2012
DOI: 10.1103/physrevb.86.174301
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Unified theory of spin dynamics in a two-dimensional electron gas with arbitrary spin-orbit coupling strength at finite temperature

Abstract: We study the spin dynamics in the presence of impurity and electron-electron (e-e) scattering in a III-V semiconductor quantum well with arbitrary spin-orbit coupling (SOC) strength and symmetry at finite temperature. We derive the coupled spin-charge dynamic equations in the presence of inelastic scattering and provide a new formalism that describes the spin relaxation and dynamics in both the weak and the strong SOC regime in a unified way. In the weak SOC regime, as expected, our theory reproduces all previ… Show more

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Cited by 31 publications
(56 citation statements)
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“…Therefore, we obtain coupled spin and charge transport equations for SSs of a TI as well as a Rashba 2DEG. For ease of analysis, we begin with the Rashba 2DEG, which is then modified for the TI SSs.Within the parabolic band approximation, the Hamiltonian for the Rashba 2DEG (setting = 1) is [22,27]:Here m is the effective mass, k is the in-plane momentum, σ 0 is the identity matrix, σ = (σ xx + σ yŷ + σ zẑ ) where σ's are the Pauli spin matrices (we have used boldface for matrices in the spin space) and λ is the strength of spin splitting. The spin-charge dynamic equation obtained from quantum kinetic theory can be written in terms of density matrix ρ = ρ 0 σ 0 + ρ · σ (where ρ = ρ xx + ρ yŷ + ρ zẑ ) as ρ r = D rs ρ s (r, s = 0, x, y, z), where D is the diffusion matrix [22,23].…”
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confidence: 99%
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“…Therefore, we obtain coupled spin and charge transport equations for SSs of a TI as well as a Rashba 2DEG. For ease of analysis, we begin with the Rashba 2DEG, which is then modified for the TI SSs.Within the parabolic band approximation, the Hamiltonian for the Rashba 2DEG (setting = 1) is [22,27]:Here m is the effective mass, k is the in-plane momentum, σ 0 is the identity matrix, σ = (σ xx + σ yŷ + σ zẑ ) where σ's are the Pauli spin matrices (we have used boldface for matrices in the spin space) and λ is the strength of spin splitting. The spin-charge dynamic equation obtained from quantum kinetic theory can be written in terms of density matrix ρ = ρ 0 σ 0 + ρ · σ (where ρ = ρ xx + ρ yŷ + ρ zẑ ) as ρ r = D rs ρ s (r, s = 0, x, y, z), where D is the diffusion matrix [22,23].…”
mentioning
confidence: 99%
“…Previously, the voltage drop measured between a FM and a nonmagnetic (NM) contact placed on the surface of a TI was theoretically calculated either using non-equilibrium Green's function [20] or by solving the transport equations derived from Kubo formalism [21]. Here, we provide a different approach for the derivation of the coupled spin-charge transport differential equation based on quantum kinetic theory [22,23] in the diffusive limit. The experimentally measured spin signal matches well with the theory providing evidence for the spin polarized SS in our TI Bi 2 Te 3 thin film.…”
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“…(22) and (24), the charge distribution enters the spin sector, from which we determine f y and hence the spin polarization linear in E x and ∇ x T according to Eq. (25). In the last step, integrating the y spin component of Eq.…”
Section: A the "Dirty" Limit (2-d)mentioning
confidence: 99%
“…Moreover, we wish to identify the possible connections between the four phenomena. It is known, for example, that in a 2DEG at low T , the spin Hall and Edelstein effects may be related [22][23][24][25], and that such a relation can be extended to thin (quasi-2D) films as well [26]. Whether a connection exists, possibly in a modified form, also at high T or in 3D is an open question.…”
Section: Introductionmentioning
confidence: 99%