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Slow Electronic Dynamics in the Paramagnetic State of UTe2

Yo Tokunaga1 E-mail: [email protected]    Hironori Sakai1    Shinsaku Kambe1    Yoshinori Haga1    Yoshifumi Tokiwa1    Petr Opletal1    Hiroki Fujibayashi2    Katsuki Kinjo2    Shunsaku Kitagawa2    Kenji Ishida2    Ai Nakamura3    Yusei Shimizu3    Yoshiya Homma3    Dexin Li3    Fuminori Honda3,4    and Dai Aoki3,5 1ASRC1ASRC Japan Atomic Energy Agency Japan Atomic Energy Agency Tokai-mura Tokai-mura Ibaraki 319-1195 Ibaraki 319-1195 Japan
2Department of Physics Japan
2Department of Physics Kyoto University Kyoto University Kyoto 606-8502 Kyoto 606-8502 Japan
3IMR Japan
3IMR Tohoku University Tohoku University Oarai Oarai Ibaraki Ibaraki 311-1313 311-1313 Japan
4Central Institute of Radioisotope Science and Safety Japan
4Central Institute of Radioisotope Science and Safety Kyushu University Kyushu University Fukuoka 819-0395 Fukuoka 819-0395 Japan
5University Grenoble Alpes Japan
5University Grenoble Alpes CEA CEA IRIG-PHELIQS IRIG-PHELIQS F-38000 Grenoble F-38000 Grenoble France France
Abstract

125Te NMR experiments in field (HH) applied along the easy magnetization axis (the aa-axis) revealed slow electronic dynamics developing in the paramagnetic state of UTe2. The observed slow fluctuations are concerned with a successive growth of long-range electronic correlations below 30-40 K, where the spin susceptibility along the hard magnetization axis (the bb-axis) shows a broad maximum. The experiments also imply that tiny amounts of disorder or defects locally disturb the long-range electronic correlations and develop an inhomogeneous electronic state at low temperatures, leading to a low temperature upturn observed in the bulk-susceptibility in HaH\|a. We suggest that UTe2 would be located on the paramagnetic side near an electronic phase boundary, where either magnetic or Fermi-surface instability would be the origin of the characteristic fluctuations.

A recently discovered heavy-fermion superconductor UTe2[1] attracted particular attention, because of the strong possibility of spin-triplet Cooper pairing, which is a natural candidate for topological superconductivity (SC) in a bulk material [2, 3, 4, 5]. The formation of the spin-triplet pairing was experimentally suggested from tiny decrease in NMR Knight shift below the SC transition temperature TSC1.6T_{\rm SC}\sim 1.6 K [6, 7, 8], and an exceptionally large upper critical field Hc2H_{c2} far exceeding the Pauli-limiting field [1, 9, 10, 11, 12]. The spin-triplet pairing was further supported by the later discovery of a field-induced reentrant SC in high magnetic field (HH) over 40 T [12, 10, 11, 13] and multiple SC phases under applied pressure [14, 15].

UTe2 was initially proposed to be located at the paramagnetic end of the uranium-based ferromagnetic (FM) superconductor series, where SC is mediated by FM fluctuations [1]. This was based on the scaling analysis of the bulk spin-susceptibility below 9 K [1], and the temperature (TT) dependence of μ\muSR relaxation [16]. However, a key difference separating UTe2 from the other FM superconductors is the absence of a long-range magnetic order in the ground state, and as a consequence, the nature of spin fluctuations has been found to be much more complex than originally thought. NMR 1/T21/T_{2} measurements implied the development of slow and longitudinal fluctuations around 20 K in HaH\|a [17]. The zero-field μ\muSR experiment also observed similar fluctuations, but only below 5 K [16]. These fluctuations were attributed to possible FM instability of the material. On the other hand, more recent neutron scattering experiments detected antiferromagnetic (AFM), incommensurate fluctuations with a qq-vector of (0, 0.57, 0) [18, 19]. The AFM fluctuations are developing from higher TT, and saturated below about 12 K [19], similar to the TT-dependence of NMR 1/T1T1/T_{1}T [17]. Because of the puzzling results from the different probes, a unified picture of fluctuations has not yet emerged for UTe2.

