Magnetic anisotropy of the van der Waals ferromagnet Cr2Ge2Te6 studied by angular-dependent XMCD
Abstract
The van der Waals ferromagnet Cr2Ge2Te6 (CGT) has a two-dimensional crystal structure where each layer is stacked through van der Waals force. We have investigated the nature of the ferromagnetism and the weak perpendicular magnetic anisotropy (PMA) of CGT by means of X-ray absorption spectroscopy and X-ray magnetic circular dichroism (XMCD) studies of CGT single crystals. The XMCD spectra at the Cr edge for different magnetic field directions were analyzed on the basis of the cluster-model multiplet calculation. The Cr valence is confirmed to be 3+ and the orbital magnetic moment is found to be nearly quenched, as expected for the high-spin 3 configuration of the Cr3+ ion. A large ( eV) trigonal crystal-field splitting of the level caused by the distortion of the CrTe6 octahedron has been revealed, while the single-ion anisotropy (SIA) of the Cr atom is found to have a sign opposite to the observed PMA and too weak compared to the reported anisotropy energy. The present result suggests that anisotropic exchange coupling between the Cr atoms through the ligand Te orbitals having strong spin-orbit coupling has to be invoked to explain the weak PMA of CGT, as in the case of the strong PMA of CrI3.
I Introduction
The discovery of graphene has invoked renewed interest in the studies on two-dimensional (2D) materials including layered transition-metal chalcogenides graphene_first ; review_2 ; review_3 ; TMD_review . The 2D materials show various fascinating properties that may lead to applications for new spintronics devices. In addition, the relation between dimensionality and various physical properties has long been a major subject from a fundamental point of view. For instance, the Mermin-Wagner theorem states that a long-range magnetic order in the 2D isotropic Heisenberg model cannot be realized at finite temperature due to long-range magnetic fluctuations Mermin . Recently, van der Waals (vdW) ferromagnets, which have 2D crystal structures but show ferromagnetic order vdWFerro_review , such as Cr2Ge2Te6 (CGT) CGT_oldcalc_prop ; CGT_oldcalc_2 ; CGT_tricritical_exp ; CGT_aniso_exp ; CGT_MH_MT ; CGT_bilayer ; CGT_hydropressure ; CGT_thinfilm_mag ; ARPES1 ; ARPES2 ; EM_19_Kang and CrI3 CrI3_mono ; CrI3_giant have attracted great interest. Although the magnetism of a few to several-monolayer CGT shows soft behaviors well described by the 2D Heisenberg model CGT_bilayer , the finite Curie temperature of 61 K CGT_aniso_exp ; CGT_oldcalc_prop ; CGT_tricritical_exp and the easy magnetization axis along the -axis (out-of-plane) direction CGT_aniso_exp ; CGT_oldcalc_prop ; CGT_MH_MT indicate a finite perpendicular magnetic anisotropy (PMA) and hence a departure from the 2D Heisenberg model. On the other hand, CrI3 exhibits ferromagnetism down to monolayer thickness, which suggests a stronger PMA than CGT and is well described by the 2D Ising model CrI3_mono .
The magnetic anisotropy of a 2D ferromagnet arises primarily from (i) the single-ion anisotropy (SIA) of the magnetic ion and (ii) anisotropic exchange interaction between the magnetic ions in the 2D layer. The SIA of the Cr-based vdW ferromagnets is considered to be small because of the 3 configuration of the Cr3+ ion, which has no orbital degree of freedom, as discussed, e.g., by Lado and Fernández-Rossi CrI3_aniso_calc . On the contrary, first-principles estimates of exchange coupling by Xu et al. CrI3 Kitaev vs SIA have shown that the SIA and Kitaev-type anisotropic magnetic coupling in the Cr-based vdW ferromagnets are of comparable magnitudes and compete with each other. Furthermore, Kim et al. PRL_19_Kim have performed multi-site cluster-model multiplet calculation and attributed the strong PMA of CrI3 to anisotropic exchange coupling between Cr atoms through the iodine ligand orbitals, which has strong spin-orbit coupling (SOC). In fact, X-ray magnetic circular dichroism (XMCD) measurements at the iodine edge of CrI3 have revealed a finite orbital magnetic moment of the I electrons, implying the importance of the ligand orbitals in the PMA of the vdW ferromagnets Choi I XMCD . As for CGT, which shows a weaker PMA than CrI3, the situation is complicated and it is far from clear which of the SIA or the anisotropic exchange is responsible for the PMA PRL_19_Kim ; PCCP_19_Wang .
