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Spintronics

Spintronics studies how spin angular momentum and magnetic order are generated, transported, detected, and used to control electronic or magnetic states. Its central objects are not isolated spins but nonequilibrium spin accumulations, spin-polarized charge currents, pure spin currents, interfacial torques, and magnetization-dependent electrical signals.

A useful device separates four functions:

  1. generation, by a ferromagnetic contact, optical orientation, the spin Hall effect, or interfacial spin–momentum locking;
  2. transport, by itinerant electrons, holes, magnons, or collective magnetic order;
  3. manipulation, by precession, exchange fields, spin–orbit fields, spin-transfer torque, or spin–orbit torque;
  4. detection, through a ferromagnetic analyzer, inverse charge–spin conversion, magnetoresistance, optical rotation, or magnetic resonance.

Those stages are linked by interfaces. A large bulk polarization or spin Hall conductivity does not guarantee a large device signal if the interface absorbs, depolarizes, reflects, or shunts the relevant current.

Density and Current Operators owns microscopic current operators and the nonuniqueness of spin current when spin is not conserved. Spin–Orbit Coupling in Solids owns intrinsic and extrinsic spin Hall mechanisms. This page owns the device-level transport ledger: spin diffusion and injection, nonlocal detection, giant magnetoresistance, reciprocal conversion, spin pumping, current-induced torques, and the material constraints connecting them.

Required background. Density and Current Operators supplies spin-current and torque definitions, while Spin–Orbit Coupling in Solids supplies charge–spin conversion mechanisms.

Helpful background. Ferromagnetism provides injection and magnetoresistive context, while Boltzmann Transport provides the semiclassical transport closure.

Spin-transport literature uses several quantities all called “spin current.” They are not numerically interchangeable.

Let e>0e>0 denote the elementary charge. A spin-resolved conventional charge-current density has units A m−2\mathrm{A\,m^{-2}}. For a chosen quantization axis,

jc=j↑+j↓,js(q)=j↑−j↓.\mathbf j_c = \mathbf j_\uparrow + \mathbf j_\downarrow , \qquad \mathbf j_s^{(q)} = \mathbf j_\uparrow - \mathbf j_\downarrow .

The superscript (q)(q) marks the charge-equivalent normalization. Its current polarization is

Pj=js(q)⋅n^jc⋅n^=j↑−j↓j↑+j↓,P_j = \frac{ \mathbf j_s^{(q)}\cdot\hat{\mathbf n} }{ \mathbf j_c\cdot\hat{\mathbf n} } = \frac{ j_\uparrow-j_\downarrow }{ j_\uparrow+j_\downarrow },

for transport along n^\hat{\mathbf n}. This scalar description is adequate only when a common spin axis remains meaningful.

The angular-momentum-current tensor Qi aQ_i^{\,a} describes flow along spatial direction ii of spin angular momentum polarized along aa. Its units are angular momentum per area per time. We define

js,i a≡2eℏQi a,j_{s,i}^{\,a} \equiv \frac{2e}{\hbar} Q_i^{\,a},

so js,i aj_{s,i}^{\,a} also has units A m−2\mathrm{A\,m^{-2}}. The inverse relation is

Qi a=ℏ2ejs,i a.Q_i^{\,a} = \frac{\hbar}{2e} j_{s,i}^{\,a}.

Some authors call Qi aQ_i^{\,a} the spin current; others call js,i aj_{s,i}^{\,a} the spin current and suppress the factor ℏ/2e\hbar/2e. Every quoted spin Hall angle, interface conductance, or torque efficiency should therefore state its normalization.

For collinear transport, the spin accumulation is the splitting of spin-resolved electrochemical potentials,

μs≡μ↑−μ↓.\mu_s \equiv \mu_\uparrow-\mu_\downarrow .

For noncollinear transport it becomes a vector μs\boldsymbol{\mu}_s in spin space. It has units of energy, not magnetization. A spin density and a spin accumulation are related through the appropriate density of states and susceptibility; they are not identical variables.

We use:

  • m=M/Ms\mathbf m=\mathbf M/M_s for a ferromagnet’s unit magnetization;
  • p^\hat{\mathbf p} for the injected spin-polarization direction;
  • tFt_F for the active magnetic-layer thickness;
  • λs\lambda_s for a spin-diffusion length;
  • τs\tau_s for a spin-relaxation time;
  • θSH\theta_{\mathrm{SH}} for a spin Hall conversion ratio in an explicitly stated geometry;
  • geff↑↓g_{\mathrm{eff}}^{\uparrow\downarrow} for an effective spin-mixing conductance per area.

