Home Search Collections Journals About Contact us My IOPscience Spin and charge pumping in a quantum wire: the role of spin-flip scattering and Zeeman splitting This article has been downloaded from IOPscience. Please scroll down to see the full text article. 2011 J. Phys.: Condens. Matter 23 405301 (http://iopscience.iop.org/0953-8984/23/40/405301) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 212.182.1.153 The article was downloaded on 14/11/2012 at 07:34 Please note that terms and conditions apply. IOP PUBLISHING JOURNAL OF PHYSICS: CONDENSED MATTER J. Phys.: Condens. Matter 23 (2011) 405301 (11pp) doi:10.1088/0953-8984/23/40/405301 Spin and charge pumping in a quantum wire: the role of spin-flip scattering and Zeeman splitting T Kwapiński and R Taranko Institute of Physics, M Curie-Skłodowska University, PL-20-031 Lublin, Poland E-mail: tomasz.kwapinski@umcs.lublin.pl Received 3 June 2011, in final form 17 August 2011 Published 19 September 2011 Online at stacks.iop.org/JPhysCM/23/405301 Abstract We investigate theoretically charge and spin pumps based on a linear configuration of quantum dots (quantum wire) which are disturbed by an external time-dependent perturbation. This perturbation forms an impulse which moves as a train pulse through the wire. It is found that the charge pumped through the system depends non-monotonically on the wire length, N. In the presence of the Zeeman splitting pure spin current flowing through the wire can be generated in the absence of charge current. Moreover, we observe electron pumping in a direction which does not coincide with the propagation direction of the pulse and the spin pumping direction (spin–charge separation). Additionally, on-site spin-flip processes significantly influence electron transport through the system and can also reverse the charge current direction. 1. Introduction the ac signal. The easiest way to break the time-reversal symmetry is to add the second harmonic to the driving periodic field or use time-dependent dipole forces, [17]. The functional principle of spin pumps is closely related to charge pumps. However, a charge–spin system often reveals a fascinating phenomenon, i.e. it can generate pure spin current in the absence of charge (electron) current. Such spin pumps were studied, for example, for a two-dimensional electron gas [18], a single molecule (quantum dot, QD) [6, 19, 20] or a double QD system [11, 21]. In the last case in the presence of ac-driven perturbations the system behaves as a spin filter. Pumping effects in one-dimensional systems were reported for an oscillating potential [22, 23] or time-periodic (harmonic, bi-harmonic, pulsed) delta-like potentials applied to two sites of a wire [10, 24, 25]. Such time-dependent two-site perturbations act as electron pumping sources in these systems. It was found that the pumped charge depends monotonically (increases) with the wire length or shows a step-like behaviour, [23]. Also by applying two slowly varying orthogonal gate electric fields on different sections of the wire one can generate spin pumping, [26]. Moreover, time-dependent magnetic fields acting on two quantum wire sites can also produce the spin current [27]. Charge–spin pumps have attracted a great deal of attention from scientists and engineers due to their significant advantages and potential applications in spintronics and quantum computing. Subtle experimental techniques were applied to investigate new phenomena like conductance oscillations [1], conductance quantization [2], spin–charge separation [3] and others. Many interesting effects were found in low-dimensional systems driven by external timedependent fields like photon-assisted tunnelling (PAT) [4, 5] or quantum pumps [6–11]. A charge or spin pump is an electronic device which generates a net current flowing between unbiased leads. A quantum pump involves periodic changes of two or more device-control parameters [12, 13], which break the spatial symmetry of the system. Such electron pumps were realized experimentally, e.g. [8, 14]. Recently it was shown, both theoretically and experimentally, that an electron pump can exist also for a single time-dependent parameter (monoparametric pumping), [15, 16]. Generally a pump current can be generated by an external time-dependent signal (i) due to the absence of spatial symmetry in the system or (ii) in the case of a lack of time-reversal symmetry in 0953-8984/11/405301+11$33.00 1 c 2011 IOP Publishing Ltd Printed in the UK & the USA J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko In our studies for a row of coupled QDs (or atomic sites which form a quantum wire, QW) the source of pumping is the time-dependent potential applied to the gate electrodes forming the tunnel barriers between QDs. This potential influences the couplings in the wire (hopping integrals). The couplings vary non-homogeneously in time and form an impulse/perturbation which moves between leads, along the wire (train impulse). Because no source–drain voltage is applied to the left and right electrodes the system behaves as a charge pump or, in the presence of magnetic fields, as a spin or spin–charge pump. The system considered here reveals new physical possibilities for spin and charge pumping which are often quite different in comparison with two-site pumping sources in a wire (studied, for example, in [10, 24, 25]). Our goal is to investigate the role of the Zeeman splitting and the intradot spin-flip scattering on charge and spin pumping through a QW in the presence of a train impulse. These studies allow us to answer the following intriguing questions. Is it possible to observe the spin–charge separation effect with no Coulomb interactions in the wire? Then, next, do the pumping currents (charge and spin) change monotonically as a function of the wire length or do they oscillate? Especially interesting for us are spin pumps in the presence of both the Zeeman splitting and spin-flip scattering. It is known that coupling of a small quantum system (like a QD or QW) to its surrounding environment is usually responsible for spin decoherence or spin dissipation and can lead to spin-flip processes. A possible mechanism of spin relaxation in QDs is based on coupling of nuclear spins to those of