Locating the pseudogap closing point in cuprate superconductors: Absence of entrant or reentrant behavior

Jeffery L. Tallon, James G. Storey, John R. Cooper, and John W. Loram
Phys. Rev. B 101, 174512 – Published 21 May 2020

Abstract

Many current descriptions of the pseudogap in underdoped cuprates envision a doping-dependent transition line T*(p) which descends monotonically toward zero just beyond optimal doping. There is much debate as to the location of the terminal point p* where T*(p) vanishes, whether or not there is a phase transition at T* and exactly how T*(p) behaves below Tc within the superconducting dome. One perspective sees T*(p) cutting the dome and continuing to descend monotonically to zero at p*0.19 holes/Cu—referred to here as entrant behavior. Another perspective derived from photoemission studies is that T*(p) intersects the dome near p0.23 holes/Cu then turns back below Tc, falling to zero again around p*0.19—referred to here as reentrant behavior. By examining field-dependent thermodynamic data for Bi2Sr2CaCu2O8+δ we show that neither entrant nor reentrant behavior is supported. Rather, p* sharply delimits the pseudogap regime: For p<0.19 the pseudogap is always present, independent of T. Similar results are found for Y0.8Ca0.2Ba2Cu3O7δ. For both materials, T*(p) is not a temperature but a crossover scale, E*(p)/2kB, reflecting instead the underlying pseudogap energy E*(p) which vanishes as pp*0.19.

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  • Received 30 July 2019
  • Revised 20 April 2020
  • Accepted 28 April 2020

DOI:https://doi.org/10.1103/PhysRevB.101.174512

©2020 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Jeffery L. Tallon1,*, James G. Storey1, John R. Cooper2, and John W. Loram2,†

  • 1Robinson Research Institute, Victoria University of Wellington, P.O. Box 33436, Lower Hutt 5046, New Zealand
  • 2Cavendish Laboratory, Cambridge University, Cambridge CB3 0HE, United Kingdom

  • *jeff.tallon@vuw.ac.nz
  • Deceased.

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Vol. 101, Iss. 17 — 1 May 2020

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