energy. Consequently, Marks predicts the evolution in cluster structure with increasing cluster size to progress from icosahedral to decahedra1and finally to truncated octahedral structures. The energetics underlying the above progression results from a balancebetween the relatively lower surface energies of the fivefold symmetric structures and the elastic strain energiesinherent in them. Since the total surface energy of a cluster varies roughly as its surfacearea while its total elastic strain energy varies roughly as its volume, the latter must increase more rapidly with the cluster’s size. At a critical size, the decahedral sequenceof clusters becomesenergetically more favorable than the icosahedral sequencesince it is characterized by a smaller strain energy. It should be noted, however, that numerical estimates” failed to show stability of the decahedral structures in the intermediate cluster sizeregime. In this context, we remark that application of the modified Wulff construction requires, as input, quantities which are often difficult (or impossible) to obtain from experiments (such as elastic strain energies,surface and twinning energies). In this paper, we show how to calculate these quantities for a given model of the interaction potentials. Motivated by the above considerationsand the increasing experimental efforts aimed at determinations of the structures of metal clusters and elucidation of correlations betweenthe structure and physical and chemical properties, we embarked on a systematic study of the dependenceof the J. Chem. Phys.,subject Vol. 94,toNo. June or 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution AIPii,1license copyright, see http://jcp.aip.org/jcp/copyright.jsp 7378 C. L. Cleveland and U. Landman: Structure of nickel clusters structure of metal clusters on cluster size. Our studies are basedon unconstrainedminimizations (relaxations) of the energiesof a multitude of structural motifs, with the interatomic potentials described via the many-body embedded atom method (EAM)624 parametrizedfor nickel.65 In our studies,both the macroscopicand microscopic, atomistic approachesare pursued, thus providing a test on the adequacyof the macroscopicconcepts.We concludethat the macroscopicexpressionswhich we develop,in conjunction with accurately calculated valuesfor the characteristic energiesasinput, provide a reliableframework for structural analysis. We find that in the small cluster size regime (less than 2300 atoms), icosahedral structures are energetically preferred, while for somewhatlarger clusters,the decahedraare more stable.Furthermore, the optimal singlecrystal polyhedron doesnot becomemore favorablethan the best Marks’ decahedronof similar size for clusterssmaller than - 17 000 atoms. In the next section, we briefly review the embedded atom method. In Sec. III, we describethe developmentof macroscopicexpressionsfor the energeticsof various structural forms, aswell as provide detailsof methodsfor calculations of surface,strain, and twinning energies.Results obtained via atomistic energy minimization are presentedin Sec. IV and compared to those derived from macroscopic estimates.Finally, we summarize our results in Sec.V. c I( #i) p;(R,) ++I ,x, q$j(R,)], (1) J(#l) where@ is the spherically averagedatomic electron density, the function ~+4~ dependsonly on the speciesof atoms i andj, and R, is the distancebetweenatoms i andj locatedat Ri and Ri. Thus the background density for each atom i is determined as the superpositionof electronic densitiesfrom other atoms, evaluatedat the nucleusof the ith atom. As seenfrom Eq. ( 1)) the total cohesiveenergyof the material is expressed asa sum over all atoms in the systemof atomic energycontributions. In the EAM, the functions F and 4 are determined by choosing for them functional forms which meet certain generalrequirementsand fitting parameters in these functions to a number of bulk equilibrium propertiesof the solid such as lattice constant, heat of sublimation, elastic constants, vacancyformation energy,etc. From the severalparametrization procedures which have been suggested,we have chosenthe one describedrecently by Adams et a1.65 III. MACROSCOPIC CALCULATIONS A. Single crystals For a macroscopicsingle crystal cluster of a given size and shapewhich only has flat facets,it is simple to calculate the energyif we know the energyper atom in the bulk crystal and the surface energy (surface energy per unit area) for each type of crystal face that is exposed.The macroscopic character is invoked in the neglect of corrections to bulk II. INTERACTION POTENTIALS energyother than surfaceenergies,such as “edge”and “verAs is well known, pair potentials are generally not ade- tex” energies. Alternatively, if we are given surfaceenergiesfor all the quate for a description of the energeticsin metals due to the (possibly) relevant types of facets, we can ask what shape density dependenceof the interactions which underlie the cohesionof thesematerials. Nevertheless,for simple metals will minimize the energy under the constraint that its volume remain constant.Wulff 56s7has provided a simple con(e.g., free-electronmetals), formulations basedon densitystruction that gives the answer. Proceedfrom the origin in dependentexpressionsfor the total energy6”69(employing effective Hamiltonians within the context of pseudopoten- any direction. This direction definesthe normal to a crystal tial theory) have been used with some success.However, surface. At a distance from the origin numerically equal to since the effectiveHamiltonian formulations, basedon sec- the surfaceenergyof that surface,erect a normal plane. Go ond-order perturbation theory with respectto the electron back to the origin and repeatthe processfor all other direcion interaction, are limited to free-electron (sp-bonded) tions which may point to facetson the cluster. The smallest volume containing the origin insideall erectedplanesis simimetals, we have representedthe energeticsof the material under study (nickel) using the embeddedatom method lar (in the geometricalsense)to the minimum energyshape for a cluster of given size. The construction is perfectly gen(EAM)62-64 which has been applied recently with significant success in studies of various transition-metal sys- eral and handlesevenunfacetedsurfaces. We will call the minimum energyshapefor a material its tems.62-65,7G72 Wulff polyhedron. Someresearchersuse this term to denote The EAM is a semiempirical method which provides a an Archimedian solid, the truncated octahedron,whosesurconvenientframework for atomistic calculations for metalfaceholds six square( 100) facesand eight equilateral hexaglic systems.In this method, the dominant contribution to the onal ( 111) faces.While this shapeis indeed the minimum energyof the metal is viewed as the energyof embeddingan energyfee polyhedron for surfaceenergiesgiven by a simple atom into the local electron density provided by the other atoms of the system, representedby an embedding-energy bond-breakingcalculation,76it at best only resemblesthe minimum energy polyhedra for any realistic materials exfunction F. This dominant contribution is supplementedby cept by coincidence,so such a usageseemssomewhat misshort-range,two-body interactions due to a core-core repulleading. sion 4. The basic idea underlying this method is thus the In order to apply such macroscopic methods, we need sameas that which motivated the developmentof the effecsurfaceenergies,and possiblybulk energies,for the material and both find their roots in the dentive-medium theory,73,74 from which the cluster is made. These may be difficult to sity-functional theory.75 acquireexperimentally.Often the bestinformation available The cohesiveenergyEcoh of the metal is given in EAM for surfacesis only an averagesurfaceenergy,undifferentiatby the ansatz J. Chem. Phys., Vol. 94, No. 11,i June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters ed by crystal face. One of the problemsin applying the macroscopicapproachto small clustersis being unsurewhether any deficienciesthat may arisedo so from the method’sfundamental approximationsor from poor values for material properties. Thus such methods are frequently applied only qualitatively. However, in cases such as ours where the atomic interactions are specified,the required energiesare not difficult to obtain. This will permit us to test, in at least one case,how well the macroscopicapproach works when appliedto small clusterswhen the input energiesare precisely known. The crystaline bulk systemmay be describedas consisting of a basisof N atoms (where N is on the order of several hundred) within a parallelapipedcomputationalcell defined by three fundamentaltranslation vectors which describethe periodicity of the cell (i.e., the periodic boundary conditions). Furthermore, these vectors are treated as dynamic variableson the samelevel as atomic coordinates.77In fact, the atomic coordinates are only describedin terms of the prevailing periodicity of the bulk system.Consequently,if so desired,a uniform strain could be applied to the systemby imposing suitable constraints on the three translation vectors that representthe correspondingperiodicity of the system under the specifiedstrain. To determinethe bulk energyper atom and the density for our material (at 0 K), it is sufficient to m inimize the energyof the systemby varying the vectors defining the unit ce11,77 which we accomplishby using the conjugategradient method.” This providesus with the bulk (per atom) energy for our material and also determinesthe bulk density. Using the EAM potentials for nickel, the calculated bulk energy (per atom) is eg = - 4.450 008 08 eV and the volume per atom is 10.9163A3.79 To determinethe surfaceenergyat 0 K for an unstrained surface,we removea periodic boundary condition, creating two free surfaces,” while holding the computational cell fixed sinceit is determinedby the bulk crystal. Subsequently, we relax the energyof the systemby varying atomic coordinates using the conjugategradient procedure. The surface energyis then simply the differencebetweenour relaxedsystem’s energyand that of the relaxedbulk systemdivided by twice the area of one of the newly exposedsurfaces. We have performedsuch calculationsfor the low M iller index surfaces[ ( 100)) ( 1lo), and ( 111)] which contribute to the Wulff polyhedron. In addition, we can also insert a single ( 111) twinning fault into a bulk system, and relax both the computational cell and atomic coordinatesto obtain the twinning energy. The results of these calculations are shown in Table I. We remark that the atomic energies near the centersof the slabswere very closeto the bulk ener- 7379 gy given above,which servesas evidencethat theseslabsare bulklike in their m iddles. We also note that relaxation has very little effecton the surfaceenergiesin nickel, all of which turned out to be somewhatsmaller than the experimental, facially averagedvalue” of 0.1485 eV/A2 (2.380 J mT2) (however, the experimental value may be questioned;see Ref. 62 for a discussion). Note that the twinning energyis negative.This suggests that the m inimum energycrystal structure for theseinteractions m ight be hexagonalclosepacked (hcp) insteadof fee. If we construct an hcp bulk systemand m inimize its energy, we find that the energyper atom is lower than that of the fee systemby only 4.6 x 10 - 4 eV. This is of little if any consequencein the study presentedhere, sinceother energiesare much more important for our clusters. With theseenergies,we are in a position to construct the Wulff polyhedron for nickel. Using the zero temperature surface energies” for Lennard-Jones6-12 interactions, we can also do the samefor that material (seealso Ref. 5 1 for a more