Origin of Reversible Photoinduced Phase Separation in Hybrid

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Origin of Reversible Photoinduced Phase Separation in Hybrid Perovskites Connor G. Bischak,† Craig L. Hetherington,†,‡ Hao Wu,† Shaul Aloni,§,∥ D. Frank Ogletree,§,∥ David T. Limmer,†,§,⊥ and Naomi S. Ginsberg*,†,‡,§,⊥,# †

Department of Chemistry, University of California, Berkeley, California 94720, United States Molecular Biophysics and Integrative Bioimaging Division, §Materials Science Division, and ∥Molecular Foundry, Lawrence Berkeley National Laboratory, Berkeley, California 94720, United States ⊥ Kavli Energy NanoScience Institute, Berkeley, California 94720, United States # Department of Physics, University of California, Berkeley, California 94720, United States ‡

S Supporting Information *

ABSTRACT: The distinct physical properties of hybrid organic−inorganic materials can lead to unexpected nonequilibrium phenomena that are difficult to characterize due to the broad range of length and time scales involved. For instance, mixed halide hybrid perovskites are promising materials for optoelectronics, yet bulk measurements suggest the halides reversibly phase separate upon photoexcitation. By combining nanoscale imaging and multiscale modeling, we find that the nature of halide demixing in these materials is distinct from macroscopic phase separation. We propose that the localized strain induced by a single photoexcited charge interacting with the soft, ionic lattice is sufficient to promote halide phase separation and nucleate a light-stabilized, low-bandgap, ∼8 nm iodide-rich cluster. The limited extent of this polaron is essential to promote demixing because by contrast bulk strain would simply be relaxed. Photoinduced phase separation is therefore a consequence of the unique electromechanical properties of this hybrid class of materials. Exploiting photoinduced phase separation and other nonequilibrium phenomena in hybrid materials more generally could expand applications in sensing, switching, memory, and energy storage. KEYWORDS: Photoinduced phase transition, hybrid mixed halide perovskite, multiscale simulations, cathodoluminescence imaging, polaron

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color-tuning perovskite-based LEDs and lasers, and for incorporating hybrid perovskites in tandem solar cells.5,17 Light-induced effects, however, restrict the practical use of mixed halide hybrid perovskites.1,2,18,19 Photoluminescence (PL) and X-ray diffraction (XRD) measurements suggest that MAPb(IxBr1−x)3 (0.1 < x < 0.8) undergoes reversible phase separation into iodide-rich and bromide-rich regions when photoexcited.1 Such demixing is detrimental to photovoltaic performance because it leads to charge carrier trapping in the iodide-rich regions. Determining the microscopic mechanism behind phase separation is essential for furthering approaches to mitigate adverse photoinduced effects in devices and should expand the range of their functional applications into areas such as optical memory storage and sensing.20,21 Unfortunately, the microscopic mechanism behind this effect has been elusive because of the multiple length and time scales involved in

hotovoltaic and light-emitting devices typically operate under conditions far from equilibrium. As such, elucidating the response of functional materials to nonequilibrium driving forces is vital to understanding their fundamental physical properties and to determining their suitability for device applications. In particular, photoinduced dynamic processes are of major importance to the performance of hybrid perovskitebased devices.1−4 Hybrid perovskites are low-cost, solution processable materials that are promising for many device applications, including photovoltaics5−10 and light-emitting diodes (LEDs).11 The high device efficiencies have been attributed partly to their long charge carrier migration lengths7,12 and tolerance of structural defects.13,14 The chemical formula of hybrid perovskites is APbX3, where A is an organic cation, typically methylammonium (CH3NH3+, MA) or formamidinium (HC(NH2)2+, FA), and X is either iodide, bromide, chloride, or iodide/bromide or bromide/chloride mixtures. By varying the halide ratios in hybrid perovskites, the bandgap can be tuned across the visible spectrum.1,15,16 Precise control of the bandgap presents promising opportunities for © XXXX American Chemical Society

