Literature DB >> 29507211

Strain-induced high-temperature perovskite ferromagnetic insulator.

Dechao Meng1,2,3, Hongli Guo1,2,4,5, Zhangzhang Cui1,2,3,6, Chao Ma1,2, Jin Zhao1,2,4,5, Jiangbo Lu7, Hui Xu1,2,3, Zhicheng Wang1,2,3, Xiang Hu1,2,3, Zhengping Fu1,2, Ranran Peng1,2, Jinghua Guo6,8, Xiaofang Zhai9,2, Gail J Brown10, Randy Knize11, Yalin Lu9,2,3,10,11.   

Abstract

Ferromagnetic insulators are required for many new magnetic devices, such as dissipationless quantum-spintronic devices, magnetic tunneling junctions, etc. Ferromagnetic insulators with a high Curie temperature and a high-symmetry structure are critical integration with common single-crystalline oxide films or substrates. So far, the commonly used ferromagnetic insulators mostly possess low-symmetry structures associated with a poor growth quality and widespread properties. The few known high-symmetry materials either have extremely low Curie temperatures (≤16 K), or require chemical doping of an otherwise antiferromagnetic matrix. Here we present compelling evidence that the LaCoO3 single-crystalline thin film under tensile strain is a rare undoped perovskite ferromagnetic insulator with a remarkably high TC of up to 90 K. Both experiments and first-principles calculations demonstrate tensile-strain-induced ferromagnetism which does not exist in bulk LaCoO3 The ferromagnetism is strongest within a nearly stoichiometric structure, disappearing when the Co2+ defect concentration reaches about 10%. Significant impact of the research includes demonstration of a strain-induced high-temperature ferromagnetic insulator, successful elevation of the transition over the liquid-nitrogen temperature, and high potential for integration into large-area device fabrication processes.
Copyright © 2018 the Author(s). Published by PNAS.

Entities:  

Keywords:  X-ray absorption; defect; ferromagnetic insulator; pulsed-laser deposition; strain

Year:  2018        PMID: 29507211      PMCID: PMC5866535          DOI: 10.1073/pnas.1707817115

Source DB:  PubMed          Journal:  Proc Natl Acad Sci U S A        ISSN: 0027-8424            Impact factor:   11.205


The realization of a dopant-free ferromagnetic insulator (FMI) is critical to the fabrication of versatile spintronic devices due to the potential for dopants acting as undesirable inelastic scattering centers. In low-symmetry magnetic materials, an FMI may be realized through charge ordering in which magnetic ions occupy different atomic sites. Unfortunately, integrating such low-symmetry FMIs (1–4) into film devices presents significant challenges due to large lattice mismatch between the film and commonly used substrates, which almost universally possess high-symmetry structures. In high-symmetry structures, however, magnetic ions likely occupy identical crystallographic sites so that charge-ordering–stabilized FMI states are highly disfavored. Thus, undoped high-symmetry FMIs remain extremely rare (5–7). In fact, chemical doping has been always a prerequisite for making high-symmetry FMIs such as the colossal magnetoresistance oxides (8–12) and magnetic semiconductors (13, 14). The two well-known undoped high-symmetry FMIs, EuS and strained EuTiO3, exhibit low Curie temperatures of about 16 and 4 K, respectively (5, 7). Therefore, engineering an undoped, FMI with high symmetry and high transition temperature (TC) is highly desirable. Normally, realizing an FMI requires a nonzero energy cost (ΔE) associated with electron hopping from an occupied metal orbital to a nearby unoccupied metal orbital through the bridging ligand orbital, so that the “hops” remain virtual events (15–17). Recently, the diamagnetic perovskite LaCoO3 has been suggested as a possible high-symmetry FMI candidate due to the near-degeneracy of various spin states of the Co3+ ion, so that spin-state ordering may be readily achieved (18, 19). Such an ordering of the spin states, which may be induced through strain effects, was first theoretically proposed by Hsu et al. (20) and later by Demkov and coworkers (21) to explain the observed FM in the LaCoO3 thin films (22, 23). However, previously fabricated LaCoO3 thin films are susceptible to oxygen vacancy (Ov) ordering as observed in scanning transmission electron microscopy (STEM) studies (24–26). More recently, such Ov ordering was reported to be critical for the observed FM in nonstoichiometric LaCoO3−δ films (25, 26). Currently, the nature of the FMI state in LaCoO3 films remains unresolved, and the roles of strain and Ovs remains hotly debated. In addition to resolving these questions, it is critical to elucidate whether the LaCoO3 film can in fact yield an undoped, high-temperature FMI with the high symmetry which enables high-quality growth. In this work, we fabricated nearly stoichiometric LaCoO3 films through pulsed-laser deposition under a maximal oxygen pressure of 25 Pa, which resulted in layer-by-layer growth. Details of the sample information can be found in and . We also fabricated various LaCoO3 thin films in which the Co2+ concentration was systematically varied by tuning the oxygen pressure and film thickness. The latter increases the Co2+ defect density when the thickness is reduced below 10 unit cells (u.c.). Further experiments and first-principles calculations demonstrated that the film with minimal Co2+ under tensile strain exhibited the strongest FM state. The observed FM eventually disappears for Co2+ concentrations above ∼10%. These results indicate that LaCoO3 films under tensile strain may represent the unusual case of a high-symmetry undoped FMI with a TC above liquid nitrogen temperature. In Fig. 1, we show magnetization and resistivity vs. temperature measurements for a 30-u.c. LaCoO3 film grown under 25-Pa oxygen pressure on (001) SrTiO3 substrate. The FM transition for this film appears at about 85 K. The resistivity increases with decreasing temperature from 390 to 70 K. Below 70 K, the resistance is over the measurement limit. A high-angle annular dark-field (HAADF) image, shown in Fig. 1, was taken along the (010) direction by an aberration-corrected STEM. Long-range–ordered dark stripes associated with Co2+ state (25) or La–La elastic interactions (24) were not observed in either the present HAADF images or a variety of images taken in different areas and directions of the film, although we occasionally observed short, randomly distributed stripes in some areas (). Co and Ti L-edge electron energy-loss spectroscopy (EELS), shown in Fig. 1, reveals that the film–substrate interface is very sharp. Furthermore, the thickness oscillation fringes in the X-ray diffraction shown in Fig. 1 and the atomic force microscopy image in Fig. 1 both demonstrate the high quality of the fabricated LaCoO3 film.
Fig. 1.

