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Magnetic ground state of SrRuO3 thin film and applicability of standard first-principles approximations to metallic magnetism

  • Scientific Reports 7, Article number: 4635 (2017)
  • doi:10.1038/s41598-017-04044-6
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Abstract

A systematic first-principles study has been performed to understand the magnetism of thin film SrRuO3 which lots of research efforts have been devoted to but no clear consensus has been reached about its ground state properties. The relative t2g level difference, lattice distortion as well as the layer thickness play together in determining the spin order. In particular, it is important to understand the difference between two standard approximations, namely LDA and GGA, in describing this metallic magnetism. Landau free energy analysis and the magnetization-energy-ratio plot clearly show the different tendency of favoring the magnetic moment formation, and it is magnified when applied to the thin film limit where the experimental information is severely limited. As a result, LDA gives a qualitatively different prediction from GGA in the experimentally relevant region of strain whereas both approximations give reasonable results for the bulk phase. We discuss the origin of this difference and the applicability of standard methods to the correlated oxide and the metallic magnetic systems.

Introduction

The study of transition-metal oxide heterostructures and thin films has been an exciting field of research1,2,3,4,5. As the controlled synthesis and the combination of multiple ‘mother compounds’ become feasible, new possibilities can be realized to create the unique functionality and another angle to look at a long-standing problem from a different perspective. Simultaneously, however, it requires the further technological developments; not only for synthesizing but also for characterizing the materials. For example, the site dislocation, interface sharpness, stoichiometry and the oxygen vacancy have often been issues to understand the observed phenomena and the discrepancies between different measurements3,4,5.

Partly in this regard, first-principles approach has been playing a central role in this field from the early stage3, 4. Due to its capability of independent simulation, first-principles calculation not just provides the better understanding of experiments, but is also useful to predict or suggest a new system to have desired properties4, 6,7,8,9,10. As for the computation methods, however, there are several limitations and challenges to be overcome especially when the ‘(on-site) electronic correlation’ becomes important11, 12.

In this paper we study the magnetism of SrRuO3 (SRO113) thin film. First of all, it is an interesting system from both fundamental science and application point of view13,14,15,16,17,18,19,20,21,22,23,24. Its possible applications, for example, to the bottom electrode and field-effect devices have been discussed13. Further, a fundamental understanding of its magnetic properties is still controversial15,16,17,18,19,20,21,22,23,24. While the ferromagnetism of SRO113 has traditionally been discussed from Stoner’s picture13, 16, 25, recent studies provide new insights19, 26, 27. The relationship to its cousins (e.g., CaRuO3, Sr2RuO4, Ca2RuO4, etc), which show fairly different characteristics including antiferromagnetic insulating (AF-I) phase and superconductivity28, 29, should also be clarified. Thin film SRO113, in particular, exhibits the intriguing thickness-dependent magnetic and metal-insulator transition15,16,17,18. The nature of this transition is far from clear. For example, there is an obvious discrepancy in the previous reports regarding the critical thickness, and the ground state magnetism has not been clearly identified15,16,17,18, 20,21,22,23,24.

Here we perform a systematic and comparative investigation of SRO113 based on the standard first-principles computation methods. We elucidate the controversies in the previous calculations16, 20,21,22,23,24 and partly resolve the unsettled issues including the thickness and strain dependent transition of magnetic and electronic properties15,16,17,18, 20,21,22,23,24. The role of strain, correlation and lattice distortions are clarified. We further analyze the applicability of primary approximations, namely, LDA (local density approximation) and GGA (generalized gradient approximation), to metallic magnetism. Landau free energy analysis and the magnetization-energy-ratio plot clearly show the different tendency of favoring the magnetic moment formation. In case of thin film, as a result, LDA gives a qualitatively different prediction from GGA in the experimentally relevant region of strain whereas both approximations give reasonable results for the bulk phase. We discuss the origin of this difference and the applicability of standard methods to the correlated oxide and the metallic magnetic systems. Our work carries important information for future study especially when the experimental information is severely limited just as in the thin film or heterostructure.

Results

Bulk

SRO113 is a ferromagnetic metal (FM-M) with Curie temperature of 160 K and magnetic moment (M) of 1.1–1.7 μB/f.u.13. Orthorhombic crystal structure is stabilized below 850 K with GdFeO3-type distortion13. To investigate SRO113, we first optimized the lattice parameters and the result is in good agreement with the previous studies (Table 1)20, 21, 30, 31. A well-known trend of the underestimated/overestimated lattice parameters by LDA/GGA is clearly seen. The deviation from experimental lattice values is within ±1.2%. Rotation and tilting angles calculated by LDA and GGA are slightly overestimated (within ~1.6–2.2°) in comparison with the experimental value of 8.61° and 8.60°, respectively.

Table 1: The calculated lattice constants, Stoner I, IN(EF) and magnetic moments for c-SRO113 and o-SRO113 by LDA and GGA.

Ferromagnetic ground state is well reproduced by both LDA and GGA with the optimized and experimental lattice parameters. The calculated moments are summarized in Table 1 being consistent with the previous studies20, 30, 31. About 70% of total moment resides at Ru-site and the other amount comes from O-site due to the hybridization20, 25. GGA moment is larger than LDA by about factor of two. Here we note this unusually large difference of the calculated moments by two different exchange-correlation (XC) functionals. It may indicate either that GGA overestimates the ferromagnetism or that LDA underestimates it. This difference becomes critical when one tries to predict the ferromagnetic instability in the thin films for which the experimental detections are largely limited. This point will be highlighted and further discussed later in this paper.