Refer to caption
Figure 1: (Color online) (a) The crystal structure of UTe2, where the ladder structure of U atoms is emphasized. (b) Temperature and field dependences of the NMR Knight shift Ka(T,H)K_{\rm a}(T,H) and the bulk-susceptibility, χa(T,H)\chi_{\rm a}(T,H). The χa\chi_{\rm a} was measured in fields H=0.1=0.1 T and 1 - 7 T in 1 T step. The inset shows the resistivity data of our single crystal.

In this paper, we report 125Te-NMR experiments performed on a 125Te enriched (99%) single crystal of UTe2. The enrichment of 125Te largely enhanced NMR signal intensity and S/N ratio, allowing us to extend NMR studies to lower HH and TT than a previous report [17]. The single crystal was grown using the chemical vapor transport method with iodine as transport agent [9]. As seen in the inset of Fig. 1(b), the resistivity data of our single crystal shows a SC transition at TSC=T_{\rm SC}=1.74 K defined by the midpoint of the resistivity drop; a little lower than the highest TSCT_{\rm SC} of \sim2 K reported recently [20]. In the orthorhombic structure of UTe2 (space group No. 71, ImmmImmm, D2h25D_{2h}^{25}), U atoms in equivalent sites form a two-leg ladder structure with legs along the aa-axis and rungs along the cc-axis, with the inversion center located between the two U atoms, as displayed in Fig. 1(a) [21, 19]. On the other hand, Te atoms surrounding the ladder have two crystallographically inequivalent sites in a unit cell, so that 125Te NMR spectrum consists of two distinct peaks arising from the two inequivalent sites in HaH\|a [17]. Although we measured both peaks, there was no qualitative difference in the NMR results; here we focus on the data obtained at the lower frequency peak within two peaks.

NMR spectra were measured by recording integrated spin-echo intensities while sweeping frequency at a fixed HH. The NMR (Knight) shift was derived from the peak position of the NMR spectrum, where Cu NMR signals from metallic copper were used as markers for field calibrations. The nuclear spin-spin relaxation rate (1/T21/T_{2}) was obtained by measuring the decay of the spin-echo intensity on the peak position. The decay was found to fit an exponential function, M(2τ)exp(2τ/T2)M(2\tau)\propto\exp(-2\tau/T_{2}) as reported previously[17], where τ\tau is the time interval between the first and second pulses in the NMR spin-echo sequence.

Refer to caption
Figure 2: (Color online) Comparison of the TT dependences of NMR line width (FWHM) and Knight shift measured at several different HH in H||aH||a. The down triangles indicate the temperature below which additional NMR line broadening emerges.
Refer to caption
Figure 3: (Color online) (a) Temperature dependence of ΔW\Delta W in different fields. The inset shows the TT dependence of ΔW/H\Delta W/H. (b) Comparison of NMR spectra obtained at TT=5.5 K, 15 K and 32 K in HH=1.4 T. The horizontal axis Δf=fmeas.fpeak\Delta f=f_{\rm meas.}-f_{\rm peak} is the frequency difference from the peak frequency. The spectrum intensity is normalized by the intensity at the peak position.

Figure 1(b) shows the TT and HH dependences of bulk spin-susceptibility, χa\chi_{a} and the Knight shift KaK_{\rm a} in HaH\|a. For UTe2, the susceptibility, and thus the Knight shift, exhibit Ising anisotropy with the aa-axis as the magnetic easy axis, and the χa\chi_{a} follows a Curie Weiss behavior with a negative Weiss temperature of θ=60\theta=-60 K above 150 K [1, 13, 22]. With further decreasing TT, the χa\chi_{a} starts to increase faster than the Curie Weiss behavior, and tends to saturate below 20 K. The χa\chi_{a} becomes strongly HH dependent below 20 K, and has an additional upturn below 10 K at lower HH (2\lesssim 2 T) [1, 23, 13, 20]. In contrast, we found that the KaK_{\rm a} is totally HH independent over the whole TT region. Consequently the linear scaling obtained at higher TT between the Ka(T)K_{\rm a}(T) and χa(T)\chi_{\rm a}(T) does not work below 20 K. Below 10 K, the KaK_{\rm a} becomes almost TT independent, and thus never reproduce the low-TT upturn observed in the χa(T)\chi_{a}(T).