Current direction, electron-flow direction, interface normal, and magnetization direction must be drawn separately. Reversing any one of them can reverse a reported sign.

For spin density sas^a, a local balance equation has the form

∂sa∂t+∂iQi a=Ta−sa−seqaτsf,\frac{\partial s^a}{\partial t} + \partial_i Q_i^{\,a} = \mathcal T^a - \frac{s^a-s_{\mathrm{eq}}^a}{\tau_{\mathrm{sf}}},

where Ta\mathcal T^a is a coherent torque density and the final term represents a simple spin-flip relaxation model. When the Hamiltonian does not conserve sas^a, current and torque can be repartitioned by torque-dipole terms. The measurable content lies in the complete balance law and boundary conditions, not in a current symbol alone.

In a diffusive nonmagnetic conductor, a widely used phenomenological equation is

∂μs∂t=Ds∇2μs−μsτs+ΩL×μs+S,\frac{\partial\boldsymbol{\mu}_s}{\partial t} = D_s\nabla^2\boldsymbol{\mu}_s - \frac{\boldsymbol{\mu}_s}{\tau_s} + \boldsymbol{\Omega}_L \times \boldsymbol{\mu}_s + \mathbf S,

where DsD_s is a spin-diffusion coefficient, ΩL\boldsymbol{\Omega}_L is the Larmor-frequency vector, and S\mathbf S is a source. Without precession or a source, each steady component obeys

∇2μs=μsλs2,λs=Dsτs.\nabla^2\mu_s = \frac{\mu_s}{\lambda_s^2}, \qquad \lambda_s = \sqrt{D_s\tau_s}.

In one dimension,

μs(x)=Ae−x/λs+Bex/λs.\mu_s(x) = A e^{-x/\lambda_s} + B e^{x/\lambda_s}.

Boundary conditions discard the exponentially growing branch in a semi-infinite lead. The diffusion length is therefore not the mean free path: it combines many momentum-scattering events with a slower loss of spin memory.

If ζσ\zeta_\sigma is a spin-resolved electrochemical potential expressed in volts, define

ζs=ζ↑−ζ↓.\zeta_s = \zeta_\uparrow-\zeta_\downarrow .

For equal spin-channel conductivities in a nonmagnetic metal,

js(q)=−σ2∇ζs.\mathbf j_s^{(q)} = - \frac{\sigma}{2} \boldsymbol{\nabla}\zeta_s .

The sign follows this voltage convention. If μs\mu_s is used instead, the conversion between μs\mu_s and ζs\zeta_s must be stated. This small bookkeeping choice explains many apparent sign disagreements.

Spin injection, two-current giant magnetoresistance, and spin Hall torque geometries

Three device ledgers. (a) A ferromagnetic injector creates a spin accumulation that decays over λs\lambda_s in a nonmagnetic channel and is sampled nonlocally by a second ferromagnet. (b) A two-current resistor model gives low resistance for parallel magnetic layers and high resistance for antiparallel layers. (c) A charge current in a spin–orbit layer generates a transverse spin flux into a ferromagnet, producing a damping-like torque; reciprocal spin pumping emits angular momentum from a precessing magnet.

Consider a ferromagnet F, a nonmagnetic channel N, and an interface c. In a one-dimensional collinear diffusion model it is useful to compare spin-resistance-area products,

rN=ρNλN,r_N = \rho_N\lambda_N,

and

rF=ρFλF1−PF2.r_F = \frac{ \rho_F\lambda_F }{ 1-P_F^2 }.

Here PFP_F is the bulk conductivity polarization. Both rNr_N and rFr_F have units Ω m2\Omega\,\mathrm{m^2}. Let rcr_c and PcP_c denote the contact’s spin-averaged resistance-area product and polarization in a specified interface convention. A common idealized injection result is

Pinj≃PFrF+PcrcrF+rN+rc.P_{\mathrm{inj}} \simeq \frac{ P_F r_F + P_c r_c }{ r_F+r_N+r_c }.

Exact factors depend on whether spin-channel resistances, total contact resistance, or area-normalized conductances are used. The physical limits are more robust than any memorized prefactor:

rN≫rF,rc⟹Pinj≪PF,rc≫rF,rN⟹Pinj→Pc.\begin{aligned} r_N\gg r_F,r_c &\Longrightarrow P_{\mathrm{inj}}\ll P_F, \\ r_c\gg r_F,r_N &\Longrightarrow P_{\mathrm{inj}}\to P_c. \end{aligned}

The first limit is the conductivity-mismatch problem for a transparent ferromagnet–semiconductor contact: the channel’s large spin resistance suppresses injection. A spin-selective tunnel barrier can raise rcr_c and restore polarization. An arbitrarily resistive barrier is not automatically optimal, because it reduces charge current, signal bandwidth, and impedance matching.

