Chinese Physics Letters, 2022, Vol. 39, No. 5, Article code 057501Express Letter Neutron Spectroscopy Evidence for a Possible Magnetic-Field-Induced Gapless Quantum-Spin-Liquid Phase in a Kitaev Material $\alpha$-RuCl$_3$ Xiaoxue Zhao (赵晓雪)1†, Kejing Ran (冉柯静)2†, Jinghui Wang (王靖珲)2, Song Bao (鲍嵩)1, Yanyan Shangguan (上官艳艳)1, Zhentao Huang (黄振涛)1, Junbo Liao (廖俊波)1, Bo Zhang (张波)1, Shufan Cheng (承舒凡)1, Hao Xu (徐豪)1, Wei Wang (王巍)3, Zhao-Yang Dong (董召阳)4, Siqin Meng (孟思勤)5,6, Zhilun Lu (陆智伦)5,7, Shin-ichiro Yano8, Shun-Li Yu (于顺利)1,9*, Jian-Xin Li (李建新)1,9*, and Jinsheng Wen (温锦生)1,9* Affiliations 1National Laboratory of Solid State Microstructures and Department of Physics, Nanjing University, Nanjing 210093, China 2School of Physical Science and Technology and ShanghaiTech Laboratory for Topological Physics, ShanghaiTech University, Shanghai 200031, China 3School of Science, Nanjing University of Posts and Telecommunications, Nanjing 210023, China 4Department of Applied Physics, Nanjing University of Science and Technology, Nanjing 210094, China 5Helmholtz-Zentrum Berlin für Materialien und Energie GmbH, Hahn-Meitner-Platz 1D-14109 Berlin, Germany 6China Institute of Atomic Energy, Beijing 102413, China 7School of Engineering and the Built Environment, Edinburgh Napier University, Edinburgh EH10 5DT, United Kingdom 8National Synchrotron Radiation Research Center, Hsinchu 30077, China 9Collaborative Innovation Center of Advanced Microstructures, Nanjing University, Nanjing 210093, China Received 3 March 2022; accepted 2 April 2022; published online 5 April 2022 These authors contributed equally to the work.
*Corresponding authors. Email: slyu@nju.edu.cn; jxli@nju.edu.cn; jwen@nju.edu.cn
Citation Text: Zhao X X, Ran K J, Wang J H et al. 2022 Chin. Phys. Lett. 39 057501    Abstract As one of the most promising Kitaev quantum-spin-liquid (QSL) candidates, $\alpha$-RuCl$_3$ has received a great deal of attention. However, its ground state exhibits a long-range zigzag magnetic order, which defies the QSL phase. Nevertheless, the magnetic order is fragile and can be completely suppressed by applying an external magnetic field. Here, we explore the evolution of magnetic excitations of $\alpha$-RuCl$_3$ under an in-plane magnetic field, by carrying out inelastic neutron scattering measurements on high-quality single crystals. Under zero field, there exist spin-wave excitations near the $M$ point and a continuum near the $\varGamma$ point, which are believed to be associated with the zigzag magnetic order and fractional excitations of the Kitaev QSL state, respectively. By increasing the magnetic field, the spin-wave excitations gradually give way to the continuous excitations. On the verge of the critical field $\mu_0H_{\rm c}=7.5$ T, the former ones vanish and only the latter ones are left, indicating the emergence of a pure QSL state. By further increasing the field strength, the excitations near the $\varGamma$ point become more intense. By following the gap evolution of the excitations near the $\varGamma$ point, we are able to establish a phase diagram composed of three interesting phases, including a gapped zigzag order phase at low fields, possibly gapless QSL phase near $\mu_0H_{\rm c}$, and gapped partially polarized phase at high fields. These results demonstrate that an in-plane magnetic field can drive $\alpha$-RuCl$_3$ into a long-sought QSL state near the critical field.
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DOI:10.1088/0256-307X/39/5/057501 © 2022 Chinese Physics Society Article Text In the past few years, $\alpha$-RuCl$_3$ with the honeycomb structure has been studied extensively in the pursuit of Kitaev quantum spin liquids (QSLs), which result from the bond-dependent anisotropic Kitaev interactions,[1–4] different from the triangular-, kagome-, or pyrochlore-structured QSL candidates with geometrical frustration.[5,6] Now, it is well established that the ground state of $\alpha$-RuCl$_3$ is actually a zigzag ordered state.[7–11] However, taking advantages of the spatial anisotropy of the Ru$^{3+} d$ orbitals and the close-to-ideal bond configurations, it has been shown that there exists a large Kitaev interaction between the effective spin-1/2 moments.[12–17] Due to the presence of the Kitaev interaction, the zigzag order phase is in proximity to the Kitaev QSL phase,[10,18–20] although there also exist some non-Kitaev terms that make the system deviate from the QSL phase.[21–32] This provides the opportunity that by tuning the competing interactions, the zigzag magnetic order can be suppressed and a QSL state may be achieved.[33–41] In fact, there are accumulating reports that an external magnetic field applied within the honeycomb plane can suppress the magnetic order effectively and drive the system into a magnetically disordered state, utilizing various experimental probes, including magnetization,[9,42–45] specific heat,[42,43,46–54] neutron scattering,[9,45,46,55,56] nuclear magnetic resonance,[43,49,57,58] thermal conductivity and thermal Hall conductivity,[50,59–66] Raman, microwave, and terahertz spectroscopy,[67–72] magnetodielectric,[73] magnetic torque,[59] resonant torsion magnetometry,[74] electron spin resonance,[75,76] and thermal expansion and magnetostriction measurements.