In order to evaluate the contribution of the SIA of Cr to the magnetic anisotropy, XMCD studies at the Cr edge are expected to give essential information. So far Cr -edge XMCD has been reported for CGT Fumega XMCD and CrI3 Frisk_XMCD with line-shape analysis using cluster-model calculation, but no information about the contributions of the Cr electrons to the PMA has been explored. In the present work, we have carried out Cr -edge XMCD measurements of CGT single crystal under magnetic fields applied to different crystallographic directions and subsequent cluster-model multiplet calculation to estimate the SIA energy of the Cr atom centered in the CrTe6 octahedron.
II methods
Single crystals of CGT were synthesized using a flux method. High purity Cr, Ge and Te powders were mixed in a molar ratio of 2:6:36; the extra Ge and Te were used as a flux. The mixture was loaded in an alumina crucible and sealed in an evacuated quartz tube. A ball of alumina fiber was placed on top of the crucible. The quartz tube was placed in a furnace, heated to 700 ∘C, held for 5 hours, and then slowly cooled down to 480 ∘C over a period of 3 days. This was followed by centrifugation to remove the flux.
X-ray absorption spectroscopy (XAS) and XMCD measurements at the Cr edge were performed at beam line BL23SU of SPring-8 and beam line BL-16A of Photon Factory at High Energy Accelerator Research Organization (KEK-PF). The measurement at SPring-8 was performed under a magnetic field of T parallel to the -axis of the sample. The XAS and XMCD spectra were recorded in the total electron yield mode. Right- () and left () circularly polarized x-rays were switched at a frequency of 1 Hz in order to eliminate time-dependent background from the obtained XMCD spectra. The sample temperature () during the measurement was set to 20 K, well below the Curie temperature. The sample was cleaved in the vacuum chamber prior to the measurements to obtain fresh surfaces. Magnetic-field-direction dependence of XMCD spectra was measured at the BL-16A of KEK-PF. Polarization switching was made at a frequency of 10 Hz. Magnetic field of T was applied parallel and perpendicular to the -axis. Signals were recorded in the total electron-yield mode.
To investigate the electronic structure which contributes to the ferromagnetism, configuration-interaction cluster-model multiplet calculations have been conducted. Figure 1(a) shows the crystal structure of CGT. Each Cr atom is surrounded by six Te atoms, forming a CrTe6 cluster. It constitutes the CrGeTe3 layer, which are stacked through vdW force. The CrTe6 cluster is slightly elongated along the -axis CGT_oldcalc_prop , as shown in Fig. 1(b), which means that the Cr electrons are under a nearly octahedral, trigonally distorted crystal field. The following parameters of the cluster model are used to reproduce the experimental XMCD spectra: the Cr 3-3 Coulomb energy , the Cr 2-3 Coulomb energy , the charge-transfer energy from the Te 5 to Cr 3 levels, the Slater-Koster parameter () between the Cr 3 and Te 5 orbitals, the crystal-field splitting 10 ( eV) between the Cr and levels (apart from the - covalency contribution), and the trigonal crystal-field splitting between the and orbitals. [For the definition of 10 and , see Fig. 1(c).] As for the parameter values, we follow the empirical relationship fujimori_para and employ eV, eV, and eV as being relevant to Cr3+ tellurides. The SOC parameter of the Cr orbital is taken to be 35 meV.
