Terahertz conductivity of the magnetic Weyl semimetal Mn{}_{3}Sn films

Terahertz conductivity of the magnetic Weyl semimetal MnSn films

Bing Cheng    Youcheng Wang    D. Barbalas The Institute of Quantum Matter, Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA    Tomoya Higo Institute for Solid State Physics, University of Tokyo, Kashiwa, 227-8581, Japan    S. Nakatsuji The Institute of Quantum Matter, Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA Institute for Solid State Physics, University of Tokyo, Kashiwa, 227-8581, Japan    N. P. Armitage The Institute of Quantum Matter, Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA Japan Society for the Promotion of Science, International Research Fellow, Institute for Solid State Physics, The University of Tokyo, Kashiwa 277-8581, Japan
July 20, 2019
Abstract

MnSn is a non-collinear antiferromagnet which displays a large anomalous Hall effect at room temperature. It is believed that the principal contribution to its anomalous Hall conductivity comes from Berry curvature. Moreover, dc transport and photoemission experiments have confirmed that MnSn may be an example of a time-reversal symmetry breaking Weyl semimetal. Due to a small, but finite moment in the room temperature inverse triangular spin structure, which allows control of the Hall current with external field, this material has garnered much interest for next generation memory devices and THz spintronics applications. In this work, we report a THz range study of oriented MnSn thin films as a function of temperature. At low frequencies we found the optical conductivity can be well described by a single Drude oscillator. The plasma frequency is strongly suppressed in a temperature dependent fashion as one enters the 260 K helical phase. This may be associated with partial gapping of the Fermi surfaces that comes from breaking translational symmetry along the c-axis. The scattering rate shows quadratic temperature dependence below 200 K, highlighting the possible important role of interactions in this compound.

preprint: AIP/123-QED

The anomalous Hall effect (AHE) conventionally occurs in ferromagnetic metals (FMs) and is usually interpreted as an effect beyond the ordinary Hall effect that arises from spontaneous magnetizationNagaosa et al. (2010). It can arise based on three different mechanisms: side jump scattering, skew scattering, and intrinsic effects. The latter arises through Berry curvature. This Berry curvature is determined by the geometry of Bloch wavefunctions and acts in many ways as an effective magnetic field in momentum space. Recently, the possibility of an intrinsic AHE in systems without net magnetization has been explored, such as in spin liquid and antiferromagnetic systemsMachida et al. (2010); Nakatsuji, Kiyohara, and Higo (2015); Kiyohara, Tomita, and Nakatsuji (2016); Nayak et al. (2016). One of the most promising possibilities are non-collinear antiferromagnets. In most antiferromagnets with collinear spins, the Berry curvature is zero. However theory has found that in a triangular spin structures with non-collinear moments a Berry curvature can be presentChen, Niu, and MacDonald (2014); Yang et al. (2017). One of the most likely realizations for this physics is MnSnNakatsuji, Kiyohara, and Higo (2015), which has attracted recent attention because of its unique magnetic structure and symmetries. Below T 420 K, it undergoes an antiferromagnetic transition and enters a non-collinear inverse triangular spin stateTomiyoshi et al. (1986); Ohmori et al. (1987) that shows a large anomalous Hall conductivity, Nernst effect, and magneto-optical Kerr effect (MOKE) Nakatsuji, Kiyohara, and Higo (2015); Ikhlas and et al. (2017); Higo and et al. (2018). The system transitions to a helical (spiral) spin structure on cooling below 260 K in which the AHE is quenched Sung et al. (2018); Ohmori et al. (1987); Cable, Wakabayashi, and Radhakrishna (1993).

First-principle band structure calculations of MnSn showed multiple pairs of Weyl nodes and three-dimensional linear dispersions in momentum space that have been confirmed by recent photoemission experimentsKuroda and et al. (2015). MnSn is of particular applications interest because in the non-collinear inverse triangular spin state, the system also exhibits a very small net magnetic moments of  3 m/Mn that allows the magnetic state and the AHE to be controlled and manipulated with external field, while giving negligible fringe field itself. This makes this system of interest for next generation memory devices and THz spintronics. In this regard THz dynamics of MnSn are particularly important for applications.