The GGA trend of stronger (than LDA) preference for ferromagnetic solutions is also found in the magnetic stabilization energy: ΔELDA = ΔEFM − ΔEPM = −7.8 meV/f.u. and ΔEGGA = −106 meV/f.u. for o-SRO113 (orthorhombic SRO113). For c-SRO113 (cubic SRO113), ΔELDA = −14 meV/f.u. and ΔEGGA = −102 meV/f.u.

To have further understanding, we performed the fixed spin moment (FSM) calculations which have not been reported before in these materials. Our result is summarized in Fig. 1. The aforementioned magnetic behavior, namely the enhanced (suppressed) ferromagnetism by GGA (LDA), is again clearly manifested in this plot (see blue and red lines in Fig. 1). Note that this is not just the effect from the different lattice constants given by GGA and LDA optimization. Even when the same crystal structures were used, GGA total energy more favors the ferromagnetic solution than LDA; compare the blue-solid line (filled triangles) with the yellow-dashed line (open circles), and compare the green-dotted line (open triangles) with the red-dashed-dotted lines (filled circles). It is also noted that the GGA-optimized crystal structure is more favorable to ferromagnetism than the LDA structure; compare the blue solid line (filled triangles) with the green dotted lines (open triangles), and compare the yellow-dashed line (open circles) with the red-dashed-dotted lines (filled circles).

Figure 1
Figure 1

FSM calculation result of total energy for c-SRO113 as a function of M. The lines are obtained from the fitting to the Landau free energy. The open triangles (green) and open circles (yellow) refer to the LDA results with the GGA-optimized structure and the GGA results with the LDA-optimized structure, respectively. The nonmagnetic state is set to be the zero reference energy.

The ferromagnetism in ruthenates has been understood traditionally based on the Stoner model13, 16, 25. Therefore, it would be fruitful to estimate the Stoner parameter (I) from our FSM calculation results. Landau free energy can be written as,

E(M)=E(0)+( a 2 / 2 ) M 2 +( a 4 / 4 ) M 4 +,
(1)

where E(M) is the total energy as a function of magnetic moment (Fig. 1). The uniform spin susceptibility is given by

χ 1 = 2 E M 2 | M = 0 = a 2 = 1 2 ( 1 N ( E F ) I ) ,
(2)

where N(EF) is the non-spin-polarized density of states (DOS) per spin at Fermi level (EF). The calculated Stoner I and IN(EF) are presented in Table 1. The LDA result is in good agreement with the previous study25. Both LDA and GGA results satisfy the Stoner’s criterion of ferromagnetism and the calculated magnetic moments are in reasonable range consistent with experiments. The calculated I and I N(EF) values by GGA are larger than those of LDA by ~17% and ~40%, respectively. Namely, the stronger preference for FM solution by GGA (than LDA) can also be seen in these parameters. We once again emphasize that this cannot be attributed to the lattice effect. It is rather directly related to the parameterization of XC functional itself and thus requires further understanding at the more fundamental level. Our result demonstrates that the special care needs to be paid in ruthenates and related systems when one uses first-principles methods even within the standard XC approximations.

Undistorted thin films: 1a × 1a lateral unitcell

Now let us turn our attention to the thin film. The previous calculations and experimental results are not quite consistent with one another regarding, for example, the thickness-dependent magnetic states on SrTiO3 substrate13, 15,16,17,18, 20,21,22,23,24. Since SRO113 thin film and its magnetic property have been studied often within 1a × 1a lateral unitcell (uc)16, 20, we focus on 1a × 1a films before considering the effect of tilting/rotational distortions of RuO6 octahedra.

Our results are summarized in Fig. 2. The calculated magnetic moments by GGA (red circles) and LDA (blue triangles) are presented as a function of strain. Figure 2(a–c) shows the result of the 3-uc, 2-uc, and 1-uc thick SRO113 films, respectively. In the 1a × 1a lateral uc, antiferromagnetic spin order can not be simulated and the finite moment indicates the ferromagnetic order as in the previous studies16, 20. It is noted that GGA more prefers the ferromagnetic solution than LDA, which is the same tendency as observed in the calculations of bulk SRO113.

Figure 2
Figure 2

The calculated Ru moments of (a) 3-uc, (b) 2-uc, and (c) 1-uc thick c-SRO113 by LDA (blue solid lines; triangles) and GGA (red solid lines; circles) as a function of strain. The zero strain is set to the optimized lattice parameters of the bulk structure by each XC functional (Table 1). The vertical dashed lines represent the strains realizable by NdGaO3 (blue), Sr2RuO4 (light blue), SrTiO3 (orange), DyScO3 (magenta), and GdScO3 (red) as substrates.

One general feature found in Fig. 2 is that the ferromagnetism is suppressed by compressive strain. Both LDA and GGA predict the zero moment or paramagnetic phase under the large enough compressive strain. Importantly, however, the difference between GGA and LDA leads to a different prediction for the existence of ferromagnetic order and the critical value of strain below (above) which the magnetic moment or ferromagnetic order vanishes (sets in). In GGA, the ferromagnetic order is robust for 3-uc, 2-uc, and 1-uc films, which is significantly different from the LDA predictions of ≤−0.5 (3-uc)–0.0% (2-uc).