Real interfaces add:

  • spin-dependent interface transmission;
  • spin-memory loss from interfacial disorder and spin–orbit coupling;
  • interface states and Fermi-level pinning;
  • current crowding and nonuniform contact geometry;
  • magnon-assisted and inelastic channels;
  • proximity magnetism and intermixing.

Bulk polarization, contact polarization, and the polarization delivered to the channel are therefore distinct experimental quantities.

In a lateral nonlocal geometry, one ferromagnet injects current into a nonmagnetic channel while a distant ferromagnet detects voltage in a nominally open circuit. This separation strongly suppresses ordinary charge-voltage backgrounds.

For a narrow one-dimensional channel, an ideal form is

RNL≡VNLI≃±PinjPdetRNe−L/λN,R_{\mathrm{NL}} \equiv \frac{V_{\mathrm{NL}}}{I} \simeq \pm P_{\mathrm{inj}}P_{\mathrm{det}} R_N e^{-L/\lambda_N},

where

RN=ρNλNAN.R_N = \frac{\rho_N\lambda_N}{A_N}.

The sign changes between parallel and antiparallel injector–detector magnetizations. Some papers define ΔRNL\Delta R_{\mathrm{NL}} as the full parallel-minus-antiparallel difference, which adds a factor of two. Finite contact widths, spin absorption, multidimensional spreading, and interface resistances change the prefactor.

A transverse field rotates the diffusing spins. For injection along one spin axis, the ideal Hanle response contains

RNL(B)∝∫0∞dt4πDstexp⁡(−L24Dst−tτs)×cos⁡(ΩLt).\begin{aligned} R_{\mathrm{NL}}(B) \propto \int_0^\infty & \frac{\mathrm dt}{ \sqrt{4\pi D_s t} } \exp \left( - \frac{L^2}{4D_s t} - \frac{t}{\tau_s} \right) \\ &\times \cos(\Omega_L t). \end{aligned}

The diffusion kernel sums over all travel times; the cosine records precession. The characteristic dephasing field satisfies roughly

∣ΩL∣τs∼1,ΩL=gμBℏB|\Omega_L|\tau_s \sim 1, \qquad \boldsymbol{\Omega}_L = \frac{g\mu_B}{\hbar}\mathbf B

for an isotropic gg factor. Reliable extraction of DsD_s and τs\tau_s may require contact-induced relaxation, drift, anisotropic gg tensors, stray fields, nuclear fields, and magnetic switching to be modeled rather than absorbed into a single Lorentzian.

Giant magnetoresistance (GMR) is the dependence of a metallic multilayer’s resistance on the relative orientation of neighboring magnetic layers. It is a nonequilibrium transport effect, not simply the equilibrium energy that favors one alignment.

The Mott two-current picture begins with weak spin-flip scattering: majority and minority carriers conduct approximately in parallel and experience different resistances. For two identical ferromagnetic layers, let R↑R_\uparrow and R↓R_\downarrow be the resistance of one layer for spin quantized along its magnetization. In the parallel state,

RP=2R↑R↓R↑+R↓.R_P = \frac{ 2R_\uparrow R_\downarrow }{ R_\uparrow+R_\downarrow }.

In the antiparallel state, each channel encounters one majority-like and one minority-like layer, so

RAP=R↑+R↓2.R_{\mathrm{AP}} = \frac{ R_\uparrow+R_\downarrow }{ 2 }.

Thus

RAP−RPRP=(R↑−R↓)24R↑R↓≥0.\frac{ R_{\mathrm{AP}}-R_P }{ R_P } = \frac{ (R_\uparrow-R_\downarrow)^2 }{ 4R_\uparrow R_\downarrow } \ge 0.

Defining

β=R↓−R↑R↓+R↑,\beta = \frac{ R_\downarrow-R_\uparrow }{ R_\downarrow+R_\uparrow },

the same result becomes

ΔRRP=β21−β2.\frac{\Delta R}{R_P} = \frac{\beta^2}{1-\beta^2}.

This resistor network captures the sign and intuition, but not quantitative multilayers. Current-in-plane (CIP) and current-perpendicular-to-plane (CPP) geometries sample bulk and interface scattering differently. In CPP structures, the Valet–Fert theory solves spin-dependent diffusion with bulk asymmetries, interface resistances, finite spin-diffusion lengths, and spin accumulation. Layer thicknesses much larger than λs\lambda_s do not contribute coherently to spin contrast throughout their full volume.