III results and discussion
Figure 2 shows Cr -edge XAS and XMCD spectra of CGT under the out-of-plane magnetic field of 3 T at = 20 K. The applied magnetic field was high enough to saturate the magnetization of CGT because the magnetization saturates below T CGT_tricritical_exp . The tail of the Te XAS peak overlapping the Cr XAS spectrum has been subtracted assuming a hyperbola. Arctangent steps at the and edges have also been subtracted from the Cr XAS as usual. On the other hand, the XMCD signals predominantly come from the magnetic Cr atoms, and there is no need to subtract signals from the Te atoms.
Figure 3 shows comparison of the measured Cr XMCD spectrum with those calculated using the cluster model assuming the Cr valences of 4+, 3+, 2+ high-spin states, and 2+ low-spin states. The experimental spectrum shows three negative peaks and one positive peak at the edge, and one negative peak and two positive peaks at the edge. The comparison shows that the calculation for the Cr3+ state reproduces the experimental spectrum better than those for the Cr2+ and Cr4+ states. Thus, one can conclude that the Cr atom in CGT is in the state (with the high-spin configuration), and not in the nor state.
III.1 Spin and orbital magnetic moments
The orbital and effective spin magnetic moments are quantitatively estimated from the XAS and XMCD spectra using the XMCD sum rules Carra ; Thole . For the edge ( transition), the sum rules are given by:
where () is an XAS spectrum taken with (), , and are the orbital magnetic moment, spin magnetic moment, and magnetic dipole moment, respectively, in units of Bohr magneton /Cr atom. () stands for the absorption coefficient for photon helicity parallel (antiparallel) to the Cr majority spin direction. is the number of holes in the valence shell. By applying the sum rules to the spectra in Fig. 2, the orbital magnetic moment of /Cr atoms has been obtained, consistent with the quenched orbital magnetic moment in the configuration of Cr3+. The effective spin magnetic moment of /Cr atom has been obtained, where the and are the spin magnetic moment and the magnetic dipole moment, respectively. In a high-symmetry environment of the Cr atom as in CGT, is negligibly small compared to dipole_1 ; dipole_2 . Therefore, since is nearly zero, we regard as the total magnetic moment . The value is consistent with that of the reported saturation magnetization of CGT, 2.2 - 2.9 /Cr atom CGT_MH_MT ; CGT_aniso_exp ; CGT_oldcalc_prop .
III.2 Crystal-field splitting
In order to study the anisotropies of the electronic and magnetic properties of CGT, XMCD measurements under different magnetic field directions have been made. Figure 4 shows the Cr XAS and XMCD spectra taken with magnetic fields applied to the out-of-plane (-axis) and in-plane (-plane) directions. The XMCD spectra show small but clear differences between the different magnetic-field directions, while the spectral line shapes of the XAS spectra are relatively insensitive to the field direction. To identify the origin of the spectral differences between the different field directions, cluster-model multiplet calculations have been conducted assuming the Cr valence to be 3+. The effects of the elongation of the CrTe6 octahedron along the -axis CGT_oldcalc_prop are taken into account as a trigonal crystal-field splitting of the level as shown in Fig. 1(c), where the triply-degenerate level is split into the non-degenerate and doubly-degenerate levels. Here, for a positive (negative) trigonal crystal field , the level is located above (below) the level. Figures 5(b) and (c) show the calculated spectra without and with the trigonal crystal field, respectively, compared with experiment [Fig. 5(a)]. Without the trigonal crystal field, i.e., [Fig. 5(b)], there is no difference in the XMCD spectra between the out-of-plain and in-plane magnetic fields. On the other hand, the calculated XMCD spectra under the trigonal crystal field of 0.2 eV show finite differences between the out-of-plain and in-plane magnetic fields, as shown in Fig. 5(c), and well explain the experiment [Fig. 5(a)]. Thus we conclude that the differences in the XMCD spectra taken with the different magnetic-field directions are attributed to the elongation of the CrTe6 octahedron along the -axis.