Note that, in the experimentally accessible strain range, GGA gives a qualitatively different prediction from LDA especially for the case of 1-uc. Vertical dashed lines indicate the strain values corresponding to the available substrates. Within the −2–+1.5% range, LDA gives zero (or very small) moment while GGA predicts magnetic phase and the moment is quite large. It should be noted that the zero strain in our calculations is set to be the LDA/GGA-optimized lattice parameters obtained by each XC functional and therefore two values at a given strain value represent the different in-plane lattice parameters; larger in GGA case and smaller in LDA.

As an example, let us first consider the mono-layer SRO113 grown on NdGaO3 substrate (dark-blue vertical lines)32. Due to the lattice mismatch, this corresponds to the −1.81% of compressive strain situation. For this case, GGA predicts the ferromagnetic spin order while LDA solution is nonmagnetic. The same is true for the case of Sr2RuO4 substrate33 which corresponds to −1.55% compressive strain. Our result therefore raises a question about the predictive power of standard first-principles methodology. On the one hand, it shows that the special care needs to be paid in the first-principles study of correlated oxide thin films and/or heterostructures even with the standard XC energy functionals. On the other, our result calls the further method development which can better describe the electronic correlations and the structural properties. We note that in this kind of systems conventional experimental techniques are often less useful. In this sense, correlated oxide heterostructure and thin film pose a new challenge to the first-principles methodology (see Discussion).

Another notable example is SRO113 film on SrTiO3 substrate (−0.38% compressive strain). Contrary to the previous experimental reports15,16,17,18, there is no clear magnetic-to-nonmagnetic and metal-to-insulator (MI) transition in both of our GGA and LDA results. In 1-uc case, GGA result is ferromagnetic with ~1.4 μB/Ru while a significantly smaller magnetic moment of ~0.2 μB/Ru is found in LDA (Fig. 2(c)). It may seem inconsistent not only with experiments but also with the previous LDA16, 20 calculations since they report the magnetic to non-magnetic transition as the SRO layer thickness is reduced although the critical thickness is still under debate15,16,17,18, 20. It should be noted however that in the previous LDA16 studies, the experimental SrTiO3 lattice parameter (3.905 Å) is taken for the calculations. According to our optimized lattice parameters, this corresponds to +0.69% tensile strain for the case of LDA and −2.08% compressive strain for GGA, both of which are significantly different from the experimental situation of −0.38% compressive strain. In fact, our results of +0.69% tensile and −0.38% compressive strain are consistent with the previous calculations16, 20. At the correct strain of SRO113 on SrTiO3 (−0.38%), the LDA magnetic moment gradually decreases from 3-uc to 1-uc which may be understood as a magnetic to non-magnetic transition observed in experiments. In GGA, however, ferromagnetism survives down to 1-uc thickness. This behavior is double checked by other codes, namely, OpenMX and ecalj.

It is clear that understanding the SRO113 thin film based on 1a × 1a is quite limited. The tilting and rotation distortions can play important roles in determining the electronic and magnetic property.

Distorted thin films: 2 a× 2 a lateral unitcell

The octahedral distortion (tilting and rotation of RuO6 cage) and the use of enlarged lateral uc can lead to a qualitatively different ground state solution. The 2-uc-thick SRO113 is found to have FM-M ground state in the strain range of about −3 to +2.5%. At ~3%, G-type-like (i.e., all the nearest-neighbor couplings are antiferromagnetic) AF-I is stabilized in both LDA and GGA with Ru-site magnetic moment of 0.74 μB/Ru (LDA) and 1.51 μB/Ru (GGA). It is markedly different from the strained bulk SRO113 for which ferromagnetic ground state is fairly robust over a wide range of strain and G-type AF-I state is not stable30, 31.

To understand the detailed electronic structure and its relation to the magnetism, we focus on the thinnest case (i.e., 1-uc thick) in the remaining part of this subsection. The ground state phase diagram as a function of strain is presented in Fig. 3; (a) LDA and (b) GGA. The first thing to be noted is that both XC functionals predict FM-M and AF-I ground state in the large compressive and large tensile strain region, respectively. The size of magnetic moment is generally larger in GGA than LDA, which is the same feature found in the previous cases of bulk and undistorted thin film.

Figure 3
Figure 3

The calculated M of 1-uc 2 a ×  2 a o-SRO113 by (a) LDA and (b) GGA as a function of strain. The different types of ground configurations (FM-M, AF-M, and AF-I) are presented by background colors. The vertical dashed lines represent the strains realizable by NdGaO3 (blue), Sr2RuO4 (light blue), SrTiO3 (orange), DyScO3 (magenta), and GdScO3 (red) as substrates.

In the experimentally more accessible range, however, LDA and GGA give qualitatively different solutions. In the GGA phase diagram (Fig. 3(b)), AF-I is the ground state around zero strain region (≤±1% strain) while LDA predicts either FM-M or antiferromagnetic metal (AF-M). The AF-M phase of LDA (which is absent in GGA phase diagram) is attributed to the smaller energy splitting between d xy and d yz,zx states near EF. Thus, for the case of SrTiO332, DyScO332 or GdScO314 substrate, we have two different predictions regarding the ground state property from two standard XC functionals. It therefore raises a serious question about the predictive power of the current first-principles method to describe the correlated oxide thin film and/or heterostructure for which the experimental information is often limited. Further investigation and development are urgently necessary.