EffectState variable controlling resistanceTypical structure
Anisotropic magnetoresistance (AMR)angle between current and one magnetic order parametersingle magnetic conductor
GMRrelative orientation of metallic magnetic layersmetallic spin valve or multilayer
Tunneling magnetoresistance (TMR)relative orientation across a tunnel barriermagnetic tunnel junction
Spin Hall magnetoresistancespin reflection and absorption at a spin–orbit-metal/magnet interfacebilayer
Colossal magnetoresistance (CMR)coupled magnetic, electronic, and structural statecorrelated magnetic oxide

For an ideal spin-conserving tunnel junction, Jullière’s model gives

TMR≡RAP−RPRP≃2P1P21−P1P2,\mathrm{TMR} \equiv \frac{ R_{\mathrm{AP}}-R_P }{ R_P } \simeq \frac{ 2P_1P_2 }{ 1-P_1P_2 },

where P1P_1 and P2P_2 are tunneling density-of-states polarizations. Crystalline symmetry filtering, barrier defects, bias, temperature, magnons, and interface resonances can invalidate this simple density-of-states formula.

Spin–orbit coupling permits reciprocal conversion between longitudinal charge flow and transverse spin flow. To make signs explicit, suppose a charge current flows along +x^+\hat{\mathbf x}, spin angular momentum flows along +z^+\hat{\mathbf z}, and its polarization is +y^+\hat{\mathbf y}. We define the sign of the spin Hall angle by

js,z y=θSHjc,x.j_{s,z}^{\,y} = \theta_{\mathrm{SH}} j_{c,x}.

Changing the interface normal or choosing electron flow instead of conventional current changes the verbal handedness. The tensor relation, axes, and sign convention should accompany every number.

The intrinsic Berry-curvature contribution, skew scattering, side jump, and the conventional spin-current operator are developed in Spin–Orbit Coupling in Solids. At the device level, a measured conversion also depends on

t,λs,ρ,geff↑↓,interface transparency,current shunting.t, \quad \lambda_s, \quad \rho, \quad g_{\mathrm{eff}}^{\uparrow\downarrow}, \quad \text{interface transparency}, \quad \text{current shunting}.

A fitted torque efficiency is therefore not automatically the intrinsic bulk spin Hall angle.

The inverse spin Hall effect converts an injected spin flux into a transverse charge signal. Onsager reciprocity constrains direct and inverse linear-response coefficients after all time-reversal-odd variables, especially magnetization, are transformed consistently. It does not excuse ignoring open-circuit boundary conditions or sign conventions.

At a two-dimensional inversion-asymmetric interface, the Edelstein effect produces a nonequilibrium spin accumulation from an in-plane electric field. Its reciprocal converts an injected spin accumulation or flux into a two-dimensional charge current. This interfacial spin density is not the same object as a bulk transverse spin Hall current, even though both can generate similar torques.

A precessing magnet can emit spin angular momentum into an adjacent conductor. For a slowly varying unit magnetization, the pumped angular-momentum current per area is

Qspump=ℏ4π[gr↑↓m×m˙−gi↑↓m˙].\mathbf Q_s^{\mathrm{pump}} = \frac{\hbar}{4\pi} \left[ g_r^{\uparrow\downarrow} \mathbf m\times\dot{\mathbf m} - g_i^{\uparrow\downarrow} \dot{\mathbf m} \right].

Here gr↑↓g_r^{\uparrow\downarrow} and gi↑↓g_i^{\uparrow\downarrow} are the real and imaginary parts of the spin-mixing conductance per area in the stated convention. The receiving material develops a backflow spin accumulation; replacing the bare conductance by geff↑↓g_{\mathrm{eff}}^{\uparrow\downarrow} folds that backflow and spin loss into an effective interface parameter.

Spin pumping adds damping to a magnetic film:

Δα=∣γ∣ℏ4πMstFgeff↑↓.\Delta\alpha = \frac{ |\gamma|\hbar }{ 4\pi M_s t_F } g_{\mathrm{eff}}^{\uparrow\downarrow}.

Inverse spin Hall voltage, terahertz emission, or a nonlocal detector can register the emitted spin current. A linewidth increase alone is not unique proof of spin pumping: two-magnon scattering, radiative damping, eddy currents, inhomogeneous broadening, and magnetic proximity effects require controls.

Spin pumping and spin-transfer torque are reciprocal interfacial processes. One exports angular momentum from a moving magnet; the other absorbs angular momentum from an incident nonequilibrium spin distribution.