In this work, we take advantage of recent technical advances in thin film preparation Higo et al. (2018) to present the first THz range optical study of a polycrystalline MnSn thin film. We found the complex optical conductivity can be well reproduced by a single Drude oscillator, indicative of excellent metallic conduction. The plasma frequency of the Drude oscillator is suppressed with lowering temperature below 200 K, which strongly hints at the partial gap opening below the phase transition to the helical phase at 260 K. The scattering rate has an approximately quadratic dependence on temperature at low temperature, before crossing over to a weaker temperature dependence above the 250 K scale. These features enable us to set the upper limits of the effective mass and mobility for free carriers and supports the notion of a correlated Weyl phase in MnSn.

Figure 1: (Color online) Magnetic structure of MnSn film in (a) magnetic helical phase below 260 K and (b) magnetic inverse triangular phase above 260 K. Top view of (c) helical phase and (d) inverse triangular phase. (e) dc resistivity of polycrystalline MnSn film.

Polycrystalline MnSn films were deposited to a thickness of 100 nm by DC magnetron sputtering at room temperature onto Si/SiO substrates from a MnSn target. The sputtering power and Ar gas pressure are 60 W and 0.3 Pa. The film is post-deposition annealed at 500C for 1 h. The annealing procedure after the deposition crystallizes the as-deposited amorphous film into a polycrystalline form of MnSn. Further details of the deposition and sample treatment can be found in Higo et al. (2018). XRD revealed that the almost randomly oriented polycrystalline MnSn film. This has been shown recently to allow the large anomalous Hall effect comparable to the bulk MnSn. Higo et al. (2018).

Complex values of the THz transmission of these films were measured in a home-built THz time-domain spectroscopy (TDTS) spectrometer with a closed-cycle 7 T superconducting magnet. The complex conductivity can be extracted by using the appropriate expression in the thin film approximation: Cheng et al. (2016). Here is the complex transmission function as referenced to a bare substrate, () is the complex optical conductivity, is the thickness of the film, and is the index of refraction of the substrate. is the small thickness difference between samples and reference substrates, and is the vacuum impedance, which is approximately 377 .

Fig. 1(a) to (d) depict the magnetic structure schematically of MnSn. As mentioned above, below a Neel temperature T = 420 K, MnSn orders in an inverse triangular spin configuration with negative vector chirality in the kagome lattice [Fig. 1(b)]. Mn moments lie in the ab plane and form 120 angles with each other [Fig. 1(d)]. In each magnetic primitive unit cell, there are two triangles along the vertical direction related by inversion symmetry. In this phase, a very large anomalous Hall conductivity is observed at zero field which originates from non-zero Berry curvature in momentum space induced by the cluster multipole orderSuzuki et al. (2017). Furthermore, Weyl nodes in the bulk and Fermi arcs on the surface was predicted by band structure calculations in this phase, which have been confirmed by photoemission measurementsKuroda and et al. (2015). dc transport displays a negative magnetoresistance with , which is regarded as a signature of the chiral anomaly that describes the breakdown of chiral symmetry in Weyl semimetals when presenting parallel electric and magnetic fieldsKuroda and et al. (2015). Our previous study has found that, below 260 K, the MnSn thin film undergoes a magnetic phase transition to the helical magnetic stateHigo et al. (2018) [Fig. 1(a)]. For each triangle, the Mn moments still lie in plane with 120 pattern, but the moment of each triangle is rotated by an angle about the vertical direction forming a helical structure [Fig. 1(c)]. In this phase, the anomalous Hall conductivity at zero field vanishes. Both of the magnetic states are metallic. Fig. 1(e) shows that the dc resistivity increases with increasing temperature. Above 250 K, the resistivity seems to gradually saturate. This can be either because the rate of increase of the carrier density decreases or the rate of increase of the scattering rate decreases. Optical conductivity is a powerful method to sort out these possibilities. We show below that both play a role.

Figure 2: (Color online) (a) Real and (b) imaginary parts of optical conductivity of MnSn film at different temperatures. (c) Real and imaginary parts of magneto-terahertz conductivity in Faraday geometry at 6 K.