inclusiveexploration of facetingfor this and other M ie potentials, and Morse potentials, neglecting relaxation). Theseresults are comparedin Fig. 1. The Wulff polyhedronfor nickel is markedly more similar to the truncated octahedron than the one for LennardJonesium.We will seethat the differencesbetweenthesepolyhedra for nickel and Lennard-Jonesiumexactly parallel differenceswe will observein comparing our results for m icroscopicnickel clusterswith thoseof Raoult et al8 for LennardJonesium. More quantitatively, Table II compares the ratios among the ( 111), ( lOO), and ( 110) surface energiesfor nickel, Lennard-Jonesium,and an ideal material whose Wulff polyhedron is exactly the truncated octahedron.Both nickel and Lennard-Jonesiumcrystallites prefer to have their ( 100) facessomewhatnearerto their centersthan does the truncated octahedron (i.e., the ratio yloo/y,, , for these materials is smaller than 2/d), increasingthe relative area of those faces.Both also have ( 110) facets which the truncated octahedronlacks, but in nickel that facet is very narrow (less than one nearest-neighbordistance in width for clustersup to about 15 000 atoms) and, unlike the LennardJonescase,’thesewill never end up being advantageousfor clusters as small as the ones we will examine later on an atomistic scale. Let us now calculatethe energyE,(N) of a Wulff polyhedron containing Natoms. Since( 110) facetsdo not occur on clusters as small as the atomistic oneswe will treat later, we will omit thesefacesin this calculation. Let us usea unit of length uN for our cluster such that the distancefrom the center of given Wulff cluster of N particles to a face with TABLE I. Interfacial energiesfor unstrained nickel slabs. Interface Unrelaxed surfaceor twinning energy Relaxed surface or twinning energy (1ll)surface ( 100) surface (110)surface ( 111) twinning plane 0.094 14 eV A - 2 0.103 41 eV A-* 0.11244eVA-2 0.094 675 8 eV A-’ O.l034068eV&’ 0.112341 2eV&* -O.O000883eVA-* J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters FIG. 1. The Wulff polyhedra for (a) nickel and (b) LennardJonesium. Also shown for comparison is (c) the truncated octahedron. surfaceenergyy is numerically equalto yuN. For a given N, the surface energiesthus determine the distancesfrom the center of the cluster to its facesand specify the geometryof the polyhedronso that we may calculatethe areasof its faces AllI and Al, and its volume V. For nickel, we find (with energyin units of eV and lengths in units of A) that E,(N) = Eg(N) + 8y,,,A,,, + 6y,ooA,, E,N + Cu”,, (2) where C = 0.014970 96. Sincethe volume is given as = F’= 8Am Y,IIU,/~ + ~mo~m~d3 = cl&./3 (3) and the volume per atom V/N = 10.9163,we can conclude that uN = 12.9812N 1’3and obtain for the Wulff polyhedron energy Ew(N) = EON+ 2.522 79N2’3. (4) 6. Multitwinned particles 1. lcosahedra An icosahedron(seeFig. 2) may be thought of as being composedof 20 distorted tetrahedral units all meetingat the center and each sharing three of its faces with neighboring units, leaving the last face to serve as one of the external icosahedralsurfacefacets.Crystallographically, eachfaceof the tetrahedronis an fee ( 111) face and the plane of atoms which two neighboringtetrahedrashareis a twinning plane, or put in other words, the stacking sequencein the direction normal to this plane is mirrored in it, ignoring the distortion of the tetrahedron. Twenty perfect tetrahedral units, however, cannot be put together to make an icosahedron.If surface vertices of neighboringunits are aligned,the units themselveswill overlap at the icosahedron’scenter. To make a proper icosahedron, the tetrahedral units must be strained to make three of their sides, those meeting at the central vertex, about 5% shorter than the three which lay on the surface.This sort of strain is easy to accommodatewithin the Parrinello-Rahman description” employedfor extendedsystems,in order to obtain the bulk and surfaceenergiesrequired for calculations of the cluster energiesas describedabove. For an unstrainedsystem,eachfundamentaltranslation vector defining the periodically repeatedcell could be taken as an integral multiple of one of the conventional primitive translation vectors for an fee material [each pair of which definesa ( 111) plane1. This situation is representedin Fig. 3. In this figure, all the distancesOA, OB, OC, AB, BC, and AC are equal. In order to apply icosahedralstrain, we need only changethe translation vector c so that the distancesOC, AC, and BC become4.894...% smaller than they were originally. [For further discussionof this sort of description of icosahedral(and decahedral)materials, seeRef. 59.1When minimizing the energy of a system with such a computational cell, the only parameter which we may vary is the volume. Doing so, and comparing with the corresponding result for the unstrained bulk, gives a strain energy (per atom) for uniform icosahedralstrain of E’, = 0.032 921 95 eV and a volume per atom of 11.0124A3, slightly greater than that for an unstrainedsystem. It is instructive to use Ino’s5’expressionfor the energy due to a uniform icosahedralstrain, with the elastic constants C,, , C,, , and C, for our model of nickel, which are given in Ref. 65. The resulting value for the strain energyis 0.0349eV. The agreementbetweenthis value and that obtained hereby direct minimization indicates that for our interactions, nickel under uniform icosahedralstrain is within the region of linear elastic behavior. If we removethe periodic boundary condition associated with translation vector c, we create two surfaceslike the OADB plane in Fig. 3, which under the type of strain described abovecorrespondsto the exposedface of a tetrahedral unit in an icosahedron.Fixing the shapeof the computational cell as beforeand relaxing atomic coordinatesyields a surfaceenergyof 0.0795eV/A’, nearly 16% lower than the unstrained value. (Without relaxation, the icosahedralsurface energy would have been 0.0894 eV/A’.) Notice that unlike the caseof the unstrainedcrystal (cf. Table I), surface relaxation has a significant effect here. We may perform for the icosahedronan analogouscalculation to that which gave us an expression [see Eq. (4) ] for E,(N) for the Wulff polyhedron. If we ignore the twinning energy,which will be very small, we obtain (in units of eV) TABLE II. Surfaceenergyratios for nickel and Lennard-Jonesium,along with thoseneededto produce a Wulff polyhedron that is exactly the truncated octahedron. Nickel Truncated octahedron Lennard-Jonesium 1.092 1.187 2/g/3(1.154...) >m( > 1.224...) 1.054 1.118 J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters 7381 for decahedraand single crystals. In the icosahedron,strain can be relieved by letting the surface facets bow out in a nonplanarand nonuniform fashion at the expenseof surface energy (see the discussion on icosahedrain Sec. IV). The two corrections nearly cancel for the range of cluster sizes where the energiesof the icosahedracross thoseof the Wulff polyhedra, so that the prediction made on the basis of the macroscopiccalculation is deceptively good. However, we will seethat in systemsunder lower strain, such as the single crystals and the decahedra(whose uniform strain energy is 30 times smaller than the icosahedron’s) , lhe macroscopiccalculations can indeedbe usedto produce quantitatively informative energy differences betweencluster forms. 2. Decahedra FIG. 2. The icosahedron and its relationship to the tetrahedral units of which it is composed. E,(N) = (eB +&IV+ 2.02709N2'3. (5) Comparing Eqs. (4) and (5), we can determine at what valueof N the Wulff polyhedronbecomesmore energetically favorable than the icosahedron.We find the energiesequal when N = 3413. In our microscopic atomistic calculations (see Sec. IV), we will find that the two energy curves for thesetwo structural forms cross when N = 3540. However, the remarkable agreementbetweenthe macroscopic estimateand that obtainedfrom microscopic calculations is fortuitous in this case.If we comparethe macroscopically calculated icosahedralenergieswith those obtained by atomistic minimizations of icosahedralclusters’energies, we find that the “real” clusters (i.e., those obtained via atomistic minimization) act as if their strain energy is substantially smaller than the value we have usedhere. In fact, relaxation of an icosahedralcluster from the “ideal” size and shapegiven by the macroscopicapproachreducesthe energy by a fraction almost an order of magnitude larger than that Figure 4 illustrates the kinds of “decahedra”we will be concernedwith here. Of these,only the classic decahedron or pentagonaldipyramid actually has ten faces, the others being so called only becauseof their derivation from it. The classic decahedronis, like the icosahedron,composedof slightly distorted tetrahedral units, five of which are joined at a common edgeand eachof which sharestwo of its ( 111) faces as twinning planes with neighboring units and contributes two other ( 111) facesto the surfaceof the decahedron. The faceson the classic decahedronare equilateral triangles. The principal advantageof the decahedronover the icosahedronlies in its lower strain energy.Part of this is due to the lower strain in the tetrahedral units of the classic decahedronand part is becausein addition to being able to minimize strain energyby varying the volume of the units, we can also relax an additional degreeof freedom corresponding to the length of the decahedron’scentral axis, shown as a dashedline in Fig. 4(a). The relaxedclassic decahedronshareswith the icosahedron the advantageof only having ( 111) faces,but because of its much lower sphericity, its surfaceareais comparatively larger and energetically it is a poor competitor. Ino5* suggested truncating the tetrahedral units as shown in Fig. (a) FIG. 3. An unstrainedcomputational cell for fee crystals. The three vectors a, b, and c are translations under whose repeatedapplication the computational cell periodically fills all spAce. FIG. 4. (a) The classic decahedron, (b) an example of Ino’s decahedron, and Cc) an example of Marks’ decahedron. J. Chem. Phys., Vol. 94, No. Ii,1 June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7382 C. L. Cleveland and U. Landman: Structure of nickel clusters 4(b), exposing( 100) facesand making the structure more spherical.While this improvesmatters and alsoprovidesanother parameterwe may vary to m inimize the energyof the polyhedron,Ino’s decahedronis not the lowestenergystructure for any known material, sinceas the polyhedrabecome larger and larger, the single crystals becomemore favorable than either the icosahedronor Ino’s decahedronbefore the decahedronsurpassesthe icosahedron. In an attempt to m inimize the surfaceenergyof the decahedron,however, we may give each of its single crystal tetrahedral units a surface like that of the single crystal Wulff polyhedron. This motivates Marks’ modified Wulff construction*’for decahedra,resultingin a nonconvexpolyhedron like that in Fig. 4(c). In this construction, the distancesfrom the origin to eachsurfaceplane are againtaken to be simply proportional to that crystal plane’ssurfaceenergy, and in addition, new “faces” are addedin the directions corresponding to the decahedra1unit’s ( 111) twinning planes,ignoring strain. Sincethe interfacial energiesof the twinning planes are very nearly zero, these planes almost passthrough the origin and excisea wedgefrom the Wulff polyhedron that would otherwise have resulted. Thus the exposedsurfaceof a unit in the decahedron,apart from being slightly stretched to fit, looksjust like part of the surfaceof the Wulff polyhedron if the necessarystrain doesnot significantly effect the surfaceenergies.Figure 5 illustrates the relationshipbetweenthe units of which Marks’decahedronis composedand