# Surface impedance measurements on Nb$_{3}$Sn at high magnetic fields

**Authors:** Andrea Alimenti, Nicola Pompeo, Kostiantyn Torokhtii, Tiziana Spina,, Ren\'e Fl\"ukiger, Luigi Muzzi, Enrico Silva

arXiv: 1901.03819 · 2019-01-15

## TL;DR

This study measures the surface impedance of Nb$_{3}$Sn at 15 GHz in high magnetic fields up to 12 T, revealing its potential for RF applications due to high depinning frequencies and strong vortex pinning.

## Contribution

First surface impedance measurements of Nb$_{3}$Sn at high magnetic fields, providing new insights into its vortex dynamics and suitability for RF technology.

## Key findings

- Measured $
u_p$ in Nb$_{3}$Sn is several times higher than in pure Nb.
- Nb$_{3}$Sn exhibits strong vortex pinning at high frequencies.
- Results suggest Nb$_{3}$Sn's potential for high-field RF applications.

## Abstract

Nb$_{3}$Sn is a superconductor of great relevance for perspective RF applications. We present for the first time surface impedance $Z_s$ measurements at 15 GHz and low RF field amplitude on Nb$_{3}$Sn in high magnetic fields up to 12 T, with the aim of increasing the knowledge of Nb$_{3}$Sn behavior in such conditions. $Z_s$ is a fundamental material parameter that directly gives useful information about the dissipative and reactive phenomena when the superconductor is subjected to high-frequency excitations. Therefore, we present an analysis of the measured $Z_s$ with the aim of extracting interesting data about pinning in Nb$_{3}$Sn at high frequencies. From $Z_s$ we extract the vortex motion complex resistivity to obtain the $r$-parameter and the depinning frequency $\nu_p$ in high magnetic fields. The comparison of the results with the literature shows that the measured $\nu_p$ on bulk Nb$_{3}$Sn is several times greater than that of pure Nb. This demonstrates how Nb$_{3}$Sn can be a good candidate for RF technological applications, also in high magnetic fields.

## Full text

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## Figures

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## References

33 references — full list in the complete paper: https://tomesphere.com/paper/1901.03819/full.md

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Source: https://tomesphere.com/paper/1901.03819