In general, the discrepancy in the TT dependence between the bulk-χ\chi and the NMR KK implies the presence of foreign impurity phases in measured samples; the KK is insensitive to the small amounts of foreign phases, whereas the bulk-χ\chi involves contributions from both the main and foreign phases. However, this is probably not the case for UTe2, because the low-TT anomaly in the χa(T)\chi_{\rm a}(T) has been commonly observed in single crystals grown by different groups [1, 23, 13, 20]. In addition, the anomaly is strongly field-orientation dependent (not observed in H||bH||b and ||c||c), and suppressed rapidly under applied pressure [24]. Furthermore, we have observed a distinct anomaly in the TT dependence of NMR line width and 1/T21/T_{2} in the same TT region, as described below. These imply that the low-TT anomaly in the χa(T)\chi_{a}(T) does not arise from foreign impurity phases, but is rather connected to electronic properties of UTe2 [25].

Figure 2 shows the TT dependence of the NMR line width (the full width at half maximum; WFWHMW_{\rm FWHM}) measured in several different HH. In the figure, we also plotted the Ka(T)K_{\rm a}(T) obtained in the same HH. The WFWHMW_{\rm FWHM} increases with decreasing TT. At higher-TT, it entirely scales with the KaK_{\rm a}, as expected when the broadening simply arises from a small distribution of the KaK_{\rm a}. However, below about 30-40 K, the WFWHMW_{\rm FWHM} starts to increase much faster than that of the KaK_{\rm a}, as if either the onset of spontaneous magnetic ordering or the sudden growth of electronic inhomogeneity took place at low TT. The onset temperature of the broadening shifts to higher TT in higher HH, as shown by the open triangles in Fig. 2. In Fig. 3 (a), we extracted the additional broadening component as ΔW=WFWHMWΔK\Delta W=W_{\rm FWHM}-W_{\rm\Delta K}, where WΔK=αKaW_{\rm\Delta K}=\alpha K_{\rm a} with a scaling coefficient α\alpha determined above 30-40 K. Although the absolute values of ΔW\Delta W are enhanced with increasing HH, we found that all the data fall roughly on a single curve after dividing the values by HH, as seen in the inset of Fig. 3 (a). This indicates that the ΔW\Delta W is nearly proportional to HH, i.e., ΔW0\Delta W\rightarrow 0 at H0H\rightarrow 0. The ΔW\Delta W is thus field-induced, not spontaneous one.

Figure 3 (b) displays typical evolution of the NMR line profile, which corresponds to the histogram of local fields associated with the electronic inhomogeneity. As mentioned above, the spectra show a distinct broadening below 30-40 K. However, it holds nearly symmetrical and structureless profile, indicating continuous distribution of local fields in magnitude. Such a structureless profile will deny any homogeneous, long-range magnetic orderings, neither with commensurate nor incommensurate wave vector in the 1D system. Interestingly, a similar broadening has been observed in low-dimensional correlated magnets with quenched disorder, such as x-ray-irradiated organic materials [26, 27, 28], and impurity-doped spin-ladder [29, 30, 31, 32] and high-TSCT_{\rm SC} cuprates [33, 34, 35, 36]. In these materials, defects or impurities locally disturb long-range electronic correlations, induce local moments (magnetic clusters) at their neighbor sites, and develop inhomogeneous spin susceptibility. This results in discrepancy between the bulk-χ\chi and the NMR KK at low TT.

Refer to caption
Figure 4: (Color online) The TT dependence of 1/T21/T_{2} measured at several different HH in HaH\|a. The 1/T21/T_{2} starts to increase below THT_{\rm H} and exhibits a peak at TPT_{\rm P}. With further decreasing TT, the 1/T21/T_{2} shows a minimum and then increases again below about TLT_{\rm L}.
Refer to caption
Figure 5: (Color online) The TT-HH phase diagram with the contour plot of 1/T21/T_{2} in HaH\|a. The phase diagram includes the THT_{\rm H}, TPT_{\rm P} and TLT_{\rm L} extracted from the TT profile of 1/T21/T_{2}, and the other characteristic temperatures, Tχ,maxT_{\rm\chi,max}, TT^{\rm*} and TμT_{\rm\mu} reported previously from different experimental techniques.

