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Stoichiometry and defect superstructures in epitaxial FeSe films on SrTiO3

Xue-Qing Yu    Ming-Qiang Ren    Yi-Min Zhang    Jia-Qi Fan    Sha Han State Key Laboratory of Low-Dimensional Quantum Physics, Department of Physics, Tsinghua University, Beijing 100084, China   
Can-Li Song
[email protected]
   Xu-Cun Ma [email protected] State Key Laboratory of Low-Dimensional Quantum Physics, Department of Physics, Tsinghua University, Beijing 100084, China Frontier Science Center for Quantum Information, Beijing 100084, China    Qi-Kun Xue [email protected] State Key Laboratory of Low-Dimensional Quantum Physics, Department of Physics, Tsinghua University, Beijing 100084, China Frontier Science Center for Quantum Information, Beijing 100084, China Beijing Academy of Quantum Information Sciences, Beijing 100193, China
Abstract

Cryogenic scanning tunneling microscopy is employed to investigate the stoichiometry and defects of epitaxial FeSe thin films on SrTiO3(001) substrates under various post-growth annealing conditions. Low-temperature annealing with an excess supply of Se leads to formation of Fe vacancies and superstructures, accompanied by a superconductivity (metal)-to-insulator transition in FeSe films. By contrast, high-temperature annealing could eliminate the Fe vacancies and superstructures, and thus recover the high-temperature superconducting phase of monolayer FeSe films. We also observe multilayer FeSe during low-temperature annealing, which is revealed to link with Fe vacancy formation and adatom migration. Our results document very special roles of film stoichiometry and help unravel several controversies in the properties of monolayer FeSe films.

High-temperature (TcT_{\textrm{c}}) superconductivity in a number of FeSe-related compounds has attracted worldwide attention in the community of superconductors Wang et al. (2012); Guo et al. (2010); Burrard-Lucas et al. (2013); Lu et al. (2015); Miyata et al. (2015); Lei et al. (2016); Song et al. (2016); Shiogai et al. (2016); Shahi et al. (2018), with a particular focus on monolayer (ML) FeSe epitaxial films grown on SrTiO3 substrates by molecular beam epitaxy (MBE) Zhang et al. (2014); He et al. (2013); Tan et al. (2013); Ge et al. (2014); Xiang et al. (2012); Lee et al. (2014); Fan et al. (2015); Wang et al. (2016); Zhang et al. (2017); Zhao et al. (2018); Song et al. (2019). This seems understandable because the structurally simple FeSe/SrTiO3 system exhibits an unexpectedly high TcT_{\textrm{c}} (\sim 65 K or even higher) Wang et al. (2012); Zhang et al. (2014); He et al. (2013); Tan et al. (2013); Ge et al. (2014) and serves as an ideal platform to unravel the mystery of unconventional superconductivity in iron-based compounds. Since the discovery, much has been learned about electron transfer from the substrates to monolayer FeSe that significantly enhances TcT_{\textrm{c}} Guo et al. (2010); Burrard-Lucas et al. (2013); Lu et al. (2015); Miyata et al. (2015); Lei et al. (2016); Song et al. (2016); Shiogai et al. (2016); Shahi et al. (2018); He et al. (2013); Tan et al. (2013); Zhang et al. (2017); Zhao et al. (2018); Song et al. (2019), but unsolved issues including the samples themselves remain. Monolayer FeSe films prepared in different methods display a great diversity of TcT_{\textrm{c}} and the superconducting energy gap Huang and Hoffman (2017). This situation becomes especially prominent when comparing in-situ and ex-situ measurements Wang et al. (2012); Zhang et al. (2014); He et al. (2013); Tan et al. (2013); Ge et al. (2014). The actual roles played by the capping layer (e.g. amorphous Se) required for ex-situ measurements have been little investigated Zhang et al. (2014); He et al. (2013). In order to achieve the high-TcT_{\textrm{c}} superconductivity in monolayer FeSe films, the Se capping layer has to be removed via a high-temperature annealing, during which the identified phase transition from a low-doping normal state to superconductivity is controversial in nature He et al. (2013); Berlijn et al. (2014); Hu et al. .

