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arXiv · 1802.00861

Spin wave emission by spin-orbit torque antennas

Giacomo Talmelli·Florin Ciubotaru·Kevin Garello·Xiao Sun·Marc Heyns·Iuliana P. Radu·Christoph Adelmann·Thibaut Devolder
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Abstract

We study the generation of propagating spin waves in Ta/CoFeB waveguides by spin-orbit torque antennas and compare them to conventional inductive antennas. The spin-orbit torque was generated by a transverse microwave current across the magnetic waveguide. The detected spin wave signals for an in-plane magnetization across the waveguide (Damon-Eshbach configuration) exhibited the expected phase rotation and amplitude decay upon propagation when the current spreading was taken into account. Wavevectors up to about 6 rad/$\mu$m could be excited by the spin-orbit torque antennas despite the current spreading, presumably due to the non-uniformity of the microwave current. The relative magnitude of generated anti-damping spin-Hall and Oersted fields was calculated within an analytic model and it was found that they contribute approximately equally to the total effective field generated by the spin-orbit torque antenna. Due to the ellipticity of the precession in the ultrathin waveguide and the different orientation of the anti-damping spin-Hall and Oersted fields, the torque was however still dominated by the Oersted field. The prospects for obtaining a pure spin-orbit torque response are discussed, as are the energy efficiency and the scaling properties of spin-orbit torque antennas.

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Giacomo Talmelli, Florin Ciubotaru, Kevin Garello, Xiao Sun, Marc Heyns, Iuliana P. Radu, Christoph Adelmann, Thibaut Devolder. 2018-02-02. Spin wave emission by spin-orbit torque antennas. https://doi.org/10.1103/physrevapplied.10.044060

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