QD electrons where the rate of spin relaxation depends inversely on the number of nuclei in the dot [28]. Other possibilities for spin-flip scattering are spin–orbit coupling, phonon interaction or magnetic impurity. Spin-flip transitions give rise to additional steps in the electric current through a quantum system which leads to additional peaks in the conductance [29–31]. Moreover, for magnetic tunnel junctions the spin-flip processes suppress the tunnel magnetoresistance [32, 33], but in general the spin-polarized current depends on the magnetic configuration of both leads [34]. Also the conductance of an interacting QD in the presence of spin-flip tunnelling is suppressed [35]. For a magnetic QD with time-dependent pulsed bias voltage and attached to normal and ferromagnetic leads the spin-flip scattering influences the amplitude of the quantum beats in the total charge and spin currents, [36]—both currents are suppressed in that case. In our calculations we use a tight-binding Hamiltonian and the evolution operator method. This method, which can be applied for arbitrary time dependence of external perturbations (and does not require the Floquet theory), was successfully used to describe time-dependent phenomena like scattering of atoms at the surface or photon-assisted tunnelling in QD systems [37, 38]. A possible experimental realization of the considered system is based on oscillating molecules or QDs in a harmonic potential, like in a quantum shuttle [39–41]. The moving QD affects its nearest-neighbour hoppings in time and drastically influences the electron transport through the system. Alternatively, one can use coherently coupled QDs, e.g. [5, 9], with additional external Figure 1. Schematic view of a wire consisting of N sites and coupled with the left (L) and right (R) electron reservoirs. fi (t) functions stand for the time-dependent hybridization matrix elements between sites. (This figure is in colour only in the electronic version) electrodes between them. Using these electrodes one can arbitrary change in time all hopping integrals between dots. It is also possible to use mechanical vibrations or acoustic waves [42], which can influence nearest-neighbour hoppings in a wire. The organization of this paper is as follows. The model Hamiltonian of a wire and theoretical calculations are presented in section 2. Electron pumping effects through a single QD and a QW are analysed in section 3. In section 4 spin pumps are studied in the presence of the Zeeman splitting and in section 5 the role of the spin-flip scattering is discussed. Section 6 is devoted to conclusions. 2. Model and theoretical description Our model consists of a monatomic QW or coupled QDs connected with the left electrode (via the first wire site) and the right one (via the last wire site), figure 1. The hopping integrals between the first/last wire site and the left/right electrode as well as inside the wire can be changed in time. We assume that the wire remains straight during this process and the next-neighbour couplings are neglected. The time-dependent Hamiltonian written in the second quantization notation is H = H0 + V(t), where H0 = X + + εkασ E E aE akασ kασ E kα,σ V(t) = X kLσ N−1 XX i=1 i=1 σ + VkL E (t)aE a1σ + E kL,σ + N X X σ X εiσ a+ iσ aiσ , + VkR E (t)aE aNσ kRσ E kR,σ Vi (t)a+ iσ ai+1σ + (1) N X X i=1 σ Vsf a+ iσ ai−σ + h.c., (2) + + and α = L, R, operators akασ E (akασ E ), aiσ (aiσ ) are the electron annihilation (creation) operators in the α electrode or at the ith wire site, respectively. Vsf stands for the spin-flip scattering strength (the same for all QW sites) and Vkα E (t), Vi (t) are the hybridization matrix elements (hopping integrals) between the electron states in the left/right electrode and the first/last wire site or between the nearest-neighbour sites in the wire and in general one can assume VkL/R (t) = VkL/R f1/N+1 (t), E E Vi (t) = Vi fi+1 (t), (3) i.e. fi (t) functions are responsible for the time dependence of all hopping integrals. In our calculations we neglect the electron–electron correlations as we do not consider here the 2 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko many-body effects (e.g. the Kondo effect). In the case of strong Coulomb correlation one can consider the tunnelling in the neighbourhood of a single Coulomb oscillation peak [43]. In general, the Coulomb interactions play no role when the broadening of the molecular levels due to the coupling to the leads is larger than any broadening due to the interactions within the wire, [44]. Note that one-dimensional charge and spin pumps exist also for an interacting wire (Luttinger liquid) [45, 46] and spin currents can be achieved without the presence of a magnetic field [47]. In the Hamiltonian the spin index, σ , is written explicitly and is responsible for magnetic properties of the system. An external magnetic field which is applied to the wire leads to the Zeeman splitting of the wire on-site energy levels (e.g. [11, 21, 48, 49]) and thus in general εiσ 6= εi−σ . In that case the magnetic field cancels the spin degeneracy of these levels. The strength of the Zeeman splitting is expressed by the h parameter, h = εi−σ − εiσ , and its value (in our calculations) corresponds to magnetic fields which are usually used in many experiments, [48, 49]. Moreover, we assume that both leads are unpolarized. To describe the spin and charge pumping effects through the wire in the presence of time-dependent couplings we use the evolution operator method, [37, 38]. The total charge or spin pumped through the system can be obtained from the time-dependent current flowing, e.g. from the left electrode, jLσ (t). We calculate this current from the time derivative of the total number of electrons in the left reservoir, [50]: jLσ (t) = −ednLσ (t)/dt, elements can be written: ∂ i(εE − ε0σ )t 0 (t) = VE (t)e kLσ U1σ,EqLσ 0 (t), (8) UE kL ∂t kLσ,EqLσ ∂ i Uiσ,kLσ E 0 (t) = Vi (t)Ui+1σ,kLσ E 0 (t) ∂t i(ε0σ −ε0−σ )t Ui−σ,kLσ + Vi−1 (t)Ui−1σ,kLσ E 0 (t) E 0 (t) + Vsf e X ei(ε0σ −εqELσ )t UqELσ,kLσ + δi,1 δσ,σ 0 VkL E (t) E (t) i qELσ + δi,N δσ,σ 0 VkR E (t) E kRσ E kL, 2 nkRσ E 0 (t0 )|UkLσ, E E 0 (t, t0 )| . kRσ ∂ U E 0 (t) = −iVi (t)Ui+1σ,kLσ E 0 (t) − iVi−1 (t) ∂t iσ,kLσ i(ε0σ −ε0−σ )t Ui−σ,kLσ × Ui−1σ,kLσ E 0 (t) E 0 (t) − iVsf e i(ε0σ −εkLσ E )t − δi,1 δσ,σ 0 iVkL E f1 (t)e 0L 2 R 2 + f (t)U1σ,kLσ E (t) − δi,N δσ,σ 0 0 /2fN+1 (t) 2 1 × UNσ,kLσ E (t). (4) jLσ (t) = −e0f12 (t)n1σ (t) X i(εE −ε0σ )t +2eRe nkLσ U1σ,kLσ E (0)iVkL E f1 (t)e kLσ E (t) , (5) E kL (11) Here the time evolution operator, U(t, t0 ) (in the interaction representation), satisfies the equation of motion (h̄ = 1): ∂ U(t, t0 ) = Ṽ(t) U(t, t0 ), ∂t (10) A similar equation can be written for Uiσ,kRσ E 0 (t). Note that the Vsf term mixes the set of differential equations with spin σ and spin −σ via the matrix elements Ui−σ,kLσ E 0 (t). Assuming the L same strengths of the 0 parameters, 0 = 0 R = 0, the current flowing through the system can be expressed as follows: 0 i (9) 0 and similar equations for Uiσ,kRσ E 0 (t) and UkRσ,E E qRσ (t). Note that within Pthe wide∗ band limit approximation [50], i.e. for 0 α = 2π kα E ), α = L, R, and using the E Vkα E Vkα E δ(ε − εkασ 0 solutions of the corresponding equations for Ukασ,E E qα σ (t), equation (9) takes the form: E qLσ 0 kL,E X E )t U ei(ε0σ −εkRσ E E (t), kRσ, kLσ E kRσ where the left electrode occupation, nLσ (t), can be expressed in terms of the evolution operator matrix elements, [37, 38]: X 2 0 nLσ (t) = nqELσ 0 (t0 )|UkLσ,E E qLσ (t, t0 )| + X where the charge, n1σ (t), is calculated from equation (7) and Uiσ,kLσ elements are obtained from the set of differential E equations, equation (10). Here the current, equation (11), can be written coefficients, P in terms of the transmittance P i.e. j(t) = kL E nkL E (0)TLR (t) − EkR nkR E (0)TRL (t), where TLR/RL is expressed using the evolution operator elements, 0 (t). Note that, in general, TLR (t) 6= TRL (t), and one Uiσ,kL/Rσ E cannot write the current in the form of the Landauer-like formula. Thus electrons can be pumped between electrodes with no source–drain voltage [17]. The expression for the current, equation (11), together with the set of differential equations for the evolution operator elements, equation (10), are the main analytical formulae of this paper. The total charge pumped during one time-dependent cycle of a train impulse (period) through the system is obtained from Z NL/Rσ = jL/Rσ (t) dt, (12) (6) where Ṽ(t) = U0 (t, t0 ) V(t) U0+ (t, t0 ) and U0 (t, t0 ) = T Rt 0 0 exp(i t0 dt H0 (t )). In equation (5) nkασ E (t0 ) represents the initial filling of the corresponding single-particle state in the left or right leads (we assume the initial wire site occupations, niσ (t0 ) = 0). For t > t0 the charge localized at the ith wire site can be expressed in terms of the appropriate matrix elements of the evolution operator, i.e. X 2 niσ (t) = nkασ (7) E 0 (t0 )|Uiσ,kασ E 0 (t, t0 )| . E 0 kασ Assuming the same positions of all on-site energies in the wire, εiσ = ε0σ (which is reasonable for a regular wire consisting of almost identical sites) and t0 = 0, the following set of differential equations for the evolution operator matrix 3 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko and the relation NLσ = −NRσ is satisfied in our system. We assume that the external perturbation does not spread immediately through the wire but there is a kind of a wire inertia which leads to different couplings between QW sites for a given time. It means that for our wire the coupling (first QD)–(L electrode) is different in comparison with those for (first QD)–(second QD) or (last QD)–(R electrode). Here we consider two possibilities for time-dependent perturbations. The first one assumes that the couplings QD–QD and QD–electrode change in time like the Gaussian distribution function, i.e. ! [t − (t00 + (j − 1)tx )]2 fj (t) = 1 + exp − , (13) σ0 where j = 1, 2, . . . , N + 1 corresponds to the following connection: (L electrode)–(first QD) for j = 1, (first QD)–(second QD) for j = 2, . . ., (last QD)–(R electrode) for j = N +1, respectively. The parameter tx stands for a time shift of the external signal between the nearest-neighbour hoppings and for tx = 0 all hoppings are driven homogeneously (the coupling strengths change in time in the same way). σ0 corresponds to the half-width of the Gaussian signal and t00 stands for the time for the first Gaussian maximum, i.e. the maximum of the f1 function. The couplings between appropriate sites in the system are responsible for the distance between these sites (the weaker the V parameter the larger the distance between sites). Thus the perturbation described above (one-Gaussian function) leads to decrease the distance between sites (in the first stage of perturbation) and then the system returns to its initial arrangement. The second time-dependent perturbation considered in this paper has a structure of two, positive and negative, Gaussian functions which can be written as follows: ! [t − (t00 + (j − 1)tx )]2 fj (t) = 1 + exp − σ0 ! [t − t1 − (t00 + (j − 1)tx )]2 , (14) − exp − σ0 Figure 2. The case of a single QD coupled with two electrodes. Upper panels: time-dependent perturbations between the left electrode and the QD site (solid lines) and between the right electrode and the QD site (broken lines). Charge occupations of the QD site: the current flowing from the left electrode and from the right one are shown in the middle and bottom panels, respectively. The left (right) panels correspond to the one-Gaussian (two-Gaussian) perturbation. The broken and solid lines correspond to ε0 = 4 and ε0 = −4, respectively. The other parameters are tx = 5, σ = 10, VL = VR = 4, t00 = 50 and 0 = 1. where t1 is a time shift between the maxima of two-Gaussian functions. In the absence of a time shift between these functions, t1 = 0, the system is not disturbed. The examples of both kinds of perturbations are described in section 3 and depicted in figure 2, upper panels. Throughout the paper we consider no source–drain voltage (µL = µR = 0), which implies that the Fermi energy is zero, EF = 0. The current is expressed in units of 2e0/h̄ and time in h̄/ 0. In our calculations we assume large values of the t00 parameter in order to avoid the initial switch effects, which appear for t ≥ t0 = 0. The positive value of the left/right current means that electrons tunnel from the left/right electrode to the first/last QW site. we consider a wire in the absence of Zeeman splitting, i.e. ε0σ = ε0−σ = ε0 , (h = 0). Thus the current flowing through the system, charge occupations and the pumped charge do not depend on σ , i.e. jLσ (t) = jL−σ (t) = jL (t), niσ (t) = ni−σ (t) = ni (t) and NLσ = NL−σ = NL and similar relations hold for the R index. Also the spin-flip scattering is not taken into consideration in this section. 