On the other hand, intrinsic defects unavoidably occur in epitaxial FeSe films and have been found to severely influence superconductivity Chen et al. (2014); Jiao et al. (2017); Chen et al. (2017); Liu et al. (2018); Hanzawa et al. (2019); Bu et al. (2019). For example, the dumbbell-like defects and their ordering, which have been assigned to Fe vacancies Huang et al. (2016); Fang et al. (2016), are very detrimental to superconductivity Chen et al. (2014); Jiao et al. (2017); Fang et al. (2016). With regard to film stoichiometry, a recent scanning tunneling microscopy (STM) study argued an unexpected existence of at least 20%\% excess Fe in the superconducting FeSe monolayer films by annealing Se-covered FeSe monolayer on SrTiO3 and estimating the amount of newly formed multilayer FeSe islands Hu et al. (2018). This challenges the well-established 1:1 stoichiometry of FeSe for attaining superconductivity in both bulk counterpart and epitaxial films on graphene substrates Williams et al. (2009); Song et al. (2011a, b). In this study, we investigate systematically the morphology, defects and electronic structure of epitaxial FeSe thin films on SrTiO3(001) by using various post-growth annealing conditions, aiming to clarify the roles of stoichiometry.

Our experiments were conducted on two ultrahigh vacuum (UHV) STM systems (Unisoku), every of which is connected to an MBE chambers for in-situ sample preparation. The base pressure of all UHV chambers is better than 2.0 ×\times 10-10 Torr. Nb-doped SrTiO3(001) substrates (0.05 wt%\%) were degassed at 600 o{}^{\textrm{o}}C, and subsequently annealed at 1250 o{}^{\textrm{o}}C in MBE for 20 minutes to obtain a clean (2 ×\times 2) surface. High-purity Fe (99.995%\%) and Se (99.9999%\%) sources evaporated from the respective Kundsen cells were co-deposited onto the substrates under Se-rich condition. Direct current heating was used to heat the substrates, while the substrate temperature (TsubT_{\textrm{sub}}) was measured by a pyrometer. All STM topographies and spectroscopic data were acquired at 4.2 K using polycrystalline PtIr tips, which were cleaned by electron-beam heating and calibrated on MBE-grown Ag/Si(111) films prior to the measurements. Tunneling conductance spectra were collected using a standard lock-in technique with a bias modulation at 931 Hz.

Refer to caption
Figure 1: (color online) (a) Morphology of monolayer FeSe films (300 nm ×\times 300 nm, VV = 3.0 V, II = 30 pA) on SrTiO3(001) upon annealing at 530 o{}^{\textrm{o}}C. The step-terrace feature stems from a miscut of the underlying SrTiO3 substrates throughout. (b) Atomically resolved STM image (10 nm ×\times 10 nm, VV = 50 mV, II = 100 pA) of monolayer FeSe film in (a). The black square marks the (1 ×\times 1) unit cell of Se-terminated FeSe(001) surface. (c) Representative dI/dV spectrum presenting a superconducting gap of Δ\Delta \sim 15 meV on the high-temperature annealed FeSe films in (a). The setpoint is stabilized at VV = 50 mV and II = 100 pA. (d) STM topography (300 nm ×\times 300 nm, VV = 4.0 V, II = 25 pA) showing multilayer FeSe islands after annealing Se-covered monolayer FeSe films at 180 o{}^{\textrm{o}}C. (e, f) STM topographic images (10 nm ×\times 10 nm, VV = 1.8 V, II = 100 pA) of monolayer and bilayer FeSe surfaces in (d), respectively. The blue and white parallelograms correspond to the unit cells of 2 ×\times 10\sqrt{10} and 5\sqrt{5} ×\times 10\sqrt{10} surface superstructures, respectively. (g) STM topography (300 nm ×\times 300 nm, VV = 4.0 V, II = 30 pA) showing the coexistence of 1 ML and 2 ML FeSe after annealing monolayer FeSe films in MBE chamber at 180 o{}^{\textrm{o}}C. (h, i) STM topographic images (10 nm ×\times 10 nm, VV = 0.5 V, II = 100 pA) of monolayer and bilayer FeSe surfaces in (g), respectively.