Noticeable is our GGA result of AF-I ground state for SrTiO3 substrate (see Fig. 3(b)). We emphasize that this AF-I phase has never been achieved before by LDA and GGA16, 20,21,22. Since AF-I has previously been obtained only by DFT + U21, 22 or DFT + DMFT (DFT + dynamical mean-field theory)24 and it can be consistent with the recent experiments reporting an insulating state carrying no net moment17, 18, it has been discussed that the insulating gap of 1-uc SRO113 is opened by on-site Coulomb correlation24. However, Fig. 4(a) clearly shows the band-gap without the explicit inclusion of U while the gap size is smaller than that of DMFT ( E g DMFT  = 1.0 eV)24. Our result therefore implies that the insulating ground state of mono-layer SRO113 is not just attributed to the local Coulomb physics within Ru-d electrons, but the homogeneous electron approximation can describe the gap opening. It also shows that the careful consideration of lattice effect is important to simulate the experimental situation of complex oxides.

Figure 4
Figure 4

(a) The Ru-t2g DOS by GGA for 1-uc o-SRO113 at −0.5% strain. The positive and negative DOS represent the up- and down-spin parts, respectively. The Fermi level is set to zero. The non-spin-polarized DOS is shown in the inset. (b) The calculated crystal-field splitting, Δ, for 1-uc o-SRO113 by GGA as a function of strain. The inset shows Δ as a function of film thickness (the number of layers) at 0% strain.

A common trend found in both LDA and GGA phase diagram is that the tensile strain makes system antiferromagnetic while the compressive strain favors ferromagnetic. It can be simply understood by defining an energy level difference between Ru-d yz,zx and d xy state: Δ LDA / GGA ε y z , z x LDA / GGA ε x y LDA / GGA . It is straightforward to compute ε by using the standard technique of maximally localized Wannier function34, 35. At 0% strain, ΔLDA = 0.33 and ΔGGA = 0.31 eV. As the in-plane lattice parameter gets smaller (more compressive strain), Δ decreases to 0.15 (LDA) and 0.17 (GGA) eV at ~−3% while under tensile strain it becomes larger to 0.40 (LDA) and 0.38 (GGA) eV at ~+3%. The same trend is also observed in the 2-uc-thick film; Δ = 0.21 eV (LDA) and 0.20 eV (GGA) at 0% strain while Δ = 0.27 eV (LDA) and 0.27 eV (GGA) at ~+3% strain where AF-I is stabilized. The calculated results of ΔGGA is presented in Fig. 4(b). In the large Δ limit (large tensile strain regime), the separation between ε yz,zx and ε xy is large and it approximately corresponds to the (two-band) half-filled case within the ionic picture of Ru4+ (see inset of Fig. 4(a)) as in the case of Ca2RuO436. Thus the antiferromagnetic spin order is naturally stabilized via superexchange. On the other hand, the small Δ limit (compressive strain) basically corresponds to the bulk SRO113 regime in which ferromagnetic order is stable.

The inset of Fig. 4(b) shows the calculated ΔGGA as a function of SRO thickness. A decreasing trend is clearly noticed as the number of layers increases. Since this is a qualitatively consistent trend with the magnetic transition observed in the several experiments as a function of layer thickness, our result implies that the Δ plays an important role in the thickness-dependent transition. Therefore it is probably not understood solely from N(EF) and Stoner’s criterion16, but rather comparable with the case of SrVO3/SrTiO3 in which the lifted orbital degeneracy plays an important role to induce the MI transition37, 38. We do not find any systematic trend in N(EF) over the range of strain. In the sense that the FM-M to AF-I transition occurs in between 2- and 1-uc thickness, our GGA result is not in quite good agreement with experiments which report the transitions in between 5- and 4-uc15, or 4- and 3-uc17, 18, or 3- to 2-uc16. Further inclusion of electron correlations might be needed to correctly describe the Δ and other electronic properties19, 38,39,40,41,42,43.

It might be informative to see DFT + U44 results. In spite of its static Hartree-Fock nature, it has been used to study SRO11321, 22. With a fixed U value to a recent cRPA (constrained random phase approximation) result (U = 3.5 eV24) and at a −0.5% compressive strain (close to SrTiO3 value), AF-I phase is found to be the ground state. For 1-uc thickness, Eg = 1.1 (1.6) eV and M = 1.47 (1.60) μB/Ru in LDA + U (GGA + U). In 2-uc thickness, Eg = 0.9 (1.3) eV and M = 1.41 (1.57) μB/Ru in LDA + U (GGA + U).

Discussion

Our results show that the prediction of the magnetic ground state of complex oxide thin film or heterostructure is a challenge to the current first-principles methodology. Without further information such as structural property and/or magnetic order (usually known from experiment in the case of bulk), it is difficult to make a prediction for thin film SRO113. Note that LDA and GGA are not a bad choice to describe the bulk SRO113 in the sense that both predict the correct FM-M ground state. Although some detailed features in the electronic structure are not well captured by LDA or GGA (e.g., Hubbard-like state ~−1.3 eV below the Fermi energy; see, ref. 45), these standard approximations provide reasonable descriptions of this metallic bulk material. Arguably, they are better than other improved but static methods to take orbital-dependent correlations into serious account such as DFT + U11. It is therefore surprising to see such a large difference between LDA and GGA in this system.

We first note that this difficulty is related to the complex nature of correlated oxides in which the spin, orbital, and lattice degree of freedom are tightly coupled to each other. On the one hand, it is the reason why the parameter-free first-principles techniques are strongly requested. On the other hand, this complexity makes the first-principles description be a greater challenge. Note that an improved description of electronic correlations cannot immediately be the right answer unless it can simultaneously give the better description of the other degrees of freedom such as lattice. For example, if we resort to DMFT approximation to get a better electronic structure of ruthenates, we have to describe the force and the lattice relaxation simultaneously at the same level. This development is technically non-trivial46,47,48. Similar issues and related intrinsic ambiguities can also be found in other techniques such as SIC-DFT (self-interaction corrected DFT) and hybrid functional.