3.1. Single QD pump First we study the pumping effect for a system consisting of one site (single QD) coupled with two electrodes. The couplings change in time but there is a time shift between the left and right couplings, figure 2, upper panels—the left (right) panel for one-Gaussian (two-Gaussian) perturbations. A similar system was also considered in [8], but the couplings were switched on and off alternately from zero to maximal 3. Pure charge pumps To find the basic reactions of the one-dimensional system to the Gaussian-like time-dependent perturbations in this section 4 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko pump which will be discussed further. This asymmetry is very visible for the two-Gaussian perturbation, right panels. To find the total charge pumped from the left electrode to the right one, NL , one should integrate the left current jL (t) over time. In figure 3 the charge pumped through a single QD system is shown as a function of the time shift parameter, tx , for different values of ε0 as well as the one-Gaussian perturbation (upper panel) and the two-Gaussian perturbation (bottom panel). If there is no time shift between f1 and f2 functions, tx = 0, the charge is not pumped—in this case f1 and f2 functions are the same and the system is driven homogeneously. For a very large value of the tx parameter, the net charge also equals zero as both functions f1 and f2 are quite separate (do not overlap each other). √The maximal value of the net charge is observed for tx = σ . It is interesting that, for ε0 = 0 (thick lines), the charge does not flow through the system although tx 6= 0. In this case the system is symmetrical in the energy scale and the total occupation of the QD site remains constant. For ε0 6= 0 and in the presence of a time-dependent perturbation, the QD occupation changes in time which leads to the charge pumping effect. Note that for the one-Gaussian perturbation and positive ε0 the pumped charge is positive with the same absolute values as for negative ε0 (not shown here). For the two-Gaussian perturbation and negative ε0 , the charge flows from the right to the left electrode (for small tx ), or in the reverse direction (for larger tx ). The opposite conclusion is valid for positive ε0 . Figure 3. Charge pumped through a single QD as a function of tx for ε0 = 0, −2 and −4 (thick solid, broken and thin solid lines, respectively). The upper (lower) panel corresponds to the one-Gaussian (two-Gaussian) perturbation. The other parameters are as in figure 2. values (quantum ratchets). The QD occupation and the current flowing from the left and right electrodes in the presence of these perturbations are shown in the middle and bottom panels in figure 2. The broken and solid lines correspond to different positions of the on-site QD energy, ε0 = 4 and ε0 = −4, respectively. The charge occupations of these sites are characterized by two local minima (for negative ε0 ) or maxima (for positive ε0 ) which appear for maximal values of the left and right couplings, i.e. for t = 50 and 55, and are related to the extremes of the f1 and f2 functions. This conclusion is also valid for the two-Gaussian perturbation, right panels. It is interesting that for negative ε0 , the QD occupation, n1 (t), decreases for larger couplings VL/R (t) and increases for smaller VL/R (t). The opposite relation holds for positive ε0 . If both functions f1 and f2 do not change in time the current does not flow through the system as we consider here the same chemical potentials of both leads. In the presence of time-dependent perturbations the current oscillates in time. Depending on the position of ε0 , for a given time, it can be positive or negative. It is interesting that the left (right) current is equal to zero for the extremal values of the f1 (f2 ) function. Moreover, the right and left currents seem to be strictly time-shifted by the tx parameter. However, there are small differences between both currents—compare, for example, the maximal values of jL (t) and jR (t) (solid lines, right panels). Additionally, the current curves look like an ‘odd’ function for the one-Gaussian perturbation (left panels) but the precise calculations show that these curves are non-symmetrical and the system behaves as an electron 3.2. Quantum wire pump In this subsection we consider pumping effects through a short QW subjected to external time-dependent perturbations (train impulse). First, we analyse the case of a QW consisting of three sites and in figure 4 we show the net charge pumped through the system as a function of the on-site energy, ε0 , and the time shift parameter, tx . The upper (bottom) panel corresponds to the one-Gaussian (two-Gaussian) perturbation. Before the external impulse starts the system is characterized √ by three molecular states localized at ε0 and ε0 ± V1 2 ' ε0 ± 5.6. In the presence of the time-dependent perturbations the parameter V1 changes, which moves these peaks in the energy scale. Thus the maximal pumped charge is observed for larger ε0 , i.e. ε0 ' ±6.8. For negative values of ε0 the charge at the first QW site flows out to the left electrode (if the coupling of the left electrode with the first QD increases) and, due to nonzero coupling between the first and second QW sites, electrons flow from the second site to the first one in order to compensate the charge which escapes from the first site. This is the reason that, for negative ε0 , the pumped charge flows from the right electrode to the left one. The opposite conclusion is valid for positive values of ε0 . This result is crucial as it concerns spin current devices and will be discussed in section 4. It is interesting that electron charge is pumped through the system also for small absolute values of ε0 (but for ε0 = 0 the current is zero, cf figure 3). It is related to a nonzero value of the wire density of states (DOS) at the Fermi level for