Introduction

Although ILM formation for driven nonlinear lattices is well established1,2, temperature activated ILMs3 observed in the α-U4 and NaI5 atomic lattices in thermal equilibrium are not well understood. First, the intensities of ILM signatures (comparable to the normal phonons4,5) are higher than expected for a dilute concentration. Second, ILM signatures do not follow the expected exponential thermal activation law3, but rather appear abruptly at a high temperature followed by modest growth with increasing temperature5,6. Third, associated with ILM formation are softened normal phonons positioned at frequencies just below the ILM features4,5; coherent modifications to extended modes are not expected for a random distribution of ILMs. Finally, the observed single value of the ILM frequency4,5 is unexpected since classical simulations predict a distribution of frequencies7,8.

Alternatively, Burlakov9 demonstrated theoretically the formation of dynamical patterns for optically driven anharmonic lattices that resemble a train of equal ILMs10. Such dynamical patterns allow for indirect experimental evidence of ILMs based on dynamical breaking of the lattice translational symmetry9,10. Similar patterns with ILM constituents were also shown theoretically for the forced-damped Fermi-Pasta-Ulam lattice11 and an ILM pattern was predicted for the α-U crystal lattice under ion bombardment12. For continuous systems driven far from equilibrium, dynamical patterns are often observed13 and analogous trains of solitons date back to 1895 with the cnoidal wave trains of Korteweg and De Vries14. Unlike with these driven systems, however, here we report ILMs forming a dynamical pattern within the equilibrium thermal vibrations of a crystal. These results could not have been anticipated from previous work on pattern formation in driven systems since such patterns disappear in the absence of the non-equilibrium driving force.

Results

Figure 1 shows lattice excitation spectra collected near the NaI spectral gap centered near 10 meV for curved sections of Q-E space (momentum-energy). Figure 1a shows data collected for Q directed near the <111> axis for the energy range of interest (9 to 11 meV) at both low QL and high QH in similar reciprocal space regions. On increasing temperature from 496 K to 614 K a sharp peak develops in the gap near 10.5 meV for both QL and QH, consistent with the previously reported ILM5. On further increasing temperature to 636 K, however, the ILM peak in the gap disappears. The disappearance is particularly clear at QL, where the multiphonon background is smaller15, but it is also reproduced in the QH section. Next, with another small temperature increase to 659 K the ILM peak reappears in the gap for both QL and QH sections. There is also a new feature appearing around 5.8 meV in the acoustic part of the spectrum below the gap, but only in the QL section. Figure 1b shows data collected in a section with Q directed near the <011> axis. These results appear complimentary to those in Fig. 1a. First, from 496 K to 614 K, as the ILM peak forms in Fig. 1a, no feature appears in the gap in Fig. 1b. But then on heating from 614 K to 636 K, as the ILM peak in Fig. 1a disappears, a peak appears in the gap at 10 meV labeled ILM*. Finally, at 659 K as the ILM peak is recovered in Fig. 1a, ILM* disappears in Fig. 1b. Figure 1c shows data in a section along the <100> axis. This appears to be a mixture of what appears in Fig. 1a and 1b; on heating from 496 K to 614 K a weak ILM signature develops in the gap, followed by a weak ILM* signature at 636 K and very little in the gap at 659 K. Taken together the results of Fig. 1 indicate that the ILMs appearing along <111> at 614 K collectively reorient into <011> to form the ILM* feature at 636 K and then move back to <111> at 659 K.

Figure 1
figure 1

Lattice excitation spectra derived from a curved section of momentum-energy (Q-E) space as a function of temperature.

The Q space sampled in these spectra changes with E . The curved dashed-line section in the pictures above the data sets shows where the detector banks are projected in the NaI reciprocal lattice for energies between 9 meV and 11 meV (where the ILM feature forms5). The grey outlined boxes with Q labels indicate the volume of Q space integrated within the plane. Out-of-plane integration for these sections was kept fully open and accounts for about ±0.6 reduced lattice units (r. l. u.) in the out of plane [0,k,-k] direction for energies between 9 and 11 meV. (a) Includes low QL and high QH sections near the <111> axis just inside the zone. The integration boxes in this case were rotated by 57° with QL 0.2 by 0.9 r. l. u. and QH 1 by 0.5 r. l. u. (b) An intermediate QM region located near the <011> axis; integrating K = [-2,-1.7] and H = [-0.5,1]. (c) A low Q region positioned mainly along <100>; integrating K = [-0.25,0.25] and H = [0,2].