the single crystal Wulff polyhedron. For uniform decahedra1strain, we may calculate the strain energy, and surface energiesfor the ( 100) face, the ( 111) “capping” face which touchesthe axis of the decahedron, and the (111) “notch” (or reentrant) face which makesMarks’ decahedronnonconvex,as well as the twinning planeenergy,by m inimizing the energyof systemswith two- or three-dimensionalperiodic boundary conditions, in a mannersimilar to our treatment of icosahedralstrain. The detailsof such calculationsare much more involved than the icosahedralcaseand are given in Appendix A. The resulting uniform strain energy per atom is e = 1.124426X 10- 3 eV. The volume per atom is 10.9186A3, only 0.02% more than that of the perfect singlecrystal. Table III displaysthe resultsfor the surfaceand twinning energies,with the ( 110) surface omitted for simplicity [for nickel clusters in the rangeof sizeswe concentrateon in this paper, ( 110) facets FIG. 5. The “tetrahedral” units of Marks’decahedron(left) and their relation to the Wulff polyhedron (right). do not occur]. Notice that in contrast to the icosahedral case,relaxation effectsfor surfaceenergiesare small. Comparisonwith Table I showsthat the changefrom the surface energiesof an unstrainedcrystal are also small. The percentagechangefor the capping ( 111) face is - 0.26%, that for the reentrant ( 111) faceis - 0.5 l%, and that for the ( 100) face is - 0.48%. The twinning plane energy, although slightly larger and with the oppositesign than the unstrained case,is still negligible. Given this information, we may seekan equationfor the energyof the best Marks’decahedron,for a given volumeor number of particles,just as we did for the Wulff polyhedra. This evaluationis describedin Appendix B where we obtain for the optimal Marks’decahedronlacking ( 110) facets,the expressionfor the cluster’senergyas a function of the numberofatomsinit,E,(N);seeEq. (Bl). If we compareED (N) with the Wulff polyhedron’senergy E,(N) from Eq. (4), we can estimatethat the single crystal will becomemore favorable than a Marks’decahedron whenNZ 17 000.Clearly, clustersof this sizemay have ( 110) facets-in fact their width would be about one nearest-neighbordistance.Our neglectof them, however,occurs on both the Wulff polyhedronand the decahedron.They will effect the energiesof both kinds of shapessimilarly and that effect will be small since they are much smaller than the other faces.For nickel, at least,we do not feel that our estimation would be improvedenoughto warrant the increasein the complexity of the derivation given in Appendix B. As we will seefrom comparing energydifferencesbetweenm icroscopicatomistic clustersof lessthan about 5000atoms with corresponding macroscopic ones, the macroscopic treatment of clusters can be expectedto be quantitatively quite good for clustersmuch smaller than 17 000 atoms. IV. MICROSCOPIC CALCULATIONS A. Single crystals and icosahedra Prior to describing our m icroscopic, atomistic treatment, it is appropriateto discussthe nomenclaturethat we will usefor different structural modelsof singlecrystal clusters. In general,it is not possibleto fit an arbitrary numberof atoms together in the shapeof any given polyhedron, especially one like the Wulff polyhedronfor nickel, the lengthsof whoseedgeshavenonsimpleratios. In addition, we examine clusterswhich depart from the ideal shape,not only because no clusters of m icroscopicdimensionsexist for that precise shape,but alsosincewe do not know apriori how reliablethe macroscopiccalculationsare for such small clusters. Some of the cluster shapeswhich we examinealreadyhaveconventional names,suchasthe cuboctahedron,the truncated octahedron, and the icosahedron.Others have no namesoutside the community of scientists studying small clusters and therefore needto be introduced for clarity. The most extensivem icroscopicstudy to date is that of Raoult et aZ.* who studied the structure of Lennard-Jones m icroclustersand who havenamedmany cluster modelsfor the first time. Sincethere are no precedents,we will adopt much of their terminology in this paper. All the fee singlecrystal shapeswhich we will consider may be thought of as originating from a cubewhosecenter is J. Chem. Phys., Vol. 94, No. 11.1 June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters 7383 TABLE III. Interfacial energiesfor nickel decahedra. Interface Unrelaxed surfaceor twinning energy ( 111) surface (capping) ( ill) surface (notch) ( 100) surface Twinning plane 0.094 60eV A;-’ 0.094 80 eVA-’ O.l0306eVA-’ Relaxed surfaceor twinning energy the origin and whoseeight verticespoint in the ( 111) directions. A cube,along with someother Platonic and Archimedean solids, is shown in Fig. 6. There are two fundamental families of such cubesthose with an atom at the origin and those with an fee octahedral site there.*’ We will generallydiscussonly atom-centered clusters in this section, becausethe octahedral-sitecentered clusters have little new to offer after the atom-centeredoneshavebeenexamined.Apart from the decahedra,if the number of atoms in a single-crystalcluster is odd, the cluster is atom centered; if even, octahedral site centered. Other polyhedracan be producedby “shaving off layers of atoms correspondingto crystal planeswe want to exposeon the surface.When shavingoff any face of atoms, we also removeall other similar ones,sincewe want to keepthe shapeswe consider as symmetric, and therefore as small in number, as possible.Repeatedlyshaving ( 111) facesfrom a cubeallows us to successivelyproduce,at leastapproximately, a sequenceof shapeslike the Archimedeansolids in Fig. 6. It also enablesus to produce many other intermediate shapesas well. However, we cannot produceclustersof arbitrary shape,as we could macroscopically,sinceatoms must be removedas discrete units. This aspectof atomicity is revealedexplicitly in the way the choice of a particular geometric shapefor a cluster re- FIG. 6. A sequenceof Platonic and Archimedian solids demonstrating the duality of the octahedron and the cube. Shown are (a) the cube; (b) the truncated cube; (c) the cuboctahedron; (d) the truncated octahedron; and (e) the octahedron. 0.094423 3 eVA-’ O.O941898eVA--2 O.l029129eVA-* 0.0001663eVA-2 stricts the number of atoms which it can contain. If we want to construct an icosahedronor cuboctahedron,we must use a number of atoms in the set {13,55, 147,309,561, ...I. or to construct a truncated octahedron,we must choosefrom {38, 201, 1289,4033, ...}. etc. This posesthe questionof which modelswe should consider?The truncated octahedron [Fig. 6 (d) ] is an obvious choicesinceof all the namedshapes,it is closestto the Wulff polyhedron. We also consider local variations from this shapesinceit occurs sparselyand we want to examinesimilar shapesto fill the gapsin cluster size,as well as explore its local neighborhood in configuration space. Many of the modelswhich we haveconsideredare lessthan encouraging. In this paper, we concentrateon the more energeticallyfavorable models and a posteriori explain the principles that m ight have led us to such models from the outset. Let us construct our clusters from cuboctahedra[Fig. 6(c) ] which have the convenient property that removing one atomic layer from each of its faces producesthe next smallercuboctahedron.(A similar observationholds for the icosahedra.) This causesthe difference in the number of atoms betweena cuboctahedronand the next one in size to be as small as possible.Taking the sequenceof cuboctahedra,84we find that only for every fourth one can a truncated octahedron be produced by shaving off ( 111) planes of atoms. Nevertheless,Raoult et al.’ have defineda sequence of clusters (named“model C”) which closelyresembletruncatedoctahedraand which can be madefrom everycuboctahedron. Accordingly, a cluster belongs to model C if its ( 111) facesare just further from the center than would be the casefor the truncated octahedronand consequentlyare slightly smaller in comparisonwith the ( 100) faces.In this context, we remark that the Wulff polyhedron also has its ( 111) facesslightly further from its center than the truncated octahedrondoes.For any cuboctahedron,we havemerely to shave off ( 111) planes until we come to the last one further from the origin than the ideal truncated octahedral distance.Thus we have four model C clustersfor every truncated octahedron.85 Another sequenceof clustersmay be obtainedby exposing ( 110) facets.Given any model C cluster, we can simply strip off the line of atoms at the edgewhere two ( 111) faces meet. This produces a small (110) face consisting of two parallel lines of atoms. Following Raoult et al., we call these HKI clusters.86 The last sequenceof single-crystal clusters which we considerare cuboctahedra.Many previousresearchershave studiedthem, eventhough the shapeis not very optimal, J. Chem.Phys.,Vol.94,No.11,1 June1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7384 C. L. Cleveland and U. Landman: Structure of nickel clusters becauseof the special relationship, alluded to earlier, that the cubocthedronhas with the icosahedron.Not only do the two sequencescontain clusters with the same numbers of atoms,but any cuboctahedralcluster can convert to an icosahedralone,and vice versa,by meansof a simple twinning transformation.” Thus the competitionbetweenicosahedra and cuboctahedrais more direct and physical than that involving other single-crystalclusters,which generallycannot convert to other high symmetry clusters without gaining or losing atoms or at least undergoingsubstantialatomic rearrangement. Finally, we will also include in our m icroscopiccalculations the icosahedra,which are expectedto be energetically optimal for the smallestclusters,and sincewe wish to investigate as a function of cluster size the transition from icosahedra to other structural forms, such as single crystals and cuboctahedra. In Table IV some of the geometric properties of these clusters are collected. Here and elsewhere,m denotesthe numberof atomson an edgejoining a ( 111) faceand a ( 100) face; n denotesthe number of atoms on an edgebetweena ( 111) face and any non-( 100) face-either ( 111) or ( 110) for our clusters.The number of atoms on an edgebetweena ( 100)faceand a ( 110) faceon an HKI cluster is alwaystwo. First we will plot ,vsN “’ the energies(obtainedby energy m inimization using the EAM potentials) of theseclusters less the bulk energy of the same number of atoms EB (N) = l BN divided by LV”~. Using macroscopicconsiderationsas a guide, we expectthat the total energyof a given cluster shape, with N atoms and surface area S, could be expressedin the form5’ E(N) = E&v + E&v + ep, (6) whereeBis the bulk energyper atom, 6, is the uniform strain energyper atom (zero for the single-crystalclusters), and cy is an averagesurface energy per unit area for that cluster shape.Denoting by a a geometric factor suitable for that shape,we may write [E(N) -ESN]/N2'3~=E,N1'3+aEY. (7) Equation (7) is an approximateequality becausequite large clustersmay be necessarybeforethe surfaceareacan be well approximatedby aN 2’3for a given cluster shape. Thus a simple macroscopicapproach would lead us to expectthat plotting the energiesof m icroscopicsingle-crystal clusters in this way will producehorizontal lines ranked according to how well they m inimize surfaceenergy,while the icosahedralcurve will be a straight line with a positive slopecausedby its internal strain. In the upper panel of Fig. 7, we display the results of energym inimization for m icroscopicsingle-crystalclusters and the aboveexpectationsare born out. We also find that icosahedralclustersare most favorablefor clusterscontaining lessthan 3540atoms,at which point the truncatedoctahedra and model C clustersare very competitive with each