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First-principles study of ultrafast spin dynamics in FemB20 (m = 1, 2) clusters

Lu Xin Xie Meng-Lin Liu Jing Jin Wei Li Chun Georgios Lefkidis Wolfgang Hübner

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First-principles study of ultrafast spin dynamics in FemB20 (m = 1, 2) clusters

Lu Xin, Xie Meng-Lin, Liu Jing, Jin Wei, Li Chun, Georgios Lefkidis, Wolfgang Hübner
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  • In this study, we use first-principles calculations to investigate the geometry, the electronic and the magnetic structure as well as to propose the laser-induced ultrafast spin dynamics on the tubular FeB20 and Fe2B20 clusters. Our results show that the FeB20 is a stable configuration when its Fe atom gets preferably adsorbed inside the B20 tube, while the Fe2B20 is more stable configuration when one of its two Fe atoms is located inside and the other outside the boron tube. In the latter cluster, due to the higher number of d states introduced by the additional magnetic atom, the density-of-states in the low-energy region becomes higher, thus leading to richer spin dynamics. The different local geometries of the two Fe atoms lead to a multitude of many-body states with high degree of spin-density localization. Based on the calculated ground state and excited states and by using suitably tailored laser pulses we achieve ultrafast spin-flip and spin crossover scenarios for both structures. Besides, the spin-flips reach a high fidelity (above 89.7%) and are reversible, while the crossovers have lower fidelity (below 78%) and are irreversible. We also propose an ultrafast spin-transfer process from Fe2 to Fe1 for Fe2B20. The present investigation, in which we predict various ultrafast spin dynamic taken by magnetic atoms absorbed inside and outside of tubular boron clusters, is expected to provide significant theoretical guidance for the future experimental implementation and the potential applications of the relevant spin logic functional devices.
      Corresponding author: Jin Wei, jinwei@snnu.edu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 11504223, 11872309) and the Natural Science Basic Research Plan in Shaanxi Province of China (Grant No. 2017JM1033)
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  • 图 1  优化后的团簇结构 (侧视图和俯视图) (a) B20; (b) FeB20; (c) Fe2B20; 其中, 俯视图中的键长单位为 Å

    Figure 1.  Side- and top-viewed optimized geometries of clusters: (a) B20; (b) FeB20; (c) Fe2B20. The bond lengths are in Å.

    图 2  FeB20与Fe2B20的SAC-CI能级, 黑色虚线表示单重态, 红色实线表示三重态. 其中, 各自旋动力学所涉及的有关初、末态在未考虑自旋轨道耦合时的能级位置被明确标出

    Figure 2.  The SAC-CI energy levels of clusters FeB20 and Fe2B20. The singlet and triplet terms are denoted by the black dashed and red solid lines, respectively. The related terms from which the involved initial and final states in the spin dynamics to be discussed later originate before the inclusion of SOC are marked.

    图 3  超快自旋翻转动力学 (a) FeB20团簇的自旋翻转过程; (b) Fe2B20团簇的自旋翻转过程. 其中各动力学中初态、末态和中间态分别由黑色虚线、红色实线和点线表示

    Figure 3.  Ultrafast spin flip scenarios: (a) Spin-flip process in FeB20; (b) spin-flip process in Fe2B20. The initial, final, and intermediate states involved in each of the spin-flip processes are represented by the black dashed, red solid, and dotted lines, respectively.

    图 4  Fe2B20团簇上得到的超快自旋转移动力学, 其中初态、末态和中间态分别由黑色虚线、红色实线和点线表示

    Figure 4.  Ultrafast spin-transfer scenario in Fe2B20. The initial, final, and intermediate states involved in the spin-transfer process are represented by the black dashed, red solid, and dotted lines, respectively.

    图 5  超快自旋交叉动力学 (a) FeB20团簇的自旋交叉过程; (b) Fe2B20团簇的自旋交叉过程; 其中各动力学中初态、末态和中间态分别由黑色虚线、红色实线和点线表示

    Figure 5.  Ultrafast spin crossover scenarios: (a) Spin-crossover process in FeB20; (b) spin-crossover process in Fe2B20. The initial, final, and intermediate states involved in each of the spin-crossover processes are represented by black dashed, red solid, and dotted lines, respectively.

    图 A1  团簇FeB20与Fe2B20的其他稳定构型

    Figure A1.  Other stable geometries of clusters FeB20 and Fe2B20.

    表 1  Fe2B20中具有单磁中心自旋局域能态的能量、自旋期望值及自旋密度

    Table 1.  Energies, spin expectation values, and spin density of the states with spin localized on one single magnetic atom for cluster Fe2B20.

    StructureStateEnergy/eV$ \left\langle { {S}_{x} } \right\rangle $$ \left\langle { {S}_{y} } \right\rangle $$ \left\langle { {S}_{z} } \right\rangle $Spin density
    Fe1Fe2B20
    $ \left| {1} \right\rangle $00.38–0.8700.0011.9190.015
    $ \left| {2} \right\rangle $0.001–0.590.7300.0011.9110.015
    $ \left| {5} \right\rangle $0.5130.21–0.4200.0020.9460.023
    $ \left| {6} \right\rangle $0.515–0.120.4600.0020.9620.023
    $ \left| {17} \right\rangle $1.7970.16–0.7200.0221.4730.224
    $ \left| {18} \right\rangle $1.797–0.420.0500.0130.8390.13
    Fe2B20$ \left| {19} \right\rangle $1.7970.260.6700.0211.4320.22
    (B: θ = 90°, φ = 90°)$ \left| {25} \right\rangle $2.0020.41–0.3500.0041.0990.120
    $ \left| {26} \right\rangle $2.003–0.230.5400.0051.1890.133
    $ \left| {39} \right\rangle $2.658–0.02–0.6301.1140.0840.261
    $ \left| {41} \right\rangle $2.659–0.010.6301.1140.0840.261
    $ \left| {56} \right\rangle $2.9480.42–0.6300.0261.4120.305
    $ \left| {57} \right\rangle $2.949–0.520.5500.0261.4110.303
    DownLoad: CSV

    表 2  各自旋动力学过程中初、末态的能量、自旋期望值与自旋密度

    Table 2.  Energies, spin expectation values, and spin densities of the initial and final states of each scenario.

    ScenarioStructureStateEnergy/eV$ \left\langle { {S}_{x} } \right\rangle $$ \left\langle { {S}_{y} } \right\rangle $$ \left\langle { {S}_{z} } \right\rangle $Spin density
    Fe1Fe2
    Flip FeB20$ \left| {4} \right\rangle $ 1.021 –0.94 0 0 1.291
    (B: θ = 90°, φ = 90°) $ \left| {6} \right\rangle $ 1.022 0.94 0 0 1.291
    Fe2B20 $ \left| {8} \right\rangle $ 0.856 0 0 0.89 0.006 1.785
    (B: θ = 0°, φ = 90°) $ \left| {9} \right\rangle $ 0.857 0 0 –0.89 0.006 1.785
    Transfer Fe2B20$ \left| {1} \right\rangle $ 0 0.38 –0.87 0 0.001 1.919
    (B: θ = 90°, φ = 90°) $ \left| {41} \right\rangle $ 2.659 0.01 0.63 0 1.114 0.084
    CrossoverFeB20$ \left| {6} \right\rangle $ 1.022 0.94 0 0 1.291
    (B: θ = 90°, φ = 90°) $ \left| {7} \right\rangle $ 1.133 0 0 0 0
    Fe2B20$ \left| {37} \right\rangle $ 2.371 0 0 0 0 0
    (B: θ = 90°, φ = 90°)$ \left| {45} \right\rangle $ 2.784 0 –0.52 0 0.090 0.873
    DownLoad: CSV

    表 3  超快自旋动力学过程所需的激光参数, 其中 θφ为入射激光在球坐标系下的方位角, γ为入射激光振动方向和光平面的夹角, FWHM为激光脉冲的半高全宽

    Table 3.  Laser parameters for the achieved scenarios. Here, θ and φ denote the angles of the incidence in spherical coordinates, and γ is the angle between the polarization of the light and the optical plane. FWHM is the full width at half maximum of the laser pulse.

