Anisotropic magnetic excitations from single-chirality antiferromagnetic state in Ca-kapellasite
Abstract
We present a 35Cl NMR study for spin perfect kagome antiferromagnet Ca-kapellasite (CaCu3(OH)6Cl0.6H2O) with a magnetic transition at K. The static magnetic structure in the ground state has been determined to be a chirality-ordered state, which is selected by a finite Dzyaloshinskii-Moriya interaction. The low-energy magnetic excitations in the ordered state are investigated by the nuclear spin-lattice relaxation rate measurement. We detect a weakly temperature dependent contribution in the magnetic fluctuations perpendicular to the kagome plane in addition to the dispersive spin-wave contribution in the kagome plane. The low-energy magnetic excitations from the coplanar spin structure are attributed to the zero mode originating from the flat band in this kagome antiferromagnet.
The ground state of quantum magnets with spin has been intensively discussed because the quantum fluctuations destabilize the canonical magnetic ordering and give rise to a new state of matter known as the spin liquid state. balents-Nature464 This prominent quantum effect emerges when the magnetic ordering is suppressed at very low temperatures by the competing interactions among several spins. One commonly recognized example is the geometrical frustration effect for antiferromagnetically interacting spins on a triangular lattice. Magnets with triangle-based spin configuration such as kagome and pyrochlore networks for two-dimensional (2-D) and three-dimensional (3-D) structures are also candidates for experimental realization of the spin liquid state. In fact, the spin liquid state has been observed in herbertsmithite (2-D) shores-JACS127 ; norman-RMP88 ; han-Nature492 ; imai-PRL100 ; fu-Science350 ; jeong-PRL107 and Yb2Ti2O7 (3-D). ross-PRX1 ; chang-natcom3 ; tokiwa-natcom7 A recently found new candidate for a spin liquid material is the Kitaev ferromagnet, for which theory suggests that the spin-orbit coupled anisotropic frustration leads to a spin liquid ground state. kitaev-anphy321 ; nasu-NatPhy12 In the spin liquid state the spin-spin interactions extend to the distance, yet the spins maintain the dynamics. As a result the elemental excitation can be fractionalized and fermionic spinon excitations were observed in -RuCl3 sandilands-PRL114 ; kasahara-Nature559 and Ir based magnets singh-PRL108 ; kitagawa-Nature554 . In the case of Yb2Ti2O7 the monopole excitations were observed. tokiwa-natcom7 Experimental observation of fractionalized magnetic excitations is not only striking evidence for the spin liquid state, but also a characteristic potentially applicable to the quantum computation. Although fractional magnetic excitations were predicted only for the spin liquid state without any magnetic ordering, in kagome antiferromagnets low-energy magnetic excitations can be generated even in the magnetically ordered state because of the macroscopic degeneracy left in the ground state.
Magnetic excitations in the ordered state are generally understood as the bosonic magnons which can be perfectly explained by spin-wave theory. yildirim-PRB73 ; matan-PRL96 In the kagome antiferromagnet, however, a flat band known as the zero mode appears at zero energy in the magnon dispersion for a coplanar magnetic state chalker-PRL68 ; harris-PRB45 and its effect on the magnetic properties have not been revealed because the flat band can infinitely populate low-energy excitations. chernyshev-PRB92 As the zero mode is the spin excitations perpendicular to the kagome plane, we could interpret that the spin component perpendicular to the kagome plane is disordered, while the in-plane components are ordered. Experimental input is crucially important to advance understanding about low-energy excitations in kagome antiferromagnets, but so far no experimental results have been reported due to the lack of suitable materials that show a regular magnetic ordering on the perfect kagome network.

