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      Resolving the role of femtosecond heated electrons in ultrafast spin dynamics

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          Abstract

          Magnetization manipulation is essential for basic research and applications. A fundamental question is, how fast can the magnetization be reversed in nanoscale magnetic storage media. When subject to an ultrafast laser pulse, the speed of the magnetization dynamics depends on the nature of the energy transfer pathway. The order of the spin system can be effectively influenced through spin-flip processes mediated by hot electrons. It has been predicted that as electrons drive spins into the regime close to almost total demagnetization, characterized by a loss of ferromagnetic correlations near criticality, a second slower demagnetization process takes place after the initial fast drop of magnetization. By studying FePt, we unravel the fundamental role of the electronic structure. As the ferromagnet Fe becomes more noble in the FePt compound, the electronic structure is changed and the density of states around the Fermi level is reduced, thereby driving the spin correlations into the limit of critical fluctuations. We demonstrate the impact of the electrons and the ferromagnetic interactions, which allows a general insight into the mechanisms of spin dynamics when the ferromagnetic state is highly excited, and identifies possible recording speed limits in heat-assisted magnetization reversal.

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          Most cited references5

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          Ultrafast Spin Dynamics in Ferromagnetic Nickel

          Physical Review Letters, 76(22), 4250-4253
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            Scaling and critical slowing down in random-field Ising systems.

            Fisher (1986)
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              The ultimate speed of magnetic switching in granular recording media.

              In magnetic memory devices, logical bits are recorded by selectively setting the magnetization vector of individual magnetic domains either 'up' or 'down'. In such devices, the fastest and most efficient recording method involves precessional switching: when a magnetic field B(p) is applied as a write pulse over a period tau, the magnetization vector precesses about the field until B(p)tau reaches the threshold value at which switching occurs. Increasing the amplitude of the write pulse B(p) might therefore substantially shorten the required switching time tau and allow for faster magnetic recording. Here we use very short pulses of a very high magnetic field to show that under these extreme conditions, precessional switching in magnetic media supporting high bit densities no longer takes place at well-defined field strengths; instead, switching occurs randomly within a wide range of magnetic fields. We attribute this behaviour to a momentary collapse of the ferromagnetic order of the spins under the load of the short and high-field pulse, thus establishing an ultimate limit to the speed of deterministic switching and magnetic recording.
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                Author and article information

                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group
                2045-2322
                05 February 2014
                2014
                : 4
                : 3980
                Affiliations
                [1 ]I. Physikalisches Institut, Universität Göttingen , Friedrich-Hund Platz 1, 37077 Göttingen, Germany
                [2 ]Instituto de Ciencia de Materiales de Madrid, CSIC , Cantoblanco, 28049 Madrid, Spain
                [3 ]San Jose Research Center, HGST , a Western Digital Company, 3403 Yerba Buena Rd., San Jose, California 95135, USA
                [4 ]Institut für Physik, Universität Greifswald Felix-Hausdorff-Straβe 6, 17489 Greifswald , Germany
                Author notes
                Article
                srep03980
                10.1038/srep03980
                3913971
                24496221
                42b1cdda-e10a-49c7-bdeb-f5bb55bc4029
                Copyright © 2014, Macmillan Publishers Limited. All rights reserved

                This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses/by/3.0/

                History
                : 10 October 2013
                : 15 January 2014
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