Bulletin of the American Physical Society
APS March Meeting 2022
Volume 67, Number 3
Monday–Friday, March 14–18, 2022; Chicago
Session D52: Magnetization and Spin Dynamics II: YIG-based and AFM Materials
3:00 PM–6:00 PM,
Monday, March 14, 2022
Room: McCormick Place W-475A
Sponsoring
Unit:
GMAG
Chair: Rico Schoeneman, Los Alamos National Laboratory
Abstract: D52.00003 : Spin-wave amplification using spin-orbit torque in ultra-thin BiYIG/Pt microscopic waveguide
3:24 PM–3:36 PM
Presenter:
Hugo Merbouche
(Westfälische Wilhelms-Universität Münster)
Authors:
Hugo Merbouche
(Westfälische Wilhelms-Universität Münster)
Boris Divinskiy
(Institute for Applied Physics, University of Muenster)
Diane Gouéré
(Unité Mixte de Physique CNRS-Thales)
Aya El Kanj
(Unité Mixte de Physique CNRS-Thales)
Romain Lebrun
(Unité Mixte de Physique CNRS-Thales)
Vincent Cros
(Unité Mixte de Physique CNRS-Thales)
Paolo Bortolotti
(Unité Mixte de Physique CNRS-Thales)
Vladislav E Demidov
(Institute for Applied Physics, University of Muenster)
Sergej O Demokritov
(Institute for Applied Physics, University of Muenster)
Abdelmadjid Anane
(Unité Mixte de Physique CNRS-Thales)
By applying a dc current in the Pt, the effective damping is decreased due to the SOT that compensate the Gilbert damping. Once the current reaches a threshold value, the vanishing effective damping allows for the onset of the auto-oscillation (AO) regime. However, SWs strongly interact with the AO, preventing their amplification (as similarly observed in other studies). Using an rf and DC pulse scheme, we propagate rf-excited SWs before the onset of non-linearities and observe their clear amplification. Above the critical current, the SW intensity exponentially increases with the propagation distance (negative effective damping), up to a 12 µm amplification length (corresponding to a 5 time increase in intensity over 10 µm). Furthermore, we evidence the key role of the vanishing effective magnetization of the BiYIG film that suppresses the non-linear interactions that have so far prevented the amplification of propagating SWs using SOT.
This experiment sheds new light on the influence of SOT on propagating SWs and pave the way toward an efficient magnonic amplifier using DC current.
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