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Comment on "Proper and improper chiral magnetic interactions"
KTH. Univ Paris Saclay, CEA, CNRS, SPEC, F-91191 Gif Sur Yvette, France..
Uppsala Univ, Dept Phys & Astron, Box 516, SE-75120 Uppsala, Sweden..
Uppsala Univ, Dept Phys & Astron, Box 516, SE-75120 Uppsala, Sweden..
Uppsala Univ, Dept Phys & Astron, Box 516, SE-75120 Uppsala, Sweden..
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2022 (English)In: Physical Review B, ISSN 2469-9950, E-ISSN 2469-9969, Vol. 105, no 2, article id 026401Article in journal (Refereed) Published
Abstract [en]

In a recent paper by dos Santos Dias et al. [Phys. Rev. B 103, L140408 (2021)], a critique of earlier works analyzing low-energy spin Hamiltonians is put forth. To be precise, it is the large noncollinear contributions to the Dzyaloshinskii-Moriya interaction (DMI) that is the main concern of dos Santos Dias et al. In this Comment, we clarify the microscopic mechanisms for the large DMI that can be found in noncollinear magnets. Furthermore, we outline the complementary nature of the different parametrizations of a spin Hamiltonian, with strengths and weaknesses of both approaches. Specifically, we stress the physical insight in the interpretation of the DMI, when decomposed in microscopic electron and spin densities and currents.

Place, publisher, year, edition, pages
American Physical Society (APS) , 2022. Vol. 105, no 2, article id 026401
National Category
Condensed Matter Physics
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URN: urn:nbn:se:kth:diva-309261DOI: 10.1103/PhysRevB.105.026401ISI: 000752562600002Scopus ID: 2-s2.0-85123413200OAI: oai:DiVA.org:kth-309261DiVA, id: diva2:1643030
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QC 20220308

Available from: 2022-03-08 Created: 2022-03-08 Last updated: 2022-06-25Bibliographically approved

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Delin, Anna

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