Received: October 24, 2016 Revised: January 23, 2017

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Nano Letters characterizing the behavior both experimentally and theoretically. We find that these novel photoinduced processes arise because hybrid materials, including inorganic−organic perovskites, have physical properties that differ substantially from both traditional inorganic and organic semiconductors. In particular, hybrid perovskites have elastic moduli that fall in between those of pure inorganic and organic solids,22,23 aiding in their tolerance of structural defects while maintaining longrange order. Hybrid perovskites also have a high static dielectric constant, resulting in strong electron−phonon coupling, and large polarizabilities, resulting in small exciton binding energies.24−26 These macroscopic properties reflect the broad range of time scales characterizing molecular motion in these materials. For example, motions associated with freely rotating organic cations and facile halide migration have been implicated in the large dielectric constant of the material27,28 and in hysteresis upon charging.29,30 Understanding the interplay between and molecular origin of the mechanical and electronic properties of these hybrid materials provides insight into how a hierarchy of bonding energies can result in multifaceted collective phenomena. These insights will lend predictive power to the development of new high-performance functional materials. Here we describe how photoinduced phase separation in mixed halide hybrid perovskites can be mediated through strain-induced phase separation at the locations of polarons photogenerated charge carriers and their accompanying lattice distortions. The heterogeneous nature of this nonequilibrium halide phase separation that we reveal starkly contrasts the macroscopic domains that would form under equilibrium conditions. We combine cathodoluminescence (CL) imaging, a powerful tool for characterizing the nanoscale optical properties of hybrid perovskite films,14,31,32 and multiscale modeling, a set of techniques to bridge molecular and mesoscopic scales, to observe and explain the dynamic process of photoinduced phase separation. After prolonged illumination, small clusters enriched in one halide species are observed to localize near grain boundaries, which is consistent with the effects of polaronic strain in both our molecular and mean-field phenomenological models and the associated phase diagram that we construct. The transient dynamics of cluster formation are characterized by an initial latency and stochastic fluctuations in their formation. The process of cluster formation is captured with the phenomenological theory at intermediate electron− phonon coupling and consists of photogenerated polarons finding, stabilizing, and subsequently becoming trapped in halide composition fluctuations. Additional imaging and calculations validate the proposed requirement that polarons reside specifically within the lower bandgap phase-separated regions to ensure their stability and suggest a path toward new optical memory or detection applications. To observe the nanoscale features of photoinduced phase separation, we fabricated mixed halide hybrid perovskite films for CL imaging. We made a series of films with varying iodide/ bromide ratios (Figure 1a) and ultimately selected MAPb(I0.1Br0.9)3 for further investigation because of its spectrally distinct iodide-rich and bromide-rich regions. When initially photoexciting the MAPb(I0.1Br0.9)3 film, we observe a single emission peak at 540 nm, corresponding to well-mixed halides. Upon continued illumination, a second spectral feature appears at 690 nm (Figure 1b), which corresponds to iodide-rich content and is thus indicative of phase separation (Figure 1c).

Figure 1. Band gap tunability, PL spectra before and after light soaking, CL experimental setup, and CL/SE images at steady state. (A) PL spectra of MAPb(IxBr1−x)3 films with x = 0 (green), x = 0.2 (yellow), x = 0.5 (orange), x = 0.7 (red), and x = 1 (black). (B) PL spectra of MAPb(I0.1Br0.9)3 before (green) and after (red) light soaking for 5 min. (C) Schematic of phase separation and reversibility in MAPb(IxBr1−x)3 where yellow and blue spheres represent I− and Br−, respectively, the red and white pill shapes represent MA, and the lead atoms (not shown) are located in the center of the octahedra. (D) Schematic of CL acquisition and light soaking. (E) SE, CL, and SE/CL overlay after light soaking for 5 min at 100 mW/cm2. The scale bar is 2 μm.

