Scaling of the superconducting gap with orbital character in FeSe
ORAL
Abstract
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
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Presenters
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Luke Rhodes
Department of Physics, Royal Holloway University of London
Authors
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Luke Rhodes
Department of Physics, Royal Holloway University of London
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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
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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
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Daniil Evtushinsky
Institute of Physics, Ecole Polytechnique Federale Lausanne
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Matthias Eschrig
Department of Physics, Royal Holloway University of London
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Timur Kim
Diamond Light Source, Diamond Light Source, Harwell Campus, Didcot, OX11 0DE, United Kingdom