Next we discuss low-energy spin dynamics. Figure 4 shows the TT-dependence of 1/T21/T_{2} measured at several different HH. Although the spectrum broadening was observed at low TT, a unique T2T_{2} value was obtained at each temperature on the peak position of the spectrum. We found that there are two characteristic structures in the temperature profile of 1/T21/T_{2}. At the lowest HH of 0.68 T, 1/T21/T_{2} increases gradually below THT_{\rm H}\sim30 K and exhibits a broad peak at TPT_{\rm P}\sim16 K. The THT_{\rm H} agrees with the temperature below which the NMR line width shows the sudden broadening in Fig. 3. With further decreasing TT, 1/T21/T_{2} shows a minimum and then increases again below about TLT_{\rm L}\sim7 K. We can see that the high-TT anomaly (the red-colored region) is substantially enhanced and broadened with increasing HH, whereas the low-TT anomaly (the blue-colored region) is not much affected by HH.

In Fig. 5, we summarize the TT-HH phase diagram of UTe2 in HaH\|a. The phase diagram includes the THT_{\rm H}, TPT_{\rm P} and TLT_{\rm L} extracted from the temperature profile of 1/T21/T_{2}. These temperatures are certainly connected to characteristic temperatures, Tχ,maxT_{\rm\chi,max}, TT^{\rm*} and TμT_{\rm\mu} reported previously; it has been reported that the χb(T)\chi_{b}(T) shows a broad maximum at Tχ,maxT_{\rm\chi,max}[1, 23, 37], and resistivity, thermal-expansion and specific-heat data show anomalies at TT^{\rm*} [38, 39, 25]. TμT_{\rm\mu} is defined here as the temperature below which the μ\muSR relaxation rate shows a rapid increase at zero-field [16]. For UTe2, it has been argued that the energy scale of Tχ,maxT_{\rm\chi,max} corresponds to that of the field induced metamagnetic transition for H||bH||b [23, 37, 25]. In addition, the Kondo temperature has been estimated to be 20-26 K, thus also close to Tχ,maxT_{\rm\chi,max}. As we will discuss later, our experiments imply that long-range electronic correlations also start to develop within the U-ladder below THTχ,maxT_{\rm H}\simeq T_{\rm\chi,max}.

In general, 1/T21/T_{2} is given by the sum of electronic and nuclear contributions, 1/T2=(1/T2)el+(1/T2)nu1/T_{2}=(1/T_{2})^{\rm el}+(1/T_{2})^{\rm nu}. The (1/T2)nu(1/T_{2})^{\rm nu} originates from the spin-spin coupling between like nuclei, and hence, should be proportional to the square root of isotope concentration. For UTe2, 1/T21/T_{2} values are nearly identical between the natural abundance (7%7\%) and 125Te enriched (\sim99%) sample [17], and hence (1/T2)el(1/T2)nu(1/T_{2})^{\rm el}\gg(1/T_{2})^{\rm nu}. Further, the electronic contribution consists of two terms, (1/T2)el=(1/T2)el+(1/T2)el(1/T_{2})^{\rm el}=(1/T_{2})^{\rm el}_{\|}+(1/T_{2})^{\rm el}_{\bot} with (1/T2)elG(0)(1/T_{2})^{\rm el}_{\|}\propto G_{\|}(0) and (1/T2)elG(ωNMR)(1/T_{2})^{\rm el}_{\bot}\propto G_{\bot}(\omega_{\rm NMR}), where ωNMR\omega_{\rm NMR} is the NMR frequency and Gα(ω)=hα(t)hα(0)exp(iωt)𝑑tG_{\alpha}(\omega)=\int_{-\infty}^{\infty}\left<h_{\alpha}(t)h_{\alpha}(0)\right>\exp(i\omega t)dt is the spectral density of the fluctuating hyperfine field, hα(t)h_{\alpha}(t). Thus, (1/T2)el(1/T_{2})^{\rm el}_{\|} is driven by the longitudinal component of magnetic fluctuations at nearly zero frequency (of the order of kHz or lower), while (1/T2)el(1/T_{2})^{\rm el}_{\bot} is driven by the transverse (\bot) components of the fluctuations at the NMR frequency (\sim0.1 GHz) [40]. The latter fluctuations also generate the nuclear spin-lattice relaxation process 1/T11/T_{1}, which, however, has been found to show no significant anomaly at low-TT for each direction of HH [6, 17]. Therefore, the low-TT anomalies observed in 1/T21/T_{2} are attributed to the (1/T2)el(1/T_{2})^{\rm el}_{\|}, thus demonstrating the occurrence of extremely slow and longitudinal fluctuations of the h(t)h_{\|}(t) in the kilohertz or less regions along the aa-axis.