When placed in the dark, the halides remix and the red emission peak disappears on a similar time scale. We illuminate the sample with a 405 nm LED for light soaking inside a scanning electron microscope (SEM) fitted with CL collection capabilities (Figure 1d) and then scan the electron beam to probe photoinduced iodide-rich cluster formation at the nanoscale. The electron beam by itself cannot induce phase separation (see Supporting Information). Figure 1e shows a secondary electron (SE) image, CL image, and a SE/CL overlay collected after 5 min illumination at 100 mW/cm2, demonstrating that the iodide-rich regions localize to grain boundaries in steady state. Although the size of the bright spots in the CL image results from a convolution of iodide cluster size and a B

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Figure 2. Steady-state stabilities and dynamic mechanism for photoinduced phase separation. (A) Photoinduced polaron trapping and associated energy scales associated with phase separation. Color scheme is the same as in Figure 1 with the addition of lead atoms represented by gray circles. (B) Snapshot of the 99% isosurface of excess charge density taken from the molecular dynamics (MD) simulation. (C) Free energies per unit cell for MAPb(IxBr1−x)3 with varying composition in the ground (red) and photoexcited (blue) states, computed from MD simulations (circles) and mean field theory (solid lines). (D) Mean field theory temperature−composition phase diagram in the ground (red) and photoexcited state (blue) with the path through the phase diagram from initial state (star) to demixed state (circle) observed experimentally. Areas beneath the red and blue coexistence curves indicate demixed states. (E) The extent of demixing (i.e., purity of demixed regions found by tracing the blue coexistence curve in D) as a function of electron−phonon coupling and temperature computed from mean field theory in the photoexcited state.

energy calculations and path integral molecular dynamics of a pseudopotential-based model of an excess charge,36 shown in Figure 2b and Video S1, we find that high spatial overlap between the lattice and a single-charge density distribution generates sufficient strain to drive local phase separation at room temperature. By contrast, uniform bulk strain could be relaxed through global volume changes, precluding phase separation. Figure 2c shows the free energy with and without the excess charge as a function of composition, βΔF(x), within a volume characteristic of the charge distribution’s extent. This charge and the lattice deformation field that surrounds it together form a polaron that we predict to have an average size of 8 nm and binding energy Ep = 0.08 eV (Figure 2a). As discussed below, the lower bandgap of the iodide-enriched phase energetically stabilizes and spatially traps the polaron. To relate these findings to the experimental observations, we have distilled them into a simple analytical theory. Modeling the phase separation with a Landau−Ginzburg Hamiltonian with linear coupling between strain and composition fields37 and applying a semiclassical description of the excess charge,38 we parametrize and evaluate a theory for photoinduced phase separation (see Supporting Information). As shown in Figure 2c, this model is capable of describing the underlying free energy surfaces predicted from molecular dynamics simulations. Within a mean-field approximation, we determine the full temperature−composition phase diagram for both ground- and photoexcited states (Figure 2d). We confirm experimentally

large carrier migration length, individual clusters are still visible within each grain. Molecular simulations suggest that photoinduced phase separation arises when charged excitations generate sufficient lattice strain to destabilize the solid solution, favoring demixing. Using a classical point charge model27,33 we find that mixed I/ Br perovskites undergo demixing transitions as a function of temperature with a critical temperature of 190 K (Figure S1), consistent with the well-mixed films made experimentally at room temperature. Analysis of Br/Cl perovskites find a similarly low critical solution temperature of 140 K. For I/Cl perovskites, however, the critical solution temperature (1800 K) is found to be well above room temperature, consistent with experimental observations that such mixtures are unstable.34 While direct experimental evidence of temperature-induced demixing is hampered experimentally by low ion conductivities, these predictions are in reasonable agreement with other theoretical estimates.35 By analyzing the relative energetic contributions to the heat of mixing, we find that elastic effects from lattice mismatch are much larger than specific chemical interactions, which leads to a demixing transition that depends strongly on strain (Figure S2). As illustrated in Figure 2a, upon light absorption weakly bound electron−hole pairs, with binding energies Ex ≈ 0.03 eV,25 rapidly dissociate, easily creating free charges. These charges deform the surrounding lattice through electron−phonon coupling, which is expected to be significant given the ionic nature of the material. Using free C

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Figure 3. Formation and evolution of iodide-rich clusters. (A) PL spectra after different light soaking times at 50 mW/cm2. (B) Normalized PL intensity versus time (red) and normalized simulated cluster size versus time (black) with standard error values (blue). (C) Duty cycle for CL image series. CL image series with (D) 10 and (E) 30 s of light soaking between each CL image. The scale bars are 2 μm. (F) CL image series of a single domain with 10 s of light soaking between each CL image. The color scale indicates iodide-rich CL intensity, which convolves carrier migration length with feature size. The scale bar is 200 nm. (G) A series of snapshots from a cluster formation simulation of a 100 nm region with iodide-rich regions in yellow and bromide-rich regions in blue.

that varying the film temperature over a range of 50 K is insufficient to induce demixing, but does increase the demixing rate by increasing halide mobility (Figure S3). We also map the degree of demixing as a function of temperature and electron− phonon coupling, α, in the photoexcited state (Figure 2e). Previous PL studies confirm that the stable iodide-rich cluster phase is at approximately MAPb(I0.8Br0.2)3,1 which agrees with our predicted phase diagram and PL measurements. To confirm the validity of our thermodynamic model for photoinduced phase separation, we demonstrate experimentally both the ability of polarons to stabilize iodide-rich clusters and that large electron−phonon coupling is required to cause halide phase separation. For the latter, we show both experimentally and with the phenomenological model that reducing the electron−phonon coupling in the system by replacing MA+ with less polar Cs+ reduces the tendency to phase separate (Figure S4), consistent with the phase diagram in Figure 2e. To demonstrate that the local presence of a polaron stabilizes iodide-rich clusters in the hybrid perovskites, specifically in MAPb(I0.1Br0.9)3, we first generate iodide-rich clusters with a 405 nm excitation source. We then illuminate the film with 635 nm light, generating charge carriers only in pre-existing iodiderich clusters. The 635 nm light stabilizes these clusters but does not generate new ones (Figure S5 and S6), confirming that the continued presence of photogenerated carriers is required for cluster stability. Having established a model for the thermodynamics of halide phase separation, we focus on the dynamics of the formation and evolution of iodide-rich clusters, which further constrains

our model. To monitor the formation of iodide-rich clusters in bulk, we collected a series of PL emission spectra under constant light-soaking at 50 mW/cm2 (Figure 3a) and plot the integrated intensity of iodide-rich emission as a function of time as it grows to a finite value proportional to the illumination intensity (Figure 3b, red). To resolve the emergence and evolution of iodide-rich clusters, we alternate between light soaking and CL imaging (Figure 3c). Figure 3d and 3e (Videos S2 and S3) show overlaid CL and SE image sequences with 10 and 30 s intervals of light soaking, respectively. After some latency, iodide-rich clusters begin to emerge and grow primarily in number. They quickly reach a maximum size, suggesting that cluster nucleation rather than growth limits the rate of phase separation. We also find using CL microscopy that the rate of cluster formation increases with illumination intensity (Figure S7, Video S4 and S5). To gain insight into the microscopic dynamics leading to cluster formation, we examine the photoinduced progression within single domains with both CL (Figure 3f and Figure S8) and simulations (Figure 3g). Simulations of the clustering process are performed by solving our phenomenological theory numerically on a lattice (Video S6). We observe similar dynamics in both experiment and simulation, such as the formation of both transient and stabilized clusters. An ensemble average of independent simulated clustering events yields a curve that characterizes the clustering process (Figure 3b, black), which agrees with the experimentally observed PL intensity growth in time (red) and its illumination power dependence (Figures S9 and S10). We find that the 5−10 s D