[77,78] Nevertheless, whether the disordered phase under field is the long-sought QSL phase,[50–53,55–68,72,74–79] and if it is, whether it is gapless or gapped,[43,46,49,55,57] remain hotly debated. Furthermore, there are also some controversies on whether the field divides the phase diagram into two parts, or three parts with a QSL phase intermediate between the low- and high-field phases.[43,46–51,53,55–65,74–79] In this Letter, we aim to solve these problems by carrying out inelastic neutron scattering (INS) measurements on the magnetic field evolution of the magnetic excitations with finer field step of 0.5 T, higher energy resolution of 0.15 meV, and stronger field strength up to 13 T, as compared to the previous INS works under fields.[55,56] Under zero field, the magnetic excitations are composed of the spin-wave excitations associated with the zigzag magnetic order,[10,15,80] and a continuum hypothesized to be the fractional excitations associated with the Kitaev QSL state,[10,18–20,81] which are around the $M$ and $\varGamma$ points, respectively. Under an external magnetic field applied within the $ab$ plane, the spin-wave excitations around the $M$ point are gradually suppressed and vanish around the critical field $\mu_0H_{\rm c}\approx7.5$ T, accompanying the suppression and disappearance of the zigzag magnetic order. On the other hand, the continuum near the $\varGamma$ point still persists when the spin waves vanish. These results are evident that the continuum around the $\varGamma$ point represents the fractional excitations associated with the QSL state, and the phase near $\mu_0H_{\rm c}$ is the QSL phase. By following the gap evolution of the continuum, we can divide the phase diagram into three phases, including the low-field gapped zigzag ordered state, intermediate possibly gapless QSL, and gapped partially polarized phase. Single crystals of $\alpha$-RuCl$_3$ were grown by the chemical vapor transport method using commercially purchased anhydrous $\alpha$-RuCl$_3$ powders.[15,81] The plate-like crystals are shiny and black with a typical size of 60 mg per piece. Magnetic susceptibility measurements were performed using the vibrating sample magnetometer option integrated in a physical property measurement system (PPMS-9T) from Quantum Design. The results showed that the sample had a single magnetic transition temperature. The specific heat measurements were also conducted on PPMS-9T. Neutron scattering measurements were conducted on two cold-neutron triple-axis spectrometers, FLEXX located at Helmholtz-Zentrum Berlin (HZB), and SIKA located at Australian Nuclear Science and Technology Organization (ANSTO),[82] both utilizing a fixed-final-energy mode with $E_{\rm f}=5.0$ meV under double-focusing conditions for both the monochromator and analyzer.
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Fig. 1. (a) Dependence of the magnetic transition temperature $T_{\rm N}$ as a function of the in-plane magnetic field $\mu_0H$ for $\alpha$-RuCl$_3$, obtained from the magnetization and specific heat data. The inset shows the schematic honeycomb crystal lattice of $\alpha$-RuCl$_3$ with the zigzag magnetic order. (b) Field dependence of the integrated intensities of the magnetic Bragg peak (0.5, 0, 1). The inset is a contour map showing the elastic scans through (0.5, 0, 1), under magnetic field applied along the [$-1$, 2, 0] direction with strength ranging from 0 to 9 T. Black solid curves through data are guides to the eyes. The errors represent one standard deviation throughout this study.
The energy resolutions for both instruments were $\sim $0.15 meV (full width at half maximum).  Two batches of samples, both weighed $\sim $2 g in total, were labeled as samples I and II. Sample I and II arrays consisted of 20 and 22 pieces of single crystal, respectively. The former was used for measurements on both FLEXX and SIKA, whilst the latter was only measured on SIKA.  They were coaligned using a backscattering Laue x-ray diffractometer and glued onto aluminum plates by hydrogen-free Cytop grease. These crystals were well aligned so that the overall mosaic spreads were both less than 3$^\circ$, as determined from the rocking scans through the (0, 0, 3) and (1, 0, 0) Bragg peaks. All measurements were carried out in the ($H,\,0,\,L$) plane with magnetic field applied along the [$-1$, 2, 0] direction. A hexagonal structure, with the routinely adopted lattice parameters $a=b=5.96$ Å, and $c=17.20$ Å, was used throughout this study. The wave vector $\boldsymbol{Q}$ was expressed as ($H,\,K,\,L$) in reciprocal lattice unit (r.l.u.) of $(a^{*}, b^{*}, c^{*}) = (4\pi/\sqrt3a, 4\pi/\sqrt3b, 2\pi/c)$.
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Fig. 2. (a) Constant-$\boldsymbol{Q}$ scans at the $M$ point (0.5, 0, 2) of the two-dimensional Brillouin zone, with applied field up to 13 T. (b) The same as (a) but at the Brillouin zone center $\varGamma$ point (0, 0, 2). (c) The scans similar to those in (b) but with finer field step of 0.5 T ranging from 7 to 8.5 T, around the critical field of 7.5 T. (d) Constant-$\boldsymbol{Q}$ scans at the $\varGamma$ point (0, 0, $L$) with different $L$'s under zero field. All measurements were performed on sample I at $T=1.8$ K. Here, (a) and (b) were both measured on FLEXX triple-axis spectrometer while (c) and (d) were measured on SIKA. Solid lines are guides to the eyes, and black dotted horizontal lines represent background signals.
