high pressure µsr study of quantum phase transition in ...many kinds of hkaf have been investigated...

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High pressure μSR study of quantum phase transition in CeNiAsO H. Guo, *1, *2 Y. Luo, *1 I. Watanabe, *2 and Z. Xu *1 The discovery of superconductivity in LaFeAsO 1-y F y systems 1) triggers not only a new search of the iron- based superconductors, but also studies of the Kondo effect when La is replaced by magnetic ions such as Ce. The Fe 3d electrons in such systems usually undergo a spin-density-wave (SDW) transition at about 140 K on top of the much lower temperature where the 4f elec- trons become magnetically ordered. 2) In order to study the 4f electronic properties, we therefore focused on a Ni-based compound, namely, CeONiAs, instead of Fe- based compounds since the Ni ions are not long-ranged magnetically ordered in these compounds, as observed by experiments and theoretical calculations. 3) Our previous studies including magnetic suscepti- bility, transport, and thermal dynamic measurements show that CeONiAs undergoes two successive magnet- ic transitions at T 1 = 9.3 K and T 2 = 7.3 K, respective- ly, and these two transitions can be suppressed both by hydrostatic and chemical pressures (P ). When P> 4 kbar, T 1 can be hardly seen, while T 2 is continuously suppressed with a critical value of P c 6.3 kbar. Re- sistivity measurements indicate that there is a quan- tum phase transition at P c . In order to reveal the role of magnetic correlations around the quantum critical point (QCP), and the evolution of magnetic structure with pressure, we have performed µSR experiments with gas pressures up to 6.1 kbar on CeONiAs 0.9 P 0.1 , where the substitution of As by P is expected to reduce P c . During the high pressure µSR measurement, most of the muons are stopped at the pressure cell made of Cu, and therefore, muon spin precession is hardly observed even when magnetic ordering appears in the sample, which limits our analyses of the evolution of the magnetic structure with pressure from the obser- vation of muon spin precession in the zero field (ZF) measurement. Alternatively, we performed transverse field (TF) measurements and the spectra were fitted using the following function: A(t)= A ini cos(γ μ Bt + φ)exp(-λt) (1) where A int is the initial asymmetry, γ μ is the muon gyromagnetic ratio, B is the magnetic field, and λ is the muon spin relaxation rate. Figure 1(a) shows the temperature dependence of the initial asymmetry, A ini at ambient pressure (A.P.) and P = 6.1 kbar. At A.P., A ini is nearly tempera- ture independent at high temperatures, and decreases sharply below approximately 10 K. No further signif- icant change is observed below 10 K due to the low *1 Department of Physics, Zhejiang University *2 RIKEN Nishina Center Fig. 1. Temperature dependence of the extracted param- eters. (a) The initial asymmetry. (b) The muon spin relaxation rate, λ. The arrows indicate the magnetic transition temperatures. signal-to-background ratio. The transition tempera- ture is suppressed to approximately 6 K when P = 6.1 kbar. Fig. 1(b) shows the temperature dependence of the muon spin relaxation rate λ. The substantial in- crease of λ below about 10 K and 6 K, respectively, at A.P. and P = 6.1 kbar is consistent with the results of the temperature dependence of A ini . The appear- ance of the internal field will increase the internal field distribution width at the muon site, thus enhancing the muon spin relaxation rate. Owing to the usage of a pulsed muon source, the increase in muon spin relaxation rate will usually lead to a decrease in the initial asymmetry. Thus, our current results confirm the magnetic ordering from the microscopic view point. The application of high pressures up to 6.1 kbar also confirms that the magnetic ordering is suppressed by pressure. Unfortunately, valuable information about the evolution of the internal field with the pressure cannot be obtained since we cannot observe the muon spin precession directly as mentioned above. References 1) Y. Kamihara, H. Hiramatsu, M. Hirano, R. Kawamura, H. Yanagi, T. Kamiya, and H. Hosono, J. Am. Chem. Soc. 128, 10012 (2006). 2) J. Zhao, Q. Huang, C. de la Cruz, S. Li, J. W. Lynn, Y. Chen, M. A. Green, G. F. Chen, G. Li, Z. Li, J. L. Luo, N. L. Wang, and P. Dai, Nature Materials 7, 953 (2008). 3) T. M. McQueen, T. Klimczuk, A. J. Williams, Q. Huang, and R. J. Cava, Phys. Rev. B 79, 172502 (2009). - 261 - -2. Atomic & Solid State Physics (Muon) RIKEN Accel. Prog. Rep. 48 (2015)

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Page 1: High pressure µSR study of quantum phase transition in ...many kinds of HKAF have been investigated as the candidate for the ideal kagome spin lattice material. Another new candidate