other, as expected since their shapesbracket that of the Wulff polyhedron.As expected,we alsofind the ( 110) faceting of HKI clusters to be energetically unfavorable for smaller clusters and to becomemore attractive as cluster sizes increase,although we do not explore clusters large enough for it to becomethe optimal structural form. The cuboctahedrondoesnot competeat all with the other clusters in this size range. However, extrapolation” of the cuboctahedraland icosahedralenergiesenablesus to estimate that the cuboctahedralsare favoredover the icosahedralsfor clusterslarger than about 14 000 atoms. At this point we wish to comparethe resultsobtainedvia the atomistic energym inimization with thoseof macroscopic calculations.To perform macroscopiccalculationsfor an unrelaxedatomic cluster, we must be able to associatea polyhedron with it; i.e., we must take the cluster and find its set of surfaceplanes.This definesthe polyhedron and allows us to calculateits volume and various surfaceareas,which are usedin a macroscopiccalculationof the cluster’senergy.We note that sincewe are dealingwith rather small,atomic clus- TABLE IV. Single crystal atom-centeredclusters and icosahedra:number of atoms N, number of atoms on an edgebetweena ( 111) and a ( 100) face m, number ofatoms on an edgebetweena ( 111) faceand a non-( 100) facen. Each truncated octahedroncan be producedfrom the cuboctahedronin the same row by removing one or more setsof eight ( 111) planes,and ifone fewer set of ( 111) planesis removedfrom eachtruncated octahedron,the model C cluster in the samerow is produced. Icosahedra/cuboctahedra” Truncated octahedra N m n 147 309 561 923 1415 2057 2869 3871 5083 6525b o/4 O/5 O/6 O/7 O/8 o/9 o/10 o/11 o/12 o/13 4/l 5/l 6/l 7/l 8/l 9/l 10/l 1 l/l 12/l 13/l Model C N m ” 201 3 3 1289 5 5 4033 7 7 HKI N m n N m n 405 711 1139 1709 1925 2735 3739 4957 5341 4 5 6 7 6 7 8 9 8 3 3 3 3 5 5 5 5 7 369 675 1103 1673 1865 2675 3679 4897 5257 2 3 4 5 4 5 6 7 6 4 4 4 4 6 6 6 6 8 “Form and n, the left-hand value is for icosahedra;the right is for cuboctahedra. ‘Not studied here. J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters 5 53 cu’ z $3 hy: fci “, ui’s: 8,” x 0-e. o---E)---*--- Q---Q---Ct---@..--Q X -, x HKI * 4 F -& 5 $3, Y-s: 2d %* sd 7385 would initially be discouraged.All the singlecrystal clusters would have scaled energy differencessubstantially lower than any of the icosahedra,and for smaller clustersthe deficiency would be much worse. However, upon closer examination, we observedthat the relative ordering in energy of the clusters of similar size had beenremarkably improved. Results in which the energeticsof various structural modelsare comparedmay be presentedin various ways. In particular, we may use as our referencenot E&V, but the energiesof the membersof a standard referencefamily of clusters, such as the cuboctahedra, somewhat as van de Waa140does.The advantageof this approachover using the bulk energy as referenceis that it subtracts cluster surface energiesas well. While this is unimportant when presenting energiesobtained via atomistic m inimization, it is advantageouswhen displaying energiesfrom macroscopiccalculations for small clusters, sincesuch a subtraction can largely correct for systematicerrors, such as may be connectedwith the positioning of the surfaceplanes.We will usethe cuboctahedron as our referencecluster sinceit has no strain energy, it occurs at frequent intervals for better interpolation, and it will not be greatly m issedfrom the figures since it is such a poor competitor. Resultsobtainedby atomistic energym inimization and via macroscopiccalculations which take surface planes to passthrough surfaceatoms are shown in Fig. 8. At the top, the m icroscopic results, using an interpolation88 formula based on m icroscopic cuboctahedraare displayed. At the bottom, we show the results for macroscopicsingle-crystal polyhedra, using an interpolation formula basedon macroscopic cuboctahedra.The icosahedralcurve in both figures is the one obtained from our m icroscopiccalculationssince the macroscopicapproachfails to provide an accurateestimate for this structure, as discussedin Sec.III. The overall agreement between the results obtained by the two approachesis remarkable.Note, however, the overestimation of the energiesof the HKI clustersby the macroscopiccalculations. Nevertheless,this discrepancydecreasesas clusters become larger and the m icroscopic HKI clusters become more competitive energetically. The use of cuboctahedralreferenceenergiesinstead of bulk ones does not affect the relative energeticordering of clusters of similar size, regardlessof which convention is employedfor positioning the surfaceplaneswith respectto atomic ones. The advantageof using cuboctahedralreference energieslies in being able to changethe conventional location of the surfaceplanesin order to improve the relative energeticordering of clustersof similar size,sinceonly clusters of similar size can energeticallycompetewith one another.89 *sQ--.o ---Q.-~~---EP-.-c3---0 ,.QQBL Y HKI d.0 0.0 IA.0 I;.0 IA.0 do NV3 FIG. 7. In the upper panel of this figure, the minimized energiesof microscopic single clusters are representedrelative to the bulk, together with those of the icosahedra. In the lower panel, also relative to the bulk, are shown the energiesresulting from macroscopiccalculations for unrelaxed versions of the same clusters, along with the same icosahedral curve. In these macroscopiccalculations, surface planes were taken to fall between atomic layers. ters, it may make a substantial differencewhere we define those surfaceplanesto fall. We m ight choosefor one to cut through the atoms in the surfacelayer of its facet. Alternatively, we m ight choosefor the surface plane to fall outside that plane by a distanceequal to one-half the layer spacing for that crystal face.Each choiceproducesa different energy for every cluster we examine. First, let us take a surfaceplane to lie abovethe surface atoms by one-half a layer spacing. Results of macroscopic calculations with this convention are shown in the lower panel of Fig. 7. The overall energiesare are in adequate agreementwith the correspondingm icroscopicones,shown in the upper panel of Fig. 7, with the scaledenergy differencesin the figure too low by 0.03 eV for large clusters and worsefor smallerones.However, the relative ordering of the clusters in energy, particularly the truncated octahedron, model C, and HKI clusters, is poorly articulated and frequently wrong, evenfor larger ones. Let us explorea different conventionfor positioning the surface planes in the macroscopic calculation and move theseplanesso that they passthrough the cluster’s surface atoms. If we were to plot the results in the usual way, we B. lcosahedra There is substantialinterest in the characteristicsof relaxed icosahedralclusters. As we pointed out in Sec. III, systemsunder uniform icosahedralstrain have a relatively large strain energy. Nonetheless,m icroscopically relaxed icosahedral clusters are energetically favored over other typesevenfor clustersof severalthousandatoms.It is worthwhile to examinethe nature of the relaxation of icosahedral J. Chem. Phys., Vol. 94,toNo. Juneor1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject AIP11,l license copyright, see http://jcp.aip.org/jcp/copyright.jsp 7386 C. L. Cleveland and U. Landman: Structure of nickel clusters N ‘i X. .. ‘ic A- 561 N= 55 147 1415 2869 5063 2I 9 &t _ -. -x- - -.-.* ..-I-‘F _ _ _ -x---_ _ .+-.*&-...c.-~ _ --Q- - - +.‘&*--- 3 .-SC Z+ ‘% % f / )RA 70 t iI -? T I 0.0 I 2.0 I 4.0 I 6.0 I 8.0 I 10.0 12.0 Shell Number x. --_ FIG. 9. The energiesof vertex atoms on successiveshells of icosahedraof various sizes. Lines connect energiescorresponding to atoms in different shells in the same icosahedron.Results for icosahedracomprising three, five, seven,nine, and elevenshellsare shown. The 55-atom, two shell icosahedron is also shown, but with a dashedline. x- - _ _ x * ____ +-_..*-A----&.-----A --__ +X-.* -‘x----x.-~-~+ +--A-+..*: 1 x + bdi )RA I 6.0 / 8.0 I I 10.0 12.0 NV’ 1 I 14.0 16.0 18.0 FIG. 8. In the top graph, the minimized energiesof microscopicclustersare represented,relative to an interpolated cuboctahedralenergy.In the bottom graph, equivalentmacroscopicquantities are displayed,with the exception of the curve for icosahedra,which is the sameas in the upper graph. clusterswhich enablesthem to competeenergeticallyas well as they do. As mentioned above, we may analyze the energy of a cluster atom by atom. In Fig. 9 we display how the energies of atoms on the fivefold axeschangeas we move from the insideof a cluster to its outside.We observea great regularity with overall cluster sizeif we comparethe outermostlayer of each cluster and then successivelyproceed inwards. Our overall observationis that the energiesof atoms in the outer shellsof theseclustersare very similar, but that as the interior of the cluster is penetrated,energiesincrease.The further one penetrates,the greater is the increasein atomic energy with a particular concentrationof energyat the center of the cluster. Sincea large part of the cohesiveenergy in metals derivesfrom the embeddingof the metal ions in the electronic chargedensity of the medium, atoms will seekto occupy positionswhich optimize that embeddingenergy.Consequently,atoms on the outer shellsof the cluster attempt to compensatefor the m issingof neighborswhich would have beenpresentin the bulk by displacinginward toward regions of higher electronic density. (The optimal structure is of course a balance between the cohesiveembeddingenergy and the core-core repulsions.) The atoms that experience the greatestlossof electronicembeddingdensity are the ones at the outside verticesof the cluster. Under the geometryof the icosahedron,theseatoms can only move to a region of higher electronicdensityby pressingdirectly on atomsat the verticesof the shell below theirs. Becausethe vertex atoms form a linear chain from the outside of the cluster to its center, and since the stresson theseatoms is radial, stress accumulatesalong the fivefold axes and especially at the clusters’centers. It is not surprising that the energy of an atom at a cluster’scenteris still increasingalmost as strongly with the cluster’s radius when the cluster hasten or 11shells as when it had two or three. (We suspectthis behavior to be largely independentof the interatomic interaction for potentials that favor close-packedstructures, since the geometry of the icosahedronalmost forces such a concentration of stress.) Similar analysisto that leading to the results shown in Fig. 9 could also be made for atoms on the edgesadjoining faceson shells within the icosahedraor atoms on the faces themselves.By way of definition, let us say that asidefrom the vertex atoms on an icosahedralshell, we also have edge atoms, which adjoin two faces,but do not include the vertex atoms, and face atoms, which include every atom that is neither a vertex or an edgeatom. It is worth pointing out that although unrelaxedclustersshowa considerablevariation in atomic energiesfor the edgeatoms in a shell, or for the face atoms in a shell, the edgeenergiesare remarkably uniform within a given shell of a cluster after relaxation, as are those of the face atoms. For example,in the 1l-shell, 5083 atom icosahedron, the standard deviation of energies of edge atoms is greatestfor the tenth shell, where it is 0.003 27 eV, as comparedwith an edgeaveragefor that shell of - 4.4 183 eV. For the samecluster, the standard deviation of energies of face atoms is greatest for the 11th shell, where it is 0.005 02 eV, as comparedto a facial averagefor that shell of - 3.93929 eV. Within a given shell of an icosahedron,the energydifferencebetweena pair of