From susceptibility and specific heat measurements on $\alpha$-RuCl$_3$, the relation between the magnetic transition temperature $T_{\rm N}$ and the applied in-plane magnetic field $\mu_0H$ is obtained, as presented in Fig. 1(a). It clearly shows that $T_{\rm N}$ decreases with increasing field, indicating that the magnetic order is weakened and disappears at $\mu_0H_{\rm c}=7.5$ T. The magnetic field dependence of the integrated intensities for the magnetic Bragg peak (0.5, 0, 1) by elastic neutron scattering measurements is plotted in Fig. 1(b). With the gradual increase of external field strength, the intensities of the Bragg peak are reduced correspondingly, also implying that the magnetic ordering is being suppressed and ultimately vanishes at around 7 T. These results are consistent with previous reports that an in-plane external field will suppress the magnetic order of $\alpha$-RuCl$_3$.[9,42–45] Based on some previous experiments,[10,15,20,80,81] the magnetic excitations are basically converged at the $M$ and $\varGamma$ points in the two-dimensional Brillouin zone. Specifically, the gapped sharp excitations around the $M$ point are the spin-wave excitations ascribed to the zigzag magnetic order, while the ones around the $\varGamma$ point exhibiting broad continuous characteristics are suggested to be the fractional magnetic excitations bestowed by the proximity to the Kitaev QSL state of $\alpha$-RuCl$_3$.[10,15,18,20,81] To observe the evolutions of these two types of excitations with respect to the applied field, we thus performed constant-$\boldsymbol{Q}$ scans at the $M$ point (0.5, 0, 2) and $\varGamma$ point (0, 0, 2). Some of the representative data are shown in Fig. 2. In Fig. 2(a), the excitations at the $M$ point are enhanced from 0 to 3 T, which may be due to the spectral weight transfer of the magnetic Bragg peak. As shown in Fig. 1(b), the peak intensity has a great drop from 0 to 3 T. With the field further increasing, the intensity is suppressed and almost vanishes at 7.5 T and above. As shown in Fig. 2(b), the excitations at the $\varGamma$ point are gradually suppressed with the field for $\mu_0H\le7.5$ T, similar to those at the $M$ point. More importantly, at 7.5 T, the peak feature of the excitations at the $\varGamma$ point disappears, resulting in a featureless continuous profile in energy expected for a QSL. At 9 and 13 T, the intensities become stronger, while there are no magnetic scattering intensities at the $M$ point for the field strength exceeding 7.5 T, indicating that the system enters a partially polarized state, in which the magnetic moments are forced to be partially aligned with field. Furthermore, by more detailed measurements around the critical field of 7.5 T, as shown in Fig. 2(c), we can find the peak feature of the excitations at the $\varGamma$ point reappears after 8 T. Overall, the featureless and continuous scan profiles at 7.5 and 8 T are quite distinct from others. At other fields, the scan reaches its background $\gtrsim$1 meV, below which the intensity rises due to the incoherent elastic scattering. On the other hand, the data points for 7.5 and 8 T are well above the background level at 1 meV, and remain finite when extended to zero energy. From these results, we can judge that the excitations are gapless at 7.5 and 8 T, but gapped at other fields, at least on a qualitative level. This issue will be discussed further in the latter part of this work. In most previous neutron scattering experiments on $\alpha$-RuCl$_3$, the $L$-dependence of the continuous excitations at the $\varGamma$ point is typically not taken into account, and the models are normally based on the two-dimensional magnetic structure, ignoring the interlayer interactions. In Ref. [56], it has been pointed out that the excitations at the $\varGamma$ point actually follow a cosine form, indicating a nonnegligible interlayer magnetic coupling. We have also measured the excitations at $M$ and $\varGamma$ points with different $L$'s. In Fig. 2(d), we show four representative scans at different $L$'s at zero field. The data show apparent $L$ dependence, consistent with Refs. [45,56]. Nevertheless, the evolution of the excitations with the field is similar for different $L$'s, as shown in the Supplementary Material.
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Fig. 3. Magnetic excitation spectra along the [100] direction under different magnetic fields. (a)–(c) Measured at 1.8 K. (d) Measured at 25 K. Data of (b) were obtained from SIKA, and the rest were from FLEXX. $H=0$ and 0.5 r.l.u. correspond to the high-symmetric $\varGamma$ and $M$ points, respectively. White cross dots mark experimental data points. In all the panels, left regions ($-0.5 < H < 0$ r.l.u.) are symmetrized from the right ($0 < H < 0.5$ r.l.u.) for better visualizing purpose. Note that according to the linear scans in Fig. 2, there are still finite intensities below 1.5 meV at the $\varGamma$ point at 7.5 T, so the data in (b) should not be misinterpreted as there is a gap below 1.5 meV.
To better visualize the evolutions of the magnetic excitations with the field, we have performed a series of energy scans at various $\boldsymbol{Q}$ values, and obtained the excitation spectra along the [100] direction under different field strengths at the base temperature as plotted in Fig. 3. For comparison, the spectra at 25 K, well above the $T_{\rm N}$, are also plotted. The data in Fig. 3(b) are from SIKA, and the rest are all from FLEXX. Since the measurements were carried out on similar instruments with the same sample I, the results are similar and comparable (see the Supplementary Material for more details). Figure 3(a) clearly shows that there are two types of excitations, on the one hand the spin wave excitations, with an energy gap around 1.6 meV, disperse upwards from the $M$ point ($H=\pm0.5$ r.l.u.), and reach the band top at the $\varGamma$ point; on the other hand at the $\varGamma$ point, there is another type of excitations. Although they seem to have a dispersion similar to the spin waves, they are shown to be incompatible with the spin waves but are a continuum representing the fractional excitations resulting from the QSL phase instead.