Visualizing Orbital-selective Quasiparticle Interference in the Hund's Metal State of FeSe.
High temperature superconductivity (HTS) in Cu-based materials is generated by strong electronic correlations due to proximity of the Mott insulator phase. By contrast, the undoped phase proximate to Fe-based HTS is never an insulator. But this striking distinction may be deceptive because, while only a single Cu d-orbital is active in the former compounds, up to five Fe d-orbitals are active in the latter. In theory, such orbital multiplicity allows an unusual new state, referred to as an orbital-selective Hund's metal, to appear. In this state, strong Hund's coupling aligns the Fe spins thereby suppressing the inter-orbital charge fluctuations. The result is orbital selectivity of correlations wherein electrons associated with some orbitals become strongly incoherent but coexist with coherent quasiparticles associated with other orbitals of the same atom. A distinguishing experimental signature would be that quasiparticle spectral weights $Z_m$ associated with each different orbital m would be highly distinct, effectively resulting in orbital selectivity of quasiparticles. To search for such effects associated with Fe-based HTS, we visualize quasiparticle interference resolved by orbital content in FeSe, and discover strong orbitally selective differences of quasiparticle $Z_m$ on all detectable bands. Measurement of QPI amplitudes on the \alpha-, \epsilon- and \delta-bands of FeSe reveals that $Z_{xy}<Z_{xz}<<Z_{yz}$ for a wide energy range and throughout k-space. Moreover, the magnitudes and ratios of these quasiparticle weights are consistent with those deduced independently from the properties of orbital-selective Cooper pairing. All these data indicate that orbital-selective strong correlations dominate the Hund's metal state underpinning superconductivity in FeSe, a situation that would be of broad fundamental significance if true for Fe-based superconductors in general.
Publisher URL: http://arxiv.org/abs/1802.02266
DOI: arXiv:1802.02266v1
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