atoms chosenfrom two different categories(vertex, edge,or face) is much greater J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters than the energydifferencebetweenany pair of atoms within any single category. Fargeset aL9 consider similar issuesfor clusters whose atoms interact through a Lennard-Jones 6-12 potential. They show how the spacingbetweenpairs of adjacentatoms lying on one of the fivefold axes of an icosahedral cluster changesin moving from the inside of a cluster out, and for a given distance from the center, how it changeswith cluster size. We call this spacing the radial nearest-neighbordistance. Furthermore, they examinethe nearest-neighbordistancebetweenatoms near the center of a face for eachof the shells of which an icosahedralcluster is composed.We take this to mean the distance betweenthose two atoms in the shell nearestthe center of a face, whether one of the atoms is exactly in the centeror not, and call it the tangential nearestneighbor distance for that shell. In Fig. 10, we show the results for the icosahedral clusters that we have studied, which are qualitatively similar to the results of Fargeset al. although somewhatlarger in degree.We note that both the c;i -Bulk 4, Shell Pail r c-4 gp L-4 -0E an as fE a ci Shell kig2@ 8 ci -2 -a53 2C” 4 3 2 $J e 0 3 z c-4 -yt: 2.0 I 4.0 Total Number 6.0 a.0 10.0 12.0 of Shells in Icosahedron FIG. 10. In the top graph, the distancesbetweenadjacent atoms on a fivefold axis ofan icoshedralcluster are shown. The curves connect distancesin different clusters betweenatoms in the same two shells and are marked by the pair of shell numbers involved. In the bottom graph, the distance between the two atoms in a shell closest to the center of one of its faces is shown, marked by the number of the shell. Note that the numbering of shells is such thatshell zerohasone atom,shellonehas12,etc. 7387 radial and tangentialdistancesbetweenatoms decreasenonuniformly as we move from the outside toward the inside of the cluster. Furthermore, as we consider larger and larger clusters, the distancesat the surfaceof the clusters increase and the distancesnear its center decrease.For the icosahedral clusters we have examined,the radial nearest-neighbor distanceis alwayslessthat the nearest-neighbordistancein a perfect bulk crystal, while the tangential nearest-neighbor distanceis larger than that distancefor a cluster’s outer layers and smaller for its inner ones. Farges et a1.9 also provide information about the convexity of faces on the 923-atom, six-shell icosahedralLennardJones cluster and suggestthat the convexity is more or less uniform from shell to shell for any given icosahedral cluster. Following their suggestion,we take a radial unit vector through the center of a face and project onto it two vectors pointing from the center of the cluster, with one pointing to a vertex atom on that faceand the other pointing to the atom closestto the face’scenter. We definethe layer position of the faceto be the meanof theseprojecteddistancesand the layer distortion to be their difference. We find for the sixshell icosahedralcluster that the ratio of the distortion for the outermost shell to the differencebetweenthe layer position of the two outermost shells is about 13%. Fargeset al., obtain 9% for an apparently similar quantity for their LennardJones material. They observethat this ratio increasesin a nearly linear mannerwith shell number if it is also calculated for the interior shells of the cluster, suggestinga uniformity of convexity throughout the shells of the cluster. We also observea roughly linear relation betweenshell number and this ratio. Moreover we note that this ratio, for a given shell number within a containing icosahedralcluster, is remarkably independentof the size of the cluster containing it. An alternative measure of the convexity of a surface may be obtainedin the following manner: Let us definetwo spheres.One is chosenso that its center is at the center of the icosahedralcluster and its surfacepassesthrough the vertex atoms on a given shell of the cluster. The other is chosenso that its surfacepassesthrough the vertex atoms of a particular face and also through the atom closest to the center of that face (or rather through the projection of that atom’s position onto the radial unit vector through the center of the face). As the mean curvature C of the face,we take the reciprocal of the radius of the secondsphere,although the face will tend to be flatter in its center than at its edges.To normalize this curvature in a way that should be independentof which of the shells we are examining if they are all similar, we multiply it by the radius R, of the first sphere.Thus if the faceswere completely Rat, the product would be zero, while if the cluster had relaxed to a perfect sphere, it would be unity. Results are shown in Fig. 11.We find that as expected, this relative curvature uniformly decreasesas we move to larger and larger clusters, since it ultimately must conform to the macroscopiclimit. C. Decahedra The principle difficulty in studying the energies of Marks’decahedrais the richnessof the parameterspace[see Figs.4(c) and 51.As a simplification,we ignore( 110)faces J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7388 C. L. Cleveland and U. Landman: Structure of nickel clusters 8 d 8 d $8 vo -7 ;: 6 8 6 -a B---+-49 w I 2.0 I 4.0 Total Number I 6.0 I a.0 I 10 $ II 10.0 FIG. 12. An Ino’s decahedronwith m = 7 and n = 5 is shown on the left. On the right is shown the resulting Marks’ decahedronif theoutermost line of atoms on eachtwinning plane is removed.This decahedronhass = 1 and p = 2 as well as m = 5 and n = 5. of Shells in lcosahedron FIG. 11. The relative curvature of faceson shells within icosahedraof various sizes. sincein the rangeof cluster sizeswhich we study, such faces do not appearto be favorable. Even so, we have two inequivalent kinds of ( 111) faces,which we have called capping facesand notch faces.Thus while we can specify one of our single-crystalpolyhedra without ( 110) facesjust by listing the number of atoms on the edgejoining ( 100) and ( 111) faces m and the number of atoms on the edgejoining two ( 111) facesn, we will find an additional parameteris needed for decahedra.For decahedra,we will use m to denote the number of atoms on an edgejoining a ( 100) face and a capping ( 111) face, n to denote the number of atoms on the other kind of edgeon a (100) face, which connectsit with either a notching ( 111) face or if no notching has occurred with a neighboring (100) face, andp to denotethe number on an edgejoining the two kinds of ( 111) face.This notation is the sameas that usedby Raoult et al* Instead ofp, however,we shall usually refer to s = p - 1, the number of ( 111) notching planeswhich havebeenremovedfrom the sidesof eachdecahedra1unit to producethe desiredMarks’decahedron. We chooseto do this since our schemefor organizing the plethora of Marks’ decahedrarefers each back to the Ino’s decahedronfrom which it could be madeby notching, and which is simply a Marks’ decahedronwith s = 0 [see Figs. 4(b) and 4(c) 1. An Ino’s decahedronand any Marks’ decahedronthat can be obtainedfrom it by notching all belong to the same “family.” Two Ino’s decahedrabelong to the same family if for them m - n, which measuresthe “squareness”of the ( 100) face, has the samevalue. Thus in Fig. 12, both the Ino’s decahedronand the Marks’ decahedron belongto family m - n = 2. The Ino’s decahedronhas m = 7, n = 5, s = 0 (andp = l), while the Marks’ decahedronhasm=S,n=5,s=l (andp=2). If we take any Ino’s decahedronand beginnotching it at the twinning planes,we find that, relative either to bulk energiesor cuboctahedralenergies,a sharp minimum exists. In Fig. 13 we show the results for family four, i.e., the set of decahedraarising from notching an Ino’s decahedronwith m---=4. Similar calculations were performed for members of families two, six, and eight. The geometriesof the decahedra1 clusters which we investigatedare given in Table V. We observed that as one moves to larger and larger clusters, the number of the energeticallyoptimal family increasesand the degreeof notching of the optimal member of that family increasesas well. The results of thesecalculations are summarized in Fig. 14, where we display the energiesfor those decahedra1 clusters with energieslower than any other decahedron of similar size, along with the curve of microscopic icosahedralenergieswhich we have seenin so many of the other figures.We concludethat icosahedrabecomeunstable with respect to Marks’ decahedrafor clusters larger than about 2300atoms. In examining Fig. 14, we note that minimum energy decahedratend to havesquare ( 100) facesand that the size of those faces and the depth of the notch embracing them increaseswith increasingcluster sizejust aswe would expect from macroscopicconsiderations.To make the comparison with macroscopicexpectationsmore quantitative, we show ii.0 A.0 Ii.0 Nm Ii.0 Ii.0 ‘LO FIG. 13. The energiesof the decahedra1family four relative to the bulk energyof the samenumber of atoms. The solid lines connect memberswith the same degreeof notching, while the dashed lines connect each cluster with that one producedfrom it by further notching and with its parent cluster from which it was similarly produced.Thes value for eachsolid curve is usedto denote it, while each cluster is marked by its m and n values. J. Chem. Phys., Vol. 94, No. ii,1 June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters 7389 TABLE V. Decahedra1clusters: numbers ofatoms N, number ofatoms on an edgebetweenacapping ( 111) and a ( 100) face m, number ofatoms on the other type of edgeon a ( 100) face n, and the depth of the notch s, for the decahedra1families 2,4,6, and 8, corresponding to decahedrathat may be produced by various degreesof notching from Ino’s decahedrawith m - n = 2,4, 6, and 8, respectively. Family 2 N m 207 409 711 1133 1695 2417 3319 4421 192 389 686 1103 1660 2377 3274 4371 142 324 606 1008 1550 2252 3134 4216 461 838 1355 2032 2889 3946 6 7 8 9 10 11 12 3 4 5 6 7 8 9 10 1 2 3 4 5 6 7 8 1 2 3 4 5 6 5 Family 4 Family 6 Family 8 n s N m n s N m n s N m n s 3 4 5 6 7 8 9 10 3 4 5 6 7 8 9 10 3 4 5 6 7 8 9 10 5 6 7 8 9 10 0 0 0 0 0 0 0 0 1 1 1 1 499 851 1333 1965 2767 3759 4961 484 831 1308 1935 2732 3719 434 766 1228 1840 2622 3594 339 646 1083 1670 2427 3314 7 8 9 10 11 12 13 5 6 7 8 9 10 3 4 5 6 7 8 1 2 3 4 5 6 3 4 5 6 7 8 9 3 4 5 6 7 8 3 4 5 6 7 8 3 4 5 6 7 8 0 0 0 0 0 0 0 1 1 1 1 1 1 2 2 2 2 2 2 3 3 3 3 3 3 971 1513 2215 3097 4179 5481 1493 2190 3067 4144 1428 2110 2972 4034 1308 1965 2802 3839 1745 2547 3549 9 10 11 12 13 14 8 9 10 11 6 7 8 9 4 5 6 7 3 4 5 3 4 5 6 7 8 4 5 6 7 4 5 6 7 4 5 6 7 5 6 7 0 0 0 0 0 0 1 1 1 1 2 2 2 2 3 3 3 3 4 4 4 3397 4569 5911 13 14 15 5 6 7 0 0 0 1 1 1 1 2 2 2 2 2 2 2 2 3 3 3 3 3 3 results for family four in Fig. 15, where in the macroscopic calculations the surfaceplanesare taken to cut through surface atoms. In the upper panel energiesobtained via microscopic, atomistic energyminimizations are shown relative to 27 c.4 . %I0 cuboctahedral energies,and in the lower panel, the corresponding macroscopic results are displayed. For reference, the microscopic icosahedralenergiesare shown in the upper graph. We find excellent agreementbetween the ordering provided by the macroscopic calculations and the microscopic results. In evaluating the quality of the decahedra1 results, it should be borne in mind that the decahedrausedin the macroscopiccalculation are made from unrelaxed,classic decahedraand not macroscopicdecahedrawhosegeometries are consistent with the bulk system whose energy we minimized under decahedra1strain. Using the latter geometries insteadresults in an overall lowering of the macroscopic energies,reducing the overall energy shift betweenthe two panelsof Fig. 15. D. Other clusters I d.0 El0 6.0 I;.0 Ii.0 1Lo Ii.0 NV3 FIG. 14. Those decahedra1sequenceswe have studied which have somewhere an energy lower than any other decahedra1sequenceof corresponding size. Each curve is marked with its degreeof notching s and eachdecahedron’s point is marked with its m and n values. The icosahedral curve, obtained from microscopic energy minimization, is included for comparison. In addition to the abovestructures, other model structures of atomic clusters have been examined in order to check that we haveindeedconsideredmost of the structural motifs relevant to our study of the energeticsof nickel clusters. Thus, e.g.,we havestudied “model B” of Raoult et a&* which is a shift from the truncated octahedronin the opposite direction to that taken by model C, so that it has smaller ( 100) faces.As expected,this is energeticallyquite unfavorable. Furthermore, unlike the Lennard-Jonesiumclusters of Raoulteta1.,8 removing the12vertexatomsontheicosahe- J. Chem. Phys.,subject Vol. 94,toNo. 11,l June or 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution AIP license copyright, see http://jcp.aip.org/jcp/copyright.jsp 7390 C. L. Cleveland and U. Landman: Structure of nickel clusters 6 ‘? 