Thermal Spin Wave Noise as a Probe for the Dzyaloshinskii-Moriya Interaction

Interfacial Dzyaloshinskii-Moriya interaction (DMI) is a key ingredient in the stabilization of chiral magnetic states in thin films. Its sign and strength often determine crucial properties of magnetic objects, like their topology or how they can be manipulated with currents. A few experimental techniques are currently available to measure DMI quantitatively, based on the study of domain walls, spin waves, or spin-orbit torques. In this Letter, we propose a qualitative variant of spin wave methods. We rely on magnetic noise from confined thermal spin waves in domain walls and skyrmions in perpendicularly magnetized thin films, which we probe with scanning nitrogen-vacancy center relaxometry. We show both numerically and experimentally that the sign of the DMI can be inferred from the amplitude of the detected noise, which is affected by the nonreciprocity in the spin wave dispersion. Furthermore, we also demonstrate that the noise distribution around the contour of magnetic skyrmions reveals their Néel or Bloch nature, giving therefore also insight into the strength of DMI involved in their stabilization.

Authors

Institutions

Publication Details

Journal
Physical Review Letters
Published
2025-09-24
DOI
https://doi.org/10.1103/dvbq-9z5f
Citations
1
Primary Topic
Magnetic properties of thin films
Type
article
Field-Weighted Citation Impact
1.25
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Thermal Spin Wave Noise as a Probe for the Dzyaloshinskii-Moriya Interaction

Van Tuong Pham, Maxime Rollo, Joo-Von Kim, Aurore Finco et al.
1 citations
Physical Review Letters
Magnetic properties of thin films
1.25
article

Thermal Spin Wave Noise as a Probe for the Dzyaloshinskii-Moriya Interaction

Van Tuong Pham, Maxime Rollo, Joo-Von Kim, Aurore Finco, Olivier Boulle, Rodrigo Guedas, Pawan Kumar, V. Jacques, Joseba Urrestarazu-Larrañaga
article en
1 citations

Abstract

Interfacial Dzyaloshinskii-Moriya interaction (DMI) is a key ingredient in the stabilization of chiral magnetic states in thin films. Its sign and strength often determine crucial properties of magnetic objects, like their topology or how they can be manipulated with currents. A few experimental techniques are currently available to measure DMI quantitatively, based on the study of domain walls, spin waves, or spin-orbit torques. In this Letter, we propose a qualitative variant of spin wave methods. We rely on magnetic noise from confined thermal spin waves in domain walls and skyrmions in perpendicularly magnetized thin films, which we probe with scanning nitrogen-vacancy center relaxometry. We show both numerically and experimentally that the sign of the DMI can be inferred from the amplitude of the detected noise, which is affected by the nonreciprocity in the spin wave dispersion. Furthermore, we also demonstrate that the noise distribution around the contour of magnetic skyrmions reveals their Néel or Bloch nature, giving therefore also insight into the strength of DMI involved in their stabilization.

Physical Review LettersVol. 135(13)
Centre de Nanosciences et de Nanotechnologies (FR), Laboratoire Charles Coulomb (FR), Spintronique et Technologie des Composants (FR)
Openalex Percentile: Top 17%
Magnetic properties of thin films
1.25
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.