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Nano Letters initial lag time corresponds to a characteristic time scale for a polaron to become trapped in a spontaneous fluctuation of higher iodide concentration, which is limited by the ions’ diffusivity rather than the polaron’s diffusivity. During the following 10−90 s, a trapped polaron stabilizes an iodide-rich cluster and accumulates more iodide, and more clusters form within the film. Subsequently, cluster growth stops, as cluster size is limited to the deformation region of the polaron, and cluster number is limited by the total number of photogenerated charges. Although the time scales for these dynamics are considerably longer than the lifetime of a single polaron, continuous illumination enables newly generated polarons to replace recombining ones.39 Newly generated polarons continue to stabilize clusters due to the much larger mobility of the excess charge relative to the iodide, resulting in a characteristic localization time for the polaron that is much smaller than the characteristic time for a cluster to relax. By measuring the PL of the iodide-rich clusters at different intensities (Figure S9), which correspond to different steadystate polaron densities, we estimate the size of the clusters to be 8−10 nm in diameter (Figure S11), which is in agreement with our theoretical prediction. During later times, the clusters migrate to grain boundaries to relieve strain (Figure 1e). We rule out that the enhanced CL emission near the grain boundaries comes from outcoupling effects due to the film topography because previous CL studies on lead halide perovskite thin films did not observe such effects.14 The confluence of multiple physical processes that couple disparate length and time scales gives rise to the decidedly peculiar photoinduced phase separated state. For example, because the strain field applied by each polaron is limited in spatial extent, the photoexcited steady state of the system consists of a series of isolated nanoscale clusters rather than the expected large, single iodide-rich domain of a low-temperature equilibrium state in the dark (Figure 3d). Further, because polarons preferentially localize in iodide-rich regions, the composition of the remaining material is neither predicted nor observed to deviate from its preillumination halide mixture ratio (Figure 1b), as though it were still in the dark. Last, because the iodide-rich clusters are limited to nanoscale sizes, their coarsening dynamics do not abide by familiar, universal scaling laws. We have established that the unusual interplay between the electronic and mechanical properties in hybrid perovskite materials results in local, excited-state phase behavior that differs substantially from the ground state due to polaronic strain. Photoinduced phase separation is a general phenomenon in hybrid perovskites that has been observed in both polycrystalline films and single crystals and with different organic cations.1 We further find both experimentally and theoretically that it occurs with other halide mixtures, such as in MAPb(BrxCl1−x)3 thin films (Figures S12 and S13). Our study shows that the unique combination of mobile halides, substantial electron−phonon coupling, and long-lived charge carriers is required for photoinduced phase separation. Decreasing defect concentrations to reduce vacancy-mediated halide migration or lowering electron−phonon coupling could significantly reduce photoinduced effects and improve compatibility with device applications at ambient conditions. For instance, it has been shown that Cs-doped FAPb(IxBr1−x)3 films are much more phase-stable under illumination than undoped films, likely due to a decrease in the electron−phonon coupling.5

Taking advantage of the generality of photoinduced phase separation could provide new opportunities for expanding the functional applications of mixed halide hybrid perovskites. Because of their sensitive spectral photoresponse, these materials could be used in sensing, switching, or memory applications. In fact, we have demonstrated a first step toward memory storage by transiently patterning the local halide composition (Figure S6). Because we show that a single excited charge is responsible for locally changing the structure and composition of the material, truly nanoscale memory elements could even be realized via single charge injection. More broadly, the commonality in the electronic and mechanical properties among a rapidly growing library of new hybrid materials suggests that nonequilibrium processes in these materials are similar and could be exploited for new device applications. The coordinated multiscale methodologies that we have developed could also uncover the nature of other nonequilibrium phenomena in other dynamic materials, for example in energy storage40 or electronically correlated materials,41for which their complexity necessitates a multifaceted approach, capable of bridging molecular and mesoscopic length scales.

