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Spin polarization engineering in d-wave altermagnets

Mohsen Yarmohammadi, 1, ∗ Marco Berritta, 2 Marin Bukov, 3 Libor Šmejkal, 3, 4, 5 Jacob Linder, 6 and Peter M. Oppeneer 2 1 Department of Physics, Georgetown University, Washington DC 20057, USA Department of Physics and Astronomy, Uppsala University, Box 516, SE-75120 Uppsala, Sweden 3 Max Planck Institute for the Physics of Complex Systems, Nöthnitzer Str. 38, 01187 Dresden, Germany

4 Max Planck Institute for Chemical Physics of Solids, Nöthnitzer Str. 40, 01187 Dresden, Germany

5 Institute of Physics, Czech Academy of Sciences, Cukrovarnická 10, 162 00 Praha 6, Czech Republic 6 Center for Quantum Spintronics, Department of Physics, Norwegian University of Science and Technology, NO-7491 Trondheim, Norway

(Dated: October 6, 2025)

arXiv:2510.02452v1 [cond-mat.mtrl-sci]

2

Oct 2025

2 Altermagnets host unconventional spin-polarized bands despite zero net magnetization, but controlling their spin structure remains challenging. We propose a multi-field approach to engineer spin polarization in d-wave altermagnets using gating, optical driving, and in-plane electric fields, which enable tunable and switchable polarizations along multiple directions. Optical driving induces out-of-plane (z) polarization, while gating and in-plane fields generate x- and y-polarizations via the Edelstein effect, all of which are experimentally detectable. We further find that spin- and band-selective doping induces chiral optical activity, a feature unique to altermagnets. Our approach provides a versatile route for full control of spin polarization in altermagnets.

Introduction.—Altermagnets are a new class of magnetic materials [1–4] that break the traditional division between ferromagnets and antiferromagnets and exhibit unconventional properties [1–12]. Despite zero net magnetization, their spin symmetries and nonrelativistic electronic structure yield symmetry-protected, alternating spin polarization in momentum space. Spin-

nating spin polarization in momentum space. Spin-
momentum locking can appear in d-, g-, or i-wave

forms [1–3, 6, 8, 13], with d-wave altermagnets predicted to host unusual current-driven spin effects, including exotic spin torques, spin-orbit torques, and spin-splitter currents [10, 14–18].

Initial experimental indications of altermagnetic properties and functionalities were reported [19–23], however, precise control of their spin polarization remains a key challenge for spintronics. Previous static approaches—strain, doping, or (anti)ferroelectric tuning [24–32]—can face limits such as lattice instabilities and poor tunability, while dynamical methods provide greater flexibility [33–39]. Specifically, Floquet engineering, using periodic driving to modify quantum systems [33–35, 40], can reshape band structures and spin textures [41–44], enabling non-equilibrium spin transport.

The spin Edelstein effect (generation of a nonequilibrium spin polarizations from an applied electric field in systems with spin-orbit coupling (SOC)) [45– 48] usually relies on SOC and spin-momentum locking, while the orbital Edelstein effect can occur even without SOC [49–54]. Recently, an out-of-plane electric field was shown to generate altermagnetic spin polarization in certain monolayer antiferromagnets [55]. Additionally, various current-induced spin polarization effects were proposed, including relativistic variants in altermagnetic interfaces [56], nonrelativistic variants in bulk altermagnets [57], p-wave antialtermagnets [58–60], and chiral spin-textured magnets [61].

In this Letter, we propose a multi-field platform, absent in the previous proposals, for more complete control of spin polarization in two-dimensional (2D) d-wave altermagnets. The method unifies electrostatic gating, optical driving, and in-plane electric fields. Gating induces Rashba spin-orbit coupling (RSOC) [37, 38, 55, 62, 63], while circularly polarized light (CPL) generates anisotropic spin textures and spin polarization

erates anisotropic spin textures and spin polarization
along z-direction [37, 38]. In addition, in-plane elec-

tric fields produce spin Edelstein polarizations along xand y-directions. Proposed materials include thin films of d-wave altermagnets KV 2 Se 2 O [18], RbV 2 Te 2 O [64], RuO 2 [5, 10, 21, 65], and κ-CL [7], noting RuO 2 remains debated.

Without CPL, gating and in-plane electric fields generate spin Edelstein polarizations of opposite sign along xand y-directions. Adding CPL breaks this reversal symmetry, yielding strongly anisotropic polarizations. We demonstrate large, tunable, and switchable spin polarizations enabled by light-controlled band topology [66] and symmetry breaking, offering a route to full spin control in altermagnets. Intrinsic altermagnetic order can also generate chiral optical activity under spin-selective doping, opening routes to spin-resolved photonic technologies [64, 67, 68].

Effective Hamiltonian model.—We consider a 2D Rashba d-wave altermagnet, as illustrated in Fig. 1(a), for both d x 2 −y 2 and d xy pairing symmetries [69], described by the Hamiltonian

HR⃗ k = ℏ2 (k2x + k2y ) 2me σ0 + h(⃗k ) σz + λ (kx σ y − ky σx ) , (1)