In this study, we focus on a 2-D kagome antiferromagnet Ca-kapellasite (CaCu3(OH)6Cl0.6H2O), yoshida-JPSJ86 which has a magnetically perfect kagome network of Cu spins. The magnetism in Ca-kapellasite is understood on the basis of the model, fak-PRL109 ; kermarrec-PRB90 ; boldrin-PRB91 ; bieri-PRB92 ; iqbal-PRB92 in which the long range interaction across the hexagon is finite in addition to the nearest and next nearest interactions and . [Fig. 1 (a)] Within the family of kapellasite materials colman-CM20 ; colman-CM22 , Ca-kapellasite is the most interesting because of the antiferromagnetic . The ground states for antiferromagnetic were theoretically investigated only from the classical limit without quantum fluctuation effects. messio-PRB83 In the phase diagram and ground states reside very close to each other when is small, which is the case for Ca-kapellasite. The ground state in the real material will be selected by further interactions, such as Dzyaloshinskii-Moriya (DM) interaction which is intrinsic for the kagome network. elhajal-PRB66 The DM vector perpendicular to the kagome plane stabilizes the coplanar magnetic state [Figs. 1 (b), (c)] opening a gap for the zero mode. chernyshev-PRB92
Previous bulk property measurements yoshida-JPSJ86 revealed a weak magnetic ordering at K from the peaks in the in-plane magnetization and the heat capacity. From the 35Cl NMR experiment for a powdered sample a peak in the spin-lattice relaxation rate at and spectrum broadening below were observed as the evidence for static magnetic ordering. ihara-PRB96 In the ordered state, the dispersive magnon excitations were observed as the term in the heat capacity and the term in . In addition to these magnon contributions Ca-kapellasite has nontrivial magnetic excitations which introduce -linear temperature dependence both in the heat capacity and . As this temperature dependence is reminiscent of a Fermi liquid state in conductors, one would invoke a fermionic nature for the low-energy excitations.
To identify the origin of nontrivial magnetic excitations, we performed 35Cl NMR experiments on crystalline samples. From the NMR spectra and measurements in field applied parallel () and perpendicular () to the kagome plane, we found that the ordered state is highly anisotropic due to the coplanar magnetic structure. Moreover, we revealed that the magnetic excitations are also anisotropic and that the weakly temperature dependent contribution was observed only in the axis component. We discuss the zero mode in kagome antiferromagnets as a possible origin of the orientation ordered magnetic excitations.
The 35Cl NMR experiment was performed for a single crystal with a typical dimension of mm3. The sample was mounted on a single axis rotator, with which the field direction can be tuned from the axis ( to the axis ). The NMR spectra were obtained by a single Fourier transformation at fixed field when the linewidth is narrow at high temperatures, and by recombining several Fourier transformations during the field sweep for the broad spectra at low temperatures. The peak frequency/field and their standard error were estimated by fitting the obtained spectrum with a Gaussian function. For the high field NMR experiment, we used the high superconducting magnet in the Institute for Materials Research, Tohoku University.

Figure 2 shows the temperature dependence of the Knight shift . Temperature-independent term was subtracted from the total shift. The solid lines in Fig. 2 are the uniform susceptibility multiplied by the hyperfine coupling constants for and , which are mT/ and mT/ sup . At high temperatures above K follows as expected for a paramagnetic state. At low temperatures deviates from due to the formation of short-range ordering structure. The in-plane Knight shift goes down to zero around , suggesting a degrees structure in the ordered state, for which the transferred hyperfine fields are canceled out at the Cl sites on the trigonal axis. (inset of Fig. 2) Remarkably, the out-of-plane Knight shift levels off around and remains finite even in the ordered state. We can exclude any extrinsic magnetization from impurities and defects as the source of finite because such contributions would not shift the peak positions but increase the linewidth of the NMR spectrum. The finite evidences that the -axis susceptibility is finite and thus the low-energy magnetic excitations survive partially in the antiferromagnetically ordered state. We will discuss the dynamics of this low-energy mode later.

Anisotropic behavior was also observed in the linewidth. As shown in Fig. 3 (a), (b), the emergent line broadening associated with magnetic transition was observed only in . The small increase in the linewidth for further confirms that the finite -axis susceptibility does not originate from magnetic impurities. In the temperature dependence of full width at the half maximum [FWHM, Fig. 3 (c)] the onset of the line broadening was observed slightly above in . The precursor to the magnetic transition is ascribed to the growth in the coherent length for interactiong spins. In the ordered state a broad spectrum without apparent structure was observed. In contrast, in magnetic line broadening at the lowest temperature is approximately mT, which is of that in . The finite line broadening in can be ascribed to a field misalignment of less than degrees. From these results we can conclude that the internal fields at the Cl site orient parallel to the kagome plane, and its amplitude is distributed.
