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Spin Hall Effect Guang-Yu Guo ( ) Physics Dept, National Taiwan - PowerPoint PPT Presentation

Spin Hall Effect Guang-Yu Guo ( ) Physics Dept, National Taiwan University, Taiwan ( ) (A Colloquium Talk in Department of Physics, National Taiwan University, 22 April 2014) Plan of this Talk I.


  1. Spin Hall Effect Guang-Yu Guo ( 郭光宇 ) Physics Dept, National Taiwan University, Taiwan ( 國立臺灣大學物理系) (A Colloquium Talk in Department of Physics, National Taiwan University, 22 April 2014)

  2. Plan of this Talk I. Introduction, overview and outlook 1. What is spin Hall effect 2. Spin Hall effect observed in semiconductors 3. Large room-temperature spin Hall effect in metals 4. Spintronics, magneto-electric devices and spin Hall effect 5. Spin-off’s: Topological insulators and spin caloritronics II. Ab initio calculation of intrinsic spin Hall effect in solids 1. Motivations 2. Berry phase formalism for intrinsic Hall effects. 3. Intrinsic spin Hall effect in platinum III. Gigantic spin Hall effect in gold and multi-orbital Kondo effect 1. Gigantic spin Hall effect in gold/FePt 2. Spin Hall effect enhanced by multi-orbital Kondo effect. 3. Quantum Monte Carlo simulation IV. Summary

  3. I. Introduction, overview and outlook 1. What is spin Hall effect Lorentz force q × v B 1) Ordinal Hall Effect [Hall 1879] Edwin H. Hall (1855-1938) 2) Anomalous Hall Effect [Hall, 1880 & 1881] 3) Extrinsic spin Hall Effect [Dyakonov & Perel, JETP 1971] Spin current spin current Spin-orbit interaction dV r ( ) ( s L ⋅ ) Charge current dr (Mott or skew scattering)

  4. 4) Intrinsic spin Hall effect (1) In p-type zincblende semiconductors [Science 301, 1348 (2003)]   2    5 Luttinger model 2 2 = γ + γ − γ ⋅ H ( ) k 2 ( k S )   0 1 2 2 2 m 2   Dirac monopole  k   X = i + F k Equation of motion i il l m λ e  e > 0 (hole) k = E i i       k e λ  Anomalous velocity X = − k × E 3 m  k λ n h = 10 19 cm -3 , μ = 50 cm /V·s, σ = e μ n h = 80 Ω -1 cm -1 ; σ s = 80 Ω -1 cm -1 n h = 10 16 cm -3 , μ = 50 cm /V·s, σ = e μ n h = 0.6 Ω -1 cm -1 ; σ s = 7 Ω -1 cm -1

  5. (2) In a 2-D electron gas in n-type semiconductor heterostructures [PRL 92, 126603] Rashba Hamiltonian Universal spin Hall conductivity

  6. 2. Spin Hall effect observed in semiconductors (a) in n-type 3D GaAs and InGaAs thin films [Kato et al. , Science 306, 1910 (2004)] Attributed to extrinsic SHE because of weak crystal direction dependence.

  7. (b) in p-type 2D semiconductor quantum wells [PRL 94 (2005) 047204] Attributed to intrinsic SHE.

  8. (c) Spin Hall effect in strained n -type nitride semiconductors [Chang, Chen, Chen, Hong, Tsai, Chen, Guo, PRL 98, 136403; 98, 239902 (E) (2007)] wurtzite n -type (5nm In x Ga 1-x N/3nm GaN) superlattice (x=0.15)

  9. 3. Large room-temperature spin Hall effect in metals Nature 13 July 2006 Vol. 442, P. 176 (direct) spin Hall effect fcc Al σ sH = 27~34 ( Ω cm) -1 ( T = 4.2 K) inverse spin Hall effect

  10. [Saitoh, et al., APL 88 (2006) 182509] [PRL98, 156601; 98, 139901 (E) (2007)] σ sH = 240 ( Ω cm) -1 ( T = 290 K) Assumed to be extrinsic!

  11. [Hoffmann, IEEE Trans. Magn. 49 (2013) 5172]

  12. 4. Spintronics, magneto-devices and spin Hall effect 1) Spintronics (spin electronics) Three basic elements: Generation, detection, & manipulation of spin current. Ferromagnetic leads Usual spin current generations: Problems: magnets and/or magnetic fields needed, and difficult to integrate with semiconductor technologies. (a) non-magnetic metals, (b) ferromagnetic metals and (c) half-metallic metals. (1) Direct spin Hall effect would allow us to generate pure spin current electrically in nonmagnetic microstructures without applied magnetic fields or magnetic materials, and make possible pure electric driven spintronics which could be readily integated with conventional electronics. (2) Inverse spin Hall effect would enable us to detect spin current electrically, again without applied magnetic fields or magnetic materials.