8 9& :’ I$ 2 1. Z “0’00 u”$ A $a I 8 FQ & s* 9 $P z-co 8s yP 2 gc2 9 r P 8.0 10.0 12.0 ,,,I,3 14.0 16.0 18.0 FIG. 15. In the upper graph the minimized microscopicenergiesfor family four are representedrelative to the cuboctahedralenergy. In the lower figure, the correspondingmacroscopicresultsare shown, where we have taken eachsurface’splane to passthrough its atoms. The microscopic results for the icosahedron(squares) are shown in the upper graph as well. dral clusters makes them worse competitors energetically. This type of variation never seemsto be advantageousfor any cluster types and we havenot systematicallyexploredit. We have also created monotwins of someof the singlecrystals, which invariably lowered the cluster’s energy,but to a degreeso small comparedto other energydifferencesasto be uninteresting.For example,the untwinnedHKI cluster with 3679atoms has a total energyof - 15 766.341eV. The correspondingtwinned cluster hasa total energyonly 0.086eV, or 0.28 K lower. There is another largegroup of clustersthat we havenot extensivelystudied simply becausethey are too numerous: those with broken symmetry, i.e., clusters with incomplete shells,or those hybridized from piecesof severalclustersof the more symmetric type which we have considered.Such clusters may be abundant under experimentalconditions. For example,for clusters producedvia a laser-vaporization cluster source, where at low helium pressuresthe principal mechanismof cluster growth is by monomer addition, the oddsthat the number of atomsin a cluster turns out to be one of the valuesfor which an energeticallyoptimum, symmetric shapecan be made are small. Similarly, for clusters which evolve from molten droplets, evaporation of excessatoms will essentiallyceaseprior to any solidification becauseof the large binding energyfor surfaceatoms ( - 3.5 eV). The systematic trends revealedfrom our study of the more symmetric structural forms guide us as to which structures may develop when the number of atoms in a cluster does not correspond to one of the symmetric structures which we have considered.The easiestway to interpolate numbersof atoms is by breaking the symmetry of the clusters. One could usemodel C type faceson part of a cluster’s surfaceand thosefrom a truncated octahedronelsewhere.If somewhat fewer atoms are required, some vertex atoms m ight be removed,or if the cluster is big enough,some( 110) faces applied. In the decahedra,there may be variation among the five tetrahedral units. In general,the surfaceof each single crystal piece will attempt to resemblea piece from the Wulff polyhedron even for clusters that are quite small. Exceptionsare the icosahedra,where we expectthat the best clustersof lower symmetry will have an icosahedral core with a partial outer shell whoseatoms are as compactly arrangedas possible.To avoid energeticallyexpensivesharp atomic stepson a cluster’ssurface,the simplestprocedureis to take a larger cluster in the family in questionand remove whole atomic planesat a time. It is worth pointing out that the truncated octahedra,model C’s, and HKI are all singlecrystal clusters related to eachother by just such operative transformations and, except for the HKI clusters of small sizes,all havesimilar energies.This indicatesthat interpolation between similar high-symmetry configurations may provide someinformation about energiesof clustersof intermediatesizes. In order to illustrate these ideas, we have considered clusters with 201 atoms. Of the high-symmetry structures which we have studied so far, only a truncated octahedron can haveexactly this many atoms.On the other hand, as we seefrom the upper half of Fig. 7, the icosahedrahavea much lower scaledenergythan the truncated octahedrain this size range (N “3 -6). The question naturally arises as to whether some less symmetric icosahedrally based cluster with 201 atoms m ight be lower in energy than the highly symmetric truncated octahedron. A cluster with the desirednumber of atoms may be constructed by addingextra atomsto a 147-atomicosahedronor removing excessatoms from a 309-atom icosahedron.For the purposeof our illustration, we have chosenthe second construction,attempting to removewhole planesofatoms at a time. Accordingly, starting from a 309-atomicosahedron, we pick a vertex and removeall five surfaceplanesthat meet at it, exposingpart of the 147-atomcore. We continue this processby removing planesof atoms on facets adjacentto the area we have already cleared until we have 201 or less atoms left. In fact, following this procedure results in our casein a cluster containing 200 atoms to which one atom is replacedat the edgeof the partial shell which capsthe 147atom icosahedralcore. Direct m inimization of the energyof that cluster yields a total energy E(N) = - 807.076 eV which is slightly below that of the corresponding201-atom truncated octahedron ( - 807.003eV). The resulting cluster is shown,front and back, in Fig. 16,where atoms belonging to the 147-atomicosahedralcore are light gray and those J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters I FIG. 16. Front and back views ofa low symmetry 201-atom cluster with an icosahedralcore of 147atoms (light gray) and a capping partial shell of 54 atoms (dark gray) constructed as detailed in the text. of the capping partial shell are dark gray (the extra 201st atom is the dark gray one nearestthe center of the left image). It is of interest to note that the effect of this extra atom is rather large. The energy of the corresponding200-atom icosahedrally basedcluster is - 803.353eV, while that of the 201-atom truncated octahedron with one of its vertex atoms removed is - 802.589eV, markedly increasing the energetic advantageof the icosahedrally based cluster as comparedwith the 201-atomcase. We would like to note that other construction methods that we haveattempted,including somewhich involved molecular dynamics simulated annealing,resultedin clusters of substantially higher energythan the onewhich we havedemonstrated here. While we have undoubtedly not exhausted all the possible construction schemes,our result indicates that it is possibleto achieve energetically competitive lowsymmetry clusters by starting from judiciously chosenhighsymmetry structures and removing whole atomic planesat a time, as discussedabove.Our generalconclusion is that in attempting to build low-symmetry clusters whosenumber of atoms is incompatible with high-symmetry structures, the energy differencesbetweenthe latter (such as displayed in Fig. 8) provide guidance in choosing the high-symmetry structural motif on which to base the construction of the low-symmetry clusters. 7391 energies and the modified Wulff construction due to Marks” (seeSec.III) 1. Basedon comparisonsbetweenthe results of atomistic energyminimization and the macroscopic formulas which we developed [see Eqs. (4), (5)) and (Bl ) 1, we concludethat theseformulas, in conjunction with accurately calculated, or experimentally measured, cohesive, surface,and strain energies[which in our studieswere obtainedusing the EAM potentials (seeSets. II and III, and the Appendices] allow a rather reliable framework for structural analysis. The macroscopic approach is particularly useful in assessingthe relative energetic merits of various structural motifs (seethe comparisonsbetweenthe results of microscopic and macroscopic calculations in Sec. IV) and thus aids in the analysisof experimentaldata. The evolution with size of the optimal structures of nickel, as well as Lennard-Jonesium(after the results of Ref. 8) clusters is summarized in Fig. 17. As seen from Fig. 17(a), our microscopic, atomistic calculations basedon the EAM many-body interactions predict that the optimal structures of nickel clusters containing less than -2300 atoms belong to the icosahedral sequence.Larger clusters are predicted to optimally assumeMarks’ decahedra1geometries, while for clusters containing more than - 17 000 atoms, single crystal structures and their monotwins are energetically favored. Observe that we predict, on a macroscopic basis, that the evolution of optimal structures from the decahedra1sequenceto the single crystal sequencehappens for much smaller cluster sizesfor nickel that has been predicted* for Lennard-Jonesium,where on the order of 10’ atoms are expectedto be necessary.The transition for ener- SINGLE CRYSTALS AND MONOTWINS MARKS DECAHEDRA V. SUMMARY In this paper we have investigatedusing both a macroscopic approach and atomistic energy minimizations, the sizedependenceof the evolution of structures in metal (nickel) crystallites ranging in size from small clusters containing tens of atoms to rather large ones made of thousands of atoms. In our studies we have used many-body interaction potentials obtainedvia the embeddedatom method (seeSec. II), which include as a dominant contribution to the cohesive energy of the metal the embeddingenergy of the metal ions in the local electron density provided by the other atoms in the system. In addition, we compare our results to those obtained previously, employing simple pair-potential models. One of the aims of our study is to test and assessthe adequacyof macroscopicconceptsbasedon the Wulff construction and variants thereof [i.e., considerationsof elastic ICOSAHEDRA L-J (a) (W FIG. 17. Diagrams, summarizing the evolution of optimal structural motifs, vs the number of atoms in nickel clusters (obtained in this study) and in Lennard-Jonesium (after the results of Ref. 8). The results in (a) correspond to calculations including in the set of possible structures those of Marks’ decahedra.The results in (b) were obtained without the inclusion of Marks’ decahedrain the set of possiblestructures. Solid lines divide structures which belong to different internal structural forms (icosahedra, denoted by IC; Mark’s decahedra; and the single crystals and their monotwins, denoted by TO for truncated octahedra, model C, HKI, or W for other Wulff-type structures). Dashedlines divide structures which have the same internal form, but differ in their surface configuration (these are all single crystals and their monotwins). J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7392 C. L. Cleveland and U. Landman: Structure of nickel clusters getically favored structures between the icosahedral sequenceand the Marks’ decahedra1sequenceis predicted to occur for somewhatlarger clusters in nickel than for LennardJonesium (2300 vs 1600atomsac’ ). In this context, we remind