To explain the reduction of from 30 K to we assume a coplanar degrees spin structure, where all spins are in the kagome plane. Then, we can consider two different spin configurations; the positive- and negative-chirality spin configurations, depending on the direction of the spin rotation as shown in Fig. 1 (b), (c). In the magnetic structure on the kagome network all the Cu triangles possess the same chirality, whereas in the state both chirality are arranged alternatively. As the transferred hyperfine fields are canceled for both spin configurations, the spectrum broadening in is caused purely by dipole fields. The dipole fields at the Cl site have only the -axis component for the positive chirality, and in-plane component for the negative chirality. The details of the dipole field calculation are given in the supplemental material. sup As our experimental result unveils that the internal fields appear only along the kagome plane, we conclude that all the spins form the negative-chirality spin configuration. Thus, we suggest that the negative-chirality magnetic structure is realized in Ca-kapellasite.
The chirality of spins on a triangle is selected by the DM interaction, namely the vector perpendicular to the triangular plane, elhajal-PRB66 whereas the in-plane component introduces a non-coplanar spin structure. The coplanar and negative-chirality magnetic structure suggests that is perpendicular to the kagome plane and pointing down as Fig. 1 (c). The thermal Hall effect was also consistently explained by the negative-chirality state. doki-PRL121 The negative-chirality state was also suggested for a sister compound Cd-kapellasite okuma-PRB95 , and YCu3(OH)6Cl3. zorko-PRB100 In Cd-kapellasite the abrupt increase in susceptibility above the magnetic ordering temperature was explained as the precursor to the magnetic state from symmetry considerations. A similar upturn was also observed in Ca-kapellasite. yoshida-JPSJ86
It should be noted that the state has a freedom of global spin rotation. If the spin directions were locked to a certain direction with respect to the external field orientation, only two kinds of antiparallel dipole fields would be generated at the Cl site, which results in a two-peak NMR spectrum. From our results, however, a broad NMR spectrum without any structure was observed as shown in Fig. 3 (a). We thus suggest that state forms a domain to induce distributed internal fields at the Cl sites.

Next we measured the nuclear spin-lattice relaxation rate to explore the low-energy magnetic excitations in the ordered state. As shown in Fig. 4, becomes anisotropic below . In shows a peak at due to the critical fluctuations near the magnetic phase transition and a power-law behavior was observed in the ordered state. The exponent close to is explained by the linear spin-wave theory for the state, whereas in the peak at is suppressed and the temperature dependence below is weaker than . We suggest that the weak temperature dependence is due to the additional contribution in , which corresponds to the -linear contribution observed in the powder sample and also in the heat capacity measurement. ihara-PRB96 ; yoshida-JPSJ86
The nuclear spins excited by the rf fields are relaxed by the local magnetic fluctuations perpendicular to the external field direction. The temperature dependence observed in strongly indicates that spin fluctuations in the kagome plane are perfectly understood as the dispersive magnon excitations, while the spin fluctuations along the direction have larger weight at lower energy, as sensed by in . We address the zero mode as the origin of the low-energy excitations perpendicular to kagome plane. The finite and temperature independent -axis susceptibility is also consistently explained by the zero mode. We should note that the flat band is lifted by the DM interaction, which results in a gapped excitations. The power-law temperature dependence was observed down to K in Ca-kapellasite because the gap by DM interaction is suppressed by and which introduce dispersion to the flat band. chernyshev-PRB92 ; matan-PRL96
In Fig. 4, measured at T is shown together with the result at low field. In we observed a peak in at and temperature dependence below even at T. The peak temperature increases to K in T probably due to the weakly ferromagnetic nature of state. To reveal the origin of the increase in in high magnetic fields, further experiments are necessary. In the peak at is strongly suppressed, and the behavior appears in a narrow temperature range just below . Then the deviation from behavior was observed below K. From these results we suggest that the zero mode is more strongly suppressed by fields compared with the dispersive spin-wave contribution because of the small energy scale relevant to the flat band. The heat capacity measurement also suggests that the -linear contribution is suppressed by fields of about T. yoshida-JPSJ86

The zero mode from the state is understood as the local excitations of six spins surrounding one hexagon. harris-PRB45 [Fig. 5 (a)] Such local excitation without any long range propagation will contribute to a temperature independent as in the case of free spins. In contrast, the zero mode from the state forms a chain structure [Fig. 5 (b)], which would introduce a power-law temperature dependence defined by the evolution of the coherence length. We propose that the low-energy excitations in Ca-kapellasite can be understood as the superposed one-dimensional chains weakly connected by long range interactions , . Further experiment is required to directly observe the low-energy magnon dispersion, and possibly additional continuum excitations originating from weakly dispersing low-energy band.