We begin with superconducting monolayer FeSe films [Figs. 1(a)-1(c)], which are all prepared by depositing \sim 1.5 ML FeSe on the as-cleaned SrTiO3 substrates at TsubT_{\textrm{sub}} = 450 o{}^{\textrm{o}}C, followed by annealing at a higher temperature of \sim 530 o{}^{\textrm{o}}C. Such a post-growth annealing was found to eliminate effectively extra FeSe islands of \sim 0.5 ML [Fig. 1(a)] that was interpreted as decomposition of FeSe Zhang et al. (2017). Amorphous Se of \sim 10 ML (here 1 ML is defined as the area density of Se atoms in single-layer FeSe film, \sim 1.4 ×1015/cm2\times 10^{15}/cm^{2}) was subsequently deposited on the superconducting monolayer FeSe films, followed by annealing at lower TsubT_{\textrm{sub}} = 180 o{}^{\textrm{o}}C for 2 hours. A representative STM topographic image of the annealed films is depicted in Fig. 1(d). Apparently, multilayer FeSe islands with a coverage up to 0.45 ±\pm 0.14 ML are formed, analogous to the previous study Hu et al. (2018). More remarkably, a closer examination reveals a dominant 2 ×\times 10\sqrt{10} surface superstructure in both 1 ML and 2 ML FeSe films, marked by the blue parallelograms in Figs. 1(e) and 1(f). Occasionally, we observe some antiphase domain boundaries. As illustrated by the white dashed lines in Fig. 1(f), the boundary separates two adjacent domains of 2 ×\times 10\sqrt{10} phase that shift by one in-plane Se-Se spacing of aSe-Sea_{\textrm{Se-Se}} = 3.78 Å.

For comparison, we have also prepared another monolayer FeSe films, similar to the one in Fig. 1(a), and annealed it directly at 180 o{}^{\textrm{o}}C without prior Se deposition. Interestingly, multilayer FeSe islands develop both along the step edges and on the terraces [Fig. 1(g)], despite a relatively smaller coverage of 0.26 ±\pm 0.03 ML. Another remarkable distinction from the low-temperature annealed FeSe films with an excess supply of Se in Figs. 1(d)-(f) is that the FeSe(001) surface remains basically unchanged and exhibits no surface superstructure [Figs. 1(h) and 1(i)], except for an increase of dumbbell-like Fe vacancies in number, marked by the black ellipses in Fig. 1(h). The populated Fe vacancies were found to completely kill the superconductivity in monolayer FeSe films on SrTiO3 substrates.

In order to unravel the formation mechanism of multilayer FeSe islands, Fe vacancies and 2 ×\times 10\sqrt{10} surface superstructure, we conducted progressive annealing of the superstructural FeSe thin films [Figs. 1(d)-1(f)] at elevated temperatures, studied the surface structure, and measured the corresponding tunneling conductance spectra [Fig. 2]. With increasing TsubT_{\textrm{sub}}, the multilayer FeSe islands gradually reduce in population and eventually vanishes at 530 o{}^{\textrm{o}}C Hu et al. (2018), restoring to the superconducting monolayer phase as Fig. 1(a). Meanwhile, the 2 ×\times 10\sqrt{10} surface superstructure disappears at \sim 250 o{}^{\textrm{o}}C, and the monolayer FeSe films are populated by a considerable of randomly distributed Fe vacancies below TsubT_{\textrm{sub}} = 300 o{}^{\textrm{o}}C. As TsubT_{\textrm{sub}} is further increased, the Fe vacancies are significantly reduced, thereby recovering the Se-terminated FeSe(001) surface [Fig. 2(a)]. Moreover, the Fe vacancies are easier to be removed in 2 ML films [Fig. 2(a)]. Such a reduction of dumbbell-like Fe vacancies with post-growth annealing bears a striking resemblance to MBE-grown FeSe films on graphitized SiC(0001) substrates Song et al. (2011a), and is possibly associated with the diffusion of Fe vacancies to the edge of terraces Huang et al. (2016).