odd N. The pumped charge is rather small in this case (ε0 ≈ 0, upper panel) because the 5 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko Figure 5. Charge pumped from the left electrode as a function of the wire length, N, for ε0 = 0.5, 4.0, 5.56 and 9.0. The other parameters are V1 = 4, tx = 3, σ0 = 10 and 0 = 1. The lines serve as a guide to the eyes. figures 3 and 4. Unfortunately, in general, this conclusion is not valid and the pumping current strongly depends on the system parameters. To corroborate this effect in figure 5 we study the charge pumped along a wire as a function of the wire length, N. Note that for ε0 = 0 the net charge is not pumped through the system independently of the wire length (not shown in figure 5) but for small nonzero ε0 even–odd pumped charge oscillations are visible (thin solid line). These oscillations are characterized by the maximal values of NL for every odd-length wire but the oscillation amplitude decreases with N. The other positions of ε0 were chosen in such a way that they satisfy the condition of conductance oscillations for periods 3 and 4, [51]. Thus for ε0 = 4 (thick solid line) the oscillation period of the pumped charge is 3 and for ε0 = 5.56 (broken line) the period is 4. As one can see the pumped charge changes non-monotonically as a function of N and oscillates with the wire length (similarly to the conductance oscillation effect). These oscillations are very visible for short wires. For longer N there are many molecular states of the system which are localized near (below and above) the Fermi energy and they all play a role in pumping in both directions. Thus the oscillation amplitude of NL decreases with N. We have found that the charge current oscillates as a function of N for |ε0 | < 2V1 —molecular states which lie between ε0 − 2V1 and ε0 + 2V1 (which corresponds to the wire bandwidth) are responsible for these oscillations. For the case of |ε0 | > 2V1 the pumped current increases with N, see the dotted line in figure 5 for ε0 = 9.0. It results from the fact that most external molecular states of the wire are shifted with N and tend to ε0 ± 2V1 . Thus for the large positive ε0 one of these states, which lies close to ε0 − 2V1 , moves towards the Fermi energy. For longer wires there are no significant differences in the energy positions of these edge states and the pumped current does not change with N. Note that in the presence of an oscillating potential the charge pumped per one cycle is proportional to the frequency of an external perturbation [18, 22], and the pumping current vanishes in the adiabatic limit (ω → 0). In our studies we consider only one pumping cycle, so the pumped charge does Figure 4. The absolute value of the pumped charge through the three-site wire with the one-Gaussian (upper panel) and two-Gaussian (lower panel) perturbations versus ε0 and tx . The other parameters are as in figure 2. system is almost symmetrical in the energy scale and the occupation of QW sites is about 0.5. In comparison with the one-Gaussian impulse (upper panel) for the two-Gaussian perturbation (bottom panel)√a large value of the net charge is pumped also for |ε0 | < V1 2. In this case the V1 parameter decreases to a very small value for a moment (cf figure 2, upper right panel) and in that case the wire DOS peaks are shifted towards the Fermi energy (the current increases). Moreover, for the two-Gaussian perturbation the net charge is also pumped through the system for larger tx . It is worth noting that for short QWs the pumped charge decreases very fast for tx > σ . However, for longer wires the net charge can be nonzero even for larger tx . This effect is related to the wire capacity—the excess charge must be transported through all QW sites in order to obtain a new equilibrium state. For such a system it takes some time to get rid of the excess charge and it also leads to the pumping effect for larger tx . Thus one expects that the pumped charge should increase with the wire length, [23]. It seems true as the charge which is pumped per cycle through a short wire is rather large (about ten times) in comparison with a single QD system, see 6 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko Figure 7. Spin current pumped through a wire consisting of N = 2–5 QDs as a function of the h parameter for ε0−σ = ε0σ = 0 at h = 0 and Vi = 4, i = 1–4. The other parameters are the same as in figure 6. (e.g. in figure 3). For nonzero h electrons with spins −σ and σ are pumped in the opposite direction (there are spin-up and spin-down currents). As a consequence, the total charge flowing through the system, NLσ + NL−σ (thick solid line), is equal to zero independently of the strength of the Zeeman splitting. However, the spin current which is proportional to NLσ − NL−σ (thin solid line) is nonzero, i.e. spins are pumped through the system although there is no charge current. In the lower panel the initial positions of the QD spin-up and spin-down energy levels are not localized at the Fermi level—in the absence of Zeeman splitting we have ε0−σ = ε0σ = 1. Thus for h = 0 the electron charge is pumped from the left electrode through both QD spin levels and the total electron current is maximal, thick solid line, bottom panel. In this case, however, the total spin current (thin solid line) does not flow because spin-up and spin-down currents are equal to each other (broken curves). In the presence of the Zeeman splitting spin-up and spin-down charges (which are pumped through the system) are characterized by different values, which leads to nonzero total spin–charge currents. However, for some values of h, the total electron current does not flow but the spin current exists, e.g. for h = 2.9. Moreover, the charge current can be positive (for small Zeeman splitting) or negative for larger h which results directly from the relative positions of ε0σ , ε0−σ and the Fermi energy. It is worth noting that the charge current is symmetrical in relation to h (for positive and negative values of h the charge current is the same) whereas the spin current curves are antisymmetrical versus h = 0 (thin solid line). The next interesting question is whether the spin and charge pumping effects exist also for a QW (chain of QDs). Therefore, we