Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Rashba effect

From Wikipedia, the free encyclopedia
Momentum-dependent divisionof spin bands in two-dimensional condensed matter systems
Not to be confused with theRashba–Edelstein effect, which describes the conversion of a bidimensional charge current into a spin accumulation.

TheRashba effect, also calledBychkov–Rashba effect, is a momentum-dependent splitting ofspin bands in bulkcrystals[note 1] and low-dimensionalcondensed matter systems (such asheterostructures andsurface states) similar to the splitting ofparticles andanti-particles in theDirac Hamiltonian. The splitting is a combined effect ofspin–orbit interaction and asymmetry of the crystal potential, in particular in the direction perpendicular to the two-dimensional plane (as applied to surfaces and heterostructures). This effect is named in honour ofEmmanuel Rashba, who discovered it with Valentin I. Sheka in 1959[1] for three-dimensional systems and afterward with Yurii A. Bychkov in 1984 for two-dimensional systems.[2][3][4]

Remarkably, this effect can drive a wide variety of novel physical phenomena, especially operating electron spins by electric fields, even when it is a small correction to the band structure of the two-dimensional metallic state. An example of a physical phenomenon that can be explained by Rashba model is the anisotropicmagnetoresistance (AMR).[note 2][5][6][7]

Additionally, superconductors with large Rashba splitting are suggested as possible realizations of the elusiveFulde–Ferrell–Larkin–Ovchinnikov (FFLO) state,[8]Majorana fermions andtopological p-wave superconductors.[9][10]

Lately, a momentum dependent pseudospin-orbit coupling has been realized in cold atom systems.[11]

Hamiltonian

[edit]

The Rashba effect is most easily seen in the simple model Hamiltonian known as the Rashba Hamiltonian

HR=α(z^×p)σ{\displaystyle H_{\rm {R}}=\alpha ({\hat {z}}\times \mathbf {p} )\cdot {\boldsymbol {\sigma }}},

whereα{\displaystyle \alpha } is the Rashba coupling,p{\displaystyle \mathbf {p} } is themomentum andσ{\displaystyle {\boldsymbol {\sigma }}} is thePauli matrix vector.This is nothing but a two-dimensional version of the Dirac Hamiltonian (with a 90 degree rotation of the spins).

The Rashba model in solids can be derived in the framework of thek·p perturbation theory[12] or from the point of view of atight binding approximation.[13] However, the specifics of these methods are considered tedious and many prefer an intuitive toy model that gives qualitatively the same physics (quantitatively it gives a poor estimation of the couplingα{\textstyle \alpha }). Here we will introduce the intuitivetoy model approach followed by a sketch of a more accurate derivation.

Naive derivation

[edit]

The Rashba effect arises from the breaking of inversion symmetry in the direction perpendicular to a two-dimensional electron system. To illustrate this qualitatively, consider adding to the Hamiltonian an electric-field term that breaks this symmetry:

HE=eE0z{\displaystyle H_{\mathrm {E} }=-eE_{0}z}

Due to relativistic corrections, an electron moving with velocityv{\displaystyle \mathbf {v} } in an electric fieldE{\displaystyle \mathbf {E} } experiences an effective magnetic field in its rest frame, given by

B=v×Ec2{\displaystyle \mathbf {B} =-{\frac {\mathbf {v} \times \mathbf {E} }{c^{2}}}}

wherec{\displaystyle c} is the speed of light. This magnetic field couples to the electron spin through the spin–orbit interaction:

HSO=gμB2c2(v×E)σ{\displaystyle H_{\mathrm {SO} }={\frac {g\mu _{\mathrm {B} }}{2c^{2}}}(\mathbf {v} \times \mathbf {E} )\cdot {\boldsymbol {\sigma }}}

whereσ{\displaystyle {\boldsymbol {\sigma }}} are the Pauli matrices andgμBσ/2{\displaystyle -g\mu _{\mathrm {B} }{\boldsymbol {\sigma }}/2} represents the electron magnetic moment.