FMI state in a nearly stoichiometric LaCoO3 film under tensile strain. (A) Temperature dependences of the magnetization and resistivity of a 30-u.c. LaCoO3 film grown on (001) SrTiO3 at p(O2) = 25 Pa. The magnetization was measured by a superconducting quantum interference device (SQUID) along the in-plane direction with a 500-Oe field after field cooling. (Inset) Schematic of the LaCoO3/SrTiO3 heterostructure. (B) Cross-section STEM-HAADF image of the film taken along the (010) direction. (C) Ti and Co layer-by-layer distributions across the interface measured by STEM-EELS. (D) Synchrotron XRD measurement of the (00L) peaks. (E) Atomically flat LaCoO3 surface with terraces measured by atomic force microscopy.

FMI state in a nearly stoichiometric LaCoO3 film under tensile strain. (A) Temperature dependences of the magnetization and resistivity of a 30-u.c. LaCoO3 film grown on (001) SrTiO3 at p(O2) = 25 Pa. The magnetization was measured by a superconducting quantum interference device (SQUID) along the in-plane direction with a 500-Oe field after field cooling. (Inset) Schematic of the LaCoO3/SrTiO3 heterostructure. (B) Cross-section STEM-HAADF image of the film taken along the (010) direction. (C) Ti and Co layer-by-layer distributions across the interface measured by STEM-EELS. (D) Synchrotron XRD measurement of the (00L) peaks. (E) Atomically flat LaCoO3 surface with terraces measured by atomic force microscopy. To further examine the nature of the observed FMI, we intentionally introduced controlled levels of oxygen vacancies into the film by reducing the oxygen growth pressure and by reducing the film thickness, yielding LaCoO3−δ films. The corresponding reductions in TC and magnetization are shown in Fig. 2. We found that reducing the oxygen pressure causes TC to decrease and a dramatic reduction occurs between 10 and 15 Pa. X-ray diffraction analyses in Fig. 2 show that by reducing the oxygen pressure the out-of-plane lattice constant increases dramatically, in agreement with a previous report (27). All films discussed in this paper are coherently strained to their substrates, either SrTiO3 or (LaAlO3)0.3(Sr2TaAlO6)0.7 (LSAT). We define an effective strain by εeff =1 − c/a. In Fig. 2 the effective strain was found to match the TC variation extremely well. Thus, reducing the oxygen pressure is associated with a reduction in TC and magnetization which we attribute to a reduction in the effective tensile strain and increased nonstoichiometry.
Fig. 2.

