High pressure route to high-Tc superconductivity in the FeSe-based materials
COFFEE_KLATCH · Invited
Abstract
High pressure is an effective and clean tuning knob to tip the balance of competing interactions in the strongly correlated electron systems. Although FeSe is nonmagnetic within the nematic state below Ts = 90 K, the application of high pressure can induce a static magnetic order and promote high-Tc superconductivity. These facts make FeSe an ideal platform to study the interplay of superconductivity with magnetism and nematicity. In addition, high-Tc superconductivity can be achieved in various heavily electron-doped (HED) FeSe-derived materials, including AxFe2-ySe2, (Li,Fe)OHFeSe, and monolayer FeSe/SrTiO3. More intriguingly, a second high-Tc superconducting (SC-II) phase has been reported in the pressurized AxFe2-ySe2 and K-doped FeSe films.To shed more light on these intriguing issues, we recently performed detailed magneto-transport measurements on bulk FeSe and the HED FeSe-based materials under high pressure. For FeSe, we constructed a comprehensive T-P phase diagram featured by a dome-shaped magnetic phase interconnecting with the nematic order and the high-Tc superconductivity [1], and further demonstrated the presence of hole-like Fermi surface and enhanced spin fluctuations near the optimal Tc = 38.5 K at 6 GPa [2]. For the HED (Li1-xFex)OHFeSe, we observed the emergence of SC-II phase above Pc = 5 GPa, and uncovered a sharp transition of the normal state from a Fermi liquid for P < Pc to a non Fermi liquid for P > Pc [3]. The emergence of SC-II phase seems to be a universal phenomenon for these HED FeSe materials as also demonstrated in Lix(NH3)yFe2Se2 with the Tcmax = 55 K achieved under high pressure [4].
References:
[1] J. P. Sun, et al., Nat. Commu. 7, 12146 (2016).
[2] J. P. Sun, et al., Phys. Rev. Lett. 118, 147004 (2017).
[3] J. P. Sun, et al., ArXiv: 17007.06735.
[4] P. Shahi, et al., ArXiv: 1709.08455.
References:
[1] J. P. Sun, et al., Nat. Commu. 7, 12146 (2016).
[2] J. P. Sun, et al., Phys. Rev. Lett. 118, 147004 (2017).
[3] J. P. Sun, et al., ArXiv: 17007.06735.
[4] P. Shahi, et al., ArXiv: 1709.08455.
*This work was supported by the CAS, NSFC, and MOST of China (Grant Nos. 11574377, 2014CB921500, XDB07020100, QYZDB-SSW-SLH013).
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Presenters
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Jinguang Cheng
- Institute of Physics, Chinese Academy of Sciences
- Chinese Academy of Sciences (CAS)