Within this simplified “toy” model, the resulting Rashba Hamiltonian can be written as

HR=αR(z^×p)σ{\displaystyle H_{\mathrm {R} }=-\alpha _{\mathrm {R} }({\hat {z}}\times \mathbf {p} )\cdot {\boldsymbol {\sigma }}}

with a coupling strength

αR=gμBE02mc2.{\displaystyle \alpha _{\mathrm {R} }=-{\frac {g\mu _{\mathrm {B} }E_{0}}{2mc^{2}}}.}

This expression provides the correct functional form of the Rashba Hamiltonian but severely underestimates the coupling strengthαR{\displaystyle \alpha _{\mathrm {R} }}. A more realistic description shows that the effect originates from interband coupling (band mixing) in the crystal. The “toy” model above uses the Dirac energy gapmc2{\displaystyle mc^{2}}—on the order of MeV—as the denominator in the relativistic correction, which leads to an unrealistically small coupling. In actual materials, the relevant energy scales are the splittings between electronic bands, typically of order eV. This difference accounts for the much larger Rashba coupling observed experimentally.[14]

Before continuing we make a comment about a common misconception regarding the Rashba effect. According to theEhrenfest theorem, the average electric field experienced by an electron bound to a two-dimensional layer should vanish, because the expectation value of the force on a bound particle is zero. Applied naively, this reasoning seems to imply that the Rashba effect should not occur—an argument that led to early controversy prior to experimental confirmation. However, this interpretation is incomplete: the Rashba effect depends not on the *spatially averaged* electric field, but on the *local asymmetry* of the confining potential, which gives rise to an effective field acting on the electron spin.

Estimation of the Rashba coupling in a realistic system – tight-binding approach

[edit]

A microscopic estimate of the Rashba coupling constantα{\displaystyle \alpha } can be obtained using a tight-binding model. In many semiconductors, the itinerant carriers forming the two-dimensional electron gas (2DEG) originate from atomics andp orbitals. For simplicity, consider holes in thepz{\displaystyle p_{z}} band near theΓ{\displaystyle \Gamma } point.[15]

Two ingredients are essential to obtain Rashba splitting:an atomic spin–orbit interaction

HSO=ΔSOLσ,{\displaystyle H_{\mathrm {SO} }=\Delta _{\mathrm {SO} }\,\mathbf {L} \cdot {\boldsymbol {\sigma }},}

and an asymmetric potential in the direction perpendicular to the 2D plane,

HE=eE0z.{\displaystyle H_{E}=eE_{0}z.}

The symmetry-breaking potentialHE{\displaystyle H_{E}} lifts the degeneracy between the out-of-planepz{\displaystyle p_{z}} orbital and the in-planepx{\displaystyle p_{x}} andpy{\displaystyle p_{y}} orbitals, opening a gapΔBG{\displaystyle \Delta _{\mathrm {BG} }}. At the same time, it allows mixing (hybridization) between these orbitals, which can be described within a tight-binding approximation. The hopping amplitude from apz{\displaystyle p_{z}} state at sitei{\displaystyle i} with spinσ{\displaystyle \sigma } to a neighboringpx,y{\displaystyle p_{x,y}} state at sitej{\displaystyle j} with spinσ{\displaystyle \sigma '} is

tij;σσx,y=pz,i;σ|H|px,y,j;σ,{\displaystyle t_{ij;\sigma \sigma '}^{x,y}=\langle p_{z},i;\sigma \,|\,H\,|\,p_{x,y},j;\sigma '\rangle ,}

whereH{\displaystyle H} is the full Hamiltonian. In the absence of inversion asymmetry (HE=0{\displaystyle H_{E}=0}), this hopping vanishes by symmetry. WhenHE0{\displaystyle H_{E}\neq 0}, the matrix element becomes finite; for nearest neighbors one can write approximately

tσσx,y=E0pz,i;σ|z|px,y,i+x^,y^;σ=t0sgn(x^,y^)δσσ,{\displaystyle t_{\sigma \sigma '}^{x,y}=E_{0}\langle p_{z},i;\sigma \,|\,z\,|\,p_{x,y},i+{\hat {x}},{\hat {y}};\sigma '\rangle =t_{0}\,\mathrm {sgn} ({\hat {x}},{\hat {y}})\,\delta _{\sigma \sigma '},}

whereδσσ{\displaystyle \delta _{\sigma \sigma '}} is theKronecker delta.

The Rashba interaction can then be viewed as a second-order process: a hole hops from|pz,i;{\displaystyle |p_{z},i;\uparrow \rangle } to|px,y,i+x^,y^;{\displaystyle |p_{x,y},i+{\hat {x}},{\hat {y}};\uparrow \rangle } viat0{\displaystyle t_{0}}, then undergoes a spin flip through the atomic spin–orbit couplingΔSO{\displaystyle \Delta _{\mathrm {SO} }}, returning to|pz,i+x^,y^;{\displaystyle |p_{z},i+{\hat {x}},{\hat {y}};\downarrow \rangle }. Overall, the carrier hops one lattice spacing while flipping its spin.