the reader that the HKI, model C, and truncated octahedronare all singlecrystal clusters (seeSec.IV A) and they all serveas approximations, forced by the discrete nature of matter, of the Wulff shape.As clustersbecomelarger and larger, it becomesless and lessuseful to distinguish between clusters that only differ betweenone another by the addition or removal of a singleplaneor row of atoms,and we may just as well speakof the Wulff sequence,or that set of cluster structures that are good approximationsto the Wulff polyhedron. On the other hand, Marks’ decahedra,which are basedon fivefold symmetrical structures, do not belong either to the single crystal structures, or the icosahedral structures. The diagrams for nickel and Lennard-Jonesiumin Fig. 17(b) summarize the structural evolution vs size when Marks’decahedraare not considered.As seen,such calculations predict the emergenceof single crystal structural motifs (i.e., truncated octahedra,model C, and HKI) as optimal clusters for much smaller sizes than when Marks’ decahedraare included, while the cluster size for the icosahedral to single crystal transition in nickel (3600 atoms) is substantially greaterthan that for Lennard-Jonesium(2 100 atoms” ) . For the caseof icosahedralstructures, we find that the effect of relaxation (obtainedby atomistic minimization) of theseclusters from the “ideal” structure given by the macroscopic approach is much larger than is the casefor decahedral and single crystal structures.Theserelaxationsof icosahedral clusters lead to relief of strain by nonuniform relaxationsof atoms in the cluster, resulting in curved (i.e., nonflat) facets. Furthermore, the convexity of the structure propagatesinto the interior of the cluster (seeSec.IV B). While in this study we focus on structural motifs of high symmetry, we also demonstratethat the results which we obtained can guide the construction of energetically competitive low-symmetry clusters. In closing, we reiterate that the results presentedin this paper do not include thermal (and entropic) effects,which can lead to isomerizations between accessiblestructural forms and thus to a distribution of structures for a given size cluster. While a more comprehensiveaccount of the behavior of nickel clusters at finite temperatureswill be given elsewhere, it is instructive, within the context of this study, to comment on the stability of theseclusters at finite temperatures. As seenby molecular dynamics simulations which we have performed, almost all the types of clusters which we have considered here are stable up to the temperature at which their surface atoms begin to diffuse and the clusters can start to isomerize, generally - 1000 K dependingon cluster size. The exceptions are clusters which can convert to another of lower energy via a cooperative,nondiffusive transformation, i.e., the one which connects cuboctahedraand icosahedra.We haveobservedthat on heating,cuboctahedra undergo the multitwinning transformation well before any atomic diffusion occurs, resulting in icosahedra. As the temperature is successivelyincreasedfurther, more outer layers melt and wet a structurally unchanged solid core (i.e., statesof coexistencebetweenliquid, or quasiliquid, and solid phasesoccur). Finally, if enoughenergyis added,the cluster will melt completely. ACKNOWLEDGMENTS This researchis supported by the U.S. Department of Energy (DOE) under Grant No. FGO5-86ER-45234.Portions of the computations were carried out at the Florida StateUniversity Computing Centerthrough a DOE grant of computer time. APPENDIX A: UNIFORM DECAHEDRAL STRAIN In this appendix, we will show how the surface, twinning, and strain energiesneededfor a macroscopic calculation of the energyof oneof Marks’decahedrawere obtained. In Fig. 18, we display an unstrainedunit cell with the tetrahedral unit embeddedin it. The periodic repetition of this cell under the three translation vectors a, b, and c will fill all space.Each of these three vectors points in a (100) direction. In order to changethis unit cell into one containing a tetrahedral unit that will fit into a decahedron,we must changethesethree vectors, so that they satisfy certain constraints. We will choose to proceed so that the (100) surface createdby removing the periodic boundary condition in the c direction correspondsto the ( 100) surfacesthat occur on Ino’s or Marks’decahedra.Then the line AB on the tetrahedron will correspondto the decahedra1axis. Our first constraints come from the requirementthat the lengths of AC, BC, AD, and BD must all be the same.In terms of the transla- D C I [ - - - c,’ . ’ . * . , . * l , ’ . , , , 7 -iT / ’’ . .’ .. . . .. ,. . . ,. , . ’. .. I . . ’’ . . , , , , L , , FIG. 18. An unstrained computational cell for fee crystals. The three vectors a, b, and c are translations under whose repeatedapplication the computational cell periodically fills all space.They are currently pointing in ( 100) directions. We will apply decahedra1strain by changing thesethree vectors to onesconsistent with decahedra1symmetry. J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters vectors, this implies that tion a=b t-41) c-a = cob = 0. t-42) and We concludethat without loss of generality we can choosec to lie in the + z direction and a and b to line in the x-y plane. Further, since we can rotate the resulting setup about the z axis without changing the system’s energy, we can further take one of either a,, or b, zero. If, as is usual, we write the three translation vectors as column vectors and take them as the columns of an overall translation matrix H, I-I = M-w), we could so far chooseto write H as (A3) where (a,/Z,y,...)+ is the supremum of a, fi, y ,... . This expressioncould be simplified by simply assertingthat a lies along the x axis so that av = 0, correspondingto the case where a,>b,,, but the conjugate gradient procedure will treat a, and b,, as the two independentquantities in H, and we cannot be sure that it may not try to make b, larger than a, during minimization and must allow for that possibility. The last constraint is of coursethe requirementthat the dihedral anglebetweenthe ABC and the ABD planesbe 72”. In terms of the translation vectors, this requirementmay be written as [c - (a + b)/2l*[c + (a + b)/2] I[c-- (a+b)/2]jI[c+ 0 (A4) c, = Y a,+ (O,az--bz)+]*+ by+ (a+b)/2]1 =cos(720)* (A5) d(O,a:-b:) + a, I-I== ,/(O,b:-a:) + bY 0 7393 Equations (A4) and (A5) allow us to determinec, in terms of a, and 6,. We find (Ah) (O,b:-aaL:)+]*, where Y = 0.5,/ [ 1 + cos(72”)]/[ 1 - cos(72”)j = 0.6882.... (A7) That we haveonly two degreesof freedomleft is exactly as expected. We can volumetrically expand or contract a decahedronor changethe length of its axis and we will still havea decahedron.Other kinds of changesto the tetrahedral units will either prevent them from joining togetheror create mismatchesbetweentheir edgesand vertices. We can now fill this computational cell with an “fee” lattice of 500 nickel atoms arranged so that there are five conventional unit cells in the a direction, five in the b direction, and five in the c direction, and then minimize the energy by allowing a, and b,, to vary with the other components of H then beingdeterminedas in Eqs. (A4) and (A6). Comparing the resulting energywith the bulk energyof the same number of atoms in a perfect, unstrainedfee crystal gives us the strain energy. The Parrinello-Rahman method” returns the derivative of the potential energy with respectto each of the nine componentsof H disregardingany constraints on them. It is a small detail that we must use the chain rule to determine from thesederivatives the derivatives with respectto a, and b,, with constraints in place. For a, we have (A81 Parrinello-Rahman methods give us the first partial derivative in the sum and Eqs. (A4) and (A6) give us the second. by is of course treated in the sameway. We may remove the periodic boundary condition in the c direction and minimize the energyof the resultingslabby varying atomic positions within a fixed computational cell, obtaining the ( 100) surfaceenergyunder decahedra1strain. Unfortunately, the systemas describedis not well suited to determining the ( 111) surfaceenergiesor twinning energies,sinceit is not easyto createthe appropriateinterfaces.It might appearthat we needto go to a different kind of computational cell for which ( 111) surfaces can be easily made, such as the one in Fig. 3, reexaminethe consequences of the constraints neededfor decahedra1symmetry, and reminimize the bulk energyunder thoseconstraints, but we do not. Any translationally periodic system may have its periodicity representedthrough any three noncollinear periodic translation vectors. Imagine that the computational cell in Fig. 18 correspondsto the one that was produced by the minimization procedur~the changesare very small and do not justify a secondfigure. Instead of describingthe periodicity of this bulk systemby using a, b, and c, we could just as well have used a’ = c - a, b’ = c + b, (A9) c’ = b - a. In terms of Fig. 18,a’points from A to C, b’ points from A to D, and c’points from A to B. This is a right-hand coordinate system analogousto the one in Fig. 3 and is suited for a calculation of the (111) surface energy. Just as there the three vectors define a tetrahedron, here they defineABCD. The new parallelepipedunit cell has a volume that is twice that of the old one,so it is unsurprising that when we periodically replicate the atomic positions in the old one to see which copiesfall in the new one we find that 1000copiesdo. At this point on it is probably better to refer to Fig. 3, where a, b, and c can play the role of a’, b’, and c’. J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp 7394 C. L. Cleveland and U. Landman: Structure of nickel clusters These1000atoms are arrangedas ten ( 111) layers parallel to the sidesof the computational cell, whether we scan through the system along the a’, the b’, or the c’direction. Unfortunately, the stacking sequencefor ( 111) layers in an fee crystal only repeatsevery third layer, which meansthe new systemwill contain seriousstacking faults if periodically repeated.Fortunately this is easily repaired. We simply reduce the three new translation vectors by 10% and only keep the copiesof atoms which fall in this newer, smaller cell. We find that 93 do. Replicating these 729 remaining atoms in this newest unit cell with its periodic translation vectorsproducesexactly the sameatomic coordinatesas replicating the original 500 atoms with the original, relaxed translation vectors: they are equivalent periodic systems. Thus we have constructed a system with decahedra1strain with periodic translation vectors suitable for determining energiesinvolving ( 111) planes. In terms of Fig. 3, the two planesOACand OBCmeet at the line OC with a dihedral angle of 72”. Thus these two planes have the proper orientation for either a twinning plane or a notching ( 111) face. The other two faces of the tetrahedronOAB and ABC have the orientation of capping ( 111) faces.Thus by removing the periodic boundarycondition in the c’direction, we can determinethe surfaceenergy of the capping ( 111) facesby minimizing the energyof the resulting slabwhile holding the computational cell fixed and comparing the resulting energy with that of the bulk slab under decahedralstrain. Similarly, by removing the periodic boundarycondition in the b’direction, we can determinethe surfaceenergyof the notching ( 111) face. Leaving both periodic boundary conditions in place, we can introduce two twinning planesin the original bulk system. Look at the system as a set of nine atomic ( 111) planesparallel to the a’-c’ plane. Thesehave a stacking sequenceabcabcabc, counting away from the al-c’ plane. Let us take