Supplemental Material Controlled Self-Assembly of Periodic and Aperiodic Cluster Crystals

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Supplemental Material Controlled Self-Assembly of Periodic and Aperiodic Cluster Crystals Kobi Barkan, 1 Michael Engel, 2 and Ron Lifshitz 1, 3 1 Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel 2 Department of Chemical Engineering, University of Michigan, Ann Arbor, MI 48109, USA 3 Condensed Matter Physics 149-33, California Institute of Technology, Pasadena, CA 91125, USA (Dated: April 20, 2014) Computational and theoretical methods, potential parameters, and additional figures supplementing the discussion in the main text. DETERMINATION OF POTENTIAL PARAMETERS The LP-Gaussian potential family is given in Fourier space by (Eq. (1) in the main text) Ũ(k) = e ( k2 2σ 2 D0 + D 2 k 2 + D 4 k 4 + D 6 k 6 + D 8 k 8). (S1) The potential is self-dual in the sense that it has the same analytical form in real space (Eq. (2) in the main text), U(r) = 1 2π 0 Ũ(k)J 0 (kr)k dk = e 1 2 σ2 r 2 ( C 0 + C 2 r 2 + C 4 r 4 + C 6 r 6 + C 8 r 8), where J 0 is the zeroth-order Bessel function and with C 2i = 1 2π 4 ( 1) i 2 j i (j i)! j=i (S2) ( ) 2 j! D 2jσ 2(i+j+1). (S3) i! Given the desired values of the wavenumber ratio k n, the Gaussian width σ, and the depth of the pair potential in reciprocal space Ũmin, we run a Mathematica script to determine the coefficients {D 2j } 4 j=0 by simultaneously solving the following five equations: U(0) = C 0 = 1 2π 4 2 j j!d 2j σ 2(j+1) = 1, j=0 Ũ(1) = Ũ(k n) = Ũmin, dũ = dũ = 0. dk dk k=1 k=kn (S4) A substitution into the expressions for the coefficients {C 2i } 4 i=0 in Eq. (S3) and then into Eq. (S2) for the potential in real space completes the calculation. The values of σ are chosen so that the potentials are purely repulsive in real space, even though this is not required. All of the potential parameters used in this study are listed in Table S1. We note that the condition that the Fouriertransformed potential have two minima of exactly the same depth, positioned at two wave vectors whose ratio is exactly k n, as given by Eq. (S4), is employed here to ensure the success of the self assembly in every single run. It is beyond our current scope to test the extent at which one can stray from these exact requirements and still obtain the desired structures. Nevertheless, we know from BDL [2] that it is possible to do so, with some structures being more robust against such changes than others. The choice of Ũmin, here taken to be -0.08, is arbitrary. The only requirement is that it should be negative. COMPUTATIONAL METHODS The main part of the simulations is performed with the HOOMD molecular dynamics (MD) simulation package [1] with either N = 1024 particles or N = 16384 particles in the NV T ensemble at mean densities 0.1 c 2.0. The interaction potential is cut off at r = 10, shifted and smoothed close to the cut-off to avoid truncation errors and discontinuities. Due to the relatively high density and the frequent particle overlap at our high densities, up to 500-1000 neighbors can be contained within the cut-off range, which is over an order of magnitude more than in typical (non-cluster) crystals with standard potentials (e.g. Lennard-Jones), slowing down the simulation. Total simulation times are 10 7 or 10 8 MD simulation steps, which means that typical simulation run times on a single GPU core are between a few hours and a few days. We verify the findings of all cluster crystals in several ways: (i) using N P T ensemble simulations; and (ii) repeating some of the simulations using a second MD package independent of HOOMD. Overall, we ran five simulations at each of the mean densities c {0.1, 0.2,..., 2.0} and for each of the five potentials a total of 500 simulations. Diffraction patterns were obtained using a Fast Fourier Transform of delta scatterers positioned at the centers of the particles. All observables (diffraction patterns, radial distribution functions, cluster sizes) were time averaged over 100 snapshots to minimize noise. The meanfield densities shown in Fig. 2 of the main text and in Fig. S6 below were obtained numerically by minimizing the mean-field free-energy, as described by BDL [2]. In order to obtain high resolution images more efficiently we