Treating this sequence as a second-order perturbation, the resulting Rashba coupling constant scales as

αat0ΔSOΔBG,{\displaystyle \alpha \approx {\frac {a\,t_{0}\,\Delta _{\mathrm {SO} }}{\Delta _{\mathrm {BG} }}},}

wherea{\displaystyle a} is the lattice spacing. Because the relevant energy denominators are of order eV rather than MeV (as in the naive relativistic model), this estimate yields a Rashba coupling several orders of magnitude larger, in agreement with experimental observations.

Application

[edit]

Spintronics - Electronic devices are based on the ability to manipulate the electrons position by means of electric fields. Similarly, devices can be based on the manipulation of the spin degree of freedom. The Rashba effect allows to manipulate the spin by the same means, that is, without the aid of a magnetic field. Such devices have many advantages over their electronic counterparts.[16][17]

Topological quantum computation - Lately it has been suggested that the Rashba effect can be used to realize a p-wave superconductor.[9][10] Such a superconductor has very specialedge-states which are known asMajorana bound states. The non-locality immunizes them to local scattering and hence they are predicted to have longcoherence times. Decoherence is one of the largest barriers on the way to realize a full scalequantum computer and these immune states are therefore considered good candidates for aquantum bit.

Discovery of thegiant Rashba effect withα{\displaystyle \alpha } of about 5 eV•Å in bulk crystals such as BiTeI,[18] ferroelectric GeTe,[19] and in a number of low-dimensional systems bears a promise of creating devices operating electrons spins at nanoscale and possessing short operational times.

Comparison with Dresselhaus spin–orbit coupling

[edit]
Main article:Dresselhaus effect

The Rashba spin-orbit coupling is typical for systems with uniaxial symmetry, e.g., for hexagonal crystals of CdS and CdSe for which it was originally found[20] and perovskites, and also for heterostructures where it develops as a result of a symmetry breaking field in the direction perpendicular to the 2D surface.[2] All these systems lack inversion symmetry. A similar effect, known as the Dresselhaus spin orbit coupling[21] arises in cubic crystals of AIIIBV type lacking inversion symmetry and inquantum wells manufactured from them.

See also

[edit]

Footnotes

[edit]
  1. ^More specifically, uniaxial noncentrosymmetric crystals.
  2. ^AMR in most common magnetic materials was reviewed byMcGuire & Potter 1975. A more recent work (Schliemann & Loss 2003) focused on the possibility of Rashba-effect-induced AMR and some extensions and corrections were given later (Trushin et al. 2009).

