Scaling of the superconducting gap with orbital character in FeSe

ORAL

Abstract

It is often hypothesized that superconductivity in the iron-based superconductors is mediated by a spin-fluctuation pairing mechanism, however direct evidence of this pairing is challenging to obtain. Here we present a high-resolution angle-resolved photoemission spectroscopy (ARPES) study on the three-dimensional superconducting gap of FeSe. We observe a direct scaling between the dyz orbital weight at the Fermi level and the size of the superconducting gap at both the hole and electron pockets. Suggesting that superconducting pairing is mediated by strong, local Coulomb interactions.

We then present an ARPES-derived tight binding model which quantitatively takes into account all the features present in the nematic phase of FeSe; including spin-orbital coupling, nematic ordering, and most crucially the incoherence of an electron pocket. Using this model, we show that the calculated momentum dependence of the superconducting gap, assuming spin-fluctuation mediated superconductivity, directly reproduces the experimental results.

These findings provide both experimental and theoretical support for spin-fluctuation mediated superconductivity in FeSe.

L.C. Rhodes et. al. (2018) arXiv:1804.01436

Presenters

  • Luke Rhodes

    Department of Physics, Royal Holloway University of London

Authors

  • Luke Rhodes

    Department of Physics, Royal Holloway University of London

  • Matthew Watson

    University of St Andrews, School of Physics and Astronomy, University of St. Andrews, Diamond Light Source, School of Physics and Astronomy, University of St Andrews, St. Andrews KY16 9SS, United Kingdom

  • Amir Haghighirad

    Karlsruhe Institute of Technology, 76021 Karlsruhe, Germany, Institute for Solid-State Physics, Karlsruhe Institute of Technology, Institute for Solid State Physics, Karlsruhe Institute of Technology

  • Daniil Evtushinsky

    Institute of Physics, Ecole Polytechnique Federale Lausanne

  • Matthias Eschrig

    Department of Physics, Royal Holloway University of London

  • Timur Kim

    Diamond Light Source, Diamond Light Source, Harwell Campus, Didcot, OX11 0DE, United Kingdom