Figs. 2(a) and (b) show the real and imaginary parts of the optical conductivity measured at different temperatures. At the low temperature of 5 K, the real part of the optical conductivity displays a well-defined conductivity peak centered at zero frequency with is an increasing function of frequency, indicative of good metallic behavior. With increasing temperature, the peak becomes broader and flattens. When further increasing temperature above 250 K, becomes flat and show weak temperature dependence. In the THz region, no phonons or other absorptions are observed. In this regard, we can use a simple Drude model to fit the optical conductivity:

(1)
Figure 3: (Color online) (a) Drude fit for real and imaginary parts of terahertz conductivity at 6 K. (b) Temperature dependent plasma frequency. (c) Temperature dependent scattering rates and its power-law fit.

Here, represents a background polarizability that originates from absorptions above the measured spectral range including phonons and electronic interband transitions. is an index that represents a possible sum over a number of the Drude oscillators. An example fit to the data at 5K is shown in Fig. 3(a). One can see that both the real and imaginary parts of the optical conductivity at 5 K can be well simulated by a single Drude oscillator.

The temperature dependent plasma frequency /2 is displayed in Fig. 3(b). One can see that /2 has very strong temperature dependence. From 5 K to 200 K, the plasma frequency increases quickly with temperature, but above 200 K it saturates. The plasma frequency is determined by carrier density and effective mass via the expression . A decreasing plasma frequency indicates the carrier density decreases or effective mass of carriers increases, or both of these effects play partial roles. As shown in Fig. 1(a) and (c), below 250 K MnSn film enters a helical magnetic state. In this state, along the axis, the magnetic moment m (along a axis) or m (along b axis) of Mn varies approximately as a sinusoidal function of the axis. This may cause partial gapping of the Fermi surface due to Fermi surface nestingFawcett (1988). In this regard, the decreasing plasma frequency with cooling may hint to the possible partial gap opening as temperature is lowered. A recent LDA calculation shows that in the helical phase, not only are Weyl points annihilated, but gaps open in the band structure in some regions of momentum space, and in other regions very flat bands form that should have small spectral weightPark and et al. (2018). This is consistent with the decreasing plasma frequency with lowering temperature.

Fig 3(c) shows the scattering rate () as a function of temperature. The overall trend is that the scattering rate decreases as temperature is lowered. However, the behavior above and below 250 K is quite different. Below 200 K, the scattering rates behave in a typical metallic fashion with power law describing the data. The temperature exponent is extracted to be = 1.9 0.1. The value of being close to 2 may indicate a quasi-Fermi-liquid behavior. In contrast, above 200 K, the scattering rate increases more slowly and seems to be saturating above 250 K. This unusual temperature dependence may be related to the fact that in the inverse triangular magnetic state, the Berry phase of the Weyl fermions may exempt some backscatterings.

We have also performed extensive measurements in perpendicular magnetic field (Faraday geometry) at low temperature, but saw essentially no effect of field in the THz range. As shown in Fig. 2(c), even at 7 T, still exhibits a textbook Drude form and does not exhibit any signature of a cyclotron resonance peak (CR). At a particular magnetic field, the CR frequency is determined by the cyclotron mass of the charge carriersWu et al. (2015). The absence of CR in the THz region suggests that these carriers have a large cyclotron mass which pushes the CR to lower frequency. A rough upper limit for CR given by this study is 0.1 THz at 7 T, which means the mass must be larger than 2 electron masses. This is an extremely large number for semimetals systems close to having Weyl band structure. The electronic mobility is estimated to be much smaller than 30 cmVs. The large cyclotron mass and low mobility at 6 K strongly indicate even in the high-temperature Weyl phase, the Weyl fermions will have large effective mass and low mobility. Recent photoemission experiment have shown that MnSn exhibits a Weyl semimetal phase with notable electronic correlationKuroda and et al. (2015). Our observation is consistent with this in that correlations will dress the carriers and increase their effective mass.

In conclusion, we have studied the THz-range optical response of MnSn thin films. The system shows a good metallic state in the whole temperature range. Magneto-terahertz conductivities at 6 K do not exhibit field dependence and strongly indicate the quasiparticles have large effective mass and low electronic mobility, consistent with the fact that MnSn is a correlated electron system. The suppression of the plasma frequency at low temperatures is consistent with the expected gapping of the Fermi surface in the spatially modulated helical phase.

