The complex phase diagrams of strongly correlated oxides arise from the coupling between physical and electronic structure. This can lead to a renormalization of the phase boundaries when considering thin films rather than bulk crystals due to reduced dimensionality and epitaxial strain. The well-established bulk RNiO3 phase diagram shows a systematic dependence between the metal-insulator transition and the perovskite A-site rare-earth ion, R. Here, we explore the equivalent phase diagram for nickelate thin films under compressive epitaxial strain. We determine the metal-insulator phase diagram for the solid solution of Nd1-yLayNiO3 thin films within the range 0 ≤ y ≤ 1. We find qualitative similarity between the films and their bulk analogs, but with an overall renormalization in the metal-insulator transition to lower temperature. A combination of x-ray diffraction measurements and soft x-ray absorption spectroscopy indicates that the renormalization is due to increased Ni–O bond hybridization for coherently strained thin films.
The rich phase diagram of many strongly correlated oxides offers the possibility of creating devices and heterostructures displaying novel functionality. Such devices can exploit sharp metal-insulator transitions, for instance, for use in resistive switches and phase-change memories. Indeed, the idea of a Mott transition field effect transistor, or Mott-FET, has been considered as a potential alternative to conventional Si-based technologies because of the absence of extrinsic limitations – such as short channel effects – due to the high carrier densities characteristic of these oxides.1,2 In this regard, the rare-earth nickelate perovskites (RNiO3) comprise an ideal model system, as the influence of the electronic correlations on phase behavior can be tuned by the choice of rare earth cation (R), temperature, dimensionality, and applied stress.3
The metal-insulator transition in RNiO3 is driven by interactions between Ni-3d and O-2p electrons which are sensitive to changes in structure and temperature.3 The transition may be modified by three forms of stress. The first is intrinsic, arising from steric limitations of the RNiO3 distorted perovskite structure. The ideal perovskite structure consists of |${\rm NiO}_6^{3 - }$| octahedra linked at their corners with R3+ ions in the interstices. The R3+ ion is relatively too small to fit this ideal structure, exerting an internal stress that is accommodated by a rigid rotation of the |${\rm NiO}_6^{3 - }$| octahedra. This rotation decreases the Ni–O–Ni bond angle away from the ideal value of 180°, narrowing the bands. The metal-insulator transition temperature, TMI, thus decreases with increasing R3+ ion size, varying from 570 K for HoNiO3 to 130 K for PrNiO3·La3+ is so large that LaNiO3 remains metallic to zero temperature. The transition temperature can be tuned continuously using solid solutions of rare earths.4,5 A second form of stress, external hydrostatic pressure, decreases the rotation of the octahedra, thereby decreasing TMI.6–8
Thin films of RNiO3 experience a third form of stress due to mismatch of the lattice and thermal expansion to the substrate, in addition to the intrinsic internal stress. Epitaxial growth of pure NdNiO3 films on a variety of substrates has shown a renormalization of TMI with respect to the bulk, that is, TMI is increased (decreased) by tensile (compressive) in-plane strain, an effect which is attributed to an increase (decrease) of the Ni–O–Ni, bond angle which affects films in the same way as the bulk.9–14 Alternatively, it has been suggested that tensile in-plane stress may lead to a novel breathing distortion that creates two inequivalent Ni sites; charge transfer between these sites increases TMI.15
Comparison of films is complicated by misfit dislocations, which partially relieve epitaxial strain and create strain gradients through the film thickness. Misfit strain can be controlled by growing defect-free films in registry (i.e., without misfit dislocations) with a low-misfit substrate, such as LaAlO3. It has been shown that, in such films, rotation of the |${\rm NiO}_6^{3 - }$| octahedra accommodates about half the epitaxial strain; the other half leads to octahedral distortions (i.e., elongation along the c-axis.).16
The strong effects of epitaxial strain across the RNiO3 phase diagram should be understood to enable novel device integration and to further the fundamental understanding of the relation between atomic structure and electronic properties. Previous work using the different misfits of various substrates to tune the transition has suffered from inconsistencies in the growth.9,14 Systematic results may be obtained by tuning the rare-earth composition with Nd1-yLayNiO3 (0 ≤ y ≤ 1) solid solutions while maintaining the same growth conditions. In this work, we study such alloyed films grown in registry with LaAlO3(001) substrates (pseudocubic indexing is used throughout), providing low-defect films with a homogeneous compressive strain; in addition, we use sample preparation aimed to avoid oxygen vacancies.9 We characterize the transport, structural, and electronic properties of the films using resistivity measurements, synchrotron diffraction crystal truncation rod data, and x-ray absorption spectroscopy. From this, we produce an electronic phase diagram for thin films resembling that of the bulk, but with lower transition temperatures (renormalization) due to the effect of epitaxial strain.
