# Magnetism trends in doped Ce-Cu intermetallics in the vicinity of   quantum criticality: realistic Kondo lattice models based on dynamical   mean-field theory

**Authors:** Munehisa Matsumoto

arXiv: 1904.13160 · 2020-05-11

## TL;DR

This study uses realistic electronic structure calculations and dynamical mean-field theory to analyze magnetism trends near quantum criticality in doped Ce-Cu intermetallics, revealing a crossover in magnetic behavior relevant for permanent magnet design.

## Contribution

It presents a realistic Kondo lattice model based on DMFT to describe quantum criticality and magnetism in doped Ce-Cu intermetallics, connecting theory with experimental magnetic trends.

## Key findings

- CeCu$_6$ doped with Au crosses a magnetic QCP at 0.2<x<0.4.
- The magnetic behavior in Au-doped CeCu$_6$ is similar to that in Co-doped CeCu$_5$.
- The study discusses implications for coercivity in rare-earth permanent magnets.

## Abstract

The quantum critical point (QCP) in the archetypical heavy-fermion compound CeCu$_6$ doped by Au is described, accounting for the localized $4f$-electron of Ce, using realistic electronic structure calculations combined with dynamical mean-field theory (DMFT). Magnetism trends in Ce(Cu$_{1-\epsilon}$Au$_\epsilon$)$_6$ are compared with those in Co-doped CeCu$_{5}$, which resides on the non-ferromagnetic side of the composition space of one of the earliest rare-earth permanent magnet compounds, Ce(Co,Cu)$_5$. The construction of a realistic Doniach phase diagram shows that the system crosses over a magnetic quantum critical point in the Kondo lattice in $0.2<x<0.4$ of Ce(Cu$_{1-x}$Co$_x$)$_5$. Comparison between Au-doped CeCu$_6$ and Co-doped CeCu$_5$ reveals that the swept region in the vicinity of QCP for the latter thoroughly covers that of the former. The implications of these trends on the coercivity of the bulk rare-earth permanent magnets are discussed.

## Full text

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## Figures

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## References

85 references — full list in the complete paper: https://tomesphere.com/paper/1904.13160/full.md

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Source: https://tomesphere.com/paper/1904.13160