References

[edit]
  1. ^E. I. Rashba and V. I. Sheka, Fiz. Tverd. Tela – Collected Papers (Leningrad), v.II, 162-176 (1959) (in Russian), English translation: Supplemental Material to the paper by G. Bihlmayer, O. Rader, and R. Winkler, Focus on the Rashba effect, New J. Phys.17, 050202 (2015),http://iopscience.iop.org/1367-2630/17/5/050202/media/njp050202_suppdata.pdf.
  2. ^abYu. A. Bychkov and E. I. Rashba, Properties of a 2D electron gas with a lifted spectrum degeneracy, Sov. Phys. - JETP Lett.39, 78-81 (1984)
  3. ^G. Bihlmayer, O. Rader and R. Winkler, Focus on the Rashba effect, New J. Phys.17, 050202 (2015)
  4. ^Yeom, Han Woong; Grioni, Marco, eds. (May 2015)."Special issue on electron spectroscopy for Rashba spin-orbit interaction"(PDF).Journal of Electron Spectroscopy and Related Phenomena.201:1–126.doi:10.1016/j.elspec.2014.10.005.ISSN 0368-2048. Retrieved28 January 2019.
  5. ^McGuire, T.; Potter, R. (1975). "Anisotropic magnetoresistance in ferromagnetic 3d alloys".IEEE Transactions on Magnetics.11 (4):1018–1038.Bibcode:1975ITM....11.1018M.doi:10.1109/TMAG.1975.1058782.
  6. ^Schliemann, John; Loss, Daniel (2003). "Anisotropic transport in a two-dimensional electron gas in the presence of spin-orbit coupling".Physical Review B.68 (16) 165311.arXiv:cond-mat/0306528.Bibcode:2003PhRvB..68p5311S.doi:10.1103/physrevb.68.165311.S2CID 119093889.
  7. ^Trushin, Maxim; Výborný, Karel; Moraczewski, Peter; Kovalev, Alexey A.; Schliemann, John; Jungwirth, T. (2009). "Anisotropic magnetoresistance of spin-orbit coupled carriers scattered from polarized magnetic impurities".Physical Review B.80 (13) 134405.arXiv:0904.3785.Bibcode:2009PhRvB..80m4405T.doi:10.1103/PhysRevB.80.134405.S2CID 41048255.
  8. ^Agterberg, Daniel (2003). "Anisotropic magnetoresistance of spin-orbit coupled carriers scattered from polarized magnetic impurities".Physica C.387 (1–2):13–16.Bibcode:2003PhyC..387...13A.doi:10.1016/S0921-4534(03)00634-8.
  9. ^abSato, Masatoshi & Fujimoto, Satoshi (2009). "Topological phases of noncentrosymmetric superconductors: Edge states, Majorana fermions, and non-Abelian statistics".Phys. Rev. B.79 (9) 094504.arXiv:0811.3864.Bibcode:2009PhRvB..79i4504S.doi:10.1103/PhysRevB.79.094504.S2CID 119182379.
  10. ^abV. Mourik, K. Zuo1, S. M. Frolov, S. R. Plissard, E. P. A. M. Bakkers and L. P. Kouwenhoven (2012). "Signatures of Majorana Fermions in Hybrid Superconductor-Semiconductor Nanowire Devices".Science Express.1222360 (6084):1003–1007.arXiv:1204.2792.Bibcode:2012Sci...336.1003M.doi:10.1126/science.1222360.PMID 22499805.S2CID 18447180.{{cite journal}}: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)
  11. ^Lin, Y.-J.; K. Jiménez-García; I. B. Spielman (2011)."Spin-orbit-coupled Bose-Einstein condensates".Nature.471 (7336):83–86.arXiv:1103.3522.Bibcode:2011Natur.471...83L.doi:10.1038/nature09887.PMC 11493149.PMID 21368828.S2CID 4329549.
  12. ^Winkler, Ronald.Spin-orbit Coupling Effects in Two-Dimensional Electron and Hole Systems(PDF). New-York: Springer Tracts in Modern Physics.
  13. ^L. Petersena & P. Hedegård (2000). "A simple tight-binding model of spin–orbit splitting of sp-derived surface states".Surface Science.459 (1–2):49–56.Bibcode:2000SurSc.459...49P.doi:10.1016/S0039-6028(00)00441-6.
  14. ^P. Pfeffer & W. Zawadzki (1999). "Spin splitting of conduction subbands in III-V heterostructures due to inversion asymmetry".Physical Review B.59 (8):R5312–R5315.Bibcode:1999PhRvB..59.5312P.doi:10.1103/PhysRevB.59.R5312.
  15. ^Typically in semiconductors the Rashba splitting is discussed for thes-like conduction band around theΓ6{\displaystyle \Gamma _{6}} point. Here we focus on thep bands, but the same hybridization mechanism betweenp ands states underlies the Rashba splitting nearΓ6{\displaystyle \Gamma _{6}}.
  16. ^Bercioux, Dario; Lucignano, Procolo (2015-09-25). "Quantum transport in Rashba spin–orbit materials: a review".Reports on Progress in Physics.78 (10) 106001.arXiv:1502.00570.Bibcode:2015RPPh...78j6001B.doi:10.1088/0034-4885/78/10/106001.ISSN 0034-4885.PMID 26406280.S2CID 38172286.
  17. ^Rashba Effect in Spintronic Devices
  18. ^Ishizaka, K.; Bahramy, M. S.; Murakawa, H.; Sakano, M.; Shimojima, T.; et al. (2011-06-19). "Giant Rashba-type spin splitting in bulk BiTeI".Nature Materials.10 (7). Springer Science and Business Media LLC:521–526.Bibcode:2011NatMa..10..521I.doi:10.1038/nmat3051.ISSN 1476-1122.PMID 21685900.
  19. ^Di Sante, Domenico; Barone, Paolo; Bertacco, Riccardo;Picozzi, Silvia (2012-10-16). "Electric Control of the Giant Rashba Effect in Bulk GeTe".Advanced Materials.25 (4). Wiley:509–513.doi:10.1002/adma.201203199.ISSN 0935-9648.PMID 23070981.S2CID 33251068.
  20. ^E. I. Rashba and V. I. Sheka, Fiz. Tverd. Tela - Collected Papers (Leningrad), v.II, 162-176 (1959) (in Russian), English translation: Supplemental Material to the paper by G. Bihlmayer, O. Rader, and R. Winkler, Focus on the Rashba effect, New J. Phys.17, 050202 (2015).
  21. ^Dresselhaus, G. (1955-10-15). "Spin-Orbit Coupling Effects in Zinc Blende Structures".Physical Review.100 (2). American Physical Society (APS):580–586.Bibcode:1955PhRv..100..580D.doi:10.1103/physrev.100.580.ISSN 0031-899X.

Further reading

[edit]

External links

[edit]
Retrieved from "https://en.wikipedia.org/w/index.php?title=Rashba_effect&oldid=1334191129"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp