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Heat-conserving three-temperature model for ultrafast demagnetization in nickel
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.ORCID iD: 0000-0002-5974-6160
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.ORCID iD: 0000-0003-1018-9647
Örebro University, School of Science and Technology. Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.ORCID iD: 0000-0001-8007-5392
Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden.
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2022 (English)In: Physical Review B, ISSN 2469-9950, E-ISSN 2469-9969, Vol. 106, no 17, article id 174407Article in journal (Refereed) Published
Abstract [en]

Multireservoir models are widely used for modeling and interpreting ultrafast magnetization dynamics. Here we introduce an alternative formulation to existing three-temperature models for the treatment of spin, electron, and lattice temperatures in magnetization dynamics simulations. In contrast to most existing models of calculations of energy transfer between reservoirs in these types of simulations, the heat distribution of the spin and lattice subsystems is evaluated during the simulation instead of being calculated a priori. The model is applied to investigate the demagnetization and remagnetization of fcc Ni, when subjected to a strong laser pulse. In particular, our model results in a fast interplay between the electron and spin subsystems which reproduces the main features of experimental data for fcc Ni significantly better than most reported three-temperature models. We also show that the way in which the electron, spin, and lattice heat capacities are described can have a significant impact on the simulated ultrafast dynamics. By introducing spin-lattice couplings in the simulation, it is shown that these explicit interactions only have a marginal impact on the magnetization dynamics of fcc Ni, albeit it is more pronounced for higher laser pulse powers. 

Place, publisher, year, edition, pages
American Physical Society , 2022. Vol. 106, no 17, article id 174407
National Category
Condensed Matter Physics
Identifiers
URN: urn:nbn:se:oru:diva-104671DOI: 10.1103/physrevb.106.174407ISI: 000929827800003Scopus ID: 2-s2.0-85142310719OAI: oai:DiVA.org:oru-104671DiVA, id: diva2:1741286
Funder
Knut and Alice Wallenberg Foundation, 2018.0060Swedish Foundation for Strategic ResearchEU, European Research Council, 854843-FASTCORRSwedish Research Council, 2019-03666Swedish Research Council, 2016-05980Swedish Research Council, 2019-05304Swedish Research Council, 2018-05973StandUpAvailable from: 2023-03-03 Created: 2023-03-03 Last updated: 2023-03-14Bibliographically approved

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Thonig, DannyEriksson, Olle

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