Figure 2 shows Q-E slices taken at 567 K and 636 K constructed from multiple scans using MSlice16, see methods for details. Figure 2a shows that ILM*, appearing as a constant energy 10 meV streak in the gap, is dispersionless in [H,-3,-3]. Similarly, Figure 2b shows that ILM* is also dispersionless in [-2,K,K]. The dispersionless character is consistent with localization and is similar to that observed for the [111] ILM observed previously5. Figure 2c shows that along with the appearance of ILM* comes a fragmentation of the TO mode near the X high symmetry point into at least three features, labeled α, β and γ. This fragmentation can also be seen to extend to other parts of reciprocal space; compare Fig. 2a with Fig. 2d and Fig. 2b with Fig. 2e. Fragmentation is also evident at 636 K in Figs. 1a and 1b. No significant changes occur in the longitudinal acoustic (LA) or transverse acoustic (TA) phonon dispersion curves along [-2,K,K], as can be seen by comparing the curves below 9 meV in Figs. 2b and 2e. Figure 3 shows constant Q cuts taken at 636 K near six X high-symmetry points. For the (0\(\overline{3}\)\(\overline{3}\)) X point (Fig. 3a) the spectrum has strong α and γ peaks. However, for the (0\(\overline{1}\)\(\overline{1}\)) X point (Fig. 3b) the spectrum contains β and γ, but no α peak. This difference is surprising since (0\(\overline{1}\)\(\overline{1}\)) and (0\(\overline{3}\)\(\overline{3}\)) probe the same polarization and are both transverse for the NaI lattice. Next consider Fig. 3e, the (\(\overline{2}\)\(\overline{1}\)\(\overline{1}\)) X point, it is unlike either Fig. 3a or Fig. 3b in that it has α and β, but no γ. The (\(\overline{1}\)\(\overline{2}\)\(\overline{2}\)) X point (Fig. 3c) appears similar to (\(\overline{2}\)\(\overline{1}\)\(\overline{1}\)) with α and β peaks in the spectrum. The (\(\overline{3}\)\(\overline{2}\)\(\overline{2}\)) X point (Fig. 3f) appears to have no clear TO features. Finally, the (\(\overline{2}\)\(\overline{3}\)\(\overline{3}\)) X point (Fig. 3d) contains mostly α and γ with a weak β peak. Following the ILM* peak intensity going from Figs. 3c to 3d to 3f and to 3e shows that its intensity decreases and finally vanishes as the orientation moves away from [011] towards [100]. This is consistent with the [011] orientation deduced for ILM* from Fig. 1. These results show that with the appearance of the [011] ILM*s the TO splits into three modes with symmetry-breaking coherent structure.

Figure 2
figure 2

Phonon dispersion Q-E slices along [H,-3,-3] and [-2,K,K] along with a Q cut.

All slices and the cut section are indicated schematically in the image at right center. The out of plane [0,k,-k] direction is constrained to k = [-0.25,0.25] for all panels. (a) Slice along [H,-3,-3] with the [0,K,K] constrained to K = [-3.2,-2.8] at 636 K. (b) Slice along [-2,K,K] with [H,0,0] constrained to H = [-2.2,-1.8] at 636 K. (c) Cuts taken within the white dotted line section of (a) indicated by arrow at both 636 K and 567 K. The range for K along [0,K,K], H along [H,0,0] and k along [0,k,-k] (designated kmk for k minus k) are indicated at the top of the panel. Slices (d) and (c) are the same as (a) and (b) respectively, except at 567 K.

Figure 3
figure 3

A series of Q cuts at six X high-symmetry points.