[81] Intriguingly, as shown in Fig. 3(b), at the critical field of $\mu_0H_{\rm c}=7.5$ T, while the spin-wave excitations at the $M$ point completely disappear, the continuum at the $\varGamma$ point persists. This strongly indicates that the disordered phase at $\mu_0H_{\rm c}$ is the long-sought QSL phase featuring fractional excitations. Furthermore, the excitations appear to extend below 1 meV and become gapless. Compared Fig. 3(b) with the spectra in the paramagnetic phase shown in Fig. 3(d), while it is similar that the spin waves both disappear, and both feature a possibly gapless continuum, the two spectra show clear differences in their boundaries of the continua, suggesting that the field-induced possibly gapless QSL is distinct from the paramagnetic phase above $T_{\rm N}$. By further increasing the field up to 13 T, the spin waves at the $M$ point are still absent. On the other hand, the gap at the $\varGamma$ point reopens and becomes larger than that at zero field. Furthermore, the intensities of the excitations also become more intense. The gapped excitations dispersing from the $\varGamma$ point look like gapped ferromagnetic spin excitations. However, the excitations of a magnetic-field-driven partially polarized state may not be necessarily consistent with those of a ferromagnetic ground state under zero field, as the excitations are dependent on the Hamiltonians. For example, in our recent work on YbZnGaO$_4$, we have found that in the fully polarized state the excitations disperse from the $M$ point as expected for antiferromagnetic excitations, instead of from the $\varGamma$ point as expected for ferromagnetic excitations, because of the presence of dominant antiferromagnetic interactions in YbZnGaO$_4$ under zero field.[83] Returning to the case of $\alpha$-RuCl$_3$, we think that similar excitations of the partially polarized and ferromagnetic states indicate the presence of a dominant ferromagnetic Kitaev interaction, as suggested in previous works.[16,17,59,81] Summarizing the results in Figs. 2 and 3, and in Figs. S1 and S2 in the Supplementary Material, we can obtain a phase diagram of $\alpha$-RuCl$_3$ based on the gap size in Fig. 4. Here, we define the energy gap as the energy where the intensity starts to rise in the low-$E$ regime. According to the gap size, we can divide the phase diagram into three regions. The first one is the gapped zigzag ordered phase at low fields. The gap size is reduced with field, in concomitant with the suppression of the magnetic order with field as shown in Fig. 1. Around the critical field, there is a narrow regime featuring possibly gapless continuous excitations. From our measurements, we estimate the range to be about 0.5 T. By changing the way for the determination of the gap, the evolution of the gap size with the magnetic field away from the critical regime may be different, but the gapless nature at 7.5 and 8 T remains to be the same. As we show above, the magnetic order is completely suppressed here, and the excitation continuum is consistent with gapless QSL, and is therefore labeled so. With further increasing field, the magnetic moments are forced to be aligned with the field. The gap reopens and the gap size increases monotonically with field. Since the saturation field is up to above 60 T,[42] we label this phase as the gapped partially polarized phase. We have measured the excitations with different $L$ values. It can be seen from Fig. 4 that while the gap size has some difference at different $L$'s, the overall trend is similar. Such a three-zone phase diagram with an intermediate QSL phase between the low-field zigzag ordered phase and a high-field partially polarized phase featuring two quantum critical points is different from those with only two phases, i.e., a low-field zigzag ordered phase and high-field QSL phase, divided by a quantum critical point.[48,49] The phase space for the QSL state is also significantly narrowed down. On the other hand, it is consistent with literature, which features a zigzag order, QSL, and possibly topologically trivial phase.[57,61,63,72]
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Fig. 4. Field-evolution of the energy gap and the phase diagram. The left cyan zone denotes the gapped zigzag ordered state (gapped ZZ), central brown column represents the possibly gapless QSL state, and the right dark blue zone is the gapped partially polarized state (gapped PP). The purple stars and red circles denote the data measured on sample I with $L=2$ r.l.u. obtained from SIKA and FLEXX, respectively. The dark blue triangles represent the data measured on SIKA on sample II with $L=1.5$ r.l.u.
From our careful neutron scattering measurements on several batches of high-quality single crystals of $\alpha$-RuCl$_3$ on different spectrometers, we have obtained comprehensive excitation spectra as well as their evolutions under external magnetic field. These results allow us to answer the three important questions we raise above. First, the disordered phase near the critical field is indeed the QSL phase. This is evident from the fact that while the spin waves associated with the magnetic order are completely suppressed, the continuum associated with the fractional excitations of the QSL state survives. Second, the QSL phase is possibly gapless. We note that in Refs. [61,64], a half-integer quantized plateau of the thermal Hall conductivity around the critical field was reported. This indicates the presence of a Kitaev QSL state with gapped bulk and gapless edge featuring Majorana fermions. On the other hand, another report on the thermal Hall conductivity did not observe the 1/2 plateau.[63] While this controversy remains to be solved, we believe that our direct measurements on the magnetic excitations by INS provide clear evidence that the excitations of the QSL are very likely to be gapless. Third, there is a small but finite intermediate QSL regime between the gapped zigzag order and gapped partially polarized phase. By comparing the spectra of this field-induced gapless QSL phase [Fig. 3(b)] with those of the zero-field paramagnetic phase above $T_{\rm N}$ [Fig. 3(d)], we believe they are distinctive, although the latter phase may also feature fractional excitations.[20,84] To summarize, we have conducted INS experiments on $\alpha$-RuCl$_3$ single crystals to investigate the evolution of the magnetic excitations with an in-plane magnetic field. Our results show clearly that the spin-waves excitations around the $M$ point are suppressed in accordance with the suppression of the magnetic order. Near the critical field of $\sim $7.5 T, the spin waves disappear but the possibly gapless continuum around the $\varGamma$ point is present, indicating the emergence of a pure gapless QSL phase. Based on the evolution of the gap with field, we obtain a three-zone phase diagram, which consists of a low-field gapped zigzag order phase, an intermediate-field gapless QSL, and a high-field gapped partially polarized state. These results constitute as evidence that an intermediate in-plane magnetic field induces a pure QSL phase in $\alpha$-RuCl$_3$. Acknowledgments. The work was supported by the National Key Research and Development Program of China (Grant No. 2021YFA1400400), the National Natural Science Foundation of China (Grant Nos. 11822405, 12074174, 12074175, 92165205, 11904170, 12004249, 12004251, and 12004191), the Natural Science Foundation of Jiangsu Province (Grant Nos. BK20180006, BK20190436, and BK20200738), the Shanghai Sailing Program (Grant Nos. 20YF1430600 and 21YF1429200), and the Fundamental Research Funds for the Central Universities. The experiment at FLEXX was carried out under the proposal (Grant No. 17205993-CR) using beamtime allocated in the HZB-CIAE collaboration on the scientific use of instruments. The experiments at SIKA were carried out under the proposal (Grant Nos. P5844 and IC6741).