Suppressed FM in LaCoO3−δ films on SrTiO3 substrates with released effective strain or with nonstoichiometry. (A) Temperature dependence of magnetization in LaCoO3−δ films measured along the in-plane direction with a 500-Oe applied field after field cooling. (B) XRD scans of films grown with varied pressures. The fringes are total thickness oscillations indicating high-quality growth. (C) Dependences of TC and effective strain on the growth pressure. (D) XAS spectra of films with varied thicknesses. (E) XANES spectra of films with varied thicknesses alongside reference spectra of bulk samples. Reprinted with permission from ref. 32, copyright (2006) by the American Physical Society. (F) Thickness dependences of TC and Co valence measured by both XAS and XANES. (G) STEM-EELS oxygen K-edge spectra of three representative LaCoO3 films. (H) EELS oxygen K edge of the three different blocks, each about 10 u.c., in the 30-u.c. nearly stoichiometric film.

Suppressed FM in LaCoO3−δ films on SrTiO3 substrates with released effective strain or with nonstoichiometry. (A) Temperature dependence of magnetization in LaCoO3−δ films measured along the in-plane direction with a 500-Oe applied field after field cooling. (B) XRD scans of films grown with varied pressures. The fringes are total thickness oscillations indicating high-quality growth. (C) Dependences of TC and effective strain on the growth pressure. (D) XAS spectra of films with varied thicknesses. (E) XANES spectra of films with varied thicknesses alongside reference spectra of bulk samples. Reprinted with permission from ref. 32, copyright (2006) by the American Physical Society. (F) Thickness dependences of TC and Co valence measured by both XAS and XANES. (G) STEM-EELS oxygen K-edge spectra of three representative LaCoO3 films. (H) EELS oxygen K edge of the three different blocks, each about 10 u.c., in the 30-u.c. nearly stoichiometric film. Reducing the film thickness (at a constant growth pressure of 15 Pa) allows the TC to be tuned more systematically while the effective strain remains relatively constant at ∼3.5% in thicker films and ∼3.3% in the 5-u.c. film. To probe the Co valence, we measured the Co L-edge and K-edge using soft X-ray absorption (XAS) and X-ray absorption near-edge structure (XANES) as shown in Fig. 2 , respectively. In a LaCoO3 film under tensile strain, Co3+ ions may exist in either the low-spin t2g6eg0 state (LS, S = 0) or the high-spin t2g4eg2 state (HS, S = 2) (19). The introduction of Ovs, however, could stabilize Co2+ HS states (S = 1.5) with an orbital occupancy of t2g5eg2 (26, 28, 29). Quantitative XAS spectral analysis using atomic multiplet plus the crystalline-field calculation (30, 31) was performed to extract the individual concentrations of the three spin states (more details in ). Additionally, the Co valence was quantitatively analyzed by comparing the measured XANES spectra to the reference spectra with a well-determined Co valence in a pseudocubic structure (32). The dependences of TC and Co valence (both from the XAS and XANES) on the layer thickness are shown in Fig. 2. Both decrease drastically as the thickness is reduced below 10 u.c. The coincidence of TC and Co valence transitions suggests that the introduced nonstoichiometry suppresses the FM. Since the oxygen K edge is very sensitive to changes in the valence of the transition metal, we performed its STEM-EELS measurements to double check the Co valence obtained from XAS and XANES. We studied three representative samples on SrTiO3 substrates (more details in ), including a thick film (30 u.c., 25 Pa), a thin film (7 u.c., 15 Pa), and a poorly oxygenated thick film (30 u.c., 1 Pa). The average oxygen K-edge spectra in Fig. 2 show that the 7-u.c. film exhibits a very weak preedge peak likely due to rich concentrations of Ov. From the line-by-line scans in the well-oxygenated 30-u.c. film, we do not observe clear trends of this prepeak weakening as the layer approaches the interface. To improve the signal quality and enable better comparison, we average the spectra of the top 10 layers, middle 10 layers, and interfacial 10 layers of the 30-u.c. films. We observe that the middle block has a slightly stronger prepeak than the surface and interfacial blocks, as shown in Fig. 2. To better understand the interplay between strain, off-stoichiometry, and FM in LaCoO3 we performed first-principles density-functional theory (DFT) calculations, the details of which are shown in . Consistent with previous investigations, the ground state of the strained LaCoO3 is FM for a = 3.905 Å due to the high concentrations of HS Co3+ and FM coupling between the nearest HS and LS Co3+ (20, 21). Our calculations show that the FM in LaCoO3 will indeed be suppressed by increasing the Ov density. Such Ovs introduce extra electrons which generate HS Co2+ atoms containing half-occupied e orbitals which support antiferromagnetic (AFM) superexchange between half-occupied orbitals, which decreases the magnetization. LaCoO3 films with three different Ov concentrations were investigated using (1Ov/32Co), (1Ov/16Co), and (1Ov/8Co) u.c. (Fig. 3). Stoichiometric LaCoO3 without Ov was also explored using three structural models discussed above, all yielding similar results. One can see that when the concentration is only 1Ov/32Co (9.4% Co2+), the magnetization only decreases slightly from 2 μB/Co to 1.6 μB/Co. This is because the AFM coupled HS Co2+ atoms only affect the local magnetic state. When the concentration increases to 1Ov/16Co (12.5% Co2+), the magnetization decreases dramatically to 0.2 μB/Co as the two Co2+ atoms introduce a long-range AFM coupling into the u.c. (more details in ). For an even higher concentration of 1Ov/8Co (25% Co2+), the magnetization is close to zero. This behavior may be well described by a step function with an inflection point near a Co2+ concentration of 10%, in excellent agreement with our experimental results. The Ov-ordered LaCoO3−δ thin films have been studied by Biškup et al. (25). Here we studied films with Ov concentrations much less than that of the previous work. Although details did not agree, both studies showed fewer magnetizations in Ov-occupied films than Ov-free films.
Fig. 3.