To summarize, we found the anisotropic spectrum broadening in the ordered state of Ca-kapellasite, which is consistently explained as the negative-chirality state. From the measurement in and we conclude that the in-plane component of the low-energy magnetic excitations are dominated by the spin-wave contribution. Moreover, we unveiled weaker temperature dependence for the magnetic excitations along the axis. These nontrivial excitations are consistent with the finite susceptibility along axis and also -linear contribution to the heat capacity. We suggest that these excitations can be generated from the flat band in the kagome antiferromagnet when it obtains a weak dispersion due to long range interactions.
Acknowledgements.
We would like to acknowledge Jun Ohara and Kazuki Iida for fruitful discussions. Part of this work was performed at the High Field Laboratory for Superconducting Materials, Institute for Materials Research, Tohoku University (Project Nos. 17H0046, 18H0015, 19H0037). This study was partly supported by the Grant-in-Aid for Young Scientist B Grant Number JP15K17686 and JSPS KAKENHI Grant Numbers JP18K03529, JP19H01832, and JP19H01846.References
- (1) L. Balents, Nature 464, 199-208 (2010).
- (2) M. P. Shores, E. A. Nytko, B. M. Bartlett, D. G. Nocera, J. Am. Chem. Soc. 127, 13462 (2005).
- (3) T.-H. Han, J. S. Helton, S. Chu, D. G. Nocera, J. A. Rodriguez-Rivera, C. Broholm, and Y. S. Lee, Nature 492, 406-410 (2012).
- (4) M. R. Norman, Rev. Mod. Phys. 88, 041002 (2016).
- (5) T. Imai, E. A. Nytko, B. M. Bartlett, M. P. Shores, and D. G. Nocera, Phys. Rev. Lett. 100, 077203 (2008).
- (6) M. Fu, T. Imai, T.-H. Han, and Y.-S. Lee, Science 350, 655 (2015).
- (7) M. Jeong, F. Bert, P. Mendels, F. Duc, J. C. Trombe, M. A. de Vries, and A. Harrison, Phys. Rev. Lett. 107, 237201 (2011).
- (8) K. A. Ross, L. Savary, B. D. Gaulin, and L. Balents, Phys. Rev. X 1, 021002 (2011).
- (9) L.-J. Chang, S. Onoda, Y. Su, Y.-J. Kao, K.-D. Tsuei, Y. Yasui, K. Kakurai, and M. R. Lees, Nat. Commun. 3, 992 (2012).
- (10) Y. Tokiwa, T. Yamashita, M. Udagawa, S. Kittaka, T. Sakakibara, D. Terazawa, Y. Shimoyama, T. Terashima, Y. Yasui, and Y. Matsuda, Nat. Commun. 7, 10807 (2016).
- (11) A. Kitaev, Ann. Phys. 321, 2-111 (2006).
- (12) J. Nasu, J. Knolle, D. L. Kovrizhin, Y. Motome, R. Moessner, Nat. Phys. 12 912 (2016).
- (13) L. J. Sandilands, Y. Tian, K. W. Plumb, Y.-J. Kim, and K. S. Burch, Phys. Rev. Lett. 114, 147201 (2015).
- (14) Y. Kasahara, T. Ohnishi, Y. Mizukami, O. Tanaka, S. Ma, K. Sugii, N. Kurita, H. Tanaka, J. Nasu, Y. Motome, T. Shibauchi, and Y. Matsuda, Nature 559, 227 (2018).