the last four of these and rotate them 180”about their normals and put them back so that stackingsequenceis abcabcbacabc..., wherewe have periodically extendedthe sequenceand indicated the twinning planeswith capital letters for clarity. Thesetwo twinning planesare quite close together,but the twinning energy will turn out to be so small that there is little point in being more careful. We can now reminimize the bulk energyin the presenceof these twinning planes, and by comparing the resulting minimum energy with the energyof the bulk system under decahedra1strain we can determinethe twinning energyappropriate to the decahedron. The numerical results for nickel, obtainedby the above method, may be found in Table III. APPENDIX B: ENERGY OF IDEAL DECAHEDRA In this section,we will walk through a calculation using the modified Wulff construction of the energy of a Marks’ decahedrongiven the energy results of the previous appendix. However, insteadof carrying out the construction for an unstrainedsinglecrystal, it is appropriateto carry it out for a crystal under uniform decahedra1strain. Thus the normals to the surfaceswill not quite point in the samedirections as they would were no strain applied, and the faceswill be of different sizes.Becausethe bulk strain energyis so small, this can make a very large differencein our estimate of the size theseclusters must be before single crystal clusters or monotwins of the samesize are energeticallypreferable. We will neglect ( 110) faceting, for reasonsdiscussedin the sectionon macroscopiccalculations.All distancesin this sectionwill be in units of UN,introduced in that samesection. From the computationalcell which gavethe lowest bulk energyfor the given constraints, we know the normals to the ( 100) plane, as well as the ( 111) capping plane and the ( 111) twinning and notching planes.From the surfaceenergieswe found, we know how far eachsurfaceplaneshould be from the origin. Thus if n is the unit vector normal to a surface whose surface energy is y, a point r can be on the planeif it satisfiesn-r = y. If we haveanother plane adjoined to this one at an edge,the equationsof the edgefollow from the requirement that the equationsof both planes must be simultaneouslysatisfied,and a vertex where two edgesmeet is at a point where the two sets of equationsdescribing the edgeshold simultaneously.Thus the determination of all the coordinatesof all the vertices is a straightforward exercise. In the caseof the decahedron,we only have three different vertices to find: a vertex of the ( 100) face; the vertex where the capping facesmeet; and where a twinning plane, notching face, and capping face all meet. Let us take a coordinate system with the origin at the center of the polyhedron and where the z axis runs along what will be the axis of the decahedron(we simply take the twinning energy to be zero for the purposesof performing the modified Wulff construction). We take the x axis to be in the ( 100) direction and thus passingthrough the center of a ( 100) face. We place the y axis so that a right-handed orthogonal coordinate system is created. Looking at the (100) face whose outward normal is in the +x direction, we find that one of its vertices is at (0.1029, 0.0417, 0.0421), the other four being given by changingthe sign on one or both of they and z components. Notice that the height of the (100) face exceedsits width. This is not much affectedby the very small energy differencesbetweenthe capping and notching ( 111) faces, but arisesbecausethe notching planesare more parallel to the ( 100) planeunder decahedra1 strain than the cappingplanes are and thereforecut more deeplyinto it. It is interesting that stretching the crystal out laterally to make it fit the decahedron makes its (100) face narrower rather than wider. The vertex where the (upper) capping faces meet is found at (0, 0, 0.1165). The lower capping faces meet at a point just like the upperonewith the sign on the z coordinate changed. A vertex at the top of the notch, where capping, twinning, and notching ( 111) planesall intersect, is at (0.0801, 0.5821,0.0586). Others of its kind may be generatedby reversing one or both of the signs on they and z coordinates. And of course, for each vertex on the decahedron,there is another that can be found by rotating the decahedronabout the z axis by a 72”angle. With explicit coordinatesfor all the vertices, we can certainly calculate the areasof each type of face with a little planegeometry,as well as the volume of the decahedron.On J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp C. L. Cleveland and U. Landman: Structure of nickel clusters the way we discover that the width and height of the ( 100) face are 0.0833 and 0.0842, respectively,while the height of the notch at its center is 0.1172 and the width of one of the notch’s faces is 0.0282. The width of the capping face at its widest point is 0.1164, slightly smaller that the height of the notch as we should expect by now, and the length of the decahedron’saxis is 0.2330. While the notching plane normal makes an angle with the ( 100) plane normal of 54”as it must, the capping plane normal makes an angle of 54.13” with it. For reference,in the unstrained crystal, both of these angleswould be 54.74”,and in an unrelaxed classic decahedron, the capping plane’s angle with the (100) direction would be 52.62”. Equating the known bulk density under strain and equating it to A’, the number of particles that may be in the decahedron,divided by the decahedron’svolume in units of u,,, cubed, allows us once more to find a connection between uN and N, specifically uN = 13.1607NI” A. The area in units of U; of a single notch face is 0.002 837, so in all, the notch surface area is 0.028 37. The area of a single capping face is 0.008 564, so all the capping faceshave a combined area of 0.085 64. The area of a ( 100) face is 0.007 0 18 for a combined total ( 100) area of 0.035 09 and the area of a twinning plane is 0.017 34 for a total twinning plane surface area of 0.1734.92 Combining the bulk energy for N particles, including strain energy, together with the surface areasand energiesof the ten capping faces, ten notching faces, ten twinning planes, and five ( 100) faces, we finally find the energy of a decahedronof N particles in electron volts. E,(N) = (cB + t$‘)N + 2.493 87N2”, (Bl) where the uniform strain energy per atom of the decahedron <= 1.124426x10-‘eV. ‘Elemental and Molecular Clusters, edited by G. Benedek and M. Pac- chioni (Springer, Berlin, 1988). edited by P. Jena, B. K. Rao, and S. N. Khanna (Plenum, New York, 1987). ‘Atomic and Molecular Clusrers, edited by E. R. Bernstein (Elsevier, Amsterdam, 1990). ‘Mircoclusters, edited by S. Sugano, Y. Nishina, and S. Ohnishi (Springer, Berlin, 1987). ’B. Raoult and J. Farges, Rev. Sci. Instrum. 44,430 ( 1973). bJ. 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Cleveland, and U. Landman, Phys. Rev. Lett. 54, 1679 (1985). 68R N. Bamett, C. L. Cleveland, and U. Landman, Phys. Rev. Lett. 55, 2035 (1985). 69R. N. Barnett, C. L. Cleveland, and U. Landman, Phys. Rev. B 28, 1685 (1983). “E. T. Cheng, R. N. Bamett, and U. Landman, Phys. Rev. B 40, 924 (1989). “E. T. Cheng, R. N. Bamett, and U. Landman, Phys. Rev. B 41, 439 (1990). “U. Landman, W. D. Luedtke, N. A. Burnham, and R. J. Colton, Science 248,454 (1990). “K W. Jacobson,J. K. Norskov, and M. J. Puska, Phys. Rev. B 35,7423 (lb87). 74J. K. Norskov, Phys. Rev. B 26.2875 (1982). xP. Hohenberg and W. Kohn, Phys. Rev. B 136,864 ( 1964). 76Assuming fee structure, no surface relaxation, and only nearest-neighbor bonds. “M. Parrinello and A. Rahman, Phys. Rev. Lett. 45, 1196 (1980). J. Chem. Phys.,subject Vol. 94,toNo. 11,l June or 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution AIP license copyright, see http://jcp.aip.org/jcp/copyright.jsp 7396 C. L. Cleveland and U. Landman: Structure of nickel clusters ‘a Routine ZXCGR in the IMSL Fortran Subroutines for Mathematics and Statistics, edition 9.2 (IMSL, Inc., Houston, 1984). 79Whenever we report properties for extendedsystems whose energieswe have minimized, we use many decimal places.We will want to use such results in macroscopiccalculations and compare the results for different applied strains. Under different strains such properties differ by only a small percentage,so we must carry extra figures. “In general,which crystal face will be exposedwill dependon which periodic boundary condition is removed as well as the choice of computational cell and the atoms within it, as seenmore explicitly in Appendix A. ” W. R. Tyson and W. A. Miller, Surf. Sci. 62,267 ( 1977). 82J.Q. Broughton and G. H. Gilmer, J. Chem. Phys. 84,5741 (1986). a3The octahedralsite is at the geometric canter of the conventional fee unit cell. It is so called becauseits six nearestatomic neighborssit at the vertices of an octahedron. *‘All perfect cuboctahedraare atom centered. *‘These model C clusters are the sameas the onesusedby Raoult et al. (Ref. 8). Unfortunately, their description of model C doesnot produce this set of clusters, but a similar set missing every fourth member of model C. 86HKI standsfor hexakaiicosahedrons,since they have 26 sides. *‘A. Mackay, Acta Crystallogr. 15, 916 (1962). a81nterpolationof cuboctahedral or icosahedral energiesproceedsin the following way: for a given number of atoms, the cubic formula N= 1 + (lln + 15n* + 10n3)/3forthenumberofatomsintheclusteris inverted to obtain a nonintegral shell number. The energiesof the four nearestclusters of that shape, two smaller and two larger, are used to determine the four coefficientsof a cubic equation for energy usedin the region betweenthe two nearestsuch clusters. If we want to extrapolate energies,we simply usethe cubic equation in the closestregion for which one could be obtained.This method can be testedby omitting a data point, eitherinsideourdatarangeorat itsends,and thencheckinghow wellinterpolation or extrapolation can reproduceit. Accuracy is better than 1 meV. The use of a cubic equation for interpolation is deliberate. If the surface planesare taken through surfaceatoms, the shell number of a cuboctahedron or icosahedronis exactly proportional to any ofits linear dimensions, includingits”radius”r. Itisveryreasonabletoexpecttheenergyofacuboctahedron or icosahedronto have terms varying as r ‘, r ‘, and r. a91tremains unclear why taking surface planes betweenatomic layers insteadof through them should do better when estimating the overall energies of the clusters examined in this study, and worse when examining relative energeticordering betweenclusters. If we focus on relative energy differencesbetweenclusters of similar size and for that reasontake our energiesrelative to cuboctahedra,it would appear for the clusters of this study that the best location for a surface plane is just a little outside the plane that passesthrough its surface’satoms. gOThevalue of 1600atoms is given in Ref. 8 for the transition to decahedral structures from icosahedrawith all vertex atoms removed. No transition size is given for full icosahedra. 9’The value of 2 100atoms is given in Ref. 8 for the transition, with decahedra disallowed, to single crystal structures and their monotwins from full icosahedra.For icosahedramissing their vertex atoms, which we havenot consideredhere, the value reported in that referenceis 2400 atoms. 92In the modified Wulff construction, the twinning energy of a twinning plane is divided betweenthe two decahedrathat meet at it. Thus the decahedron is treated as containing ten twinning planes, two per tetrahedral unit. J. Chem. Phys., Vol. 94, No. 11,l June 1991 Downloaded 09 Feb 2004 to 130.207.165.29. Redistribution subject to AIP license or copyright, see http://jcp.aip.org/jcp/copyright.jsp