Theoretically calculated magnetizations of the tensile-strained LaCoO3-δ films with increased Ov concentrations. The three atomic pictures from left to right show the DFT calculated spin-state distribution in tensile-strained LaCoO3−δ films of 1Ov/32Co, 1Ov/16Co, and 1Ov/8Co, respectively. The atoms without density isosurface (blue colored) are LS Co3+. The rest are HS Co3+ and HS Co2+. The cyan- and yellow-colored isosurfaces have opposite spin directions.

Theoretically calculated magnetizations of the tensile-strained LaCoO3-δ films with increased Ov concentrations. The three atomic pictures from left to right show the DFT calculated spin-state distribution in tensile-strained LaCoO3−δ films of 1Ov/32Co, 1Ov/16Co, and 1Ov/8Co, respectively. The atoms without density isosurface (blue colored) are LS Co3+. The rest are HS Co3+ and HS Co2+. The cyan- and yellow-colored isosurfaces have opposite spin directions. In addition to the studies of films on SrTiO3 described above, we have performed similar experiments using LaCoO3 films grown on (001) LSAT substrates with varied thicknesses, and found similar results. In Fig. 4, we summarize the TC of all three thin-film groups, in addition to examples of films in the literature (23, 24, 26), as a function of effective strain and Co valence to create a phase diagram. Higher TCs are associated with the phase region with tensile strain and the lowest Ov concentrations. Away from this region, TC is sharply reduced or the films are nonmagnetic. The universality and substrate-independent reproducibility of these trends supports the validity and generality of this study. Therefore, the experimental findings strongly suggest that tensile strain of nearly stoichiometric LaCoO3 thin film results in a high-temperature FMI.
Fig. 4.

Phase diagram of the FM TC. The TC, effective strain εeff, and Co valence are all from experimental results. In the white-colored region, TC is below 30 K and is difficult to be quantified due to the paramagnetic background in SQUID measurements. Open circles, triangles, and squares with dots inside represent the three series of samples fabricated in this study (). The p series refer to the varying pressure films on SrTiO3. m and n series refer to the varying thickness films on SrTiO3 and LSAT, respectively. Solid-color symbols represent films from the literature (23, 24, 26).

Phase diagram of the FM TC. The TC, effective strain εeff, and Co valence are all from experimental results. In the white-colored region, TC is below 30 K and is difficult to be quantified due to the paramagnetic background in SQUID measurements. Open circles, triangles, and squares with dots inside represent the three series of samples fabricated in this study (). The p series refer to the varying pressure films on SrTiO3. m and n series refer to the varying thickness films on SrTiO3 and LSAT, respectively. Solid-color symbols represent films from the literature (23, 24, 26). Relative to other examples of undoped high-symmetry FMIs, the LaCoO3 Curie temperature is surprisingly high. A detailed understanding of this behavior is not yet clear and will require further exploration. One possible explanation is the larger overlap between the Co 3d and oxygen 2p orbitals. In other FMIs such as EuS, the FM originates in localized 4f electrons at the Eu sites and their orbital overlapping with the S 2p orbital or Eu 5d orbital (33, 34). On the other hand, our theoretical calculations show that the Co 3d orbital is much broader than the Eu 4f orbital and the superexchange interaction in LaCoO3 films (21) is more than one order magnitude larger than that in the Eu chalcogenides (34). The availability of an undoped high-symmetry and high-TC FMI is an important step toward bringing quantum-spintronic devices into the practical operation regime. Our results here indicate that the tensile-strained LaCoO3 thin film is a much better technological candidate than previous low-temperature FMIs, thanks to the material’s high TC of nearly 90 K, its high cubic symmetry, and the ability to fabricate high-quality films over large areas on conventional substrates. The realization of such an FMI provides a solid foundation for the growth and design for next-generation device fabrication.