have calculated the corresponding currents as a function of the h parameter for the symmetrical case ε0−σ = −ε0σ (i.e. ε0−σ = ε0σ = 0 at h = 0), and for a wire composed of N = 2–5 QDs, see figure 7. Note that, in this case, for arbitrary N, the total charge current does not flow through the system, independently of h. Thus, in figure 7 we show only the total spin current, NLσ − NL−σ . As one can see, for h = 0 (no Zeeman splitting) the spin current does not flow, which is in accordance with the previous results. For h 6= 0 the spin Figure 6. Charge and spin currents flowing through a single QD system, N = 1, as a function of the level separation h (Zeeman splitting parameter) for different positions of ε0σ for the vanishing magnetic field (ε0−σ = ε0σ = 0–upper panel–and εσ = ε−σ = 1–bottom panel). Thick broken (thin broken) lines correspond to NL−σ (NLσ ) and the thick solid (thin solid) lines represent charge (spin) currents. The other parameters are tx = 5, σ = 10 (one-Gaussian perturbation), VL = VR = 4 and 0 = 1. not depend on the perturbation frequency and is nonzero for a wide range of the system parameters, ε0 , tx and N. 4. Spin and charge pumps in the presence of magnetic field If a magnetic field is applied to the wire all on-site energies are split (Zeeman splitting) which leads to different values of ε0σ and ε0−σ states. Therefore, in the presence of external time-dependent perturbations, fi , electrons with spin σ can be pumped through the system in one direction and, at the same time, electrons with spin −σ can flow in the opposite direction. In that case for particular values of ε0±σ the spin current could appear although the charge current is zero. (Note that no source–drain voltage is applied to the system.) To confirm this effect in figure 6 we show electron charges which are pumped through a single-site system (QD), as a function of the Zeeman splitting parameter, h (thin and thick broken curves correspond to spins σ and −σ , respectively). In the upper panel, for no Zeeman splitting, h = 0, the QD spin levels satisfy the relation ε0−σ = ε0σ = 0 and in the presence of magnetic field both levels are separated symmetrically versus the Fermi energy, i.e. ε0−σ = −ε0σ . As one can see no charge is pumped through the system for h = 0 which is the same effect as discussed in section 4, 7 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko current appears and, for example, for N = 2 it is visible at only one current extreme (the second one appears for negative h, not shown in figure 7). Generally, for the even or odd number of N there are N or N + 1 extrema on the spin current curve. For odd N the spin current possesses a small minimum near h = 0.5 (slightly visible for N = 3 and 5) while for even N, the spin current does not flow for the same h. It results from the structure of the wire’s molecular states—only odd-length wires are characterized by a state at the Fermi level (if N is even the wire DOS is flat at the Fermi level) [51]. Thus, for example, for N = 2 and h = 0 the system is characterized by two molecular states at ±V1 (not at the Fermi level). In the presence of a magnetic field each molecular state is split and four spin states are observed (two with spins σ and two with −σ ). For small h the spin current does not flow through the system because all molecular states lie far from the Fermi level. However, for larger h the spin molecular states cross the Fermi level and the spin current appears (spin-up and -down molecular states are localized symmetrically versus EF in this case and instead of four spin current peaks we observe only two of them). For stronger and stronger magnetic fields there are no molecular states near the Fermi level and the spin current does not flow again. As the most prominent feature obtained in figure 7 we find that the total spin current pumped during one cycle of time-dependent perturbation strongly depends on the number of QW sites, N. In particular, for N = 1 only about 0.15 electron spin is pumped (figure 6, upper panel) whereas for N = 5 this value exceeds 1.6 per cycle (it is ten times larger), figure 7. This effect is related to the structure of the wire molecular states. Namely, for longer wires there are many molecular states localized symmetrically below and above the Fermi energy. For a nonzero magnetic field each state is split and (depending on the h parameter) can cross the Fermi energy. Thus even a small change in QD–QD coupling (during the time-dependent perturbation) strongly influences the site occupations. As a consequence, a high-value spin current flows through the system in the absence of the charge current. For N = 1 a single molecular state lies at the Fermi level and is very wide in comparison with the case of larger N. Thus the same time-dependent disturbance does not influence the spin current in the same way as for other N. However, all the above-mentioned values of the spin current depend on the magnetic field, h, and in general the current does not change monotonically with the wire length, see also figure 5. Only for h > ε0σ + 2V1 , which corresponds to h > 16, does the spin current increase with N, figure 7, but for the other h the sequence is different. For small h (h ' 1) the spin current oscillates with N and this effect will be discussed later. Next it is interesting to study a similar problem in the presence of nonzero charge current. Thus we consider an N-site wire with the Zeeman splitting and asymmetrically localized ε0σ and ε0−σ levels, figure 8. In contrast to figure 7 here we have chosen ε0−σ = ε0σ = 1 for h = 0 and therefore the initial positions of the QD spin-up and spin-down energy levels do not correspond to the Fermi level. As one can see, for h = 0 electrons are pumped through the system but the net pumped charge is rather small for all N. In that case the Figure 8. Charge current (upper panel) and spin current (bottom panel) through a wire consisting of N = 2–5 sites as a function of the Zeeman splitting parameter, h, for the asymmetrical case, i.e. ε0σ = ε0−σ = 1 for h = 0. Letters A and B indicate extreme points on the thick curve which are discussed in the text. The other parameters are the same as in figure 7. spin current does not flow because ε0σ = ε0−σ (bottom panel). For larger h the charge current increases and, for example, for N = 5 about 0.8 of an electron can be pumped during one time-dependent cycle (upper panel). Moreover, the charge current direction strongly depends on the magnetic field and may be positive or negative (each current peak coexists with its neighbouring dip). To explain this effect we concentrate on the two-sites wire N = 2 (thick line) which is characterized by two molecular state structures for every spin (there are two peaks in the wire DOS localized at ε ± = ε0σ ± V1 ). Thus for the small magnetic field the system is characterized by very low values of DOS near the Fermi level which leads to no charge and no spin pumping. For the larger magnetic field the molecular states ε ± cross the Fermi level at different h and the total charge pumped through the system depends on a relative distance between ε + , ε − and the Fermi level. (For a state which lies below/above the Fermi level, the pumping current is negative/positive.) Thus for h = 8 the charge current is positive (peak indicated by point A) and for a stronger magnetic field the pumping current is characterized by a local dip (point B). For larger h the charge current vanishes because both +σ and −σ molecular states are situated far from the Fermi level. It is interesting that some inflection points and extrema are also visible on the spin current curves NLσ − NL−σ , figure 8, bottom panel. For all N and for h > 0 the spin current is always negative (the current flows in one direction) 8 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko but at the same time the charge current changes its value from positive to negative, depending on the Zeeman splitting parameter. It leads to a kind of spin–charge separation, i.e. spin and charge move in opposite directions. It is surprising that this effect holds for no electron–electron interactions in the wire. The structure of NLσ − NL−σ for other N (maxima and inflection points) is related to the wire molecular states and their relative distance from the Fermi level. To conclude, by changing the Zeeman splitting parameter one can change the pumping current from the positive value to the negative one (and vice versa). This effect is very interesting because the time-dependent Gaussian-like perturbation (train impulse) moves along the wire only in one direction, from the left electrode to the right one. Thus one expects that electrons should follow this impulse, but in the considered system they can flow in the opposite direction which leads to the spin–charge separation effect. Note that in that case the direction of the spin current remains unchanged (the curves are asymmetrical versus h = 0). Figure 9. QD charge occupations nσ (solid lines) and the corresponding currents flowing from the left electrode (broken lines) as a function of time and spin-flip coupling Vsf = 0, 1 and 4 (thin, normal and thick lines) in the case of the single QD coupled with two leads. The one-Gaussian perturbation is considered with the parameters tx = 3, σ = 10, t00 = 25 and VL = VR = 4, 0 = 1, h = 1 and ε0±σ = 1 for the vanishing magnetic field. 5. Pumping effects with the spin-flip scattering the charge current, NLσ + NL−σ , pumped through the system. Thus in figure 10 we show the charge and spin currents for a single-site wire and for a different Vsf parameter as a function of the Zeeman splitting strength, h. The upper panel corresponds to the symmetrical case ε0−σ = ε0σ (the charge current does not flow in this case, see also figure 6) and the middle and bottom panels show the results for the non-symmetrical case, ε0σ = ε0−σ = 1 for h = 0. As one can see for the symmetrical case (upper panel) the absolute value of the spin current decreases with Vsf and its direction is the same for all positive (or negative) h. However, for the non-symmetrical case and for a certain range of the h parameter the absolute value of the spin current pumped in the system increases with the spin-flip scattering Vsf , (middle panel for −2 < h < +2). This interesting inversion can be explained in terms of molecular states of the system. For |h| < 2 and Vsf = 0 both spin states, ε0−σ and ε0σ , lie above the Fermi level. In the presence of the spin-flip scattering the hybridized spin states move with Vsf and one of them crosses the Fermi energy. In that case the spin current increases with Vsf , e.g. for h = 1, the lines for Vsf = 1 and Vsf = 2, middle panel. For a larger spin-flip parameter, Vsf > 2, the absolute value of the spin current decreases as the hybridized spin states move away from the Fermi level. Note that the spin current does not change its direction at different values of Vsf (for a given h). However, the charge current pumped through the system (bottom panel) can be positive or negative depending on the Vsf value and the Zeeman splitting term, h. It is worth noting that the charge current is maximal for no magnetic field and for no spin-flip scattering (thick solid line, bottom panel). For nonzero Vsf the current rapidly decreases and can be negative (changes its direction). Similar conclusions hold for a system consisting of N QD sites. We have checked that the spin and charge currents observed, e.g. in figure 8, are somewhat modified only for a small Zeeman splitting parameter. In this regime new maxima in both pumping currents can appear which lead to an increase In this section we concentrate on charge and spin pumping through a QW in the presence of the intradot spin-flip coupling, Vsf . In figure 9 we study the role of the spin-flip scattering on time-dependent occupations (solid lines) and corresponding currents flowing from the left electrode (broken lines) for different values of the Vsf parameter. A single-site wire, N = 1, and one-Gaussian time-dependent perturbation are considered. For the stationary case (before the perturbation starts, t 25) the current does not flow through the system and the charge nσ localized on the QD is constant but depends on the spin-flip strength—the occupation increases with Vsf . Such a behaviour of nσ results from the fact that in the presence of the spin-flip scattering spin-degenerate energy levels, ε0σ and ε0−σ , are replaced by new energies of the system and two peaks are q