# High Spin-Wave Propagation Length Consistent with Low Damping in a   Metallic Ferromagnet

**Authors:** Luis Flacke, Lukas Liensberger, Matthias Althammer, Hans Huebl,, Stephan Gepr\"ags, Katrin Schultheiss, Aleksandr Buzdakov, Tobias Hula,, Helmut Schultheiss, Eric R. J. Edwards, Hans T. Nembach, Justin M. Shaw,, Rudolf Gross, Mathias Weiler

arXiv: 1904.11321 · 2019-10-03

## TL;DR

This study demonstrates ultra-low magnetic damping and long spin-wave propagation lengths in Co25Fe75 heterostructures at room temperature, highlighting their potential for magnonic applications.

## Contribution

It provides the first comprehensive measurement of intrinsic damping and spin-wave propagation lengths in Co25Fe75 at room temperature, confirming their suitability for low-loss magnonic devices.

## Key findings

- Intrinsic damping as low as 3.18×10⁻⁴ in 26 nm Co25Fe75
- Spin-wave propagation length of approximately 21 μm at room temperature
- Excellent agreement between damping measurements and spin-wave propagation lengths

## Abstract

We report ultra-low intrinsic magnetic damping in Co$_{\text{25}}$Fe$_{\text{75}}$ heterostructures, reaching the low $10^{-4}$ regime at room temperature. By using a broadband ferromagnetic resonance technique, we extracted the dynamic magnetic properties of several Co$_{\text{25}}$Fe$_{\text{75}}$-based heterostructures with varying ferromagnetic layer thickness. By estimating the eddy current contribution to damping, measuring radiative damping and spin pumping effects, we found the intrinsic damping of a 26\,nm thick sample to be $$\alpha_{\mathrm{0}} \lesssim 3.18\times10^{-4}$. Furthermore, using Brillouin light scattering microscopy we measured spin-wave propagation lengths of up to $(21\pm1)\,\mathrm{\mu m}$ in a 26 nm thick Co$_{\text{25}}$Fe$_{\text{75}}$ heterostructure at room temperature, which is in excellent agreement with the measured damping.

## Full text

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## Figures

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## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1904.11321/full.md

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Source: https://tomesphere.com/paper/1904.11321