Materials and Methods

Sample Fabrication Using High-Pressure Reflective High-Energy Electron Diffraction Assisted Pulsed-Laser Deposition.

Three groups of (001) LaCoO3 thin films (summarized in ) were grown using a Pascal pulsed-laser deposition system assisted with double-differential pumped reflective high energy electron diffraction (RHEED). The SrTiO3 substrates were etched in buffered hydrofluoric acid and annealed at 930 °C in flowing oxygen to obtain the uniform TiO2 termination. All films were grown at 750 °C. The laser energy density was about 1.5 J/cm2 and the frequency was 1 Hz. The thickness of LaCoO3 films was precisely controlled by in situ RHEED oscillations, and later confirmed by ex situ X-ray reflectivity measurements. The lattice structures of films were measured by Synchrotron X-ray diffraction (XRD), carried out on BL14B1 (10 keV) at Shanghai Synchrotron Radiation Facility, 1W1A (10 keV) at Beijing Synchrotron Radiation Facility and 33-BM-C (22 keV) at Advanced Photon Source in Argonne National Laboratory.

XAS and XANES.

Co L-edge XAS measurements were performed on BL6.3.1.2 at the Advanced Light Source of Lawrence Berkeley National Laboratory and BL12B-a at the National Synchrotron Radiation Laboratory of University of Science and Technology of China (USTC). XAS spectra were recorded in the total electron yield (TEY) and total fluorescence yield (TFY) mode simultaneously. The intensities were normalized to a reference signal recorded simultaneously on a gold mesh. The energy scale was calibrated by using metallic Co foil as reference. For the XAS TEY method, the penetration depth in the LaCoO3 film was between 10 and 20 u.c. The measurements of Co K-edge XANES spectroscopy were carried out at room temperature at the beamline BL14W1 of the Shanghai Synchrotron Radiation Facility and 1W1B-XAFS of Beijing Synchrotron Radiation Facility. The signals were collected in the TFY mode at 45° with respect to the X-ray incident beam direction. Standard cobalt and iron metal foils were employed for energy calibration and fluorescence filtering, respectively. Each spectrum was collected at least three times to minimize the error.

First-Principles DFT Calculation.

The electronic and magnetic properties of LaCoO3 films on SrTiO3 substrates with different amount of Ov were elucidated using first-principles DFT calculations, as implemented in Vienna Ab initio Simulation Package (VASP). The ion–electron interactions are described by the projector-augmented wave method. We use the generalized gradient approximation (GGA) with PW91 functional. Static local electronic correlations are added to the GGA exchange-correlation potential in the GGA+U method with U = 5.27 eV and J = 1.47 eV (Co3) as Seo et al. (21) did. In our calculations, all of the atomic positions are relaxed until the force on each atom is less than 0.01 eV/Å, and all of the self-consistent electronic calculations are converged to 10−6 eV per cell. To study the Ov effect on the magnetic solution in LaCoO3 film on SrTiO3, , , and supercells were used by introducing one Ov per supercell. We used the experimental lattice constant of SrTiO3 a = 3.905 Å to fix the in-plane lattice constant of the LaCoO3 film. With this lattice constant, a 3.5% tensile strain is applied to the LaCoO3 film.

STEM.

Specimens for STEM characterization were prepared by focused ion beam along the pseudocubic (010) direction of films on SrTiO3 substrates. Specimens along (100, 110, 1-10) directions of the 30-u.c film on SrTiO3 substrate grown with P(O2) = 25 Pa were also measured which are also absent of long-range Ov order. Spherical-aberration–corrected HAADF images were acquired on a JEOL ARM200F microscope operating at 200 kV. For HAADF images, the convergence angle was about 23 mrad, and the inner and outer angles of the detectors was 90 and 370 mrad, respectively. The experimental STEM images were low-pass filtered. The intensity of every atomic column in the HAADF images was approximately proportional to Z1.7 (Z is the atomic number).
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