    ScenarioStructureInitial/Final
    state
    FidelityLaser parameters
    θ/(º)φ(º)γ/(º)FWHM
    /fs
    Amplitude
    /(atomic units)
    Energy
    /eV
    FlipFeB20$ \left| {4} \right\rangle \to \left| {6} \right\rangle $89.7%112.96.1338.9337.30.009970.299
    Fe2B20$ \left| {8} \right\rangle \to \left| {9} \right\rangle $93.5%156.4122.477.7466.20.006342.114
    TransferFe2B20$ \left| {1} \right\rangle \to \left| {41} \right\rangle $91.9%244.791.4225.392.30.007812.661
    CrossoverFeB20$ \left| {6} \right\rangle \to \left| {7} \right\rangle $77.9%61.0321.482.9318.50.007830.212
    Fe2B20$ \left| {37} \right\rangle \to \left| {45} \right\rangle $74.5%297.2356.1301.5352.00.003060.416
    DownLoad: CSV

    表 A1  FeB20 and Fe2B20团簇所计算能态在未考虑SOC和考虑SOC之后的能量值(单位: eV)

    Table A1.  Energy values of the calculated states of clusters FeB20 and Fe2B20 before and after the inclusion of SOC (in eV)

    FeB20 Fe2B20
    Before SOC After SOC Before SOC After SOC
    Singlet 1.131 (1 1A') 1.133 1.504 (1 1A') 1.489
    1.133 (2 1A') 1.134 1.850 (1 1A'') 1.857
    2.320 (1 1A'') 2.319 2.199 (2 1A') 2.203
    2.545 (SAC) 2.554 2.361 (SAC) 2.371
    2.676 (2 1A'') 2.677 2.587 (3 1A') 2.592
    2.676 (3 1A') 2.677 2.801 (2 1A'') 2.806
    3.130 (3 1A'') 3.132 2.843 (4 1A') 2.845
    3.636 (4 1A'') 3.638 2.996 (3 1A'') 3.002
    4.266 (5 1A'') 4.269 3.133 (5 1A') 3.136
    4.272 (4 1A') 4.272 3.429 (4 1A'') 3.434
    4.282 (5 1A') 4.285 3.632 (5 1A'') 3.637
    Triplet 0.000 (1 3A') 0.000 0.0005 0.001 0.000 (1 3A') 0.000 0.0007 0.002
    1.019 (2 3A') 1.021 1.021 1.022 0.508 (1 3A'') 0.511 0.513 0.515
    1.291 (3 3A') 1.271 1.271 1.294 0.851 (2 3A') 0.854 0.857 0.857
    1.293 (1 3A'') 1.295 1.313 1.317 1.545 (2 3A'') 1.548 1.551 1.570
    1.476 (2 3A'') 1.475 1.478 1.478 1.668 (3 3A') 1.673 1.673 1.673
    2.361 (3 3A'') 2.363 2.363 2.364 1.793 (4 3A') 1.797 1.797 1.797
    2.945 (4 3A'') 2.947 2.947 2.948 1.984 (5 3A') 1.989 1.989 1.989
    3.119 (5 3A'') 3.120 3.121 3.121 1.997 (3 3A'') 2.001 2.002 2.003
    3.462 (4 3A') 3.464 3.465 3.466 2.089 (6 3A') 2.093 2.094 2.094
    3.467 (6 3A'') 3.470 3.471 3.471 2.100 (4 3A'') 2.105 2.105 2.105
    3.471 (7 3A'') 3.473 3.473 3.474 2.112 (7 3A') 2.113 2.116 2.116
    3.743 (5 3A') 3.745 3.745 3.745 2.653 (8 3A') 2.658 2.658 2.659
    3.753 (8 3A'') 3.755 3.755 3.756 2.707 (5 3A'') 2.711 2.713 2.714
    3.990 (6 3A') 3.989 3.990 3.994 2.779 (9 3A') 2.784 2.784 2.784
    4.000 (7 3A') 4.003 4.008 4.008 2.783 (6 3A'') 2.787 2.788 2.788
    4.419 (8 3A') 4.421 4.421 4.421 2.934 (10 3A') 2.939 2.939 2.940
    4.435 (9 3A'') 4.436 4.436 4.438 2.943 (7 3A'') 2.948 2.949 2.952
    4.436 (9 3A') 4.438 4.440 4.440 3.144 (8 3A'') 3.150 3.151 3.152
    4.536 (10 3A') 4.528 4.528 4.539 3.301 (9 3A'') 3.305 3.306 3.306
    4.540 (10 3A'') 4.543 4.554 4.557 3.338 (10 3A'') 3.343 3.343 3.344
    DownLoad: CSV
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    Khajetoorians A A, Heinrich A J 2016 Science 352 296Google Scholar