Here it is instructive to recall that the metallic magnetism has been a challenge to the first-principles calculation49,50,51,52. A classical example is bcc Fe for which minimum energy solution of LDA is paramagnetic hcp phase (with the optimized lattice parameter)49 unlike Co and Ni53. In other words, without a priori knowledge of ferromagnetism, the situation of bcc Fe is similar with SRO113 thin film; paramagnetic ground state by LDA and ferromagnetic in GGA. Since the use of experimental lattice parameter gives the correct ferromagnetic solution in both LDA and GGA, bcc Fe is an easier case in the practical sense. In SRO113 thin film, on the other hand, the limitation of computation method is magnified due to no a priori information of structure and magnetic order.

A more detailed nature of enhanced ferromagnetism by GGA functional can be seen in Fig. 5 where the PBE (Perdew-Burke-Zunger) correction of spin-polarized energy density with respect to LDA is presented as a function of inverse density (r s ) and density gradient (s) for the relative spin-polarization (ζ). The calculated values of

α XC Δ ε XC PBE ( r s , ζ , s ) Δ ε XC LDA ( r s , ζ )
(3)

are represented by color. Here Δ ε XC PBE ( r s ,ζ,s)= ε X unif ( r s ,0)[ F XC ( r s ,ζ,s) F XC ( r s ,0,s)] and Δ ε XC LDA ( r s ,ζ)=f(ζ)[ ε XC unif ( r s ,1) ε XC unif ( r s ,0)] refer to the spin-polarized part of XC energy density within PBE and LDA, respectively. For the definitions of ε, r s , ζ, s, FXC(r s , ζ, s), and f(ζ), we follow the original PBE54 and LDA-PZ (Perdew-Zunger)55 papers. By definition, αXC represents the energy gain by GGA-PBE over LDA. In the yellow-red colored region of Fig. 5, GGA-PBE prefers the magnetic solution more than LDA while in the dark blue region LDA-like solution is favored. About 85000 real-space grid points (using OpenMX code) are plotted in this map for bcc Fe (red-colored points) and c-SRO113 (black-colored points), respectively. It is clear that both bcc Fe and c-SRO113 have large portion of grid points in the region of αXC larger than unity. It is responsible for the larger spin splitting (~ Δ ε XC / ζ ) and thus the moment formation enhanced by PBE correction.

Figure 5
Figure 5

The calculated α XC for c-SRO113 (black crosses) and bcc Fe (red crosses). About 85000 real-space grid points are obtained from the self-consistently converged electronic structure within LDA. Experimental lattice parameters are used. ζ is fixed to 0.02 which is the average value of c-SRO113. The α XC change is negligible in the range of 0 < ζ < 0.5.

Since many interesting aspects of complex oxide films and interfaces are directly or indirectly related to the metallic magnetism56,57,58,59,60, it is strongly requested to develop more reliable computation methods. One promising aspect is the same overall trend given by LDA and GGA. For example, the moment is suppressed by compressive strain in the case of 1a × 1a lateral uc (Fig. 2(a,b)). FM-M and AF-I phase in the large compressive and large tensile strain, respectively, are also consistently reproduced by LDA and GGA (Fig. 3). Further investigation of parameterization hopefully gives a way to improve approximations.

Summary

From a systematic first-principles investigation, we elucidate the controversies in the previous calculations and experiments. A part of issues has been clarified including the thickness- and strain-dependent phase transition as well as the ground state property of monolayer SRO113. The role of strain, correlation and lattice distortions are explored in detail. Applicability of LDA and GGA has been discussed in the realistic material context by using Landau free energy analysis and magnetization-energy-ratio plot. While the overall feature is commonly reproduced by both approximations, they give qualitatively different predictions for the case of thin film in the experimentally relevant region of strain. Our work provides useful information not only for ruthenates and other correlated oxides, but also for further first-principles studies in the related systems such as metallic magnetism.

Methods

We choose LDA parameterized by Perdew and Zunger55 and GGA by Perdew, Burke, and Ernzerhof54 as two representative XC functionals. The data obtained by these two functionals is presented as our main results and discussed in a comparative way. We used projector-augmented-wave (PAW) method61 as implemented in the VASP software package62. While VASP-PAW is used to obtain our main results, we also double checked some cases with other methods, confirming that our conclusions are valid. The other codes we used include OpenMX63, which is based on the norm-conserving pseudopotential and pseudoatomic orbitals, and ecalj64 based on the full-potential ‘LMTO’ or ‘PMT’ basis65.

Tetrahedron method with Blöchl correction has been used for Brillouin zone integration66, which we found is important to achieve the enough accuracy. In some cases the use of Gaussian broadening is found to give qualitatively different predictions depending on the broadening value. For bulk structure optimizations, 12 × 12 × 12 and 8 × 8 × 6 k-points were used for 5-atom uc of c-SRO113 and 20-atom uc of o-SRO113, respectively. The force criterion of 1 meV/Å was adopted for structural optimization. This choice of k meshes and the 500 eV energy cutoff were found to be satisfactory from our convergence test. For the electronic structure calculations, however, we took a denser k-grid of 16 × 16 × 16 for c-SRO113 and 12 × 12 × 10 for o-SRO113 to calculate DOS for the given optimized structures. To simulate SRO113 thin films, we considered the 3-uc, 2-uc, and 1-uc slab geometries terminated with SrO layers which is known to be the case in experimental situations13. The k-grids used for slab calculations were 12 × 12 × 2 for c-SRO113 and 8 × 8 × 2 for o-SRO113. The vacuum thickness is ≥15 Å which is large enough to simulate the experimental situation. The Ru radius is set to 1.402 Å and the Ru moment dependence on this setting is negligible (~0.01 μB).