References Anyons in an exactly solved model and beyondQuantum spin liquids: a reviewConcept and realization of Kitaev quantum spin liquidsExperimental identification of quantum spin liquidsResonating valence bonds: A new kind of insulator?Spin liquids in frustrated magnetsMagnetic order in α RuCl 3 : A honeycomb-lattice quantum magnet with strong spin-orbit couplingKitaev magnetism in honeycomb RuCl 3 with intermediate spin-orbit couplingMonoclinic crystal structure of α RuCl 3 and the zigzag antiferromagnetic ground stateProximate Kitaev quantum spin liquid behaviour in a honeycomb magnetZigzag type magnetic structure of the spin Jeff = ½ compound α-RuCl3 as determined by neutron powder diffraction α RuCl 3 : A spin-orbit assisted Mott insulator on a honeycomb latticeCrystal structure and magnetism in α RuCl 3 : An ab initio studyKitaev exchange and field-induced quantum spin-liquid states in honeycomb α-RuCl3Spin-Wave Excitations Evidencing the Kitaev Interaction in Single Crystalline α RuCl 3 Theoretical investigation of magnetic dynamics in α RuCl 3 Ferromagnetic Kitaev interaction and the origin of large magnetic anisotropy in α-RuCl3Scattering Continuum and Possible Fractionalized Excitations in α RuCl 3 Fermionic response from fractionalization in an insulating two-dimensional magnetMajorana fermions in the Kitaev quantum spin system α-RuCl3Unveiling magnetic interactions of ruthenium trichloride via constraining direction of orbital moments: Potential routes to realize a quantum spin liquidAnisotropic susceptibilities in the honeycomb Kitaev system α RuCl 3 Deriving models for the Kitaev spin-liquid candidate material α RuCl 3 from first principlesKitaev-Heisenberg Model on a Honeycomb Lattice: Possible Exotic Phases in Iridium Oxides A 2 IrO 3 Generic Spin Model for the Honeycomb Iridates beyond the Kitaev LimitHidden symmetries of the extended Kitaev-Heisenberg model: Implications for the honeycomb-lattice iridates A 2 IrO 3 Kitaev interactions between j = 1/2 moments in honeycomb Na2 IrO3 are large and ferromagnetic: insights from ab initio quantum chemistry calculationsFirst-Principles Study of the Honeycomb-Lattice Iridates Na 2 IrO 3 in the Presence of Strong Spin-Orbit Interaction and Electron CorrelationsDirect evidence for dominant bond-directional interactions in a honeycomb lattice iridate Na2IrO3Mott Insulators in the Strong Spin-Orbit Coupling Limit: From Heisenberg to a Quantum Compass and Kitaev ModelsModels and materials for generalized Kitaev magnetismChallenges in design of Kitaev materials: Magnetic interactions from competing energy scalesSignatures of magnetic-field-driven quantum phase transitions in the entanglement entropy and spin dynamics of the Kitaev honeycomb modelMagnetization processes of zigzag states on the honeycomb lattice: Identifying spin models for α RuCl 3 and Na 2 IrO 3 Proximate Kitaev system for an intermediate magnetic phase in in-plane magnetic fieldsTheory of the field-revealed Kitaev spin liquidProbing α RuCl 3 Beyond Magnetic Order: Effects of Temperature and Magnetic FieldHeisenberg–Kitaev physics in magnetic fieldsMagnetic field induced competing phases in spin-orbital entangled Kitaev magnetsProximate ferromagnetic state in the Kitaev model material α-RuCl3Identification of magnetic interactions and high-field quantum spin liquid in α-RuCl3Successive magnetic phase transitions in α RuCl 3 : XY-like frustrated magnet on the honeycomb latticeGapless Spin Excitations in the Field-Induced Quantum Spin Liquid Phase of α RuCl 3 Anisotropic Ru 3 +   4 d 5 magnetism in the α RuCl 3 honeycomb system: Susceptibility, specific heat, and zero-field NMRField-induced intermediate ordered phase and anisotropic interlayer interactions in α RuCl 3 Phase diagram of α RuCl 3 in an in-plane magnetic fieldThermodynamic Perspective on Field-Induced Behavior of α RuCl 3 Field-induced quantum criticality in the Kitaev system α RuCl 3 Evidence for a Field-Induced Quantum Spin Liquid in α - RuCl 3 Ultralow-Temperature Thermal Conductivity of the Kitaev Honeycomb Magnet α RuCl 3 across the Field-Induced Phase TransitionAngle-dependent thermodynamics of α Ru Cl 3 Thermodynamic evidence of fractionalized excitations in α RuC l 3 Thermodynamic