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Global phase diagram of a Kondo Hund impurity model and the destruction of Fermi-liquid theory

ORAL

Abstract

In many correlated materials, notably the Hund metals, the Landau Fermi-liquid coherence scale T FL is found to be very small. In this Letter, we interpret its smallness in terms of proximity to quantum critical points (QCPs): We use the numerical renormalization group (NRG) to compute the global phase diagram of the simplest three-channel spin-orbital Kondo impurity model capturing the essential physics of Hund metals. When the spin or spin-orbital Kondo couplings are tuned into the ferromagnetic regimes, we find quantum phase transitions to a singular Fermi-liquid or a novel non-Fermi-liquid phase, signalling the existence of QCPs, while T FL is suppressed to zero. The new non-Fermi-liquid phase shows frustrated behavior involving alternating overscreenings in spin and orbital sectors, with universal power laws in the spin (ω-1/5), orbital (ω1/5) and spin-orbital (ω1) dynamical susceptibilities. These power laws, and the NRG eigenlevel spectra, can be fully understood using conformal field theory arguments, which also clarify the nature of the NFL phase.

Presenters

  • Yilin Wang

    Brookhaven National Laboratory

Authors

  • Yilin Wang

    Brookhaven National Laboratory

  • Elias Walter

    Ludwig Maximilian University of Munich

  • Seung-Sup Lee

    Ludwig Maximilian University of Munich

  • Katharina M Stadler

    Ludwig Maximilian University of Munich

  • Jan Von Delft

    Ludwig Maximilian University of Munich, Physics Department, Arnold Sommerfeld Center for Theoretical Physics, and Center for NanoScience, Ludwig-Maximilians-Universität

  • Andreas Weichselbaum

    Brookhaven National Laboratory, Department of Condensed Matter Physics and Materials Science, Brookhaven National Laboratory

  • Gabriel Kotliar

    Rutgers University, New Brunswick, Rutgers University, Condensed Matter Physics, Brookhaven National Laboratory, Department of Physics and Astronomy, Rutgers University, New Brunswick, Department of Physics and Astronomy, Rutgers University