The Landau–Lifshitz–Gilbert equation with current-induced torques can be written

m˙=−∣γ∣μ0m×Heff+αm×m˙+τSTT+τSOT.\dot{\mathbf m} = - |\gamma|\mu_0 \mathbf m\times\mathbf H_{\mathrm{eff}} + \alpha \mathbf m\times\dot{\mathbf m} + \boldsymbol{\tau}_{\mathrm{STT}} + \boldsymbol{\tau}_{\mathrm{SOT}}.

For a spin flux polarized along p^\hat{\mathbf p} and absorbed by a uniform magnetic layer, the leading angular structures are

τDL=τDLm×(p^×m),\boldsymbol{\tau}_{\mathrm{DL}} = \tau_{\mathrm{DL}} \mathbf m\times \left( \hat{\mathbf p}\times\mathbf m \right),

and

τFL=τFLm×p^.\boldsymbol{\tau}_{\mathrm{FL}} = \tau_{\mathrm{FL}} \mathbf m\times\hat{\mathbf p}.

The first is called damping-like because its symmetry can oppose or reinforce Gilbert damping for a suitable trajectory. The second has the symmetry of precession about an effective field. The names describe vector form, not a unique microscopic origin.

For charge-equivalent injected spin current, a common damping-like coefficient is

τDL=∣γ∣ℏ2eMstFξDLjc,\tau_{\mathrm{DL}} = \frac{ |\gamma|\hbar }{ 2eM_s t_F } \xi_{\mathrm{DL}}j_c,

where ξDL\xi_{\mathrm{DL}} includes conversion and transmission. For a spin valve, p^\hat{\mathbf p} is set by a polarizing magnetic layer and the torque is usually called spin-transfer torque. In a spin–orbit bilayer, p^\hat{\mathbf p} can be generated by the spin Hall or Edelstein effect and the torque is usually called spin–orbit torque.

In a smoothly varying magnetic texture, current within the magnet also produces adiabatic and nonadiabatic torques:

τtexture=−(u⋅∇)m+βnam×[(u⋅∇)m].\boldsymbol{\tau}_{\mathrm{texture}} = - (\mathbf u\cdot\boldsymbol{\nabla})\mathbf m + \beta_{\mathrm{na}} \mathbf m\times \left[ (\mathbf u\cdot\boldsymbol{\nabla})\mathbf m \right].

The drift parameter u\mathbf u is proportional to current polarization, and βna\beta_{\mathrm{na}} is a nonadiabatic coefficient. This continuum form assumes a texture smooth on microscopic transport scales.

A macrospin switching estimate follows by balancing antidamping torque against magnetic damping:

jccrit∼2eℏαMstFξDLμ0Heff.j_c^{\mathrm{crit}} \sim \frac{ 2e }{ \hbar } \frac{ \alpha M_s t_F }{ \xi_{\mathrm{DL}} } \mu_0H_{\mathrm{eff}}.

Its coefficient depends on geometry, demagnetizing fields, pulse duration, temperature, incubation, and the angular dependence of torque. Real switching often proceeds by domain nucleation and wall motion rather than coherent rotation. A quoted critical current without pulse width and error probability is incomplete.

No single figure of merit ranks all spintronic materials. A useful ledger includes:

PlatformMain functionUseful attributesFrequent limitation
Metallic ferromagnet/nonmagnetinjection, GMR, spin torquehigh current density, mature interfacesshort λs\lambda_s, Joule heating
Magnetic tunnel junctionTMR readout, STT switchinglarge resistance contrast, nonvolatilitybarrier defects, write stress, stochastic switching
Heavy spin–orbit metal or semimetalspin Hall generation and inverse detectionefficient charge–spin conversionshunting, resistive loss, interface uncertainty
Semiconductor or two-dimensional channelgate control, long-distance transporttunable density and spin–orbit couplingcontact mismatch, disorder, environmental sensitivity
Magnetic insulatormagnon transport, spin pumpingnegligible electronic charge current in magnetinterface conversion and magnon relaxation
Antiferromagnet or ferrimagnetfast dynamics, compensated or low-moment operationweak stray fields, rich torque symmetryreadout, domain control, material variability

Metallic spin valves and GMR multilayers enabled compact magnetic-field sensors and hard-disk read heads. A magnetic tunnel junction uses TMR to distinguish a free layer from a reference layer. In spin-transfer-torque MRAM, the current used to read the tunnel junction also passes through it during writing. In many spin–orbit-torque designs, a lateral current in an adjacent layer writes a magnetic element while the tunnel junction provides a separate read path.

The magnetic energy barrier must satisfy

Δ≡EbkBT\Delta \equiv \frac{E_b}{k_BT}

large enough for retention, while write torque must still cross the barrier quickly and reliably. Magnetic Anisotropy owns the barrier, anisotropy, and thermal-activation ledger. Lowering EbE_b reduces write cost but also retention; increasing damping can accelerate settling while raising antidamping current.