evidence for a field-angle-dependent Majorana gap in a Kitaev spin liquidIntermediate Quantum Spin Liquid Phase in the Kitaev Material $α$-RuCl$_3$ under High Magnetic Fields up to 100 TExcitations in the field-induced quantum spin liquid state of α-RuCl3Finite field regime for a quantum spin liquid in α RuCl 3 Two-step gap opening across the quantum critical point in the Kitaev honeycomb magnet α RuCl 3 Observation of two types of fractional excitation in the Kitaev honeycomb magnetAnomalous Thermal Conductivity and Magnetic Torque Response in the Honeycomb Magnet α RuCl 3 Unusual Phonon Heat Transport in α RuCl 3 : Strong Spin-Phonon Scattering and Field-Induced Spin GapMajorana quantization and half-integer thermal quantum Hall effect in a Kitaev spin liquidUnusual Thermal Hall Effect in a Kitaev Spin Liquid Candidate α RuCl 3 Oscillations of the thermal conductivity in the spin-liquid state of α-RuCl3Half-integer quantized anomalous thermal Hall effect in the Kitaev material candidate α-RuCl3Robustness of the thermal Hall effect close to half-quantization in α-RuCl3The planar thermal Hall conductivity in the Kitaev magnet α-RuCl3High-field quantum disordered state in α RuCl 3 : Spin flips, bound states, and multiparticle continuumSignatures of low-energy fractionalized excitations in α RuCl 3 from field-dependent microwave absorptionAntiferromagnetic Resonance and Terahertz Continuum in α RuCl 3 Magnetic Excitations and Continuum of a Possibly Field-Induced Quantum Spin Liquid in α RuCl 3 Field evolution of magnons in α RuCl 3 by high-resolution polarized terahertz spectroscopyU1 snRNP regulates cancer cell migration and invasion in vitroAnisotropic magnetodielectric effect in the honeycomb-type magnet α RuCl 3 Scale-invariant magnetic anisotropy in RuCl3 at high magnetic fieldsUnconventional spin dynamics in the honeycomb-lattice material α RuCl 3 : High-field electron spin resonance studiesNature of Magnetic Excitations in the High-Field Phase of α RuCl 3 Field-induced transitions in the Kitaev material α RuCl 3 probed by thermal expansion and magnetostrictionThermal and magnetoelastic properties of α RuCl 3 in the field-induced low-temperature statesRethinking α RuCl 3 Neutron scattering in the proximate quantum spin liquid α-RuCl3Evidence for Magnetic Fractional Excitations in a Kitaev Quantum-Spin-Liquid Candidate α-RuCl3SIKA—the multiplexing cold-neutron triple-axis spectrometer at ANSTODisorder-induced broadening of the spin waves in the triangular-lattice quantum spin liquid candidate YbZnGaO 4 Universal thermodynamics in the Kitaev fractional liquid
[1] Kitaev A 2006 Ann. Phys. 321 2
[2] Savary L and Balents L 2017 Rep. Prog. Phys. 80 016502
[3] Takagi H, Takayama T, Jackeli G, Khaliullin G, and Nagler S E 2019 Nat. Rev. Phys. 1 264
[4] Wen J, Yu S L, Li S, Yu W, and Li J X 2019 npj Quantum Mater. 4 12
[5] Anderson P W 1973 Mater. Res. Bull. 8 153
[6] Balents L 2010 Nature 464 199
[7] Sears J A, Songvilay M, Plumb K W, Clancy J P, Qiu Y, Zhao Y, Parshall D, and Kim Y J 2015 Phys. Rev. B 91 144420
[8] Kim H S, Vijay S V, Catuneanu A, and Kee H Y 2015 Phys. Rev. B 91 241110
[9] Johnson R D, Williams S C, Haghighirad A A, Singleton J, Zapf V, Manuel P, Mazin I I, Li Y, Jeschke H O, Valentí R, and Coldea R 2015 Phys. Rev. B 92 235119
[10] Banerjee A, Bridges C A, Yan J Q, Aczel A A, Li L, Stone M B, Granroth G E, Lumsden M D, Yiu Y, Knolle J, Bhattacharjee S, Kovrizhin D L, Moessner R, Tennant D A, Mandrus D G, and Nagler S E 2016 Nat. Mater. 15 733
[11] Ritter C 2016 J. Phys.: Conf. Ser. 746 012060
[12] Plumb K W, Clancy J P, Sandilands L J, Shankar V V, Hu Y F, Burch K S, Kee H Y, and Kim Y J 2014 Phys. Rev. B 90 041112
[13] Kim H S and Kee H Y 2016 Phys. Rev. B 93 155143
[14] Yadav R, Bogdanov N A, Katukuri V M, Nishimoto S, van den Brink J, and Hozoi L 2016 Sci. Rep. 6 37925
[15] Ran K, Wang J, Wang W, Dong Z Y, Ren X, Bao S, Li S, Ma Z, Gan Y, Zhang Y, Park J T, Deng G, Danilkin S, Yu S L, Li J X, and Wen J 2017 Phys. Rev. Lett. 118 107203
[16] Wang W, Dong Z Y, Yu S L, and Li J X 2017 Phys. Rev. B 96 115103
[17] Sears J A, Chern L E, Kim S, Bereciartua P J, Francoual S, Kim Y B, and Kim Y J 2020 Nat. Phys. 16 837
[18] Sandilands L J, Tian Y, Plumb K W, Kim Y J, and Burch K S 2015 Phys. Rev. Lett. 114 147201