The Nd1-yLayNiO3 (0 ≤ y ≤ 1) films in this study are grown on (001)-oriented LaAlO3 substrates using molecular beam epitaxy (MBE) assisted by a radio-frequency oxygen plasma source. The bulk pseudocubic lattice parameters for NdNiO3, LaNiO3, and LaAlO3 are approximately 3.81 Å, 3.84 Å, and 3.79 Å, respectively. These values translate to a lattice mismatch of 0.5% for NdNiO3 and 1.3% for LaNiO3. LaAlO3 provides a nearly cubic template, with lattice planes rotated by <0.1° from the perovskite structure and twin boundaries typically >100 μm apart. The thicknesses of the films are held to 8 unit cells (uc). The Nd, La, and Ni metals are co-deposited in an oxygen environment with an oxygen partial pressure of 5 × 10−6 Torr. The temperature of the substrate during growth is 590 °C for each film. We utilize a quartz crystal microbalance to determine the relative stoichiometry of the metals prior to growth and ensure a growth rate of 1 layer/min. During the deposition, we monitor the film surface using reflection high energy electron diffraction (RHEED). The specular reflection shows intensity oscillations consistent with a layer-by-layer growth mode, with the peak-to-peak time corresponding to the growth of one unit cell. The observed sharp post-growth RHEED patterns along the [100] and [110] directions indicate coherent epitaxy.26 To eliminate the presence of oxygen vacancies from our films, the samples are annealed in flowing O2 for 6 hours at 600 °C following growth.
For each film, we measure the resistivity as a function of temperature (ρ-T) using a conventional van der Pauw geometry with Au contacts on the corners. We place the samples in a Quantum Design 4He cryostat to control the temperature in the range 10–300 K. Figure 1 shows the ρ-T curves obtained for 8 uc films with y = 0 (pure NdNiO3), y = 0.1 (90% Nd/10% La alloy), y = 0.25 (75% Nd/25% La alloy), and y = 0.4 (60% Nd/40% La alloy). We define the metal-insulator transition temperature, TMI, as the temperature at which ρ reaches a minimum.17 The curves for y = 0, 0.1, and 0.25 show metal-insulator transitions with TMI ≈ 155 K, 129 K, and 68 K, respectively. For y = 0.4, the film remains metallic in the entire temperature range. The high temperature metallic phase is characterized by a decrease in resistivity as the temperature is decreased (dρ/dT > 0). In the insulating state, the temperature dependence of the resistivity changes such that dρ/dT < 0. The samples with insulating ground states exhibit a temperature hysteresis in ρ around TMI upon cooling and heating the samples. The width of the maximum hysteresis window is 3 K for y = 0 and 10 K for y = 0.1 and 0.25, which also closely matches the difference in TMI upon heating and cooling. For clarity and for comparison with bulk measurements, Figure 1 shows only the data obtained upon heating.
Resistivity vs. temperature for 8 uc NdyLa1-yNiO3 thin films grown on LaAlO3. Three of the films display a metal-insulator transition at TMI ≈ 155 K (NdNiO3), 129 K (Nd0.9La0.1NiO3), and 68 K (Nd0.75La0.25NiO3); arrows in the figure indicate the approximate locations of TMI, established as the minimum of the resistivity, in each curve. The data plotted correspond to the resistivity as measured upon heating from 10 K to 300 K at a rate of 2 K/min. A temperature-related hysteresis is displayed by these films, as discussed in the main text; the cooling curve for the Nd0.75La0.25NiO3 has been omitted for clarity.
Resistivity vs. temperature for 8 uc NdyLa1-yNiO3 thin films grown on LaAlO3. Three of the films display a metal-insulator transition at TMI ≈ 155 K (NdNiO3), 129 K (Nd0.9La0.1NiO3), and 68 K (Nd0.75La0.25NiO3); arrows in the figure indicate the approximate locations of TMI, established as the minimum of the resistivity, in each curve. The data plotted correspond to the resistivity as measured upon heating from 10 K to 300 K at a rate of 2 K/min. A temperature-related hysteresis is displayed by these films, as discussed in the main text; the cooling curve for the Nd0.75La0.25NiO3 has been omitted for clarity.