Note that the intensity of electronic fluctuations in correlated electron systems is generally assumed to be structure-less in frequencies below megahertz region [26, 27]. This is mostly because the energy scale of the transfer integrals and Coulomb repulsions dominating fluctuations are all in terahertz region. However, the situation is drastically changed if the correlated electrons develop a new length scale, much longer than the atomic distance scale. The new length scale would provide extremely slow fluctuations, in particular, near an electronic phase boundary. Typical examples have been seen in organic materials near a metal-Mott insulator boundary [26, 27, 28]. In these materials, the electronic state becomes extremely sensitive to disorder when it approaches to the boundary.

Theoretically, UTe2 has been suggested to be located near a magnetic instability between FM and AFM order, where a long-range static order is suppressed by magnetic frustrations [41, 42]. Recent neutron scattering experiments also indicated an intra-ladder FM coupling together with an inter-ladder AFM coupling along the bb-axis [19]. However, for the AFM fluctuations detected by the neutron measurements, there was no signature of softening down to 2 K. Therefore, the slow electronic dynamics detected by 1/T21/T_{2} would be concerned with the development of the long-range FM correlations within the U-ladder below THT_{\rm H}. Indeed, as seen in Fig. 5, the anomaly below THT_{\rm H} is broadened and shifted to higher TT with increasing HH, suggesting the FM character of the fluctuations along the aa-axis. The observed NMR line broadening below THT_{\rm H} would be attributed to spatially distributed spin susceptibility induced by disturbing the long-range FM correlations with tiny amount of disorder or defects within the ladder [25, 43].

On the other hand, however, we can not exclude the possibility that the slow fluctuations might occur in charge channel, if the system would be located near an electronic phase boundary [26]. It is expected that the fluctuations of the charge or the electron density at the Fermi energy cause the time-dependent modulations of the hyperfine coupling strength between U spins and Te nuclei, leading to the slow fluctuations of the h(t)h_{\|}(t). As mentioned, the anomaly at TT^{*}=121512\sim 15 K has been detected not only in 1/T21/T_{2} but also in resistivity and thermodynamic measurements [38, 39, 25]. Certainly, there is some impact on electronic band structure around TT^{*}. For the electronic state of UTe2, first-principle calculations initially predict an insulating state [9], and then the correlation effect of ff-electrons causes an insulator-metal transition [41, 44, 45]. Therefore, together with the magnetic instability, Fermi surface instability might also exist in UTe2, where the Kondo effect would play a crucial role [25]. In this context, it is interesting to notice that UTe2 exhibits the slow electronic dynamics resembling disordered organic materials in the vicinity of a metal-Mott insulator boundary [26, 27, 28].

Finally, we note that the broad peak in 1/T21/T_{2} might indicate the occurrence of some symmetry lowing in the electronic state below TPTT_{\rm P}\simeq T^{*}, allowing a direct second order phase transition from the paramagnetic state to a non-unitary SC state, which is recently suggested by various experiments[46, 47, 48], but usually not allowed in the crystallographic symmetry of UTe2[49, 50, 47, 51]. Further experiments are certainly required to understand the unconventional electronic state established behind the triplet SC.