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ASSOCIATED CONTENT

* Supporting Information S

Materials and methods, an explanation for why the electron beam does not cause demixing, Figures S1−S13, Videos S1−S6, Tables S1−S2, and supporting references. This materials is available free of charge via the Internet at The Supporting Information is available free of charge on the ACS Publications website at DOI: 10.1021/acs.nanolett.6b04453. Materials and methods, an explanation for why the electron beam does not cause demixing, Figures S1−S13, Tables S1 and S2, and supporting references (PDF) Molecular dynamics simulation of a 99% isosurface of excess charge density on the perovskite lattice (MPG) Sequence of CL images of phase separation with 10 s light soaking intervals at 50 mW/cm2 (AVI) Sequence of CL images of phase separation with 30 s light soaking intervals at 50 mW/cm2 (AVI) Sequence of CL images of phase separation with 10 s light soaking intervals at 1100 mW/cm2 (AVI) Sequence of CL images of phase separation with 30 s light soaking intervals at 1100 mW/cm2 (AVI) Cluster formation simulation (MPG)

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AUTHOR INFORMATION

Corresponding Author

*E-mail: [email protected]. ORCID

Naomi S. Ginsberg: 0000-0002-5660-3586 Present Address

(H.W.) Department of Chemistry and Chemical Biology, Harvard University, Cambridge, MA 02138, United States. Author Contributions

C.G.B. and N.S.G. designed the CL and PL experiments. C.G.B fabricated the perovskite films, acquired the CL and PL data, and performed all experimental data analysis. D.T.L. designed the models and performed all simulations. C.L.H., H.W., S.A., and D.F.O. produced the CL acquisition software and provided instrument support and helpful discussion. C.G.B., D.T.L., and E

