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Quantitative modeling of spintronic terahertz emission due to ultrafast spin transport
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Theory.
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Materials Theory.ORCID iD: 0000-0002-9069-2631
2025 (English)In: Physical Review Applied, E-ISSN 2331-7019, Vol. 23, no 1, article id 014067Article in journal (Refereed) Published
Abstract [en]

In spintronic terahertz (THz) emitters, THz radiation is generated by exciting an ultrafast spin current through femtosecond laser excitation of a ferromagnetic-nonmagnetic metallic heterostructure. Although an extensive phenomenological knowledge has been built up during the last decade, a solid theoretical modeling that connects the generated THz signal to the laser induced-spin current is still incomplete. Here, starting from general solutions to Maxwell's equations, we model the electric field generated by a superdiffusive spin current in spintronic emitters, taking Co/Pt as a typical example. We explicitly include the detector shape, which is shown to significantly influence the detected THz radiation. Additionally, the electron energy dependence of the spin Hall effect is taken into account, as well as the duration of the exciting laser pulse and the thickness of the detector crystal. Our modeling leads to realistic emission profiles and highlights the role of the detection method for distinguishing key features of the spintronic THz emission.

Place, publisher, year, edition, pages
American Physical Society, 2025. Vol. 23, no 1, article id 014067
National Category
Atom and Molecular Physics and Optics Condensed Matter Physics
Identifiers
URN: urn:nbn:se:uu:diva-552354DOI: 10.1103/PhysRevApplied.23.014067ISI: 001436408100014OAI: oai:DiVA.org:uu-552354DiVA, id: diva2:1944624
Funder
Swedish Research Council, 2022-06725Knut and Alice Wallenberg Foundation, 2022.0079Knut and Alice Wallenberg Foundation, 2023.0336EU, Horizon 2020, 863155Available from: 2025-03-14 Created: 2025-03-14 Last updated: 2025-03-14Bibliographically approved

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