We would like to thank R. Matsunaga for helpful discussions. The work at JHU was supported as part of the Institute for Quantum Matter, an Energy Frontier Research Center funded by the U.S. DOE, Office of BES under Award Number DE-SC0019331. NPA also acknowledges additional support from the Japan Society for the Promotion of Science, International Research Fellows Program that supported his visit to Tokyo. Work at ISSP was supported in part by CREST JPMJCR18T3, Japan Science and Technology Agency, by Grants-in-Aid for Scientific Research 16H02209 and Program for Advancing Strategic International Networks to Accelerate the Circulation of Talented Researchers (No. R2604) from the Japanese Society for the Promotion of Science (JSPS), and by Grants-in-Aids for Scientific Research on Innovative Areas (15H05882 and 15H05883) from the Ministry of Education, Culture, Sports, Science, and Technology of Japan.

References

  • Nagaosa et al. (2010) N. Nagaosa, J. Sinova, S. Onoda, A. H. MacDonald,  and N. P. Ong, Rev. Mod. Phys. 82, 1539 (2010).
  • Machida et al. (2010) Y. Machida, S. Nakatsuji, S. Onoda, T. Tayama,  and T. Sakakibara, Nature 463, 210 (2010).
  • Nakatsuji, Kiyohara, and Higo (2015) S. Nakatsuji, N. Kiyohara,  and T. Higo, Nature 527, 212 (2015).
  • Kiyohara, Tomita, and Nakatsuji (2016) N. Kiyohara, T. Tomita,  and S. Nakatsuji, Phys. Rev. Applied 5, 064009 (2016).
  • Nayak et al. (2016) A. K. Nayak, J. E. Fischer, Y. Sun, B. Yan, J. Karel, A. C. Komarek, C. Shekhar, N. Kumar, W. Schnelle, J. Kübler, C. Felser,  and S. S. P. Parkin, Science Advances 2 (2016).
  • Chen, Niu, and MacDonald (2014) H. Chen, Q. Niu,  and A. H. MacDonald, Phys. Rev. Lett. 112, 017205 (2014).
  • Yang et al. (2017) H. Yang, Y. Sun, Y. Zhang, W.-J. Shi, S. S. P. Parkin,  and B. Yan, New Journal of Physics 19, 015008 (2017).
  • Tomiyoshi et al. (1986) S. Tomiyoshi, S. Abe, Y. Yamaguchi, H. Yamauchi,  and H. Yamamoto, Journal of Magnetism and Magnetic Materials 54-57, 1001 (1986).
  • Ohmori et al. (1987) H. Ohmori, S. Tomiyoshi, H. Yamauchi,  and H. Yamamoto, Journal of Magnetism and Magnetic Materials 70, 249 (1987).
  • Ikhlas and et al. (2017) M. Ikhlas and et al., Nat. Phys. 13, 1085 (2017).
  • Higo and et al. (2018) T. Higo and et al., Nature Photonics 12, 73 (2018).
  • Sung et al. (2018) N. H. Sung, F. Ronning, J. D. Thompson,  and E. D. Bauer, Applied Physics Letters 112, 132406 (2018).
  • Cable, Wakabayashi, and Radhakrishna (1993) J. Cable, N. Wakabayashi,  and P. Radhakrishna, Solid State Communications 88, 161 (1993).
  • Kuroda and et al. (2015) K. Kuroda and et al., Nat. Mater. 16, 1090 (2015).
  • Higo et al. (2018) T. Higo, D. Qu, Y. Li, C. Chien, Y. Otani,  and S. Nakatsuji, Applied Physics Letters 113, 202402 (2018).
  • Cheng et al. (2016) B. Cheng, L. Wu, N. J. Laurita, H. Singh, M. Chand, P. Raychaudhuri,  and N. P. Armitage, Phys. Rev. B 93, 180511(R) (2016).
  • Suzuki et al. (2017) M.-T. Suzuki, T. Koretsune, M. Ochi,  and R. Arita, Phys. Rev. B 95, 094406 (2017).
  • Fawcett (1988) E. Fawcett, Rev. Mod. Phys. 60, 209 (1988).
  • Park and et al. (2018) P. Park and et al., npj Quantum Materials 3, 63 (2018).
  • Wu et al. (2015) L. Wu, W.-K. Tse, M. Brahlek, C. M. Morris, R. V. Aguilar, N. Koirala, S. Oh,  and N. P. Armitage, Phys. Rev. Lett. 115, 217602 (2015).
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
340848
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description