Refer to caption
Figure 2: (color online) (a, b) Evolution of surface structure with annealing temperature as indicated in monolayer and bilayer FeSe(001)-2 ×\times 10\sqrt{10} films. The dimension of STM images is 15 nm ×\times 15 nm except for the one of bilayer FeSe annealed at 500 o{}^{\textrm{o}}C (10 nm ×\times 10 nm). The imaging conditions are II = 100 pA and VV = (a) 0.8 V, 0.5 V, 0.1 V, 0.05 V, (b) 0.1 V, 0.2 V, 0.1 V, 0.2 V from left to right. The duration time is 2 hours for every annealing sequence. (c) Tunneling dI/dV spectra as a function of annealing temperature. Black and blue triangles mark the onsets of valance band and conduction band throughout, respectively. Horizontal black dashes denote the band gap size of insulating FeSe films with populated Fe vacancies, while the vertical dashes are guide to eyes. The tunneling spectra are vertically offset for clarify. Setpoint: VV = 1.0 V and II = 100 pA.
Refer to caption
Figure 3: (color online) (a) STM topography (480 nm ×\times 240 nm, VV = 3.0 V, II = 10 pA) of superconducting monolayer FeSe films after kept in Se-containing MBE chamber at RT for 16 hours. (b) STM topographic image (30 nm ×\times 30 nm, VV = 3.0 V, II = 10 pA) and (c) typical dI/dV spectrum (VV = 1.0 V, II = 100 pA) on monolayer FeSe films in (a). (d) Topography (480 nm ×\times 240 nm, VV = 3.0 V, II = 10 pA) of superconducting monolayer FeSe films after kept in a clean UHV chamber at RT for 48 hours. (e) STM topographic image (30 nm ×\times 30 nm, VV = 50 mV, II = 50 pA) and (c) superconducting gap (VV = 30 mV, II = 100 pA) on monolayer FeSe films in (d). Note that the weak meandering patterns in (a) and (d) correspond to the domain boundaries of FeSe films.

Figure 2(c) plots the spatially averaged tunneling conductance dI/dV spectra measured on both 1 ML and 2 ML FeSe films as a function of annealing temperature. At TsubT_{\textrm{sub}} = 180 o{}^{\textrm{o}}C, the superstructural 2 ×\times 10\sqrt{10} surfaces are insulating with a band gap of up to 0.85 eV. As TsubT_{\textrm{sub}} is elevated, the insulating gap reduces in magnitude and the tunneling dI/dV spectra recover eventually the characteristic features of high-temperature annealed FeSe films [the top curves in Fig. 2(c)] Ding et al. (2016), leading to an insulator-to-superconductivity (metal) transition in 1 ML (2 ML) FeSe films. Apparently, the transition is more abrupt for 2 ML FeSe, echoing the easier removal of Fe vacancies upon post-growth annealing [Figs. 2(a) and 2(b)]. Note that the gap-like conductance spectra in 1 ML FeSe at TsubT_{\textrm{sub}}\geq 400 o{}^{\textrm{o}}C as seen by STM are caused by the significantly small conductance from the electron pockets around MM points of the Brillouin zone due to tunneling matrix effect, rather than indicating a real band gap. Thus the phase transition from a low-doping normal/insulating state to superconductivity upon annealing is primarily triggered by the removal of Fe vacancies. The recently observed insulating phase in monolayer FeSe films Hu et al. is essentially off-stoichiometric Fe1-xSe compound with a considerable amount of Fe vacancies. Here the Fe vacancies give rise to extra holes and reduce the effective electron carriers for superconductivity, which may be a killer of superconductivity in FeSe.

Now the cause of multilayer FeSe islands upon annealing at 180 o{}^{\textrm{o}}C becomes apparent. Firstly, the formation of Fe-vacancy superstructures provides excess Fe atoms to grow multilayer FeSe [Figs. 1(d)-1(f)]. Such argument has been convincingly corroborated in Fig. 3. By annealing monolayer FeSe films in Se-containing MBE chamber at room temperature (RT), we also find multilayer FeSe islands of 0.21 ±\pm 0.02 ML [Fig. 3(a)]. Due to the random distribution of Fe vacancies, the FeSe surface gets disordered and insulating [Figs. 3(b) and 3(c)], behaving similarly as the Fe-deficient monolayer FeSe films in Figs. 2(a) and 2(c). This shows that some Fe atoms have migrated out of the monolayer FeSe films and formed multilayer FeSe, given the fact that there exist Se residues in the MBE chamber. Actually, when a clean UHV chamber free of Se was used to keep the sample, no multilayer FeSe islands were formed [Fig. 3(d)] and the pristine FeSe(001)-1 ×\times 1 surface remains superconductive [Figs. 3(e) and 3(f)].