observed in the local DOS for ε ± = (ε0σ + ε0−σ )/2 ± (ε0σ − ε0−σ )2 +4Vsf2 /2. Thus for larger Vsf one peak is shifted below the Fermi energy, the occupation of this state increases and simultaneously the probability thatqthe electron in this state has a spin σ , (1 − (ε0−σ − ε0σ )/ (ε0σ − ε0−σ )2 +4Vsf2 )/2, also increases. In the presence of the time-dependent perturbation the charge occupation and the pumping current change in time. It is interesting that, depending on the spin-flip strength, the charge nσ can increase, decrease or remain almost unchanged. This time dependence of nσ for different values of Vsf is similar to the dependence of the QD charge occupation, see figure 2 for ε0 > EF . For larger Vsf the curve nσ (t) has a minimum for the same time interval, as in that case one peak of the DOS is localized below the Fermi energy which was also observed for ε0 = −4 in figure 2. Note that the corresponding currents flowing from the left electrode can also change direction in the presence of the spin-flip scattering (broken lines). The next interesting point is whether the spin-flip coupling influences the net spin current, NLσ − NL−σ , and 9 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko Figure 11. Charge pumped from the left electrode, NLσ and NL−σ (two upper panels) and charge and spin currents (two bottom panels) as a function of the wire length, N, for Vsf = 0–2. The other parameters are ε0σ = −2, ε0−σ = 4, h = 6, V1 = 4, tx = 3, σ0 = 10 and 0 = 1. The lines serve as a guide to the eyes. Figure 10. Spin current, NLσ − NL−σ , and charge current, NLσ + NL−σ , pumped through the one-site wire as a function of the Zeeman splitting parameter h, for the symmetrical case ε0σ/−σ = 0 for h = 0 (upper panel) and the asymmetrical one ε0σ/−σ = 1 for h = 0 (middle and bottom panels). The spin-flip couplings are Vsf = 0–4 (thick solid, thin solid, dotted, solid and broken lines, respectively). The other parameters are the same as in figure 9. values of charge for N = 2, 5, . . .. At the same time the charge NLσ does not reveal such oscillations because for ε0σ = −2 the condition for the conductance oscillations is not satisfied, [51]. Oscillations with the period of three sites are also reflected on the charge and spin currents (two lower panels). For longer wires these oscillations decrease as in this case there are many appropriate states near the Fermi level which influence the oscillation effect. It is interesting that for short wires, e.g. N = 2 or 5, the charge current, as well as the absolute values of the spin current, NLσ − NL−σ , increase with the spin-flip parameter. However, the charge current and the spin current flow in opposite directions in this case (spin–charge separation). Moreover, the spin current does not change its sign for all N while the charge current can be positive or negative depending on the wire length and the spin-flip parameter. The above results confirm that the pumped charge does not change monotonically with the wire length but it oscillates depending on the ε0±σ positions. Moreover, we have found that for a given N the pumped charge increases with the spin-flip scattering strength. of these currents as a function of Vsf (similar to the case of N = 1). The final studies in this paper are devoted to the wire-length-dependent spin and charge pumping through a QW. In figure 11 we show the charge pumped from the left electrode, NLσ , and NL−σ (the first and second panels), the charge current, (NLσ + NL−σ , the third panel), and the spin current (NLσ − NL−σ , the bottom panel) as a function of the wire length, N, for a different spin-flip parameter Vsf . A one-Gaussian time-dependent impulse acts on the wire and the asymmetrical case with the Zeeman magnetic field is considered. For Vsf = 0 and N = 1 the spin-degenerate energy levels are localized at ε0−σ = 4 and ε0σ = −2. The value of ε0−σ corresponds to the case of the conductance oscillations with the period of 3, [51]. As one can see, the pumping charge, NL−σ , oscillates with N with the maximal 10 J. Phys.: Condens. Matter 23 (2011) 405301 T Kwapiński and R Taranko 6. Conclusions [9] Blick R H, Haug R J, Weis J, Pfannkuche D, Klitzing K v and Eberl K 1996 Phys. Rev. B 53 7899 [10] Gasparian V, Altshuler B and Ortuno M 2005 Phys. Rev. B 72 195309 [11] Platero G and Aguado R 2004 Phys. 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This perturbation has influenced all hopping integrals between the nearest-neighbour sites in the system. We have found that in the presence of full spatial symmetry (and the same on-site energies which lie at the Fermi level) the current flowing from the left and right electrodes oscillates in time but no charge and no spin are pumped along the system. In other cases, the net charge can be pumped but its value strongly depends on the wire length. In the presence of a magnetic field which leads to the spin-level separation (Zeeman splitting) pure spin pumps exist in the absence of the charge current. Moreover, the spin-flip scattering, Vsf , can significantly modify the charge current and can change its direction. It leads to the spin–charge separation which manifests in opposite directions of both spin and charge currents. It is interesting that we have observed this effect in the system with no electron–electron correlations. We have also found that for the asymmetrical case the spin current increases with the strength of the spin-flip scattering. Additionally, the pumping currents (charge and spin) oscillate as a function of the wire length. Acknowledgments This work has been partially supported by grant nos N N202 263 138 and N N202 330 939 of the Polish Ministry of Science and Higher Education. References [1] Smit R H M, Untiedt C, Rubio-Bollinger G, Segers R C and van Ruitenbeek J M 2003 Phys. Rev. Lett. 91 076805 [2] van Wees B J, van Houten H, Beenakker C W J, Williamson Philips J G, Kouwenhoven L P, van der Marel D and Foxon C T 1988 Phys. Rev. Lett. 60 848 [3] Auslaender O M, Steinberg H, Yacoby A, Tserkovnyak Y, Halperin B I, Baldwin K W, Pfeiffer L N and West K W 2005 Science 308 88 [4] Oosterkamp T H, Kouwenhoven L P, Koolen A E A, van der Vaart N C and Harmans C J P M 1997 Phys. Rev. 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