2 Potential parameter Stripes 4-fold 6-fold 10-fold 12-fold σ 0.784889 0.643467 0.714178 0.685894 0.770746 C 0 1 1 1 1 1 C 2-1.11146-0.72765-0.875660-0.794085-1.09456 C 4 0.466920 0.193641 0.305132 0.252769 0.439744 C 6-0.0552546-0.0136926-0.0283173-0.0211568-0.0492739 C 8 0.00217197 0.000324970 0.000889644 0.000601617 0.00183183 D 0 17.1419 22.8844 21.6032 23.0221 17.4524 D 2-43.1030-68.9652-57.8779-63.9132-44.5109 D 4 35.4539 74.5064 52.9082 61.6601 37.5132 D 6-10.7407-34.4021-19.2394-24.3493-11.8896 D 8 1.06780 5.70885 2.3966 3.34872 1.24928 TABLE S1. Potential parameters used in this study. also employed the method of Jiang and Zhang [3]. For performing the clustering operation, we first tested a naive clustering approach using a simple cut-off to join neighboring particles. However, this did not yield reliable results because in many cases clusters were either only partially detected or nearby clusters grouped together. Using the (still simple) DBSCAN algorithm [4] solved these problems. As discussed in the text, we always use a cluster size parameter MinPts = 8 and a variable cluster distance parameter that was adjusted to yield optimal results. ADDITIONAL SIMULATION SNAPSHOTS On the following pages, we include additional (mostly larger) simulation snapshots of the observed cluster crystals and their diffraction patterns. Note that all diffraction patterns show an inner set of sharp peaks, followed by a ring with little scattering, followed by a second ring of sharp peaks together with a broad ring of diffuse scattering. The diffuse scattering is caused by the particle disorder within the clusters. [1] J. A. Anderson, C. D. Lorenz, and A. Travesset, J. Comp. Phys. 227, 5342 (2008). HOOMD-blue web page: http: //codeblue.umich.edu/hoomd-blue. [2] K. Barkan, H. Diamant, and R. Lifshitz, Phys. Rev. B 83, 172201 (2011). [3] K. Jiang and P. Zhang, J. Comput. Phys. 256, 428 (2014). [4] M. Ester, H.-P. Kriegel, J. Sander, and X. Xu, in Proceedings of the Second International Conference on Knowledge Discovery and Data Mining, edited by E. Simoudis, J. Han, and U. M. Fayyad (1996) pp. 226 231.

3 FIG. S1. Lamellar pattern formed from particles aligning into parallel stripes. Particles are still highly mobile within the stripes. Simulation parameters: N = 16384, c = 0.9, T = 0.03. FIG. S2. Periodic 4-fold cluster crystal forming a square lattice. Simulation parameters: N = 16384, c = 0.9, T = 0.03.

4 FIG. S3. Periodic 6-fold cluster crystal forming a triangular lattice. Simulation parameters: N = 16384, c = 0.7, T = 0.03. Note how a few single-particle clusters seem to be caught at the centers of large-cluster triangles. At higher densities, these proliferate to form a superlattice structure, as can be seen in Fig. S6. FIG. S4. Quasiperiodic 10-fold cluster crystal forming a pentagon Penrose (P1) tiling with some phason disorder. Simulation parameters: N = 16384, c = 0.6, T = 0.03. Clusters are identified and colored according to their size from small (blue, size 10) to large (red, size 30). Second-nearest-neighbor clusters of size 19 are connected by bonds to obtain the tiling.

5 FIG. S5. Quasiperiodic 12-fold cluster crystal forming a square-triangle-rhombus tiling with some phason disorder. Simulation parameters: N = 16384, c = 0.8, T = 0.03. Clusters are identified and colored according to their size from small (blue, size 10) to large (red, size 30). Second-nearest-neighbor clusters of size 10 are connected by bonds.

6 FIG. S6. Confirmation of superstructures of secondary lamellae and secondary clusters, as predicted by the mean-field results. At sufficiently high density and temperature (close to melting) secondary lower-density lamellae and clusters appear in the striped phase (left column) and the hexagonal phase (right column), respectively. Top row: Simulation snapshots at density c = 2.0, the highest density studied in this work, and at temperatures close to melting. To decrease noise, these snapshots are rapidly cooled to T = 0.1 (2-fold, left) and T = 0.06 (6-fold, right). Bottom row: The secondary superstructures as observed in the mean-field calculations. The mean field results shown here are identical to the insets in Fig. 2 of the main text.

7 FIG. S7. An incomplete transformation of the 12-fold quasicrystal into a compressed hexagonal phase observed at low temperature. Simulation parameters: N = 16384, c = 1.9, T = 10 3. Clusters are identified and colored according to their size from small (blue, size 10) to large (red, size 30). Second-nearest-neighbor clusters of size 20 are connected by bonds. The tiling consists of alternating rows of two types of compressed hexagonal tiles, each consisting of a pair of triangles connected by either one rectangle or two. FIG. S8. A σ-phase approximant of the 12-fold quasicrystal observed at low temperature. Simulation parameters: N = 16384, c = 1.6, T = 10 3. Clusters are identified and colored according to their size from small (blue, size 10) to large (red, size 30). Second-nearest-neighbor clusters of size 10 are connected by black bonds, revealing square, triangular, and rhombic tiles that are the same building blocks for the dodecagonal quasicrystal shown in Fig. S5. Larger clusters (of size 45), located at the centers of 12-fold rings, are connected by thick gray bonds, revealing the σ-phase approximant, where each vertex is surrounded by a pair of triangles followed by a square, another triangle, and another square, commonly denoted as 32.4.3.4. The unit cell of the approximant (four large triangles and two large squares) is highlighted green. Note the pseudo-12-fold diffraction diagram, and compare with the one in Fig. S5.