Note that every Fe vacancy brightens two adjacent Se atoms at the top layer of FeSe and leads to the dumbbell-shaped feature. Therefore, the stoichiometry of 2 ×\times 10\sqrt{10} superstructure can be readily determined as Fe5Se6, because the superstructure unit cell contains four bright Se atoms and thus two Fe vacancies in Figs. 1(e) and 1(f). It should be also noted that other Fe-vacancy superstructures coexist on the annealed FeSe films in Fig. 1(d), such as 5\sqrt{5} ×\times 10\sqrt{10} (Fe11Se14, illustrated in the lower right corner of Fig. 1f) Li et al. (2014) and 5\sqrt{5} ×\times 5\sqrt{5} (Fe4Se5) [Fig. 4(a)]. These Fe-vacancy superstructures contribute to \sim 0.2 ML FeSe, which explain well the formed multilayer FeSe islands in Fig. 3(a).

Refer to caption
Figure 4: (color online) (a) High-resolution STM topography (10 nm ×\times 10 nm, VV = 0.6 V, II = 50 pA) of superstructural 5\sqrt{5} ×\times 5\sqrt{5} (blue square) FeSe films with a thickness of 6 ML. (b) Sketched lattice model of Fe-vacancy Fe4Se5 phase. Note that the Se atoms below the Fe plane are marked by the orange spheres with light opacity. (c) Spatially-averaged dI/dV spectra (VV = 1.0 V, II = 100 pA) of FeSe(001)-5\sqrt{5} ×\times 5\sqrt{5} films at varied thickness. (d) Tunneling spectra over a wide energy range (VV = 2.0 V, II = 100 pA) showing a characteristic conductance peak in the unoccupied states. The blue dashed line is guide to the eyes.

Only the scenario of Fe vacancies and superstructures fails to account for the formed multilayer FeSe up to 0.45 ±\pm 0.14 ML in Fig. 1(d) and 0.26 ±\pm 0.03 ML in Fig. 1(g), especially considering the small population of Se vacancies in Fig. 1(g). Here we suggest a dynamical atom migration that also contributes to the formation of multilayer FeSe during the post-growth annealing process. At elevated TsubT_{\textrm{sub}}, long-range Fe atom migration may occur, rendering the invisibility of multilayer FeSe due to the limited field of view of STM. Conversely, during the low-temperature annealing, the atom migration and possible reaction with the supplied Se are responsible for the reentrance of multilayer FeSe islands. Here the atom migration might be distinctively driven by the thermal and atom density gradients during the high- and low-temperature annealing, respectively. The atom migration scenario, together with the Fe vacancies and superstructures, might help explain the mysterious FeSe stoichiometry and why monolayer FeSe films are superconductive only when the stoichiometry is nearly 1:1.

Finally, we discuss more on the Fe-vacancy-induced 5\sqrt{5} ×\times 5\sqrt{5} superstructure, which has been previously observed in alkali/alkaline-intercalated iron selenides Wang et al. (2011); Li et al. (2012); Dagotto (2013). By co-depositing Fe and Se directly at TsubT_{\textrm{sub}} = 230 o{}^{\textrm{o}}C, we obtain superstructural 5\sqrt{5} ×\times 5\sqrt{5} films with thickness of \geq 2 ML [Figs. 4(a) and 4(b)]. Plotted in Fig. 4(c) are the thickness-dependent tunneling conductance dI/dV spectra, all featuring an insulating band gap. The gap and characteristic conductance peak in the unoccupied states [Fig. 4(d)] exhibit oscillatory behavior with a period of 2 ML in magnitude (1.44 eV, 0.77 eV, 1.05 eV, 0.73 eV and 1.01 eV from 2 ML to 6 ML) and energy (1.72 eV, 1.34 eV, 1.53 eV, 1.28 eV and 1.40 eV from 2 ML to 6 ML), respectively, the cause of which merits a further theoretical investigation. On the other hand, the gap magnitude of \sim 1.44 eV in 2 ML is greater than 0.85 eV in the 2 ×\times 10\sqrt{10} superstructure [Figs. 1(c) and 1(d)]. This is most likely caused by more populated Fe vacancies in 5\sqrt{5} ×\times 5\sqrt{5} superstructure. Overall, the gap magnitude of Fe4Se5 films increases when approaching the two-dimensional limit, a consequence of poor electrostatic screening and enhanced quantum confinement.