The range for K along [0,K,K], H along [H,0,0] and k along [0,k,-k] (designated kmk for k minus k) are indicated at the top of each panel. The six X points are: (a) (0\(\overline{3}\)\(\overline{3}\)), (b) (0\(\overline{1}\)\(\overline{1}\)), (c) (\(\overline{1}\)\(\overline{2}\)\(\overline{2}\)), (d) (\(\overline{2}\)\(\overline{3}\)\(\overline{3}\)), (e) (\(\overline{2}\)\(\overline{1}\)\(\overline{1}\)) and (f) (\(\overline{3}\)\(\overline{2}\)\(\overline{2}\)). All of these cuts are indicated in the drawing at top center.

Figure 4 provides a map describing how the TO mode fragments change between the X points across Brillioun Zones. The [H,-3,-3] Q slice in Fig. 4a shows that γ is absent in a section from about H = -(1+2/3) to the zone center at H = -1. Similarly, the [H,-1,-1] Q slice in Fig. 4b shows α is absent in a section from H = -1/3 to H = +1/3. The [H,-1,-1] Q slice in Fig. 4c shows a larger section without the γ feature that extends from H = -0.5 to H = -2. The [-1,K,K] Q slices in Figs. 4d and 4e show that the α and β features appear in narrow ranges along this direction near the Γ points at K = -3 and K = -1. In Fig. 4e α and β reemerge near K = -(1+1/3). Additional weaker features at 11 meV appear near both of these Γ points, highlighted with white dashed ovals. Finally, the [-2,K,K] Q slice in Fig. 4f shows a small region where ILM*, α, β and γ all appear simultaneously near an X point.

Figure 4
figure 4

Map of the α, β and γ TO fragment coherent structure.

Regions with just β and γ intensity are shaded purple, regions with just α and β intensity are shaded green and regions with all three are shaded grey. Location where all three were not clearly visible are designated “weak”. For all slices the out-of-plane [0,k,-k] was constrained to k = [-0.25,0.25]. (a) Shows a slice along [H,-3,-3] where a segment of γ is absent in a 2/3 r. l. u. section. (b) Shows a slice along [H,-1,-1] around H = 0 where a segment of α is absent is absent in a 2/3 r. l. u. section from H = ±1/3. (c) Shows a slice along [H,-1,-1] around H = 1.5 where a larger section with γ absent is observed. (d) Shows a slice along [-1,K,K] around K = -3 where α and β are observed in a narrow section. An additional feature is indicated in the white dashed oval near 11 meV. (e) Shows a slice along [-1,K,K] around K = -1 that appears similar to the K = -3 point, including the extra feature near 11 meV. (f) Shows a slice along [-2,K,K] where all primary features α, β, γ and ILM* are visible in a region near K = -3.

Discussion

The TO mode splitting and discontinuous sectioning at fractions of a zone length are similar to zone folding effects seen with superlattices17, but here there are no corresponding superlattice Bragg reflections (in situ diffraction was monitored using Q slices near the elastic energy and showed no crystal structure changes through all measurements, as expected). Figure 5a shows how equally spaced ILM-like bond-defect modes in a 1D model give rise to dynamical superlattice properties without a structural superlattice. The 2/3 sections along [H,0,0] in NaI (Fig. 4) suggest a tripling of the unit cell along [100]. This allows for threefold splitting of the [100] TO mode into α, β and γ, while ILM*s originate along [011] and [0,-1,1] but appear at propagation wave vectors with components along [100] owing to localization. Figure 5b shows that this superlattice is commensurate with the observed 2/3 sections of the split TO mode, but that contrary to lattice theory the discontinuities in the modes all occur at zone centers rather than at zone boundaries, including the (\(\overline{1}\)\(\overline{3}\)\(\overline{3}\)) center common to all NaI superlattices. Noting that discontinuities must occur at zone boundaries suggests that the dynamical superlattice is offset in momentum space by [±1/3,0,0], implying that the dynamical superlattice itself has crystal momentum.

Figure 5
figure 5

Dynamical superlattices formed from ordered arrangements of ILM-like local modes.