[19] Nasu J, Knolle J, Kovrizhin D L, Motome Y, and Moessner R 2016 Nat. Phys. 12 912
[20] Do S H, Park S Y, Yoshitake J, Nasu J, Motome Y, Kwon Y S, Adroja D T, Voneshen D J, Kim K, Jang T H, Park J H, Choi K Y, and Ji S 2017 Nat. Phys. 13 1079
[21] Hou Y S, Xiang H J, and Gong X G 2017 Phys. Rev. B 96 054410
[22] Lampen-Kelley P, Rachel S, Reuther J, Yan J Q, Banerjee A, Bridges C A, Cao H B, Nagler S E, and Mandrus D 2018 Phys. Rev. B 98 100403
[23] Eichstaedt C, Zhang Y, Laurell P, Okamoto S, Eguiluz A G, and Berlijn T 2019 Phys. Rev. B 100 075110
[24] Chaloupka J, Jackeli G, and Khaliullin G 2010 Phys. Rev. Lett. 105 027204
[25] Rau J G, Lee E K H, and Kee H Y 2014 Phys. Rev. Lett. 112 077204
[26] Chaloupka J and Khaliullin G 2015 Phys. Rev. B 92 024413
[27] Katukuri V M, Nishimoto S, Yushankhai V, Stoyanova A, Kandpal H, Choi S, Coldea R, Rousochatzakis I, Hozoi L, and van den Brink J 2014 New J. Phys. 16 013056
[28] Yamaji Y, Nomura Y, Kurita M, Arita R, and Imada M 2014 Phys. Rev. Lett. 113 107201
[29] Chun S H, Kim J W, Kim J, Zheng H, Stoumpos C C, Malliakas C D, Mitchell J F, Mehlawat K, Singh Y, Choi Y, Gog T, Al-Zein A, Sala M M, Krisch M, Chaloupka J, Jackeli G, Khaliullin G, and Kim B J 2015 Nat. Phys. 11 462
[30] Jackeli G and Khaliullin G 2009 Phys. Rev. Lett. 102 017205
[31] Winter S M, Tsirlin A A, Daghofer M, van den Brink J, Singh Y, Gegenwart P, and Valentí R 2017 J. Phys.: Condens. Matter 29 493002
[32] Winter S M, Li Y, Jeschke H O, and Valentí R 2016 Phys. Rev. B 93 214431
[33] Ronquillo D C, Vengal A, and Trivedi N 2019 Phys. Rev. B 99 140413
[34] Janssen L, Andrade E C, and Vojta M 2017 Phys. Rev. B 96 064430
[35] Kim B H, Sota S, Shirakawa T, Yunoki S, and Son Y W 2020 Phys. Rev. B 102 140402
[36] Gordon J S, Catuneanu A, Sørensen E S, and Kee H Y 2019 Nat. Commun. 10 2470
[37] Winter S M, Riedl K, Kaib D, Coldea R, and Valentí R 2018 Phys. Rev. Lett. 120 077203
[38] Janssen L and Vojta M 2019 J. Phys.: Condens. Matter 31 423002
[39] Chern L E, Kaneko R, Lee H Y, and Kim Y B 2020 Phys. Rev. Res. 2 013014
[40] Suzuki H, Liu H, Bertinshaw J et al. 2021 Nat. Commun. 12 4512
[41] Li H, Zhang H K, Wang J, Wu H Q, Gao Y, Qu D W, Liu Z X, Gong S S, and Li W 2021 Nat. Commun. 12 4007
[42] Kubota Y, Tanaka H, Ono T, Narumi Y, and Kindo K 2015 Phys. Rev. B 91 094422
[43] Zheng J, Ran K, Li T, Wang J, Wang P, Liu B, Liu Z X, Normand B, Wen J, and Yu W 2017 Phys. Rev. Lett. 119 227208
[44] Majumder M, Schmidt M, Rosner H, Tsirlin A A, Yasuoka H, and Baenitz M 2015 Phys. Rev. B 91 180401
[45] Balz C, Janssen L, Lampen-Kelley P, Banerjee A, Liu Y H, Yan J Q, Mandrus D G, Vojta M, and Nagler S E 2021 Phys. Rev. B 103 174417
[46] Sears J A, Zhao Y, Xu Z, Lynn J W, and Kim Y J 2017 Phys. Rev. B 95 180411
[47] Bachus S, Kaib D A S, Tokiwa Y, Jesche A, Tsurkan V, Loidl A, Winter S M, Tsirlin A A, Valentí R, and Gegenwart P 2020 Phys. Rev. Lett. 125 097203
[48] Wolter A U B, Corredor L T, Janssen L, Nenkov K, Schönecker S, Do S H, Choi K Y, Albrecht R, Hunger J, Doert T, Vojta M, and Büchner B 2017 Phys. Rev. B 96 041405
[49] Baek S H, Do S H, Choi K Y, Kwon Y S, Wolter A U B, Nishimoto S, van den Brink J, and Büchner B 2017 Phys. Rev. Lett. 119 037201
[50] Yu Y J, Xu Y, Ran K J, Ni J M, Huang Y Y, Wang J H, Wen J S, and Li S Y 2018 Phys. Rev. Lett. 120 067202
[51] Bachus S, Kaib D A S, Jesche A, Tsurkan V, Loidl A, Winter S M, Tsirlin A A, Valentí R, and Gegenwart P 2021 Phys. Rev. B 103 054440
[52] Widmann S, Tsurkan V, Prishchenko D A, Mazurenko V G, Tsirlin A A, and Loidl A 2019 Phys. Rev. B 99 094415
[53] Tanaka O, Mizukami Y, Harasawa R, Hashimoto K, Hwang K, Kurita N, Tanaka H, Fujimoto S, Matsuda Y, Moon E G, and Shibauchi T 2022 Nat. Phys. (accepted)
[54] Zhou X G, Li H, Matsuda Y H, Matsuo A, Li W, Kurita N, Kindo K, and Tanaka H 2022 arXiv:2201.04597 [cond-mat.str-el]
[55] Banerjee A, Lampen-Kelley P, Knolle J, Balz C, Aczel A A, Winn B, Liu Y, Pajerowski D, Yan J, Bridges C A, Savici A T, Chakoumakos B C, Lumsden M D, Tennant D A, Moessner R, Mandrus D G, and Nagler S E 2018 npj Quantum Mater. 3 8
[56] Balz C, Lampen-Kelley P, Banerjee A, Yan J, Lu Z, Hu X, Yadav S M, Takano Y, Liu Y, Tennant D A, Lumsden M D, Mandrus D, and Nagler S E 2019 Phys. Rev. B 100 060405