To map out a diagram of electronic phases as a function of the La content, y, we determine TMI from the ρ-T measurements for 8 uc Nd1-yLayNiO3 alloys with y = 0, 0.1, 0.25, 0.4, 0.5, 0.9, 1. The resultant phase diagram is shown in Figure 2. For y ≥ 0.4, all films remain metallic down to T < 10 K, and thus we use a value of TMI = 0 for these films. The (y, TMI) points for y = 0, 0.1, and 0.25 are taken from the data shown in Figure 1. In analogy with the corresponding bulk phase diagram from Ref. 5, we also plot the transition temperatures as a function of the average size of the rare-earth ion (12-fold coordinated R3+ ionic radii as determined by Shannon18). We find that the thin film and bulk diagrams share a similar y-TMI dependence, despite the clamping effect of the substrate and the nearly two-dimensional thickness of the films.5 The value of TMI at y = 0, however, is ∼50 K lower for the NdNiO3 (bulk TMI ≈ 195 K), indicating that the MI transition temperature is shifted to lower temperatures for thin films. Furthermore, we find that a coherently strained 48 uc bulk-like NdNiO3 film grown on LaAlO3 has a TMI ≈ 156 K, matching that of the 8 uc NdNiO3. Thus, heteroepitaxial strain, rather than the reduction in dimensionality, appears to be the most likely source of the TMI shift.
Phase diagram of 8 uc (pink triangles) and bulk (brown circles) Nd1-yLayNiO3. For each specimen, TMI is plotted as a function of both y and the average ionic radius: Ravg = (1-y)RNd + (y)RLa, where RNd and RLa are the trivalent, twelvefold coordinated Shannon crystal ionic radii, from Ref. 18. The solid curves separating the metallic and insulating regions, a parabolic fit to the data, serve as a guides-to-the-eye. Bulk data are from Ref. 5.
Phase diagram of 8 uc (pink triangles) and bulk (brown circles) Nd1-yLayNiO3. For each specimen, TMI is plotted as a function of both y and the average ionic radius: Ravg = (1-y)RNd + (y)RLa, where RNd and RLa are the trivalent, twelvefold coordinated Shannon crystal ionic radii, from Ref. 18. The solid curves separating the metallic and insulating regions, a parabolic fit to the data, serve as a guides-to-the-eye. Bulk data are from Ref. 5.
In order to understand the origin of the similarities and differences between the bulk and thin film phase diagrams more thoroughly, we examine the structural properties of the thin film series using synchrotron-based x-ray diffraction. We carry out crystal truncation rod (CTR) measurements at the Advanced Photon Source at XOR beamline 33 ID-D at an x-ray energy of 16 keV. Figure 3(a) shows a comparison of the CTRs with H = 2 and K = 0 measured for 8 uc Nd1-yLayNiO3 films, with y = 0, 0.25, and 1, along with their associated fits.26 The out-of-plane lattice constants, c, of the films are determined from fits to the CTR data and compared for the three films in Figure 3(b). We observe a linear increase in c (Figure 3(b)) and the unit cell volume (Figure 3(c)) with increasing substitution of La. However, the unit cell volume of the thin films is reduced relative to their corresponding bulk analogs, as shown in Figure 3(c). This result indicates that the external strain caused by the substrate-film epitaxial mismatch leads to a reduction in bond lengths and octahedral tilt angles, as in the case of applied hydrostatic pressure.19
Structural data for 8 uc Nd1.yLayNiO3 films: (a) comparison of measured data (blue circles) and fits (red line) for the (20 L) crystal truncation rod; (b) average out-of-plane lattice constants extracted from the fits of (a); (c) comparison of unit cell volume of thin films and bulk samples. The in-plane lattice constant of the films matches that of the bulk LaAlO3 substrate (3.79 Å).
Structural data for 8 uc Nd1.yLayNiO3 films: (a) comparison of measured data (blue circles) and fits (red line) for the (20 L) crystal truncation rod; (b) average out-of-plane lattice constants extracted from the fits of (a); (c) comparison of unit cell volume of thin films and bulk samples. The in-plane lattice constant of the films matches that of the bulk LaAlO3 substrate (3.79 Å).