(a) One dimensional diatomic lattice dynamical model after Kittel18 with nearest neighbor force constants C = 1 and a mass ratio M/m = 5.2, with and without ILM-like local modes. An array of ILM-like local modes is introduced by reducing the force constants on every fourth light atom to C' = 0.7, simulating the local softening expected with ILMs. The resulting phonon dispersion curves, unfolded to the same K-space scale, show that the single optic mode is fragmented into three closely spaced segments plus the local mode dropping down further into the gap. The acoustic mode shows minimal splitting by comparison. (b) Superlattice zone scheme in the [HKK] plane for NaI with the unit cell tripled along [100] (blue lines) projected on the parent zone scheme (black lines). The purple and green sections reproduce the experimental discontinuities in the TO fragments from Fig. 4.

These observations are surprising for a crystal in thermal equilibrium. From equipartition the amplitude of the gap feature is one tenth that calculated for the 3-D NaI ILM model7 and driven 1-D and 2-D models require sufficient carrier amplitude to initiate pattern forming modulation instabilities9. Measurements on material from a third source containing an impurity gap mode present at all temperatures (not shown) showed a slightly broader-weaker ILM feature form at high temperatures. Our conclusion is that these patterns form easier with temperature than classical models suggest and depend somewhat on crystal quality. The observed single-energy ILM peak4,5 is expected for a dynamical pattern built from equal ILMs9,10. The abrupt appearance of the ILM at high temperatures followed by modest growth with increasing temperatures4,5 is consistent with a pattern of ILMs. The collective changes of ILMs between [111] and [011] orientations (Fig. 1) are expected for patterns of ILMs transitioning between configurations. Finally, the observed symmetry-breaking dynamical pattern (Figs. 24) requires coherent alterations to interatomic force constants without changing atomic arrangements, the hallmark of a dynamical pattern built from ILMs. Unlike with a random distribution of ILMs, which could be stabilized by configurational entropy3, this dynamical pattern of ILMs poses a theoretical challenge as to how it is achieved in thermal equilibrium. While simulations have shown the existence of ILMs within the thermal-equilibrium vibrational spectrum of a 2D nonlinear lattice19, ILM order in equilibrium has not been reported. However, for the conceptually similar problem of substituting atoms of a different species into a crystal, ordering transitions only occur for narrow near-stoichiometric concentrations20. By analogy, the narrow temperature range of the ILM pattern may correspond to a temperature where the ILM concentration is a rational fraction of the lattice sites, allowing for a well ordered low-energy arrangement. A limitation of this analogy is that the ILM concentration need not obey the same conservation laws as atomic substitution. Simulations of the ILMs in NaI7 show that ILMs are accompanied by local strains, including both tensile and compressive fields. A well-ordered arrangement of ILMs that overlap the compressive and tensile strain fields of adjacent ILMs would lower the strain energy, providing a possible driving force for order.

Methods

Time-of-flight inelastic neutron scattering spectra were obtained on a large single crystal of NaI(0.002Tl) (same source as crystal but different from the pure NaI powder used in Ref. [5]) mounted on a rotating furnace using the wide Angular-Range Chopper Spectrometer (ARCS) at the Spallation Neutron Source (SNS) of Oak Ridge National Laboratory. Empty can runs were collected at measurement temperatures and were subtracted from all data sets. All measurements were taken with (HKK) in the scattering plane. In the first set of measurements curved sections of Q-E space (momentum-energy) were measured with the crystal held at a single angle at temperatures near the reported ILM formation temperature (555 K5, although a subsequent calibration of the furnace at NIST indicates it was closer to 575 K): 496 K, 543 K, 567 K, 614 K, 636 K and 659 K. The orientation was such that the [100] axis of the crystal was at 39.7o with respect to the incident beam and was chosen so that nearly equivalent zone sections along the [111] direction were aligned simultaneously with the high and low angle detector regions at the energy of interest (10 meV), providing a built in consistency check. In the second set of measurements comprehensive 4-dimensional Q-E volumes of data where obtained at 567 K and 636 K, by rotating the angle between [100] and the incident beam in 1 degree steps, collecting a scan at each angle and stitching the data together using the MSlice software package in DAVE16. The angles ranged from 70o to 100o for 567 K and between 65o and 105o for 636 K.