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(18) Beal, R. E.; Slotcavage, D. J.; Leijtens, T.; Bowring, A. R.; Belisle, R. A.; Nguyen, W. H.; Burkhard, G. F.; Hoke, E. T.; McGehee, M. D. J. Phys. Chem. Lett. 2016, 7 (5), 746−751. (19) Jaffe, A.; Lin, Y.; Beavers, C. M.; Voss, J.; Mao, W. L.; Karunadasa, H. I. ACS Cent. Sci. 2016, 2, 201−209. (20) Lin, Q.; Armin, A.; Lyons, D. M.; Burn, P. L.; Meredith, P. Adv. Mater. 2015, 27 (12), 2060−2064. (21) Sutherland, B. R.; Johnston, A. K.; Ip, A. H.; Xu, J.; Adinolfi, V.; Kanjanaboos, P.; Sargent, E. H. ACS Photonics 2015, 2 (8), 1117− 1123. (22) Rakita, Y.; Cohen, S. R.; Kedem, N. K.; Hodes, G.; Cahen, D. MRS Commun. 2015, 5 (4), 623−629. (23) Sun, S.; Fang, Y.; Kieslich, G.; White, T. J.; Cheetham, A. K. J. Mater. Chem. A 2015, 3 (36), 18450−18455. (24) Onoda-Yamamuro, N.; Matsuo, T.; Suga, H. J. Phys. Chem. Solids 1992, 53 (7), 935−939. (25) Johnston, M. B.; Herz, L. M. Acc. Chem. Res. 2016, 49 (1), 146− 154. (26) Galkowski, K.; Mitioglu, A.; Miyata, A.; Plochocka, P.; Portugall, O.; Eperon, G. E.; Wang, J. T.-W.; Stergiopoulos, T.; Stranks, S. D.; Snaith, H. J.; Nicholas, R. J. Energy Environ. Sci. 2016, 9 (3), 962−970. (27) Mattoni, A.; Filippetti, A.; Saba, M. I.; Delugas, P. J. Phys. Chem. C 2015, 119 (30), 17421−17428. (28) Leguy, A. M. A.; Frost, J. M.; McMahon, A. P.; Sakai, V. G.; Kockelmann, W.; Law, C.; Li, X.; Foglia, F.; Walsh, A.; O’Regan, B. C.; Nelson, J.; Cabral, J. T.; Barnes, P. R. F. Nat. Commun. 2015, 6, 7124. (29) Unger, E. L.; Hoke, E. T.; Bailie, C. D.; Nguyen, W. H.; Bowring, A. R.; Heumüller, T.; Christoforo, M. G.; McGehee, M. D. Energy Environ. Sci. 2014, 7 (11), 3690−3698. (30) Snaith, H. J.; Abate, A.; Ball, J. M.; Eperon, G. E.; Leijtens, T.; Noel, N. K.; Stranks, S. D.; Wang, J. T.-W.; Wojciechowski, K.; Zhang, W. J. Phys. Chem. Lett. 2014, 5 (9), 1511−1515. (31) Dou, L.; Wong, A. B.; Yu, Y.; Lai, M.; Kornienko, N.; Eaton, S. W.; Fu, A.; Bischak, C. G.; Ma, J.; Ding, T.; Ginsberg, N. S.; Wang, L.W.; Alivisatos, A. P.; Yang, P. Science 2015, 349 (6255), 1518−1521. (32) Xiao, C.; Li, Z.; Guthrey, H.; Moseley, J.; Yang, Y.; Wozny, S.; Moutinho, H.; To, B.; Berry, J. J.; Gorman, B.; Yan, Y.; Zhu, K.; AlJassim, M. J. Phys. Chem. C 2015, 119 (48), 26904−26911. (33) Lewis, G. V.; Catlow, C. R. A. J. Phys. C: Solid State Phys. 1985, 18 (6), 1149. (34) Yang, B.; Keum, J.; Ovchinnikova, O. S.; Belianinov, A.; Chen, S.; Du, M.-H.; Ivanov, I. N.; Rouleau, C. M.; Geohegan, D. B.; Xiao, K. J. Am. Chem. Soc. 2016, 138 (15), 5028−5035. (35) Brivio, F.; Caetano, C.; Walsh, A. J. Phys. Chem. Lett. 2016, 7 (6), 1083−1087. (36) Kuharski, R. A.; Bader, J. S.; Chandler, D.; Sprik, M.; Klein, M. L.; Impey, R. W. J. Chem. Phys. 1988, 89 (5), 3248. (37) Cahn, J. W. Acta Metall. 1962, 10 (3), 179−183. (38) Kalosakas, G.; Aubry, S.; Tsironis, G. P. Phys. Rev. B: Condens. Matter Mater. Phys. 1998, 58 (6), 3094−3104. (39) Yang, X.; Yan, X.; Wang, W.; Zhu, X.; Li, H.; Ma, W.; Sheng, C. Org. Electron. 2016, 34, 79−83. (40) Li, Y.; El Gabaly, F.; Ferguson, T. R.; Smith, R. B.; Bartelt, N. C.; Sugar, J. D.; Fenton, K. R.; Cogswell, D. A.; Kilcoyne, A. L. D.; Tyliszczak, T.; Bazant, M. Z.; Chueh, W. C. Nat. Mater. 2014, 13 (12), 1149−1156. (41) Schmitt, F.; Kirchmann, P. S.; Bovensiepen, U.; Moore, R. G.; Rettig, L.; Krenz, M.; Chu, J.-H.; Ru, N.; Perfetti, L.; Lu, D. H. Science 2008, 321 (5896), 1649−1652.

N.S.G. wrote the manuscript and all authors revised and approved the manuscript. Notes

The authors declare no competing financial interest.

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ACKNOWLEDGMENTS CL characterization was supported by a David and Lucile Packard Fellowship for Science and Engineering to N.S.G. CL and PL at the Lawrence Berkeley Lab Molecular Foundry were performed as part of the Molecular Foundry user program, supported by the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. C.G.B. acknowledges an NSF Graduate Research Fellowship (DGE 1106400) and N.S.G. acknowledges an Alfred P. Sloan Research Fellowship and a Camille Dreyfus Teacher-Scholar Award. We thank Z. Luo for assistance with film deposition. D.T.L was supported initially through the Princeton Center of Theoretical Science.

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DOI: 10.1021/acs.nanolett.6b04453 Nano Lett. XXXX, XXX, XXX−XXX