As mentioned earlier, this type of strain effect and the resultant change in the transition temperature has been observed in previous studies of pure NdNiO3 films,11,14,20–22 but the observed renormalization across the entire phase diagram – the rigid shift to lower TMI – demonstrates the systematic effect of compressive epitaxial strain on ultrathin films for all compositions studied here (between pure NdNiO3 and LaNiO3). It should be noted that other work on thin NdNiO3 films grown on LaAlO3, however, have determined different values of TMI than that reported here, ranging from 175 K to 0 K.12,13 This difference may be explained by divergent growth conditions, as the electrical properties of RNiO3 films vary with oxygen content, which can depend sensitively on sample preparation.23,24 Further work is needed to determine what growth factors are most crucial to explain these changes. In this study, we ensure oxygen stoichiometry by using atomic oxygen during growth as well as post-growth annealing. Despite growth disparities, a renormalization for compressively strained NdNiO3 has been consistently observed, thus one can expect that the qualitative structure of the thin film phase diagram of Figure 1 is independent of growth conditions.
In addition to examining the physical structure, we determine the effects of alloying on the electronic structure of the films by performing soft x-ray absorption (XAS) measurements at the U4B beamline at the National Synchrotron Light Source (NSLS) at room temperature. We measured spectra for the Nd1-yLayNiO3 films at the O-K edge and the Ni-L2 edge at room-temperature (the x-rays are linearly polarized perpendicular to the c axis; these films show no significant linear dichroism). As a reference, we also measure a bulk LaAlO3 crystal and a 48 uc bulk-like NdNiO3 film. The pre-peak regions of the measured O-K edge spectra are shown in Figure 4. For comparison, the data are scaled to the number of Ni layers using the integrated area under the measured Ni-L2 peak, which indicates a nominal Ni3+ oxidation state for each film. The pre-peak at ∼531 eV is absent for the LaAlO3 substrate and is associated with hybridization of the Ni-3d and O-2p states that govern conduction in the system.25 As seen in the figure, the 48 uc and 8 uc NdNiO3 films have nominally identical normalized pre-peak intensities, indicating the compositional origin of this feature. We observe an increase in the peak intensity with La content for our films. Accordingly, we attribute the increasing conductivity we find with the addition of La to an increase in the Ni-3d–O-2p hybridization.
Room temperature oxygen K edge pre-peak from the x-ray absorption spectra for 8 uc Nd1-yLayNiO3 films compared with bulk LaAlO3 and a 48 uc bulk-like NdNiO3 film. This absorption corresponds to transitions from O-1s to hybridized O-2p/Ni-3d states. The spectra are normalized to the corresponding Ni-L2 peaks. The pre-peak intensity increases with decreasing TMI; the pre-peak is absent in the LaAlO3 substrate.
Room temperature oxygen K edge pre-peak from the x-ray absorption spectra for 8 uc Nd1-yLayNiO3 films compared with bulk LaAlO3 and a 48 uc bulk-like NdNiO3 film. This absorption corresponds to transitions from O-1s to hybridized O-2p/Ni-3d states. The spectra are normalized to the corresponding Ni-L2 peaks. The pre-peak intensity increases with decreasing TMI; the pre-peak is absent in the LaAlO3 substrate.
In summary, we have constructed a phase diagram for 8 uc nickelate films under compressive epitaxial strain. This phase diagram is qualitatively similar to the bulk phase diagram, but with an overall renormalization of the metal-insulator transition temperature, TMI. The reduction of TMI with respect to the bulk can be explained by the modification of the structure caused by substrate clamping. In addition, the observed change in TMI as a function of La content arises from an increase in the overlap between Ni-3d and O-2p orbitals, as has been found in the bulk due to structural modifications induced by strain and changes in the effective rare-earth ionic radii. The conclusions drawn here may be generically applicable to other strongly correlated oxide thin films experiencing metal-insulator transitions and useful for the future utilization of such materials for novel device applications.
This work was supported by DARPA Grant No. W911NF-10-1-0206 and NSF MRSEC DMR 1119826 (CRISP). Use of the Advanced Photon Source is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-06CH11357. Use of the National Synchrotron Light Source, Brookhaven National Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-98CH10886.