Investigation of magnetic ground states in mixed kagome systems(Rb1−xCsx)2Cu3SnF12 by µSR

T. Suzuki,∗1,∗4 K. Katayama,∗2 H. Tanaka,∗2 T. Goto,∗3 and I. Watanabe∗4

The Heisenberg kagome antiferromagnet (HKAF)has attracted much attention in magnetism, becauseseveral frustration and quantum effects have been in-dicated by theories. For example, in the classical spinmodel case for HKAF, the q = 0 or

√3×

√3 magnetic

structure is stabilized when the next-nearest-neighborinteraction is considered. In the case of S = 1/2 k-agome lattice, exotic magnetic ground states have beentheoretically predicted. For example, numerical calcu-lations revealed that the ground state is a magnetical-ly disordered spin liquid. In the ground state, tripletexcitations are gapped, and there exists the continu-um of low-lying singlet states below the triplet gap1).Valence-bond crystal by a periodic arrangement of s-inglet dimers has also been proposed as the magneticground state of S = 1/2 HKAF2). Experimentally,many kinds of HKAF have been investigated as thecandidate for the ideal kagome spin lattice material.

Another new candidate for the ideal kagome latticewith an exotic magnetic ground state was reportedby Ono et al. The cupric compound A2Cu3SnF12 (A= Cs, Rb), which is the subject of this study, is anewly synthesized family of S = 1/2 HKAF3,4). ForCs2Cu3SnF12, the weak-ferromagnetic behavior is ob-served below TN = 20 K, and it is suggested that theantiferromagnetic ordered state appears4). On the oth-er hand, for Rb2Cu3SnF12, the first realization of the”pinwheel” valence bond solid (VBS) ground state inthe S = 1/2 HKAF are confirmed by inelastic neu-tron measurements5). Quite recently, mixed kagomesystems (Rb1−xCsx)2Cu3SnF12 have been prepared6).By magnetic susceptibility and specific heat measure-ments on single crystals, they reported a phase dia-gram, which shows the existence of the quantum phasetransition from the VBS to the AF phase at xc = 0.53.In this concentration, the spin gap vanishes and theordered state disappears from the view point of mag-netization results.

We carried out LF-µSR measurements in x = 0.53single crystal to investigate dynamical magnetic prop-erties microscopically. Figure 1 (a) shows LF-µSRtime spectra in 200 gauss at various temperatures.It is emphasized that no disappearance of the initialasymmetry is observed. Below 3 K, time spectra arewell fitted by the two component function as follows:A(t) = A1 exp(−λ1t)+A2 exp(−λ2t). Here, A1 = 0.58,A2 = 0.42. As shown in Fig. 1 (b), λ1 increases

∗1 College of Engineering, Shibaura Institute of Technology∗2 Department of Physics, Tokyo Institute of Technology∗3 Department of Physics, Sophia University∗4 RIKEN Nishina Center

0 3 6 9 120

0.2

0.4

0.6

0.8

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Corr

ecte

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sym

metr

y

t (µs)

LF200G

19 K

5 K

4 K

3 K

1 K

0.27 K

0 3 6 9 120

0.2

0.4

0.6

0.8

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Corr

ecte

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sym

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LF-µSR

200 G

3000 G

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1000 G1500 G

0 10 200

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T = 0.27 K

(a) (c)

(b) (d)

Fig. 1. (a)Temperature dependence of the time spectra in

the LF of 200 gauss. (b) Temperature dependence of

the muon spin relaxation rate in LF 200 gauss. (c) LF-

µSR time spectra above 200 gauss up to 3000 gauss at

0.27 K. (d) LF dependence of the muon spin relaxation

rate at 0.27 K.

with decreasing temperature. LF-dependence of timespectra at 0.27 K is shown in Fig. 1 (c), and LF-dependence of relaxation rates is shown in (d). Muonspin relaxation rates are inversely proportional to LF,and such change indicates “white” frequency spectra,which means the spectra are described by summationof continuously distributed frequencies using the Red-field formula. These results suggest that the inter-nal fields fluctuate, and are consistent with reportedmacroscopic results at least down to 0.27 K.

References1) H. C. Jiang et al.: Phys. Rev. Lett. 101, 117203 (2008).2) R. R. P. Singh et al.: Phys. Rev. B 77, 144415 (2008).3) M. Muller et al.: Z. Anorg. Allg. Chem. 621, 993 (1995).4) T. Ono et al., Phys. Rev. B 79, 174407 (2009).5) K. Matan et al., Nature Phys. 6, 865 (2010).6) K. Katayama et al.: arXive:1412.5770v1 [cond-matt.str-

el].

High pressure µSR study of quantum phase transition in CeNiAsO

H. Guo,∗1,∗2 Y. Luo,∗1 I. Watanabe,∗2 and Z. Xu∗1

The discovery of superconductivity in LaFeAsO1−yFy

systems1) triggers not only a new search of the iron-based superconductors, but also studies of the Kondoeffect when La is replaced by magnetic ions such as Ce.The Fe 3d electrons in such systems usually undergo aspin-density-wave (SDW) transition at about 140 K ontop of the much lower temperature where the 4f elec-trons become magnetically ordered.2) In order to studythe 4f electronic properties, we therefore focused on aNi-based compound, namely, CeONiAs, instead of Fe-based compounds since the Ni ions are not long-rangedmagnetically ordered in these compounds, as observedby experiments and theoretical calculations.3)

Our previous studies including magnetic suscepti-bility, transport, and thermal dynamic measurementsshow that CeONiAs undergoes two successive magnet-ic transitions at T1 = 9.3 K and T2 = 7.3 K, respective-ly, and these two transitions can be suppressed both byhydrostatic and chemical pressures (P ). When P > 4kbar, T1 can be hardly seen, while T2 is continuouslysuppressed with a critical value of Pc ∼ 6.3 kbar. Re-sistivity measurements indicate that there is a quan-tum phase transition at Pc. In order to reveal the roleof magnetic correlations around the quantum criticalpoint (QCP), and the evolution of magnetic structurewith pressure, we have performed µSR experimentswith gas pressures up to 6.1 kbar on CeONiAs0.9P0.1,where the substitution of As by P is expected to reducePc.During the high pressure µSR measurement, most

of the muons are stopped at the pressure cell madeof Cu, and therefore, muon spin precession is hardlyobserved even when magnetic ordering appears in thesample, which limits our analyses of the evolution ofthe magnetic structure with pressure from the obser-vation of muon spin precession in the zero field (ZF)measurement. Alternatively, we performed transversefield (TF) measurements and the spectra were fittedusing the following function:

A(t) = Ainicos(γµBt+ φ)exp(−λt) (1)

where Aint is the initial asymmetry, γµ is the muongyromagnetic ratio, B is the magnetic field, and λ isthe muon spin relaxation rate.Figure 1(a) shows the temperature dependence of

the initial asymmetry, Aini at ambient pressure (A.P.)and P = 6.1 kbar. At A.P., Aini is nearly tempera-ture independent at high temperatures, and decreasessharply below approximately 10 K. No further signif-icant change is observed below 10 K due to the low

∗1 Department of Physics, Zhejiang University∗2 RIKEN Nishina Center

Fig. 1. Temperature dependence of the extracted param-

eters. (a) The initial asymmetry. (b) The muon spin

relaxation rate, λ. The arrows indicate the magnetic

transition temperatures.

signal-to-background ratio. The transition tempera-ture is suppressed to approximately 6 K when P = 6.1kbar. Fig. 1(b) shows the temperature dependence ofthe muon spin relaxation rate λ. The substantial in-crease of λ below about 10 K and 6 K, respectively, atA.P. and P = 6.1 kbar is consistent with the resultsof the temperature dependence of Aini. The appear-ance of the internal field will increase the internal fielddistribution width at the muon site, thus enhancingthe muon spin relaxation rate. Owing to the usageof a pulsed muon source, the increase in muon spinrelaxation rate will usually lead to a decrease in theinitial asymmetry. Thus, our current results confirmthe magnetic ordering from the microscopic view point.The application of high pressures up to 6.1 kbar alsoconfirms that the magnetic ordering is suppressed bypressure. Unfortunately, valuable information aboutthe evolution of the internal field with the pressurecannot be obtained since we cannot observe the muonspin precession directly as mentioned above.

References1) Y. Kamihara, H. Hiramatsu, M. Hirano, R. Kawamura,

H. Yanagi, T. Kamiya, and H. Hosono, J. Am. Chem.Soc. 128, 10012 (2006).

2) J. Zhao, Q. Huang, C. de la Cruz, S. Li, J. W. Lynn,Y. Chen, M. A. Green, G. F. Chen, G. Li, Z. Li, J. L.Luo, N. L. Wang, and P. Dai, Nature Materials 7, 953(2008).

3) T. M. McQueen, T. Klimczuk, A. J. Williams, Q.Huang, and R. J. Cava, Phys. Rev. B 79, 172502 (2009).

- 260 - - 261 -

Ⅲ-2. Atomic & Solid State Physics (Muon) RIKEN Accel. Prog. Rep. 48 (2015)RIKEN Accel. Prog. Rep. 48 (2015) Ⅲ-2. Atomic & Solid State Physics (Muon)

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