Advances in Condensed Matter Physics

Volume 2008, Article ID 152731, 5 pages

http://dx.doi.org/10.1155/2008/152731

## Spin Accumulation in a Quantum Wire with Rashba Spin-Orbit Coupling

^{1}Department of Physics, Hunan Normal University, Changsha, Hunan 410081, China^{2}Department of Electronics and Physics, Hunan College of Science and Engineering, Yongzhou, Hunan 425100, China

Received 22 September 2008; Revised 9 December 2008; Accepted 17 December 2008

Academic Editor: Yuri Galperin

Copyright © 2008 Xi Fu et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

#### Abstract

We investigate theoretically the spin accumulation in a Rashba spin-orbit coupling quantum wire. Using the scattering matrix approach within the effective free-electron approximation, we have demonstrated the three components of spin polarization. It is found that by a few numerical examples, the two peaks for the out-of-plane spin accumulation shift to the edges of quantum wire with the increase of propagation modes. The period of intrinsic oscillations inversely proportions to the Rashba SOC strength. This effect may be used to differentiate the intrinsic spin accumulation from the extrinsic one.

Spintronics is a rapidly developing field of research in recent years because spin-based devices are believed to be the new generation of electronic devices [1–3]. Among the research area of spintronics, the spin-orbit coupling (SOC) creates another way to manipulate spins by means of an electric field [3], which has great potential applications in the future. The Rashba spin-orbit coupling (RSOC) effect is found to be very pronounced in some semiconductor layer (e.g., InAs or InGaAs) and its strength can be controlled by gate voltage [4].

The spin polarization in two-dimensional electron gas (2DEG) systems with SOC has been attracting much attention [5–9]. Recently, the experimental observations [10, 11] of spin Hall effect (SHE) in 2DEG with SOC have given evidence of the possibility to control electron spins by an electric field. Wang and Sheng [12] have investigated the current induced local spin polarization due to weak RSOC in a narrow strip. Furthermore, Nikolić et al. [13] have demonstrated that the flow of a longitudinal unpolarized current through a ballistic 2DEG with RSOC will induce a nonequilibrium spin accumulation along the lateral edges. More recently, the out-of-plane spin Hall accumulation effect has been observed in a Rashba bar [14]. Using the nonequilibrium Green's function approach, Wang et al. [15] have studied the intrinsic oscillation of spin accumulation induced by RSOC in a quantum wire (QW) system. However, the work in [12, 14, 15] has only considered the hard-wall potential confined Rashba QWs.

In this paper, using the scattering matrix method within the effective free-electron approximation, we study theoretically the spin accumulation in a parabolic potential confined Rashba QW connected to two normal leads (without SOC) nonadiabatically, and the results are discussed and compared with the previous works [12–15]. The system under consideration is a wide-narrow-wide (WNW) geometry of structure, and the number of propagation modes in the narrow QW and wide leads is controlled by the different strength of parabolic confining potentials. The transverse direction corresponds to -axis and the longitudinal direction to -axis. Therefore, the effective mass single-electron Hamiltonian in the QW is whereis the uncoupled QW Hamiltonian while the RSOC Hamiltonian [14, 15] readsIn the above Hamiltonians, is the lateral confining potential with , and the effective electron mass and oscillator frequency, while denotes the Rashba strength, and the component of pauli matrix.

Since the Hamiltonian in the leads has no RSOC term, we assume that an unpolarized electron wave is injected from the left lead into the QW. Due to the translation invariance in the longitudinal -direction, the electron wave function in the leads can be decomposed into two components of a plane wave and a transversally confined wave function for the th mode where represents spin-up (-down) state, , and is the Hermite polynomial. Since no RSOC in the leads, the total electron energy for spin-up or -down electron is same, , where the lateral sublevel and the longitudinal wavevector .

The wave function for the weak Rashba QW is a two-components spinor and can be also decomposed into two components for spin-up and spin-down electron, respectively. The corresponding transverse ( direction) wave functions in the perturbation regime [16] can be solved aswhere and the character length related to the oscillator frequency, and the sign “" corresponding to “" state. The electron energy in the QW is , where the lateral sublevel of the th mode is and , respectively. Therefore, the longitudinal wavevectors can be expressed asfor spin-up and -down electron, respectively.

