Coupled atomistic spin-lattice simulations of ultrafast demagnetization in 3d ferromagnetsShow others and affiliations
2024 (English)In: Scientific Reports, E-ISSN 2045-2322, Vol. 14, no 1, article id 8138
Article in journal (Refereed) Published
Abstract [en]
Despite decades of research, the role of the lattice and its coupling to the magnetisation during ultrafast demagnetisation processes is still not fully understood. Here we report on studies of both explicit and implicit lattice effects on laser induced ultrafast demagnetisation of bcc Fe and fcc Co. We do this using atomistic spin- and lattice dynamics simulations following a heat-conserving three-temperature model. We show that this type of Langevin-based simulation is able to reproduce observed trends of the ultrafast magnetization dynamics of fcc Co and bcc Fe. The parameters used in our models are all obtained from electronic structure theory, with the exception of the lattice dynamics damping term, where a range of parameters were investigated. It was found that while the explicit spin-lattice coupling in the studied systems does not impact the demagnetisation process notably, the lattice damping has a large influence on the details of the magnetization dynamics. The dynamics of Fe and Co following the absorption of a femtosecond laser pulse are compared with previous results for Ni and similarities and differences in the materials' behavior are analysed. For all elements investigated so far with this model, we obtain a linear relationship between the value of the maximally demagnetized state and the fluence of the laser pulse , which is in agreement with experiments. Moreover, we demonstrate that the demagnetization amplitude is largest for Ni and smallest for Co. This holds over a wide range of the reported electron-phonon couplings, and this demagnetization trend is in agreement with recent experiments.
Place, publisher, year, edition, pages
Springer Nature, 2024. Vol. 14, no 1, article id 8138
National Category
Condensed Matter Physics Atom and Molecular Physics and Optics
Identifiers
URN: urn:nbn:se:his:diva-24985DOI: 10.1038/s41598-024-58662-yISI: 001198141000015PubMedID: 38584162Scopus ID: 2-s2.0-85189824720OAI: oai:DiVA.org:his-24985DiVA, id: diva2:1949817
Funder
Knut and Alice Wallenberg Foundation, 2018.0060Knut and Alice Wallenberg Foundation, 2021.0246Knut and Alice Wallenberg Foundation, 2022.0108EU, European Research Council, 854843-FASTCORRSwedish Foundation for Strategic ResearchStandUpSwedish Research Council, 2019-03666Swedish Research Council, 2016-05980Swedish Research Council, 2019-05304Olle Engkvists stiftelseeSSENCE - An eScience CollaborationNational Academic Infrastructure for Supercomputing in Sweden (NAISS), 2023/1-10National Academic Infrastructure for Supercomputing in Sweden (NAISS), 2023/5-454National Academic Infrastructure for Supercomputing in Sweden (NAISS), 2023/1-44Swedish Research Council, 2018-05973
Note
CC BY 4.0
Tis work was financially supported by the Knut and Alice Wallenberg Foundation (Grant Numbers 2018.0060, 2021.0246, and 2022.0108), Vetenskapsrådet (Grant Numbers 2019-03666, 2016-05980, and 2019-05304), the European Research Council (Grant Number 854843-FASTCORR), the foundation for Strategic Research SSF, and Olle Engkvist foundation. Support from STandUP and eSSENCE is also acknowledged. O.E. and A.D. also acknowledge support from the Wallenberg Initiative Materials Science for Sustainability (WISE) funded by the Knut and Alice Wallenberg Foundation (KAW). Computations were enabled by resources provided by the National Academic Infrastructure for Supercomputing in Sweden (NAISS, projects 2023/1-10, 2023/5-454, and 2023/1-44) at both the National Supercomputing Centre (NSC, Tetralith) and the PDC Centre for High Performance Computing (PDC-KTH, Dardel), partially funded by the Swedish Research Council through Grant Agreement No. 2018-05973. P.S. acknowledges support from the ANR-20-CE09-0013 UFO.
2025-04-032025-04-032025-09-29