Other platforms extend the same generation–transport–manipulation–detection logic:

  • semiconductor spin transistors seek electrical control of precession and injection;
  • graphene and other two-dimensional channels offer long transport lengths in selected regimes but are contact-sensitive;
  • magnonic devices transport angular momentum without electronic charge flow through the magnetic insulator;
  • antiferromagnetic devices exploit Néel-order dynamics and symmetry-selective readout;
  • spin caloritronics couples spin transport to heat and thermoelectric response;
  • spintronic terahertz emitters convert ultrafast spin flow into broadband charge transients.

“Low power” is not a material property. Energy per successful operation must include line resistance, pulse duration, capacitive loading, write errors, standby leakage, peripheral circuitry, and the cost of maintaining the required field or symmetry breaking.

A defensible spin-transport claim usually follows this sequence:

  1. Define every axis and normalization. Draw jc\mathbf j_c, spin-flow direction, spin polarization, interface normal, detector voltage, and magnetic order.
  2. Establish the charge baseline. Measure ordinary resistance, Hall response, current distribution, shunting, and thermoelectric backgrounds.
  3. Determine magnetic state independently. Hysteresis alone may not identify which layer or domain switched.
  4. Reverse controlled variables. Compare current, field, injector, detector, magnetization, and sample-normal reversals against the predicted parity.
  5. Fit a transport model with geometry. Contact width, spin absorption, finite thickness, and multidimensional diffusion can matter.
  6. Cross-calibrate material parameters. Resistivity, λs\lambda_s, MstFM_st_F, damping, anisotropy, and interface conductance should not all float unconstrained.
  7. Use reciprocal or orthogonal detection when possible. Direct and inverse conversion, nonlocal and local signals, or torque and pumping measurements test different parts of the ledger.
  8. Report uncertainty and model dependence. A torque efficiency extracted from one geometry is not automatically a universal bulk constant.

For torque measurements, spin-torque ferromagnetic resonance and harmonic Hall analysis can separate angular symmetries, but neither is artifact-free. Oersted fields, anomalous Nernst signals, spin Seebeck response, planar Hall mixing, nonlinear resistance, current crowding, and linewidth broadening need symmetry and thickness controls.

MistakeWhy it failsBetter practice
Calling every polarized flow a pure spin currentA spin-polarized charge current carries net chargeReport both jc\mathbf j_c and Qi aQ_i^{\,a}
Omitting ℏ/2e\hbar/2eAngular-momentum and charge-equivalent currents have different unitsState the normalization with every conversion ratio
Identifying λs\lambda_s with a mean free pathSpin diffusion combines momentum diffusion and spin relaxationReport DsD_s, τs\tau_s, and the model used
Using bulk polarization as injection polarizationInterface and channel spin resistances reshape the currentSolve or fit the boundary-value problem
Calling any magnetic resistance change GMRAMR, GMR, TMR, CMR, and spin Hall magnetoresistance have different state variablesIdentify the magnetic configuration and current path
Equating torque efficiency with spin Hall angleInterface transmission, backflow, and shunting interveneReport the full extraction model
Treating a linewidth increase as unique evidence of pumpingSeveral extrinsic processes broaden resonanceUse thickness, reference-sample, and inverse-detection controls
Inferring coherent switching from a macrospin thresholdNucleation, walls, heat, and stochasticity can dominateImage or otherwise constrain the reversal pathway
Quoting a sign without axesCurrent, electron flow, normal, and spin axes may differDraw the handed geometry
Calling a proposed device low power from current density aloneEnergy also depends on voltage, duration, errors, and circuitryReport energy per successful operation and retention

A one-dimensional nonmagnetic channel receives a localized steady spin source at x=0x=0. Away from the source,

d2μsdx2=μsλs2,\frac{\mathrm d^2\mu_s}{\mathrm dx^2} = \frac{\mu_s}{\lambda_s^2},

and μs\mu_s must remain finite as x→±∞x\to\pm\infty. Find the profile if μs(0)=μ0\mu_s(0)=\mu_0. What detector spacing reduces the signal to 1/e1/e of its interfacial value?

Solution

On the right, finiteness removes the growing exponential; on the left it removes the exponential that grows toward negative infinity. Continuity at the injector gives

μs(x)=μ0e−∣x∣/λs.\mu_s(x) = \mu_0 e^{-|x|/\lambda_s}.

The ratio at a detector a distance LL away is

μs(L)μs(0)=e−L/λs.\frac{\mu_s(L)}{\mu_s(0)} = e^{-L/\lambda_s}.