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    Wolf S A, Awschalom D D, Buhrman R A, Daughton J M, Von Molnar S, Roukes M L, Chtchelkanova A Y, Treger D M 2001 Science 294 1488Google Scholar

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    Prinz G A 1998 Science 282 1660Google Scholar

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    Bader S D, Parkin S S P 2010 Annu. Rev. Condens. Matter Phys. 1 71Google Scholar

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    Dietl T 2005 J. Magn. Magn. Mater. 290-291 14Google Scholar

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    Baibich M N, Broto J M, Fert A, Nguyen Van Dau F, Petroff F 1988 Phys. Rev. Lett. 61 2472Google Scholar

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    Beaurepaire E, Merle J C, Daunois A, Bigot J Y 1996 Phys. Rev. Lett. 76 4250Google Scholar

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    Scholl A, Baumgarten L, Jacquemin R, Eberhardt W 1997 Phys. Rev. Lett. 79 5146Google Scholar

    [10]

    Pfau B, Schaffert S, Müller L, Gutt C, Al-shemmary. A, Büttner F, Delaunay R, Düsterer S, Flewett S, Frömter R, Geilhufe J, Guehrs E, Günther C M, Hawaldar R, Hille M, Jaouen N, Kobs A, Li K, Mohanty J, Redlin H, Schlotter W F, Stickler D, Treusch R, Vodungbo B, Kläui M, Oepen H P, Lüning J, Grübel G, Eisebitt S 2012 Nat. Commun. 3 1100Google Scholar

    [11]

    Koopmans B, Ruigrok J J M, Longa F D, de Jonge W J M 2005 Phys. Rev. Lett. 95 267207Google Scholar

    [12]

    Steiauf D, Fähnle M 2009 Phys. Rev. B 79 140401Google Scholar

    [13]

    Battiato M, Carva K, Oppeneer P M 2010 Phys. Rev. Lett. 105 027203Google Scholar

    [14]

    Bigot J Y, Vomir M, Beaurepaire E 2009 Nat. Phys. 5 515Google Scholar

    [15]

    Gómez-Abal R, Hübner W 2002 Phys. Rev. B 65 195114Google Scholar

    [16]

    Zhang Z Z, Cui B, Wang G Z, Ma B, Jin Q Y, Liu Y W 2010 Appl. Phys. Lett. 97 172508Google Scholar

    [17]

    Zhang W, Liu Q, Yuan Z, Xia K, He W, Zhan Q F, Zhang X Q, Cheng Z H 2019 Phys. Rev. B 100 104412Google Scholar

    [18]

    Lefkidis G, Reyes S A 2016 Phys. Rev. B 94 144433Google Scholar

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    李春, 杨帆, Lefkidis G, Hübner W 2011 60 017802Google Scholar

    Li C, Yang F, Lefkidis G, Hübner W 2011 Acta Phys. Sin. 60 017802Google Scholar

    [20]

    Chaudhuri D, Xiang H P, Lefkidis G, Hübner W 2014 Phys. Rev. B 90 245113Google Scholar

    [21]

    Jin W, Li C, Lefkidis G, Hübner W 2014 Phys. Rev. B 89 024419Google Scholar

    [22]

    Chaudhuri D, Lefkidis G, Hübner W 2017 Phys. Rev. B 96 184413Google Scholar

    [23]

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Metrics
  • Abstract views:  5718
  • PDF Downloads:  118
  • Cited By: 0
Publishing process
  • Received Date:  10 January 2021
  • Accepted Date:  08 February 2021
  • Available Online:  11 June 2021
  • Published Online:  20 June 2021

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