In order to calculate the scattering matrix separately for spin-up and -down electron, one needs to match the wave functions at the two interfaces of wire-lead connection. For a symmetric system, one can only calculate the scattering matrix for one interface. The total scattering matrix for the system can be obtained by the symmetry property of the system [17]. Here, we first consider the left interface at as if without the right interface for electron incident from left to right. Because of the degeneracy, in the left lead , the wave functions for spin-up and -down electron can be written aswhere are the coefficients of incident mode reflecting to mode . In the QW , the wave functions for spin-up and -down electron are nondegeneratewhere are given in (5) and the coefficients of incident mode , transmitting to mode . The continuity of the wave functions at left interface gives The continuity of the derivative of the wave functions may not hold due to the existence of RSOC [16]. However, the current conservation for the system still holds [18, 19]:hence we can obtainwhere is the effective width of the QW. Multiplying and with (9) and (11), respectively, and integrating over the range of , one obtains the matrices of reflection and transmission at the interface aswithwhere the corresponding matrices elements are as follows , , , , and , respectively. Furthermore, an analogous calculation for an incident wave from the right side to the left one at interface gives matrices and . Thus, the scattering matrix at interface can be expressed as where the normalized wave amplitudes , , , and . Due to the symmetry of the system, [17] the scattering matrix at interface isTherefore, we can obtain the total wave functions in the QW asand the local spin polarization [12, 14]

In the following, we present some numerical examples of the calculated spin polarization (in units of ) in the QW at low temperatures. It should be pointed out that we only consider the weak RSOC case [16–19], that is, with , and the width of two leads supporting number of propagating modes up to . For the case of eVm [7], the incident electron energy is taken as eV (for eVm, eV). Our system is a WNW QW (); however, the actual width of QW is chosen as and the parabolic confining potential controls the number of propagation modes in the QW with the corresponding character oscillator frequency length . The electron effective mass is taken as that for InGaAs quantum well [8] and the length of QW is chosen as nm.

Figure 1 shows the 2D contour of spin polarization components for the cases of three and five propagation modes in the QW. It is noted that the components and present periodic oscillations along the longitudinal direction which comes from Rashba spin precession [15] while no oscillations presented for . This is the main difference from the results of [14] due to the different confining potential.

The polarization components versus the transverse position for different propagation modes in the QW are demonstrated in Figure 2, with the longitudinal positions for and as 0 and , respectively. More peaks and extended polarization width toward two edges of the QW have been shown with the increasing modes The component presents two inverse-direction peaks (shifting to the two edges of the QW), consequently, produces the out-of-plane spin accumulation in the QW. The spin accumulation is formed with the spin distribution polarized along the direction due to the interaction between the pseudomagnetic field arising from RSOC and the accelerating electrons [20, 21]. Moreover, the net spin polarization rather than in-plane spin accumulation is illustrated for while the present results of are qualitatively consistent with [12, 14].

Furthermore, in Figure 3 we plot the longitudinal profile of spin polarization components and at a fixed transverse position . As can be seen, due to the Rashba spin precession along the longitudinal position of QW, the period of the oscillations (with phase separation) for Rashba strength eVm is half that of the eVm case. One notes that the Rashba precession lengths and are 600 nm and 300 nm, respectively, which are consistent with the results in [14, 22]. It should be pointed out that the presented results may be observable experimentally to differentiate the intrinsic and extrinsic spin accumulation.

In conclusion, we have studied the spin polarization in a Rashba QW confined by a parabolic potential. It is found that the two inverse direction peaks of the out-of-plane spin accumulation shift to the two edges of the QW with the increasing propagation modes. Furthermore, the intrinsic oscillation of spin polarization due to Rashba spin precession can be used to identify the intrinsic spin accumulation by changing the RSOC strength.

#### Acknowledgments

This work is supported by the Nature Science Foundation of China under Grant no. 10574042, the Specialized Research Fund for the Doctoral Program of Higher Education of China under Grant no. 20060542002, and the Hunan Provincial Natural Science Foundation of China under Grant no. 06JJ2097.

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