Published March 18, 2024 | Version v1
Journal article

Temperature dependence and limiting mechanisms of the upper critical field of FeSe thin films

  • 1. Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 2. National High Magnetic Field Laboratory, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 3. Department of Chemistry, The Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 4. Department of Materials Science and Engineering, The Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 5. Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA

Description

We use magnetoresistance measurements at high magnetic field (μ0H65 T) and low temperature (T500 mK) to gain fresh insights into the behavior of the upper critical field Hc2 in superconducting ultrathin FeSe films of varying degrees of disorder, grown by molecular beam epitaxy on SrTiO3. Measurements of Hc2 across samples with a widely varying superconducting critical temperature (1.2 K Tc21 K) generically show similar qualitative temperature dependence. We analyze the temperature dependence of Hc2 in the context of Werthamer-Helfand-Hohenberg (WHH) theory. The analysis yields parameters that indicate a strong Pauli paramagnetic pair-breaking mechanism which is also reflected by pseudoisotropic superconductivity in the limit of zero temperature. In the lower Tc samples, we observe a spin-orbit scattering-driven enhancement of Hc2 above the strongly-coupled Pauli paramagnetic limit. We also observe clear deviations from WHH theory at low temperature, regardless of Tc. We attribute this to the multiband superconductivity of FeSe and possibly to the emergence of a low-temperature, high-field superconducting phase.

Additional details

Identifiers

DOI
10.1103/PhysRevB.109.094514;
arXiv
arXiv:2310.19241;
Crossref Funder ID
10.13039/100000001; 10.13039/100000015;

Publishing Information

Journal Title
Physical Review B
Journal Volume
109
Journal Issue
9
Journal Page Range
10 pgs.
ISSN
1550-235X

Optional Information

Copyright
©2024 American Physical Society
Contract/Grant/Project number
DMR-2039351; DMR-1644779; DMR2138905; DMR-2011839
Notes
Contact Email: nsamarth@psu.edu; Record automatically processed
Funding organization
National Science Foundation; U.S. Department of Energy