Superconducting phase diagram and the evolution of electronic structure across charge density wave in underdoped 1TCuδTiSe2 under hydrostatic pressure

Shuxiang Xu, Pengtao Yang, Keyu Chen, Ziyi Liu, Wuwei Cui, Qing Hu, Jianping Sun, Ran Ang, Yoshiya Uwatoko, Bosen Wang, and Jinguang Cheng
Phys. Rev. B 104, 134503 – Published 4 October 2021
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Abstract

We revisit a superconducting phase diagram and electronic structures across the charge density wave (CDW) phase transition of Cu-underdoped 1TCuδTiSe2 (δ0.03) under hydrostatic pressure. Superconductivity appears right after the complete collapse of the long-range CDW at a critical pressure of Pc2.48GPa, apart from the reported superconducting phase diagrams; it is found that the superconducting transition temperature shows a domelike pressure dependence covering a narrow pressure range with a maximum of Tcmax2.80K at 4.80 GPa. Accordingly, the residual resistivity ρ0 and temperature exponent n of normal-state resistivity (from ∼3.30 at ambient pressure to ∼2.38 at Pc and ∼4.0 at 6.50 GPa) reduce sizably while the quadratic temperature coefficient A of normal-state resistivity is enhanced by one order in magnitude; these results indicate the importance of CDW quantum fluctuation in superconducting pairing; low-T resistivity upwarps with a −lnT dependence below a characteristic temperature T* which has a domelike shape in the pressure range of 2.82–4.80 GPa. Based on two-band analysis of Hall conductivity and Kohler-fitting of magnetotransport (MR), energy bands are dominated by electron-type carriers across the CDW phase transition for P<Pc, and they reverse into hole-type for P>Pc; interestingly, the mobility of carriers increases up to five times at Pc, but carrier concentration shows a weak pressure dependence. The MR value increases with the pressure for P<Pc and then jump up to a saturated value after the collapse of the CDW. Our results show that the collapse of the CDW is accompanied by the reconstruction of the Fermi surface, and the enhancement in MR can be mainly attributed to the change of mobility. Possible mechanisms are discussed.

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  • Received 12 May 2021
  • Revised 5 August 2021
  • Accepted 13 September 2021

DOI:https://doi.org/10.1103/PhysRevB.104.134503

©2021 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Shuxiang Xu1,2, Pengtao Yang1, Keyu Chen1, Ziyi Liu1, Wuwei Cui1, Qing Hu3, Jianping Sun1,2, Ran Ang3,5,*, Yoshiya Uwatoko4, Bosen Wang1,2,6,*, and Jinguang Cheng1,2,*

  • 1Beijing National Laboratory for Condensed Matter Physics and Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China
  • 2School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100190, China
  • 3Key Laboratory of Radiation Physics and Technology, Ministry of Education, Institute of Nuclear Science and Technology, Sichuan University, Chengdu 610064, China
  • 4Institute for Solid State Physics, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa, Chiba 277-8581, Japan
  • 5Institute of New Energy and Low-Carbon Technology, Sichuan University, Chengdu 610065, China
  • 6Songshan Lake Materials Laboratory, Dongguan, Guangdong 523808, China

  • *Corresponding authors: rang@scu.edu.cn, bswang@iphy.ac.cn, and jgcheng@iphy.ac.cn

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Issue

Vol. 104, Iss. 13 — 1 October 2021

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