In summary, we have explicitly revealed by direct STM imaging that the superconductivity property in monolayer FeSe films on SrTiO3 is very sensitive to Fe vacancies. The Fe vacancy formation together with atom migration takes responsibility for the observed multilayer islands in low-temperature annealed FeSe films. Therefore, a fine control of Fe vacancies not only appears to be essential to the surface morphology and structure, but also plays a key role in the superconductivity of FeSe films.

Acknowledgements.
The work is financially supported by the Ministry of Science and Technology of China (Grants No. 2017YFA0304600, No. 2016YFA0301004, No. 2018YFA0305603), the National Natural Science Foundation of China (Grants No. 11774192, No. 11634007), and in part the Beijing Advanced Innovation Center for Future Chip.

References

  • Wang et al. (2012) Q. Y. Wang, Z. Li, W. H. Zhang, Z. C. Zhang, J. S. Zhang, W. Li, H. Ding, Y. B. Ou, P. Deng, K. Chang, J. Wen, C. L. Song, K. He, J. F. Jia, S. H. Ji, Y. Y. Wang, L. L. Wang, X. Chen, X. C. Ma,  and Q. K. Xue, Chin. Phys. Lett. 29, 037402 (2012).
  • Guo et al. (2010) J. G. Guo, S. F. Jin, G. Wang, S. C. Wang, K. X. Zhu, T. T. Zhou, M. He,  and X. L. Chen, Phys. Rev. B 82, 180520 (2010).
  • Burrard-Lucas et al. (2013) M. Burrard-Lucas, D. G. Free, S. J. Sedlmaier, J. D. Wright, S. J. Cassidy, Y. Hara, A. J. Corkett, T. Lancaster, P. J. Baker, S. J. Blundell,  and S. J. Clarke, Nat. Mater. 12, 15 (2013).
  • Lu et al. (2015) X. F. Lu, N. Z. Wang, H. Wu, Y. P. Wu, D. Zhao, X. Z. Zeng, X. G. Luo, T. Wu, W. Bao, G. H. Zhang,  and X. H. Chen, Nat. Mater. 14, 325 (2015).
  • Miyata et al. (2015) Y. Miyata, K. Nakayama, K. Sugawara, T. Sato,  and T. Takahashi, Nat. Mater. 14, 775 (2015).
  • Lei et al. (2016) B. Lei, J. H. Cui, Z. J. Xiang, C. Shang, N. Z. Wang, G. J. Ye, X. G. Luo, T. Wu, Z. Sun,  and X. H. Chen, Phys. Rev. Lett. 116, 077002 (2016).
  • Song et al. (2016) C. L. Song, H. M. Zhang, Y. Zhong, X. P. Hu, S. H. Ji, L. Wang, K. He, X. C. Ma,  and Q. K. Xue, Phys. Rev. Lett. 116, 157001 (2016).
  • Shiogai et al. (2016) J. Shiogai, Y. Ito, T. Mitsuhashi, T. Nojima,  and A. Tsukazaki, Nat. Phys. 12, 42 (2016).
  • Shahi et al. (2018) P. Shahi, J. P. Sun, S. H. Wang, Y. Y. Jiao, K. Y. Chen, S. S. Sun, H. C. Lei, Y. Uwatoko, B. S. Wang,  and J. G. Cheng, Phys. Rev. B 97, 020508 (2018).
  • Zhang et al. (2014) W. H. Zhang, Y. Sun, J. S. Zhang, F. S. Li, M. H. Guo, Y. F. Zhao, H. M. Zhang, J. P. Peng, Y. Xing, H. C. Wang, T. H. Fujita, Z. Li, H. Ding, C. J. Tang, M. Wang, Q. Y. Wang, K. He, S. H. Ji, X. Chen, J. F. Wang, Z. C. Xia, L. Li, Y. Y. Wang, J. Wang, L. L. Wang, M. W. Chen, Q. K. Xue,  and X. C. Ma, Chin. Phys. Lett. 31, 017401 (2014).