[57] Nagai Y, Jinno T, Yoshitake J, Nasu J, Motome Y, Itoh M, and Shimizu Y 2020 Phys. Rev. B 101 020414
[58] Janša N, Zorko A, Gomilšek M, Pregelj M, Krämer K W, Biner D, Biffin A, Rüegg C, and Klanjšek M 2018 Nat. Phys. 14 786
[59] Leahy I A, Pocs C A, Siegfried P E, Graf D, Do S H, Choi K Y, Normand B, and Lee M 2017 Phys. Rev. Lett. 118 187203
[60] Hentrich R, Wolter A U B, Zotos X, Brenig W, Nowak D, Isaeva A, Doert T, Banerjee A, Lampen-Kelley P, Mandrus D G, Nagler S E, Sears J, Kim Y J, Büchner B, and Hess C 2018 Phys. Rev. Lett. 120 117204
[61] Kasahara Y, Ohnishi T, Mizukami Y, Tanaka O, Ma S, Sugii K, Kurita N, Tanaka H, Nasu J, Motome Y, Shibauchi T, and Matsuda Y 2018 Nature 559 227
[62] Kasahara Y, Sugii K, Ohnishi T, Shimozawa M, Yamashita M, Kurita N, Tanaka H, Nasu J, Motome Y, Shibauchi T, and Matsuda Y 2018 Phys. Rev. Lett. 120 217205
[63] Czajka P, Gao T, Hirschberger M, Lampen-Kelley P, Banerjee A, Yan J, Mandrus D G, Nagler S E, and Ong N P 2021 Nat. Phys. 17 915
[64] Yokoi T, Ma S, Kasahara Y, Kasahara S, Shibauchi T, Kurita N, Tanaka H, Nasu J, Motome Y, Hickey C, Trebst S, and Matsuda Y 2021 Science 373 568
[65] Bruin J A N, Claus R R, Matsumoto Y, Kurita N, Tanaka H, and Takagi H 2022 Nat. Phys. (accepted)
[66] Czajka P, Gao T, Hirschberger M, Lampen-Kelley P, Banerjee A, Quirk N, Mandrus D G, Nagler S E, and Ong N P 2022 arXiv:2201.07873 [cond-mat.str-el]
[67] Sahasrabudhe A, Kaib D A S, Reschke S, German R, Koethe T C, Buhot J, Kamenskyi D, Hickey C, Becker P, Tsurkan V, Loidl A, Do S H, Choi K Y, Grüninger M, Winter S M, Wang Z, Valentí R, and van Loosdrecht P H M 2020 Phys. Rev. B 101 140410
[68] Wellm C, Zeisner J, Alfonsov A, Wolter A U B, Roslova M, Isaeva A, Doert T, Vojta M, Büchner B, and Kataev V 2018 Phys. Rev. B 98 184408
[69] Little A, Wu L, Lampen-Kelley P, Banerjee A, Patankar S, Rees D, Bridges C A, Yan J Q, Mandrus D, Nagler S E, and Orenstein J 2017 Phys. Rev. Lett. 119 227201
[70] Wang Z, Reschke S, Hüvonen D, Do S H, Choi K Y, Gensch M, Nagel U, Rõõm T, and Loidl A 2017 Phys. Rev. Lett. 119 227202
[71] Wu L, Little A, Aldape E E, Rees D, Thewalt E, Lampen-Kelley P, Banerjee A, Bridges C A, Yan J Q, Boone D, Patankar S, Goldhaber-Gordon D, Mandrus D, Nagler S E, Altman E, and Orenstein J 2018 Phys. Rev. B 98 094425
[72] Wulferding D, Choi Y, Do S H, Lee C H, Lemmens P, Faugeras C, Gallais Y, and Choi K Y 2020 Nat. Commun. 11 1
[73] Aoyama T, Hasegawa Y, Kimura S, Kimura T, and Ohgushi K 2017 Phys. Rev. B 95 245104
[74] Modic K A, McDonald R D, Ruff J P C, Bachmann M D, Lai Y, Palmstrom J C, Graf D, Chan M K, Balakirev F F, Betts J B, Boebinger G S, Schmidt M, Lawler J M, Sokolov D A, Moll P J W, Ramshaw B J, and Shekhter A 2021 Nat. Phys. 17 240
[75] Ponomaryov A N, Schulze E, Wosnitza J, Lampen-Kelley P, Banerjee A, Yan J Q, Bridges C A, Mandrus D G, Nagler S E, Kolezhuk A K, and Zvyagin S A 2017 Phys. Rev. B 96 241107
[76] Ponomaryov A N, Zviagina L, Wosnitza J, Lampen-Kelley P, Banerjee A, Yan J Q, Bridges C A, Mandrus D G, Nagler S E, and Zvyagin S A 2020 Phys. Rev. Lett. 125 037202
[77] Gass S, Cônsoli P M, Kocsis V, Corredor L T, Lampen-Kelley P, Mandrus D G, Nagler S E, Janssen L, Vojta M, Büchner B, and Wolter A U B 2020 Phys. Rev. B 101 245158
[78] Schönemann R, Imajo S, Weickert F, Yan J, Mandrus D G, Takano Y, Brosha E L, Rosa P F S, Nagler S E, Kindo K, and Jaime M 2020 Phys. Rev. B 102 214432
[79] Maksimov P A and Chernyshev A L 2020 Phys. Rev. Res. 2 033011
[80] Banerjee A, Yan J, Knolle J, Bridges C A, Stone M B, Lumsden M D, Mandrus D G, Tennant D A, Moessner R, and Nagler S E 2017 Science 356 1055
[81] Ran K, Wang J, Bao S, Cai Z, Shangguan Y, Ma Z, Wang W, Dong Z Y, Čermák P, Schneidewind A, Meng S, Lu Z, Yu S L, Li J X, and Wen J 2022 Chin. Phys. Lett. 39 027501
[82] Wu C M, Deng G, Gardner J S, Vorderwisch P, Li W H, Yano S, Peng J C, and Imamovic E 2016 J. Instrum. 11 P10009
[83] Ma Z, Dong Z Y, Wang J, Zheng S, Ran K, Bao S, Cai Z, Shangguan Y, Wang W, Boehm M, Steffens P, Regnault L P, Wang X, Su Y, Yu S L, Liu J M, Li J X, and Wen J 2021 Phys. Rev. B 104 224433
[84] Li H, Qu D W, Zhang H K, Jia Y Z, Gong S S, Qi Y, and Li W 2020 Phys. Rev. Res. 2 043015