  13. 2) Magneto-electric devices Spin-torque switching with the giant spin Hall effect of tantalum [Liu et al., Science 336, 555 (2012)]

  14. 5. Spin-off’s: Topological insulators and spin caloritronics Quantum Hall effect in conventional 2DEG [Laughlin, PRB23, 5632 (1981)] 2 2 e σ = ± ν , ν = Chern (TKNN) number xy h Quantum Hall states are insulating with 1  broken time-reversal symmetry. n ν = dk dk Ω ( ) k x x xy 2 π BZ Topological invariant is Chern number. n [Thouless et al., PRL49, 405 (1982)]

  15. 2D Topological insulators from quest for quantum spin Hall effect [Kane & Mele, PRL 95 (2005) 146801] Kane-Mele SOC Hamiltonian for graphene   † † = + λ H t c c i c s v c KM i j i z ij j < i j , > << >> ij y x E f e A B s σ = ν , σ = 0. xy xy π 2 SOC no SOC SOC is too small (<0.01 meV) to make QSHE observable! [Chen, Xiao, Chiou, Guo, PRB 84, 165453 (2011)]

  16. Evidence for quantum spin Hall effect in Quantum spin Hall effect in topological quantum wells [Koenig et al., Science phase in HgTe quantum well 318, 766 (2007)] [Bernevig, Hughes, Zhang, Science 314, 1757 (2006)] [Du et al., arXiv.1306.1925]

  17. Host a number of exotic phenemona, e.g., majorana 3D Topological insulators fermion superconductivity, axion electrodynamics [Fu, Kane, Mele, PRL98, 106803(the.)] and quantum anomalous Hall effect Bi 2 Te 3 observed in Cr 0.15 (Bi 0.1 Sb 0.9 ) 1.85 Te 3 film [Hsieh et al., Nature 460 (2009) 1101; Chang et al. Science 340, Xia et al., NP 5 (2009) 398] 167 (2013)]

  18. 2. Spin caloritronics [Bauer, Saitoh, van Wees, Nature Mater. 11 (2012) 391] Spin Nernst effect Spin Hall Effect Spin Nernst Effect [Cheng et al., PRB 2008] Spin current spin current Spin-orbit interaction dV r ( ) ( s L ⋅ ) dr

  19. Spin Seebeck effect [Uchida et al., Nature 455 (2008) 778] Thus, we could have thermally driven spintronic devices, i.e., spin caloritronics.

  20. II. Ab initio studies of intrinsic spin Hall effect in solids 1. Motivations 1) Will the intrinsic spin Hall effect exactly cancelled by the intrinsic orbital-angular-momentum Hall effect? [S. Zhang and Z. Yang, cond-mat/0407704; PRL 2005] In conclusion, we have shown that the ISHE is accompanied by the intrinsic orbital- angular-momentum Hall effect so that the total angular momenttum spin current is zero in a SOC system. For Rashba Hamiltonian, This is confirmed for Rashba system by us. However, in Dresselhaus and Rashba systems, spin Hall conductivity would not be cancelled by the orbital Hall conductivity. [Chen, Huang, Guo, PRB73 (2006) 235309]

  21. 2) To go beyond the spherical 4-band Luttinger Hamiltonian. 3) To understand the effects of epitaxial strains.

  22. 4) To understand the detailed mechanism of the SHE in metals because it would lead to the material design of the large SHE even at room temperature with the application to the spintronics. To this end, ab initio band theoretical calculations for real metal systems is essential.

  23. 2. Berry phase formalism for intrinsic Hall effects 1) Berry phase [Berry, Proc. Roy. Soc. London A 392, 451 (1984)] ε n Parameter dependent system: { ( ) ( ) } ε λ ψ λ , n n Adiabatic theorem: −  t λ i dt ε /  ( ) ( ( ) ) ( ) − γ i t n Ψ t = ψ λ t e e 0 n n λ λ t 2 Geometric phase: ∂ λ λ  t γ = λ ψ ψ d i 0 n n n ∂ λ λ 0 λ 1

  24. Well defined for a closed path ∂  γ = λ ψ ψ d i λ n n n ∂ λ 2 C Stokes theorem C =  γ λ 1 λ Ω d d λ n 2 1 Berry Curvature ∂ ∂ ∂ ∂ Ω = i ψ ψ − i ψ ψ ∂ λ ∂ λ ∂ λ ∂ λ 1 2 2 1

  25. Analogies Berry curvature Magnetic field  B  ( r ) Ω ( λ ) Berry connection Vector potential ∂ A  ( r ) ψ ψ i ∂ λ Aharonov-Bohm phase Geometric phase     ∂  2 = dr A ( r ) d r B ( r )   2 d λ ψ i ψ = d λ Ω ( ) λ ∂ λ Dirac monopole Chern number     2 2 λ Ω = = d ( ) integer d r B ( ) integer h / e λ r

  26. 2) Semiclassical dynamics of Bloch electrons Old version [e.g., Aschroft, Mermin, 1976] ∂ ε ( k ) 1  x = n , c ∂  k ∂ ϕ e e e ( r ) e    = − − × = − × k E x B x B . c c    ∂ r  New version [Marder, 2000] Berry phase correction [Chang & Niu, PRL (1995), PRB (1996)] 1 ∂ ε ( k )   = − × x n k Ω ( k ), c n  ∂ k ∂ ϕ e ( r ) e   k = − x × B , c  ∂ r  ∂ u ∂ u (Berry curvature) = − × Ω ( k ) Im n k | | n k . n ∂ ∂ k k

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