  • He et al. (2013) S. L. He, J. F. He, W. H. Zhang, L. Zhao, D. F. Liu, X. Liu, D. X. Mou, Y. B. Ou, Q. Y. Wang, Z. Li, W. Lili, Y. Y. Peng, Y. Liu, C. Y. Chen, L. Yu, G. D. Liu, X. L. Dong, J. Zhang, C. T. Chen, Z. Y. Xu, X. Chen, X. C. Ma, Q. K. Xue,  and X. J. Zhou, Nat. Mater. 12, 605 (2013).
  • Tan et al. (2013) S. Y. Tan, Y. Zhang, M. Xia, Z. R. Ye, F. Chen, X. Xie, R. Peng, D. F. Xu, Q. Fan, H. C. Xu, J. Jiang, T. Zhang, X. C. Lai, T. Xiang, J. P. Hu, N. P. Xie,  and D. L. Feng, Nat. Mater. 12, 634 (2013).
  • Ge et al. (2014) J. F. Ge, Z. L. Liu, C. H. Liu, C. L. Gao, D. Qian, Q. K. Xue, Y. Liu,  and J. F. Jia, Nat. Mater. 14, 285 (2014).
  • Xiang et al. (2012) Y. Y. Xiang, F. Wang, D. Wang, Q. H. Wang,  and D. H. Lee, Phys. Rev. B 86, 134508 (2012).
  • Lee et al. (2014) J. J. Lee, F. T. Schmitt, R. G. Moore, S. Johnston, Y. T. Cui, W. Li, M. Yi, Z. K. Liu, M. Hashimoto, Y. Zhang, D. H. Lu, T. P. Devereaux, D. H. Lee,  and Z. X. Shen, Nature 515, 245 (2014).
  • Fan et al. (2015) Q. Fan, W. H. Zhang, X. Liu, Y. J. Yan, M. Q. Ren, R. Peng, H. C. Xu, B. P. Xie, J. P. Hu, T. Zhang,  and D. L. Feng, Nat. Phys. 11, 946 (2015).
  • Wang et al. (2016) Z. F. Wang, H. M. Zhang, D. F. Liu, C. Liu, C. J. Tang, C. L. Song, Y. Zhong, J. P. Peng, F. S. Li, C. N. Nie, L. L. Wang, X. J. Zhou, X. C. Ma, Q. K. Xue,  and F. Liu, Nat. Mater. 15, 968 (2016).
  • Zhang et al. (2017) H. M. Zhang, D. Zhang, X. W. Lu, C. Liu, G. Y. Zhou, X. C. Ma, L. Wang, P. Jiang, Q. K. Xue,  and X. H. Bao, Nat. Commun. 8, 214 (2017).
  • Zhao et al. (2018) W. W. Zhao, M. D. Li, C. Z. Chang, J. Jiang, L. J. Wu, C. X. Liu, J. S. Moodera, Y. M. Zhu,  and M. H. W. Chan, Sci. Adv. 4, eaao2682 (2018).
  • Song et al. (2019) Q. Song, T. L. Yu, X. Lou, B. P. Xie, H. C. Xu, C. H. P. Wen, Q. Yao, S. Y. Zhang, X. T. Zhu, J. D. Guo, R. Peng,  and D. L. Feng, Nat. Commun. 10, 758 (2019).
  • Huang and Hoffman (2017) D. Huang and J. E. Hoffman, Annu. Rev. Condens. Matter Phys. 8, 311 (2017).
  • Berlijn et al. (2014) T. Berlijn, H. P. Cheng, P. J. Hirschfeld,  and W. Ku, Phys. Rev. B 89, 020501 (2014).
  • (23) Y. Hu, Y. Xu, Y. M. Zhang, Q. Y. Wang, S. L. He, D. F. Liu, A. J. Liang, J. W. Huang, C. Li, Y. Q. Cai, D. S. Wu, L. G. D, F. S. Li, J. Q. Fan, G. Y. Zhou, L. L. Wang, C. L. Song, X. C. Ma, X. Q. K, Z. Y. Xu, L. Zhao,  and X. J. Zhou, arXiv:1904.04662 .