Epitaxial strain is one of the key control parameters in the thin film growth. It is therefore of crucial importance to determine how to simulate the in-plane lattice parameter corresponding to the experimental situation. Note that this is a non-trivial issue because LDA- and GGA-optimized lattice parameters are both in general different from the experimental values. While the former tends to underestimate the lattice parameter, the latter overestimates (see Table 1). Thus, the naive choice of a XC functional or taking experimental lattice value can easily be misleading. Previous studies are not quite consistent in this regard. In the current study, we take the optimized lattice constant with a given XC functional as the reference value (i.e., zero strain) and define the compressive/tensile strain value with respect to it. This can be the most reasonable way to simulate the experiments and can serve as a solid reference for the future study. This point should be kept in mind when our results are compared with the previous calculation results16, 22.

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References

  1. 1.

    Ohtomo, A., Muller, D. A., Grazul, J. L. & Hwang, H. Y. Artificial charge-modulationin atomic-scale perovskite titanate superlattices. Nature 419, 378–380 (2002).

  2. 2.

    Dawber, M., Rabe, K. M. & Scott, J. F. Physics of thin-film ferroelectric oxides. Rev. Mod. Phys. 77, 1083–1130 (2005).

  3. 3.

    Mannhart, J., Blank, D. H. A., Hwang, H. Y., Millis, A. J. & Triscone, J.-M. Two-dimensional electron gases at oxide interfaces. MRS bulletin 33, 1027–1034 (2008).

  4. 4.

    Chakhalian, J., Freeland, J. W., Millis, A. J., Panagopoulos, C. & Rondinelli, J. M. Colloquium: Emergent properties in plane view: Strong correlations at oxide interfaces. Rev. Mod. Phys. 86, 1189–1202 (2014).

  5. 5.

    Stemmer, S. & Allen, S. J. Two-dimensional electron gases at complex oxide interfaces. Annu. Rev. Mater. Res. 44, 151–171 (2014).

  6. 6.

    Fennie, C. J. & Rabe, K. M. Magnetic and electric phase control in epitaxial EuTiO3 from first principles. Phys. Rev. Lett. 97, 267602 (2006).

  7. 7.

    Lee, J. H. et al. A strong ferroelectric ferromagnet created by means of spin-lattice coupling. Nature 466, 954–958 (2010).

  8. 8.

    Chaloupka, J. & Khaliullin, G. Orbital order and possible superconductivity in LaNiO3/LaMO3 superlattices. Phys. Rev. Lett. 100, 016404 (2008).

  9. 9.

    Hansmann, P. et al. Turning a nickelate fermi surface into a cupratelike one through heterostructuring. Phys. Rev. Lett. 103, 016401 (2009).

  10. 10.

    Han, M. J., Wang, X., Marianetti, C. A. & Millis, A. J. Dynamical mean-field theory of nickelate superlattices. Phys. Rev. Lett. 107, 206804 (2011).

  11. 11.

    Anisimov, V. I., Aryasetiawan, F. & Lichtenstein, A. I. First-principles calculations of the electronic structure and spectra of strongly correlated systems: the LDA + U method. J. Phys.: Condens. Matter 9, 767 (1997).

  12. 12.

    Kotliar, G. et al. Electronic structure calculations with dynamical mean-field theory. Rev. Mod. Phys. 78, 865–951 (2006).

  13. 13.

    Koster, G. et al. Structure, physical properties, and applications of SrRuO3 thin films. Rev. Mod. Phys. 84, 253–298 (2012).

  14. 14.

    Thompson, J. et al. Enhanced metallic properties of SrRuO3 thin films via kinetically controlled pulsed laser epitaxy. Appl. Phys. Lett. 109, 161902 (2016).

  15. 15.

    Toyota, D. et al. Thickness-dependent electronic structure of ultrathin SrRuO3 films studied by in situ photoemission spectroscopy. Appl. Phys. Lett. 87, 162508 (2005).

  16. 16.

    Chang, Y. J. et al. Fundamental thickness limit of itinerant ferromagnetic SrRuO3 thin films. Phys. Rev. Lett. 103, 057201 (2009).

  17. 17.

    Xia, J., Siemons, W., Koster, G., Beasley, M. R. & Kapitulnik, A. Critical thickness for itinerant ferromagnetism in ultrathin films of SrRuO3. Phys. Rev. B 79, 140407 (2009).

  18. 18.

    Ishigami, K. et al. Thickness-dependent magnetic properties and strain-induced orbital magnetic moment in SrRuO3 thin films. Phys. Rev. B 92, 064402 (2015).

  19. 19.

    Georges, A., de Medici, L. & Mravlje, J. Strong correlations from Hund’s coupling. Annu. Rev. Condens. Matter Phys. 4, 137–178 (2013).

  20. 20.

    Rondinelli, J. M., Caffrey, N. M., Sanvito, S. & Spaldin, N. A. Electronic properties of bulk and thin film SrRuO3: Search for the metal-insulator transition. Phys. Rev. B 78, 155107 (2008).