In summary, NMR 1/T21/T_{2} measurements in HaH\|a revealed slow electronic dynamics developing in the paramagnetic state of UTe2. We found that the slow fluctuations along the aa-axis emerge below Tχ,max=3040T_{\rm\chi,max}=30-40 K and have a peak around T=1215T^{\rm*}=12-15 K, followed by another rapid increase below Tμ=57T_{\rm\mu}=5-7 K. The behavior is concerned with the successive growth of long-range electronic correlations within the U-ladder below Tχ,maxT_{\rm\chi,max}, although the origin of the two anomalies is unclear at the present stage. At the low TT, possibly existing tiny amounts of disorder or defects within the ladder locally disturb the long-range correlations, and develop an inhomogeneous electronic state associated with the low-TT anomaly in the χa(T)\chi_{a}(T). We suggest that UTe2 would be located on the paramagnetic side near an electronic phase boundary, where either the magnetic or Fermi-surface instability would be the origin of the characteristic fluctuations.

Acknowledgements

We are grateful for stimulating discussions with Y. Yanase, W. Knafo, J. P. Brison, J. Flouquet, M. Horvatić, M.-H. Julien, M. Hirata and V. P. Mineev. A part of this work was supported by JSPS KAKENHI Grant Numbers 19K03726, 19H00646, 20H00130, and 20KK0061.

