2022
DOI: 10.21203/rs.3.rs-1849457/v1
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Deeply nonlinear excitation of self-normalised exchange spin waves

Abstract: Spin waves are ideal candidates for wave-based computing, but the construction of magnetic circuits is blocked by a lack of an efficient mechanism to excite long-running exchange spin waves with normalised amplitudes. Here, we solve the challenge by exploiting the deeply nonlinear phenomena of forward-volume spin waves in 200 nm wide nanoscale waveguides and validate our concept with microfocused Brillouin light scattering spectroscopy. An unprecedented nonlinear frequency shift of >2 GHz is achieved, corre… Show more

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Cited by 2 publications
(14 citation statements)
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“…The frequency step is small enough so that magnon state evolves from a preceding one. As a result, the up and down frequency sweep curves do not overlap and show a hysteretic response resulting in a large bistable frequency window of ~1.1 GHz which is similar to our previous study [14]. The nature of this bistable window is similar to those observed in a common nonlinear oscillator (e.g., Duffing oscillator) when the foldover effect takes place, although there are certain differences (see Supplementary Materials).…”
Section: Resultssupporting
confidence: 83%
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“…The frequency step is small enough so that magnon state evolves from a preceding one. As a result, the up and down frequency sweep curves do not overlap and show a hysteretic response resulting in a large bistable frequency window of ~1.1 GHz which is similar to our previous study [14]. The nature of this bistable window is similar to those observed in a common nonlinear oscillator (e.g., Duffing oscillator) when the foldover effect takes place, although there are certain differences (see Supplementary Materials).…”
Section: Resultssupporting
confidence: 83%
“…where fk,0 is the linear (small-amplitude) spin-wave frequency, Tk > 0 is the nonlinear frequency shift coefficient, and ck is canonic spin wave amplitude. In our case of forward spin waves, 𝑐 𝑘 2 ≈ 1 − cos 𝜃 ̅̅̅̅̅̅̅ , where θ is the precession angle and overbar means averaging over the waveguide width [14]. The nonlinear frequency shift coefficient in the range from k = 0 to k ≈ 20μm -1 , which is the wavenumber of spin waves excited by the CPW antenna, weakly depends on k. Then, the effect of the incident spin waves can be imagined as a shift of the whole spin wave spectrum by the value Δ𝑓 = 𝑇 𝑘 𝑐 𝑘 2 [31].…”
Section: Resultsmentioning
confidence: 99%
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