III.3 Magnetic anisotropy energies
To evaluate the SIA of the Cr ion, the ground-state energy of the cluster is calculated using the cluster model for the different magnetic field directions. Thus we find that the energy for the in-plane magnetic field is lower than the energy for the out-of-plane magnetic field by eV/Cr atom, that is, the Cr atom has the easy magnetization axis in the -plane. This is opposite to the observed PMA of CGT and furthermore its magnitude is 1-2 orders of magnitude smaller than the experimental value of eV/Cr atom CGT_aniso_exp ; CGT_bilayer as well as the first-principles-theoretical value of SIA, eV/Cr atom EM_19_Kang . The present result, on the other hand, agrees with the first-principles calculation by Wang et al. PCCP_19_Wang in that the SIA of Cr is weak and acts against PMA.
In spite of the large trigonal crystal field eV and the resulting anisotropy in the XMCD spectra, the calculated magnetic anisotropy energy is small because of the high-spin configuration, which has no orbital degree of freedom. Therefore, we consider that effects beyond the SIA evaluated using the cluster model, where only the spin-orbit coupling of the Co electrons are taken into account, may play important roles in realizing the PMA of CGT. Such effects would include anisotropic exchange coupling between Cr ions through the ligand Te electrons with strong SOC, in analogy to CrI3. In the case of CrI3, which has a stronger PMA than CGT, density functional theory (DFT) calculation CrI3_structure_info ; CrI3_aniso_calc and multi-Cr site cluster-model multiplet calculation PRL_19_Kim have clearly shown that exchange coupling between Cr ions through I orbitals explains the stronger PMA of CrI3.
In addition to the SIA of Cr and anisotropic exchange between Cr discussed above, the magnetic anisotropy of the Te electrons themselves may contribute to the magnetic anisotropy of CGT PCCP_19_Wang . Such an anisotropy could arise because the Te electrons are partially spin-polarized due to hybridization with the Cr electrons, in analogy to the magnetic anisotropy of the Pt electrons in -type FePt FePt_Solovyev ; FePt_Ikeda . In order to address this issue, further theoretical and experimental (XMCD at the Te absorption edges) studies would be necessary.
IV conclusion
We have performed XAS and XMCD measurements at the Cr edge and subsequent cluster-model calculation on CGT to investigate the electronic structure which contributes to the ferromagnetism and magnetic anisotropy. The effective spin magnetic moment obtained using the sum rules is 2.2 , consistent with previous reports, while the orbital magnetic moment is nearly zero. Subtle changes of the XMCD spectra are observed by changing the magnetic field direction, and are attributed to the distortion of the CrTe6 octahedron from comparison with cluster-model calculation including the trigonal crystal field of the cluster elongated along the axis. The magnetic anisotropy energy calculated using the cluster model is too small and has an opposite sign compared to experiment. This implies that the magnetic anisotropy of CGT cannot be explained by the SIA of Cr described by the cluster model, and that one has to take into account interaction between Cr atoms through Te ligands which have strong SOC.
Acknowledgements.
We would like to thank I. Solovyev, D. Khomskii, S. Streltsov, and K. Kugel for enlightening discussion, and M. Suzuki-Sakamaki and K. Amemiya for valuable technical support at KEK-PF. This work was supported by a Grant-in-Aid for Scientific Research from JSPS (grant Nos. 15H02109 and and 19K03741), by Center for Spintronics Research Network (CSRN), the University of Tokyo, under Spintronics Research Network of Japan (Spin-RNJ), and by the Shared Use Program of Japan Atomic Energy Agency (JAEA) Facilities (Proposal No. 2018A-E24) supported by JAEA Advanced Characterization Nanotechnology Platform as a program of ”Nanotechnology Platform” of MEXT (Proposal No. A-18-AE-0019). The synchrotron experiment at KEK-PF was done under the approval of the Program Advisory Committee (Proposal Nos. 2016S2-005), and the experiment at SPring-8 was done at the JAEA beam line BL23SU (Proposal Nos. 2018A3841). The work at Rutgers University was funded by the Gordon and Betty Moore Foundation’s EPiQS Initiative through Grant GBMF4413 to the Rutgers Center for Emergent Materials.References
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