References

  • [1] S. Ran, C. Eckberg, Q.-P. Ding, Y. Furukawa, T. Metz, S. R. Saha, I.-L.Liu, M. Zic, H. Kim, J. Paglione, and N. P. Butch, Science 365, 684 (2019).
  • [2] N. Read and D. Green, Phys. Rev. B 61, 10267-10297 (2000).
  • [3] D. A. Ivanov, Phys. Rev. Lett. 86, 268-271 (2001).
  • [4] L. Fu and E. Berg, Phys. Rev. Lett. 105, 097001 (2010).
  • [5] M. Sato, Phys. Rev. B 81, 220504 (2010).
  • [6] G. Nakamine, S. Kitagawa, K. Ishida, Y. Tokunaga, H. Sakai, S. Kambe, A. Nakamura, Y. Shimizu, Y. Homma, D. Li, F. Honda, and D. Aoki, J. Phys. Soc. Jpn. 88, 113703 (2019).
  • [7] G. Nakamine, K. Kinjo, S. Kitagawa, K. Ishida, Y. Tokunaga, H. Sakai, S. Kambe, A. Nakamura, Y. Shimizu, Y. Homma, D. Li, F. Honda, and D. Aoki, Phys. Rev. B 103, L100503 (2021).
  • [8] G. Nakamine, K. Kinjo, S. Kitagawa, K. Ishida, Y. Tokunaga, H. Sakai, S. Kambe, A. Nakamura, Y. Shimizu, Y. Homma, D. Li, F. Honda, and D. Aoki, J. Phys. Soc. Jpn. 90 064709 (2021).
  • [9] D. Aoki, A. Nakamura, F. Honda, D.X. Li, Y. Homma Y. Shimizu, Y-J. Sato, G. Knebel, J-P. Brison, A Pourret, D. Braithwaite, G. Lapertot, Q. Niu, M. Valiska, H. Harima, and J. Flouquet, J. Phys. Soc. Jpn. 88, 043702 (2019).
  • [10] G. Knebel,W. Knafo, A. Pourret, Q. Niu, M. Valiska, D. Braithwaite, G. Lapertot, M. Nardone, A. Zitouni, S. Mishra, I. Sheikin, G. Seyfarth, J.-P. Brison, D. Aoki, and J. Flouquet, J. Phys. Soc. Jpn. 88, 063707 (2019).
  • [11] G. Knebel, M. Kimata, M. Valiska, F. Honda, D. X. Li, D. Braithwaite, G. Lapertot, W. Knafo, A. Pourret, Y. J. Sato, Y. Shimizu, T. Kihara, J. P. Brison, J. Flouquet, and D. Aoki, J. Phys. Soc. Jpn. 89, 053707 (2020).
  • [12] S. Ran, I. Liu, Y. Eo, D. J. Campbell, P. M. Neves, W. T. Fuhrman, S. R. Saha, C. Eckberg, H. Kim, D. Graf, F. Balakirev, J. Singleton, J. Paglione and N. P. Butch, Nat. Phys 15, 1250 (2019).
  • [13] W. Knafo, M. Nardone, M. Valiska, A. Zitouni, G. Lapertot, D. Aoki, G. Knebel, and D. Braithwaite, Commun Phys 4, 40 (2021).
  • [14] D. Aoki, F. Honda, G. Knebel, D. Braithwaite, A. Nakamura, D. X. Li, Y. Homma, Y. Shimizu, Y. J. Sato, J. P. Brison, and J. Flouquet, J. Phys. Soc. Jpn. 89, 053705 (2020).
  • [15] D. Braithwaite, M. Valiska, G. Knebel, G. Lapertot, J. P. Brison, A. Pourret, M. E. Zhitomirsky, J. Flouquet, F. Honda, and D. Aoki, Communications Physics 2, 147 (2019).
  • [16] S. Sundar, S. Gheidi, K. Akintola, A. M. Cote, S. R. Dunsiger, S. Ran, N. P. Butch, S. R. Saha, J. Paglione, and J. E. Sonier, Phys. Rev. B 100, 140502 (2019).
  • [17] Y. Tokunaga, H. Sakai, S. Kambe, T. Hattori, N. Higa, G. Nakamine, S. Kitagawa, K. Ishida, A. Nakamura, Y. Shimizu, Y. Homma, D. Li, F. Honda, and D. Aoki, J. Phys. Soc. Jpn. 88, 073701 (2019).
  • [18] C. Duan, K. Sasmal, M. B. Maple, A. Podlesnyak, J.-X. Zhu, Q. Si, and P. Dai, Phys. Rev. Lett. 125, 237003 (2020).
  • [19] W. Knafo, G. Knebel, P. Steffens, K. Kaneko, A. Rosuel, J.-P. Brison, J. Flouquet, D. Aoki, G. Lapertot, and S. Raymond, Phys. Rev. B 104, L100409 (2021).
  • [20] P. F. S. Rosa, A. Weiland, S. S. Fender, B. L. Scott, F. Ronning, J. D. Thompson, E. D. Bauer, and S. M. Thomas, arXiv:2110.06200.
  • [21] V. Hutanu, H. Deng, S. Ran, W. T. Fuhrman, H. Thoma and N. P. Butch, Acta Cryst. B 76, 137, (2020).
  • [22] S. Ikeda, H. Sakai, D. Aoki, Y. Homma, E. Yamamoto, A. Nakamura, Y. Shiokawa, Y. Haga and Y. Onuki J. Phys. Soc. Jpn. 75 116 (2006).