  • Chen et al. (2014) T. K. Chen, C. C. Chang, H. H. Chang, A. H. Fang, C. H. Wang, W. H. Chao, C. M. Tseng, Y. C. Lee, Y. R. Wu, M. H. Wen, H. Y. Tang, F. R. Chen, M. J. Wang, M. K. Wu,  and D. V. Dyck, Proc. Natl. Acad. Sci. U.S.A. 111, 63 (2014).
  • Jiao et al. (2017) L. Jiao, S. Rößler, C. Koz, U. Schwarz, D. Kasinathan, U. K. Rößler,  and S. Wirth, Phys. Rev. B 96, 094504 (2017).
  • Chen et al. (2017) W. J. Chen, Z. J. Tian, P. Li, W. D. Luo,  and C. L. Gao, Phys. Rev. B 96, 214426 (2017).
  • Liu et al. (2018) C. Liu, J. Mao, H. Ding, R. Wu, C. Tang, F. Li, K. He, W. Li, C. L. Song, X. C. Ma, Z. Liu, L. Wang,  and Q. K. Xue, Phys. Rev. B 97, 024502 (2018).
  • Hanzawa et al. (2019) K. Hanzawa, Y. Yamaguchi, Y. Obata, S. Matsuishi, H. Hiramatsu, T. Kamiya,  and H. Hosono, Phys. Rev. B 99, 035148 (2019).
  • Bu et al. (2019) K. L. Bu, B. Wang, W. H. Zhang, Y. Fei, Y. Zheng, F. Z. Ai, Z. X. Wu, Q. S. Wang, H. L. Wo, J. Zhao, C. H. Jin,  and Y. Yin, Phys. Rev. B 100, 155127 (2019).
  • Huang et al. (2016) D. Huang, T. A. Webb, C. L. Song, C. Z. Chang, J. S. Moodera, E. Kaxiras,  and J. E. Hoffman, Nano Lett. 16, 4224 (2016).
  • Fang et al. (2016) Y. Fang, D. H. Xie, W. Zhang, F. Chen, W. Feng, B. P. Xie, D. L. Feng, X. C. Lai,  and S. Y. Tan, Phys. Rev. B 93, 184503 (2016).
  • Hu et al. (2018) Y. Hu, Y. Xu, Q. Y. Wang, L. Zhao, S. L. He, J. W. Huang, C. Li, G. D. Liu,  and X. J. Zhou, Phys. Rev. B 97, 224512 (2018).
  • Williams et al. (2009) A. J. Williams, T. M. McQueen,  and R. J. Cava, Solid State Commun. 149, 1507 (2009).
  • Song et al. (2011a) C. L. Song, Y. L. Wang, P. Cheng, Y. P. Jiang, W. Li, T. Zhang, Z. Li, K. He, L. Wang, J. F. Jia, H.-H. Hung, C. J. Wu, X. C. Ma, X. Chen,  and Q. K. Xue, Science 332, 1410 (2011a).
  • Song et al. (2011b) C. L. Song, Y. L. Wang, Y. P. Jiang, Z. Li, L. Wang, K. He, X. Chen, X. C. Ma,  and Q. K. Xue, Phys. Rev. B 84, 020503 (2011b).
  • Ding et al. (2016) H. Ding, Y. F. Lv, K. Zhao, W. L. Wang, L. Wang, C. L. Song, X. Chen, X. C. Ma,  and Q. K. Xue, Phys. Rev. Lett. 117, 067001 (2016).
  • Li et al. (2014) Z. Li, J. P. Peng, H. M. Zhang, W. H. Zhang, H. Ding, P. Deng, K. Chang, C. L. Song, S.-H. Ji, L. L. Wang, K. He, X. Chen, Q. K. Xue,  and X. C. Ma, J. Phys.: Condens. Matter 26, 265002 (2014).
  • Wang et al. (2011) Z. Wang, Y. J. Song, H. L. Shi, Z. W. Wang, Z. Chen, H. F. Tian, G. F. Chen, J. G. Guo, H. X. Yang,  and J. Q. Li, Phys. Rev. B 83, 140505 (2011).
  • Li et al. (2012) W. Li, H. Ding, P. Deng, K. Chang, C. L. Song, K. He, L. Wang, X. C. Ma, J. P. Hu, X. Chen,  and Q. K. Xue, Nat. Phys. 8, 126 (2012).
  • Dagotto (2013) E. Dagotto, Rev. Mod. Phys. 85, 849 (2013).