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.

Presenters

  • Jinguang Cheng

    Institute of Physics, Chinese Academy of Sciences, Chinese Academy of Sciences (CAS)

Authors

  • Jianping Sun

    Institute of Physics, Chinese Academy of Sciences

  • Prashant Shahi

    Institute of Physics, Chinese Academy of Sciences

  • Bosen Wang

    Institute of Physics, Chinese Academy of Sciences

  • Brian Sales

    Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge National Lab, Oak Ridge National Laborotary, Oak Ridge National Laboratory

  • Kui Jin

    Institute of Physics,Chinese Academy of Sciences, Institute of Physics, Chinese Academy of Sciences, National Laboratory for Condensed Matter Physics, , Institute of Physics Chinese Academy of Sciences, National Lab for Superconductivity, Institute of Physics, Chinese Academy of Sciences (CAS)

  • Zhou Fang

    Institute of Physics, Chinese Academy of Sciences, National Lab for Superconductivity, Institute of Physics, Chinese Academy of Sciences (CAS)

  • Guang-Ming Zhang

    Tsinghua University

  • Xiaoli Dong

    Institute of Physics, Chinese Academy of Sciences

  • Zhongxian Zhao

    Institute of Physics, Chinese Academy of Sciences, National Lab for Superconductivity, Institute of Physics, Chinese Academy of Sciences (CAS)

  • Hechang Lei

    Renmin University, Brookhaven National Laboratory, Brookhaven Natl Lab, Brookhaven National Lab

  • David Singh

    University of Missouri, Univ of Missouri - Columbia, Deparment of Physics and Astronomy, University of Missouri-Columbia

  • Takasada Shibauchi

    Department of Advanced Materials Science, University of Tokyo, University of Tokyo, Univ. Tokyo

  • Yoshiya Uwatoko

    The Institute for Solid State Physics, The University of Tokyo, University of Tokyo

  • Jinguang Cheng

    Institute of Physics, Chinese Academy of Sciences, Chinese Academy of Sciences (CAS)