- (15) Y. Singh, S. Manni, J. Reuther, T. Berlijn, R. Thomale, W. Ku, S. Trebst, and P. Gegenwart, Phys. Rev. Lett. 108, 127203 (2012).
- (16) K. Kitagawa, T. Takayama, Y. Matsumoto, A. Kato, R. Takano, Y. Kishimoto, S. Bette, R. Dinnebier, G. Jackeli, and H. Takagi, Nature 554, 341 (2018).
- (17) T. Yildirim, and A. B. Harris, Phys. Rev. B 73, 214446 (2006).
- (18) K. Matan, D. Grohol, D. G. Nocera, T. Yildirim, A. B. Harris, S. H. Lee, S. E. Nagler, and Y. S. Lee, Phys. Rev. Lett. 96, 247201 (2006).
- (19) J. T. Chalker, P. C. W. Holdsworth, and E. F. Shender, Phys. Rev. Lett 68, 855 (1992).
- (20) A. B. Harris, C. Kallin, and A. J. Berlinsky, Phys. Rev. B 45, 2899 (1992).
- (21) A. L. Chernyshev, and M. E. Zhitomirsky, Phys. Rev. B 92, 144415 (2015).
- (22) H. Yoshida, N. Noguchi, Y. Matsushita, Y. Ishii, Y. Ihara, M. Oda, H. Okabe, S. Yamashita, Y. Nakazawa, A. Takata, T. Kida, Y. Narumi, and M. Hagiwara, J. Phys. Soc. Jpn. 86, 033704 (2017).
- (23) B. Fak, E. Kermarrec, L. Messio, B. Bernu, C. Lhuillier, F. Bert, P. Mendels, B. Koteswararao, F. Bouquet, J. Ollivier, A. D. Hillier, A. Amato, R. H. Colman and A. S. Wills, Phys. Rev. Lett. 109, 037208 (2012).
- (24) E. Kermarrec, A. Zorko, F. Bert, R. H. Colman, B. Koteswararao, F. Bouquet, P. Bonville, A. Hillier, A. Amato, J. van Tol, A. Ozarowski, A. S. Wills, and P. Mendels, Phys. Rev. B 90, 205103 (2014).
- (25) D. Boldrin, B. Fak, M. Enderle, S. Bieri, J. Ollivier, S. Rols, P. Manuel, and A. S. Wills, Phys. Rev. B 91, 220408(R) (2015).
- (26) S. Bieri, L. Messio, B. Bernu, and C. Lhuillier, Phys. Rev. B 92, 060407(R) (2015).
- (27) Y. Iqbal, H. O. Jeschke, J. Reuther, R. Valentí, I. I. Mazin, M. Greiter, and R. Thomale, Phys. Rev. B 92, 220404(R) (2015).
- (28) R. H. Colman, C. Ritter, and A. S. Wills, Chem. Mater. 20, 6897 (2008).
- (29) R. H. Colman, R. Sinclair, and A. S. Wills, Chem. Mater. 22, 5774 (2010).
- (30) L. Messio, C. Lhuillier, and G. Misguich, Phys. Rev. B 83, 184401 (2011).
- (31) M. Elhajal, B. Canals, and C. Lacroix, Phys. Rev. B 66, 014422 (2002).
- (32) Y. Ihara, T. Sasaki, N. Noguchi, Y. Ishii, M. Oda, and H. Yoshida, Phys. Rev. B 96, 180409(R) (2017).
- (33) See Supplemental Material [url].
- (34) H. Doki, M. Akazawa, H.-Y. Lee, J. H. Han, K. Sugii, M. Shimozawa, N. Kawashima, M. Oda, H. Yoshida, and M. Yamashita, Phys. Rev. Lett. 121, 097203 (2018).
- (35) R. Okuma, T. Yajima, D. Nishio-Hamane, T. Okubo, and Z. Hiroi, Phys. Rev. B 95, 094427 (2017).
- (36) A. Zorko, M. Pregelj, M. Gomilšek, M. Klanjšek, O. Zaharko, W. Sun, and J. -X. Mi, Phys. Rev. B 100, 144420 (2019).