# Single ferromagnetic fluctuations in UCoGe revealed by 73Ge- and   59Co-NMR studies

**Authors:** Masahiro Manago, Kenji Ishida, Dai Aoki

arXiv: 1802.10221 · 2018-03-01

## TL;DR

This study uses $^{73}$Ge and $^{59}$Co NMR and NQR techniques to investigate the magnetic and electronic properties of the ferromagnetic superconductor UCoGe, revealing that itinerant U-$5f$ electrons drive ferromagnetism and highlighting anisotropic responses.

## Contribution

First detailed NMR/NQR analysis of UCoGe showing the role of U-$5f$ electrons and comparing its properties with related ferromagnetic superconductors.

## Key findings

- UCoGe's NQR parameters are similar to URhGe.
- Knight shifts of Ge and Co are well scaled.
- Spin susceptibilities differ along axes, affecting superconductivity.

## Abstract

$^{73}$Ge and $^{59}$Co nuclear magnetic resonance (NMR) and nuclear quadrupole resonance (NQR) measurements have been performed on a $^{73}$Ge-enriched single-crystalline sample of the ferromagnetic superconductor UCoGe in the paramagnetic state. The $^{73}$Ge NQR parameters deduced from NQR and NMR are close to those of another isostructural ferromagnetic superconductor URhGe. The Knight shifts of the Ge and Co sites are well scaled to each other when the magnetic field is parallel to the $b$ or $c$ axis. The hyperfine coupling constants of Ge are estimated to be close to those of Co. The large difference of spin susceptibilities between the $a$ and $b$ axes could lead to the different response of the superconductivity and ferromagnetism with the field parallel to these directions. The temperature dependence of the nuclear spin-lattice relaxation rates $1/T_1$ at the two sites is similar to each other above 5 K. These results indicate that the itinerant U-$5f$ electrons are responsible for the ferromagnetism in this compound, consistent with previous studies. The similarities and differences in the three ferromagnetic superconductors are discussed.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1802.10221/full.md

## References

45 references — full list in the complete paper: https://tomesphere.com/paper/1802.10221/full.md

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Source: https://tomesphere.com/paper/1802.10221