  21. 21.

    Mahadevan, P., Aryasetiawan, F., Janotti, A. & Sasaki, T. Evolution of the electronic structure of a ferromagnetic metal: Case of SrRuO3. Phys. Rev. B 80, 035106 (2009).

  22. 22.

    Gupta, K., Mandal, B. & Mahadevan, P. Strain-induced metal-insulator transition in ultrathin films of SrRuO3. Phys. Rev. B 90, 125109 (2014).

  23. 23.

    Verissimo-Alves, M., García-Fernández, P., Bilc, D. I., Ghosez, P. & Junquera, J. Highly confined spin-polarized two-dimensional electron gas in SrTiO3/SrRuO3 superlattices. Phys. Rev. Lett. 108, 107003 (2012).

  24. 24.

    Si, L., Zhong, Z., Tomczak, J. M. & Held, K. Route to room-temperature ferromagnetic ultrathin SrRuO3 films. Phys. Rev. B 92, 041108(R) (2015).

  25. 25.

    Mazin, I. I. & Singh, D. J. Electronic structure and magnetism in Ru-based perovskites. Phys. Rev. B 56, 2556–2571 (1997).

  26. 26.

    Han, Q., Dang, H. T. & Millis, A. J. Ferromagnetism and correlation strength in cubic barium ruthenate in comparison to strontium and calcium ruthenate: A dynamical mean-field study. Phys. Rev. B 93, 155103 (2016).

  27. 27.

    Jeong, D. W. et al. Temperature evolution of itinerant ferromagnetism in SrRuO3 probed by optical spectroscopy. Phys. Rev. Lett. 110, 247202 (2013).

  28. 28.

    Mackenzie, A. P. & Maeno, Y. The superconductivity of Sr2RuO4 and the physics of spin-triplet pairing. Rev. Mod. Phys. 75, 657–712 (2003).

  29. 29.

    Carlo, J. P. et al. New magnetic phase diagram of (Sr, Ca)2RuO4. Nat. Mater. 11, 323–328 (2012).

  30. 30.

    Zayak, A. T., Huang, X., Neaton, J. B. & Rabe, K. M. Structural, electronic, and magnetic properties of SrRuO3 under epitaxial strain. Phys. Rev. B 74, 094104 (2006).

  31. 31.

    Zayak, A. T., Huang, X., Neaton, J. B. & Rabe, K. M. Manipulating magnetic properties of SrRuO3 and CaRuO3 with epitaxial and uniaxial strains. Phys. Rev. B 77, 214410 (2008).

  32. 32.

    Dirsyte, R. et al. Impact of epitaxial strain on the ferromagnetic transition temperature of SrRuO3 thin films. Thin Solid Films 519, 6264–6268 (2011).

  33. 33.

    Anwar, M. S. et al. Ferromagnetic SrRuO3 thin-film deposition on a spin-triplet superconductor Sr2RuO4 with a highly conducting interface. Appl. Phys. Express 8, 015502 (2015).

  34. 34.

    Marzari, N., Mostofi, A. A., Yates, J. R., Souza, I. & Vanderbilt, D. Maximally localized Wannier functions: Theory and applications. Rev. Mod. Phys. 84, 1419–1475 (2012).

  35. 35.

    Mostofi, A. A. et al. An updated version of wannier90: A tool for obtaining maximally-localised Wannier functions. Comput. Phys. Commun. 185, 2309–2310 (2014).

  36. 36.

    Liebsch, A. & Ishida, H. Subband filling and mott transition in Ca2−x Sr x RuO4. Phys. Rev. Lett. 98, 216403 (2007).

  37. 37.

    Yoshimatsu, K. et al. Dimensional-crossover-driven metal-insulator transition in SrVO3 ultrathin films. Phys. Rev. Lett. 104, 147601 (2010).

  38. 38.

    Zhong, Z. et al. Electronics with correlated oxides: SrVO3/SrTiO3 as a mott transistor. Phys. Rev. lett. 114, 246401 (2015).

  39. 39.

    Poteryaev, A. I. et al. Enhanced crystal-field splitting and orbital-selective coherence induced by strong correlations in V2O3. Phys. Rev. B 76, 085127 (2007).

  40. 40.

    Tomczak, J. M., van Schilfgaarde, M. & Kotliar, G. Many-body effects in iron pnictides and chalcogenides: Nonlocal versus dynamic origin of effective masses. Phys. Rev. Lett. 109, 237010 (2012).

  41. 41.

    Han, M. J., Kino, H. & Kotani, T. Quasiparticle self-consistent GW study of LaNiO3 and LaNiO3/LaAlO3 superlattice. Phys. Rev. B 90, 035127 (2014).

  42. 42.

    Jang, S. W., Kotani, T., Kino, H., Kuroki, K. & Han, M. J. Quasiparticle self-consistent GW study of cuprates: electronic structure, model parameters, and the two-band theory for Tc. Sci. Rep. 5, 12050 (2015).

  43. 43.

    Ryee, S., Jang, S. W., Kino, H., Kotani, T. & Han, M. J. Quasiparticle self-consistent GW calculation of Sr2RuO4 and SrRuO3. Phys. Rev. B 93, 075125 (2016).

  44. 44.

    Dudarev, S. L., Botton, G. A., Savrasov, S. Y., Humphreys, C. J. & Sutton, A. P. Electron-energy-loss spectra and the structural stability of nickel oxide: An LSDA + U study. Phys. Rev. B 57, 1505–1509 (1998).

