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Orbital Pumping by Magnetization Dynamics in Ferromagnets

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arxiv 2309.14817 v2 pith:VKYJQ2RZ submitted 2023-09-26 cond-mat.mes-hall cond-mat.mtrl-sci

classification cond-mat.mes-hallcond-mat.mtrl-sci
keywords orbitalpumpingmagnetizationangulardynamicsmomentumferromagnetsresults
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abstract

We show that dynamics of the magnetization in ferromagnets can pump the orbital angular momentum, which we denote by orbital pumping. This is the reciprocal phenomenon to the orbital torque that induces magnetization dynamics by the orbital angular momentum in non-equilibrium. The orbital pumping is analogous to the spin pumping established in spintronics but requires the spin-orbit coupling for the orbital angular momentum to interact with the magnetization. We develop a formalism that describes the generation of the orbital angular momentum by magnetization dynamics within the adiabatic perturbation theory. Based on this, we perform first-principles calculation of the orbital pumping in prototypical $3d$ ferromagnets, Fe, Co, and Ni. The results show that the ratio between the orbital pumping and the spin pumping ranges from 5 to 15 percents, being smallest in Fe and largest in Ni. This implies that ferromagnetic Ni is a good candidate for measuring the orbital pumping. Implications of our results on experiments are also discussed.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Orbital Pumping in Ferrimagnetic Insulators

    cond-mat.mes-hall 2025-06 conditional novelty 7.0 of 10

    Orbital currents are generated directly from magnetization dynamics of the ferrimagnetic insulator BiYIG and detected in naturally oxidized Cu, with spin currents shown to dominate in Cr.

  2. Extrinsic Orbital Hall Effect and Orbital Relaxation in Mesoscopic Devices

    cond-mat.mes-hall 2025-07 conditional novelty 6.0 of 10

    Disorder enhances the orbital Hall response in 2D mesoscopic devices through skew scattering, and width-dependent decay of the orbital current yields long orbital relaxation lengths.

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