It equals 1/e1/e at

L=λs.L=\lambda_s.

The derivative jumps at x=0x=0 because the idealized injector is a delta-function source. A finite-width injector smooths that cusp.

Use

Pinj=PFrF+PcrcrF+rN+rcP_{\mathrm{inj}} = \frac{ P_Fr_F+P_cr_c }{ r_F+r_N+r_c }

to evaluate the transparent-contact and tunnel-contact limits. Explain why a very large rcr_c is not always the best device choice.

Solution

For a transparent contact, rc→0r_c\to0:

Pinj→PFrFrF+rN.P_{\mathrm{inj}} \to \frac{P_Fr_F}{r_F+r_N}.

If rN≫rFr_N\gg r_F, then

Pinj≃PFrFrN≪PF.P_{\mathrm{inj}} \simeq P_F\frac{r_F}{r_N} \ll P_F.

This is conductivity mismatch. If a spin-selective contact dominates,

rc≫rF,rN,r_c\gg r_F,r_N,

then

Pinj→Pc.P_{\mathrm{inj}}\to P_c.

However, at fixed applied voltage the charge current falls as contact resistance grows. A large rcr_c can also limit bandwidth and transfer most Joule heating or voltage stress to the barrier. The optimum depends on whether the constraint is current, voltage, power, bandwidth, or signal-to-noise ratio.

Derive the parallel and antiparallel resistances of the symmetric two-layer model and show that RAP≥RPR_{\mathrm{AP}}\ge R_P.

Solution

In the parallel state, the two channel resistances are 2R↑2R_\uparrow and 2R↓2R_\downarrow in parallel:

1RP=12R↑+12R↓.\frac{1}{R_P} = \frac{1}{2R_\uparrow} + \frac{1}{2R_\downarrow}.

Therefore

RP=2R↑R↓R↑+R↓.R_P = \frac{ 2R_\uparrow R_\downarrow }{ R_\uparrow+R_\downarrow }.

In the antiparallel state, each channel has series resistance R↑+R↓R_\uparrow+R_\downarrow, and the two equal channels are in parallel:

RAP=R↑+R↓2.R_{\mathrm{AP}} = \frac{ R_\uparrow+R_\downarrow }{ 2 }.

Their difference is

RAP−RP=(R↑−R↓)22(R↑+R↓)≥0.R_{\mathrm{AP}}-R_P = \frac{ (R_\uparrow-R_\downarrow)^2 }{ 2(R_\uparrow+R_\downarrow) } \ge0.

Equality holds only when the two spin channels scatter identically. The proof applies to the stated resistor model, not automatically to every nonlinear or quantum-coherent device.

Take g=2.0g=2.0 and τs=1.0 ns\tau_s=1.0\,\mathrm{ns}. Estimate the magnetic field at which ∣ΩL∣τs=1|\Omega_L|\tau_s=1, using μB/ℏ≃8.79×1010 s−1T−1\mu_B/\hbar\simeq8.79\times10^{10}\,\mathrm{s^{-1}T^{-1}}.

Solution

The Larmor frequency is

∣ΩL∣=∣g∣μBℏ∣B∣.|\Omega_L| = \frac{|g|\mu_B}{\hbar}|B|.

Hence

∣B∣=ℏ∣g∣μBτs≃1(2.0)(8.79×1010 s−1T−1)(1.0×10−9 s).|B| = \frac{\hbar}{|g|\mu_B\tau_s} \simeq \frac{1}{ (2.0) (8.79\times10^{10}\,\mathrm{s^{-1}T^{-1}}) (1.0\times10^{-9}\,\mathrm s) }.

Thus

∣B∣≃5.7×10−3 T=5.7 mT.|B| \simeq 5.7\times10^{-3}\,\mathrm T = 5.7\,\mathrm{mT}.

This is only a characteristic scale. Diffusive travel-time dispersion, contact absorption, and anisotropic relaxation shape the full curve.

5. Charge-equivalent and angular-momentum currents

Section titled “5. Charge-equivalent and angular-momentum currents”

A bilayer carries jc,x=8.0×1010 A m−2j_{c,x}=8.0\times10^{10}\,\mathrm{A\,m^{-2}} and has θSH=0.12\theta_{\mathrm{SH}}=0.12 in the convention js,z y=θSHjc,xj_{s,z}^{\,y}=\theta_{\mathrm{SH}}j_{c,x}. Find js,z yj_{s,z}^{\,y} and Qz yQ_z^{\,y}.

Solution

The charge-equivalent spin-current density is

js,z y=(0.12)(8.0×1010)=9.6×109 A m−2.j_{s,z}^{\,y} = (0.12) (8.0\times10^{10}) = 9.6\times10^9\, \mathrm{A\,m^{-2}}.