  45. 45.

    Takizawa, M. et al. Manifestation of correlation effects in the photoemission spectra of Ca1−x Sr x RuO3. Phys. Rev. B 72, 060404 (2005).

  46. 46.

    Leonov, I., Anisimov, V. I. & Vollhardt, D. First-principles calculation of atomic forces and structural distortions in strongly correlated materials. Phys. Rev. Lett. 112, 146401 (2014).

  47. 47.

    Park, H., Millis, A. J. & Marianetti, C. A. Computing total energies in complex materials using charge self-consistent DFT + DMFT. Phys. Rev. B 90, 235103 (2014).

  48. 48.

    Haule, K. & Birol, T. Free energy from stationary implementation of the DFT + DMFT functional. Phys. Rev. Lett. 115, 256402 (2015).

  49. 49.

    Asada, T. & Terakura, K. Cohesive properties of iron obtained by use of the generalized gradient approximation. Phys. Rev. B 46, 13599–13602 (1992).

  50. 50.

    Aguayo, A., Mazin, I. I. & Singh, D. J. Why Ni3Al is an itinerant ferromagnet but Ni3Ga is not. Phys. Rev. Lett. 92, 147201 (2004).

  51. 51.

    Mazin, I. I., Johannes, M. D., Boeri, L., Koepernik, K. & Singh, D. J. Problems with reconciling density functional theory calculations with experiment in ferropnictides. Phys. Rev. B 78, 085104 (2008).

  52. 52.

    Ortenzi, L., Mazin, I. I., Blaha, P. & Boeri, L. Accounting for spin fluctuations beyond local spin density approximation in the density functional theory. Phys. Rev. B 86, 064437 (2012).

  53. 53.

    Moroni, E. G., Kresse, G., Hafner, J. & Furthmüller, J. Ultrasoft pseudopotentials applied to magnetic Fe, Co, and Ni: From atoms to solids. Phys. Rev. B 56, 15629–15646 (1997).

  54. 54.

    Perdew, J. P., Burke, K. & Ernzerhof, M. Generalized gradient approximation made simple. Phys. Rev. Lett. 77, 3865–3868 (1996).

  55. 55.

    Perdew, J. P. & Zunger, A. Self-interaction correction to density-functional approximations for many-electron systems. Phys. Rev. B 23, 5048–5079 (1981).

  56. 56.

    Takahashi, K. S., Kawasaki, M. & Tokura, Y. Interface ferromagnetism in oxide superlattices of CaMnO3/CaRuO3. Appl. Phys. Lett. 79, 1324–1326 (2001).

  57. 57.

    Grutter, A. J. et al. Interfacial ferromagnetism in LaNiO3/CaMnO3 superlattices. Phys. Rev. Lett. 111, 087202 (2013).

  58. 58.

    Li, L., Richter, C., Mannhart, J. & Ashoori, R. C. Coexistence of magnetic order and two-dimensional superconductivity at LaAlO3/SrTiO3 interfaces. Nat. Phys. 7, 762–766 (2011).

  59. 59.

    Bert, J. A. et al. Direct imaging of the coexistence of ferromagnetism and superconductivity at the LaAlO3/SrTiO3 interface. Nat. Phys. 7, 767–771 (2011).

  60. 60.

    Hoffman, J. et al. Charge transfer and interfacial magnetism in (LaNiO3) n /(LaMnO3)2 superlattices. Phys. Rev. B 88, 144411 (2013).

  61. 61.

    Blöchl, P. E. Projector augmented-wave method. Phys. Rev. B 50, 17953–17979 (1994).

  62. 62.

    Kresse, G. & Joubert, D. From ultrasoft pseudopotentials to the projector augmented-wave method. Phys. Rev. B 59, 1758–1775 (1999).

  63. 63.

    Ozaki, T. Variationally optimized atomic orbitals for large-scale electronic structures. Phys. Rev. B 67, 155108 (2003).

  64. 64.

    The electronic structure calculation package, ‘ecalj’. https://github.com/tkotani/ecalj.

  65. 65.

    Kotani, T., Kino, H. & Akai, H. Formulation of the augmented plane-wave and muffin-tin orbital method. J. Phys. Soc. Jpn. 84, 034702 (2015).

  66. 66.

    Blöchl, P. E., Jepsen, O. & Andersen, O. K. Improved tetrahedron method for brillouin-zone integrations. Phys. Rev. B 49, 16223–16233 (1994).

  67. 67.

    Jones, C. W., Battle, P. D., Lightfoot, P. & Harrison, W. T. A. The structure of SrRuO3 by time-of-flight neutron powder diffraction. Acta Crystallogr. Sec. C: Cryst. Struct. Commun. 45, 365–367 (1989).

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Acknowledgements

We thank T. Ozaki for useful discussion. We were supported by Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (2014R1A1A2057202). The computing resource is supported by National Institute of Supercomputing and Networking/Korea Institute of Science and Technology Information with supercomputing resources including technical support (KSC-2015-C2-011).

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Affiliations

  1. Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon, 305-701, Korea

    • Siheon Ryee
    •  & Myung Joon Han
  2. KAIST Institute for the NanoCentury, KAIST, Daejeon, 305-701, Korea

    • Myung Joon Han

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Contributions

S.R. performed the calculations under the supervision of M.J.H. Both authors analyzed the results and wrote the paper.

Competing Interests

The authors declare that they have no competing interests.

Corresponding author

Correspondence to Myung Joon Han.

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