  • [23] A. Miyake, Y. Shimizu, Y. J. Sato, D. Li, A. Nakamura, Y. Homma, F. Honda, J. Flouquet, M. Tokunaga, and D. Aoki, J. Phys. Soc. Jpn. 88, 063706 (2019).
  • [24] D. Li, A. Nakamura, F. Honda, Y. J. Sato, Y. Homma, Y. Shimizu, J. Ishizuka, Y. Yanase, G. Knebel, J. Flouquet, and D. Aoki, J. Phys. Soc. Jpn. 90, 073703 (2021).
  • [25] D. Aoki, J.-P. Brison, J. Flouquet, K. Ishida, G. Knebel, Y. Tokunaga, Y. Yanase, arXiv:2110.10451.
  • [26] T. Itou, E. Watanabe, S. Maegawa, A. Tajima, N. Tajima, K. Kubo, R. Kato, K. Kanoda, Sci. Adv. 3 e1601594 (2017).
  • [27] R. Yamamoto, T. Furukawa, K. Miyagawa, T. Sasaki, K. Kanoda and T. Itou, Phys. Rev. Lett. 124, 046404 (2020).
  • [28] M. Urai, K. Miyagawa, T. Sasaki, H. Taniguchi, and K. Kanoda, Phys. Rev. Lett. 124, 117204 (2020).
  • [29] N. Fujiwara, H. Yasuoka, Y. Fujishiro, M. Azuma, and M. Takano, Phys. Rev. Lett. 80, 604 (1998).
  • [30] S. Ohsugi, Y. Tokunaga, K. Ishida, Y. Kitaoka, M. Azuma, Y. Fujishiro, and M. Takano, Phys. Rev. B 60, 4181 (1999).
  • [31] L. K. Alexander, J. Bobroff, A. V. Mahajan, B. Koteswararao, N. Laflorencie, and F. Alet, Phys. Rev. B 81, 054438 (2010).
  • [32] F. Casola, T. Shiroka, S. Wang, K. Conder, E. Pomjakushina, J. Mesot, and H.-R. Ott, Phys. Rev. Lett. 105, 067203 (2010).
  • [33] J. Bobroff, H. Alloul, Y. Yoshinari, A. Keren, P. Mendels, N. Blanchard, G. Collin, and J.-F. Marucco Phys. Rev. Lett. 79, 2117 (1997).
  • [34] M.-H. Julien, T. Feher, M. Horvatic, C. Berthier, O. N. Bakharev, P. Segransan, G. Collin, and J.-F. Marucco Phys. Rev. Lett. 84, 3422 (2000).
  • [35] S. Ouazi, J. Bobroff, H. Alloul, and W. A. MacFarlane, Phys. Rev. B 70, 104515 (2004).
  • [36] H. Alloul, J. Bobroff, M. Gabay, and P. J. Hirschfeld, Rev. Mod. Phys. 81, 45 (2009).
  • [37] W. Knafo, M. Valiska, D. Braithwaite, G. Lapertot, G. Knebel, A. Pourret, J.-P. Brison, J. Flouquet, and D. Aoki, J. Phys. Soc. Jpn. 88, 063705 (2019).
  • [38] K. Willa, F. Hardy, D. Aoki, D. Li, P. Wiecki, G. Lapertot, C. Meingast, Phys. Rev. B 104, 205107 (2021).
  • [39] Y. S. Eo, S. R. Saha, H. Kim, S.Ran, J. A. Horn, H. Hodovanets, J. Collini, W. T. Fuhrman, A. H. Nevidomskyy, N. P. Butch, M.S. Fuhrer, J. Paglione, arXiv:2101.03102.
  • [40] Y. Tokunaga, D. Aoki, H. Mayaffre, S. Kramer, M.-H. Julien, C. Berthier, M. Horvatic, H. Sakai, S. Kambe, and S. Araki, Phys. Rev. Lett. 114, 216401 (2015).
  • [41] Y. Xu, Y. Sheng and Y. Yang, Phys. Rev. Lett. 123, 217002 (2019).
  • [42] J. Ishizuka and Y. Yanase, Phys. Rev. B 103 094504 (2021).
  • [43] Y. Haga, P. Opletal, Y. Tokiwa, E. Yamamoto, Y. Tokunaga, S. Kambe, H. Sakai, arXiv:2112.13468.
  • [44] J. Ishizuka, S. Sumita, A. Daido and Y. Yanase, Phys. Rev. Lett. 123, 217001 (2019).
  • [45] A.B. Shick and W.E. Pickett, Phys. Rev. B 100,134502 (2019).
  • [46] L. Jiao, S. Howard, S. Ran, Z. Wang, J. O. Rodriguez, M. Sigrist, Z. Wang, N. P. Butch and V. Madhavan, Nature 579, 523 (2020).
  • [47] S. Kittaka, Y. Shimizu, T. Sakakibara, A. Nakamura, D. Li, Y. Homma, F. Honda, D. Aoki, and K. Machida, Phys. Rev. Research 2, 032014(R) (2020).
  • [48] I. M. Hayes, D. S. Wei, T. Metz, J. Zhang, Y. S. Eo, S. Ran, S. R. Saha, J. Collini, N. P. Butch, D. F. Agterberg, A. Kapitulnik, and J. Paglione, Science 373, 797 (2021).
  • [49] K. Machida, J. Phys. Soc. Jpn. 89, 065001 (2020).
  • [50] K. Machida, Phys. Rev. B 104 014514 (2021).
  • [51] V. P. Mineev, J. Phys. Soc. Jpn. 77, 103702 (2008).