The angular-momentum-current density is

Qz y=ℏ2ejs,z y.Q_z^{\,y} = \frac{\hbar}{2e} j_{s,z}^{\,y}.

Using ℏ/(2e)≃3.29×10−16 J s C−1\hbar/(2e)\simeq3.29\times10^{-16}\,\mathrm{J\,s\,C^{-1}},

Qz y≃3.16×10−6 J m−2.Q_z^{\,y} \simeq 3.16\times10^{-6}\, \mathrm{J\,m^{-2}}.

Since J\mathrm J equals angular momentum per unit time, this is equivalently angular momentum per area per time. The numerical values differ by the dimensional factor ℏ/2e\hbar/2e; neither should be quoted without units.

A ferromagnetic film of thickness tFt_F shows a damping increase Δα\Delta\alpha after adding a normal-metal layer. Solve the spin-pumping formula for geff↑↓g_{\mathrm{eff}}^{\uparrow\downarrow}. How should the result scale with tFt_F if the interface is unchanged?

Solution

From

Δα=∣γ∣ℏ4πMstFgeff↑↓,\Delta\alpha = \frac{ |\gamma|\hbar }{ 4\pi M_st_F } g_{\mathrm{eff}}^{\uparrow\downarrow},

one obtains

geff↑↓=4πMstF∣γ∣ℏΔα.g_{\mathrm{eff}}^{\uparrow\downarrow} = \frac{ 4\pi M_st_F }{ |\gamma|\hbar } \Delta\alpha.

For a thickness-independent interface,

Δα∝1tF.\Delta\alpha \propto \frac{1}{t_F}.

A nonzero intercept or a different thickness law can indicate bulk damping changes, magnetic dead layers, two-magnon scattering, radiative effects, or thickness-dependent material quality. It should not automatically be assigned to spin pumping.

In a uniaxial macrospin model, suppose Eb=KeffVE_b=K_{\mathrm{eff}}V and

jccrit∝αMstFξDLHeff,Heff∝KeffMs.j_c^{\mathrm{crit}} \propto \frac{ \alpha M_st_F }{ \xi_{\mathrm{DL}} } H_{\mathrm{eff}}, \qquad H_{\mathrm{eff}} \propto \frac{K_{\mathrm{eff}}}{M_s}.

At fixed geometry and material parameters other than KeffK_{\mathrm{eff}}, explain how reducing anisotropy changes retention and the idealized critical current.

Solution

The thermal-stability factor is

Δ=KeffVkBT.\Delta = \frac{ K_{\mathrm{eff}}V }{ k_BT }.

At fixed VV and TT, reducing KeffK_{\mathrm{eff}} lowers Δ\Delta linearly and therefore shortens retention exponentially in an Arrhenius model.

Because

Heff∝KeffMs,H_{\mathrm{eff}} \propto \frac{K_{\mathrm{eff}}}{M_s},

the idealized macrospin threshold also falls linearly with KeffK_{\mathrm{eff}}:

jccrit∝αtFξDLKeff.j_c^{\mathrm{crit}} \propto \frac{ \alpha t_F }{ \xi_{\mathrm{DL}} } K_{\mathrm{eff}}.

Lower anisotropy therefore eases writing while degrading retention. In a real nanomagnet, edge damage, nonuniform reversal, pulse length, temperature rise, and error-rate requirements can change the apparent scaling.

  • Density and Current Operators develops microscopic particle, charge, energy, and spin-current continuity equations.
  • Spin–Orbit Coupling in Solids owns Rashba, Dresselhaus, intrinsic, skew-scattering, and side-jump mechanisms.
  • Boltzmann Transport supplies the semiclassical collision and relaxation framework beneath diffusive conduction.
  • Hall Effect provides the charge-response tensor, sign, multiband, and inference baseline.
  • Ferromagnetism develops magnetic order, domains, hysteresis, and magnetic thermodynamics.
  • Magnetic Anisotropy connects crystal, shape, and interface energies to retention and switching fields.
  • Antiferromagnetism develops compensated order, fast dynamics, and antiferromagnetic control channels.
  • Ferrimagnetism treats compensation points and low-angular-momentum dynamics.
  • Spin Waves and Magnons owns quantized magnetic excitations, while spintronics uses interfaces to launch and detect them.
  • Skyrmions and Magnetic Textures applies current-induced torque to domain walls, vortices, skyrmions, and their gyroscopic motion.
  • Kubo Formula gives the linear-response framework behind conductivity and reciprocal conversion coefficients.
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