2

(a) (d ) ( c) ( b) (d) (c) (b) FIG. 1. (a) Schematic of a two-dimensional d-wave alter- magnet gated by ±V electrodes and illuminated by circularly polarized light (CPL, gold colored spiral). (b) Spin-resolved Fermi contours for pristine spin-up (red) and spin-down (blue) states. (c) Gating induces Rashba spin-orbit coupling, re- shaping the Fermi surface while maintaining spin balance. (d) CPL breaks this balance, generating anisotropic spin tex- Top and bottom gate electrodes with voltages ±V are included to emulate a realistic device setup. They intro- duce R SOC with st rength λ, which couples spin and mo- mentum, breaks inversion symmetry, and modifies spin splitting [37, 62, 63]. We next introduce a time-periodic vector potential for right-handed CPL, ⃗A(t) = Ad [ sin(Ωd t ), cos(Ωd t )], with driving frequency Ωd and amplitude Ad . Minimal coupling ⃗k → ⃗k − e ℏ ⃗A(t) makes the Hamiltonian time- p eriodic, HR⃗k (t)( t + T ) = HR ⃗k (t)( t) with T = 2π/Ωd (see Appendix A). In the high-frequency regime (ℏΩd ≈ 1 eV), an effective time-independent Floquet Hamiltonian is obtained via van Vleck expansion [37, 70–73]:

tures. CPL engineers out-of-plane polarization ⟨ Ŝ z ⟩ via Floquet drives, while gating and in-plane fields (E x , E y ) allow tunable and switchable control of in-plane ⟨ Ŝ x ⟩ and ⟨ Ŝ y ⟩ via the Edelstein effect. The spin polarizations are noncollinear.

where h(⃗k ) = ℏ2 D(k2x − k2y ) 2me or ℏ2 Dkx k y me , with me the elec- tron mass. The parameters 0 < D or D ≤ 1 characterize

the strength of the d x 2 −y 2 or d xy altermagnets, respectively, while ⃗σ (σ 0 ) represents the Pauli vector (identity matrix).

He ff ⃗ k ≈ HF0 (⃗k ) + [HF− 1( ⃗k ), HF+ 1( ⃗k )] ℏΩd ,

(2)

with Floquet components ν = {−1, 0, +1}: HFν (⃗k ) = 1 T T 0 HR⃗ k− e ℏ ⃗A(t)( t)ei νΩd t dt . (3)

We define A = eA d /ℏ and light-induced exchange potential ∆ = λ 2 A 2 /ℏΩ d . To leading order, we obtain the effective Hamiltonians

He ff,d x2 − y2 ⃗ k ≈ ℏ2 (k2x + k2y ) 2me + ℏ3 Ωd ∆ 2 me λ2 σ0 + ℏ2 D(k2x − k2y ) 2me + ∆ σz + λ 1 − ℏ2 ∆ D me λ2 kx σ y − 1 + ℏ2 ∆ D me λ2 ky σx , (4a) He ff,dx y ⃗ k ≈ ℏ2 (k2x + k2y ) 2me + ℏ3 Ωd ∆ 2 me λ2 σ0 + ℏ2 D kx ky me + ∆ 2 σz +λ 1 − ℏ2 ∆ D 2 me λ2 ky kx kx σ y − 1 − ℏ2 ∆ D 2 me λ2 kx ky ky σx . (4b)

In both Hamiltonians, the first term proportional to Ω d ∆σ 0 leads to a uniform energy shift—chemical potential. An additional constant spin splitting arises from the term ∆σ z (i.e., light-induced magnetization: the inverse Faraday effect [74–78]), which can shift the band structure and tune the strength of the altermagnetic order.

We note that the light-induced magnetization scales quadratically with the amplitude of the light field [74, 75]. In the d x 2 −y 2 -wave pattern, the RSOC terms are modified by ∆D, whereas in the d xy -wave pattern, a RashbaDresselhaus-type SOC emerges. Note that the d xy -wave pattern corresponds to a 45 ◦ rotation of the d x 2 −y 2 -wave pattern in both momentum and spin space.

For left-handed CPL, we employ Ω d → −Ω d , flipping the x-component of the vector potential. This reverses the magnetization term proportional to ∆ [74, 77] and inverts the RSOC anisotropy in d x 2 −y 2 -wave and the Dresselhaus SOC amplitude in d xy -wave patterns.

Since RSOC shows stronger anisotropy in the d x 2 −y 2 - than in the d xy -wave pattern, we focus on d x 2 −y 2 -wave altermagnets for highly tunable spin polarizations. It is convenient to express the effective Hamiltonian as

is convenient to express the effective Hamiltonian as He ff,dx 2 − y2 ⃗k = d0 ( k) σ0 + ⃗d(⃗k ) · ⃗σ, with eigenenergies

⃗k 0 0 ε ±⃗k = d0 ( k) ± | ⃗ d (⃗k )| and eigenstates |u ±⃗k ⟩ describing

spin-split bands. Figures 1(b)–(d) show the evolution of

spin-split bands. Figures 1(b)–(d) show the evolution of spin textures, ⟨u ±⃗k |σz |u ±⃗k ⟩, in a dx 2 −y2 -wave altermag-

net as time-reversal and inversion symmetries are sequentially broken: pristine, gated/RSOC, and under CPL.

In Fig. 1(b), without RSOC or optical driving, spin-split Fermi contours (corresponding to out-of-plane spins) are antisymmetric under C 4 rotations. Timereversal symmetry breaking remains, giving zero net magnetization despite nontrivial momentum-resolved spin textures. In Fig. 1(c), RSOC breaks inversion symmetry, distorting contours while preserving C 4 symmetry. In Fig. 1(d), CPL also breaks time-reversal symmetry, 3 inducing net z-polarized magnetization, enhancing spin contrast, and driving Floquet band reconstruction.

While CPL in combination with gating generates anisotropic in-plane spin textures [37], CPL alone does not create in-plane spin polarizations. Adding in-plane electric fields completes the scheme for engineering spin polarization across multiple components. These polarizations are mainly governed by the Edelstein effect, as noted in the introduction.

Edelstein effect.—In non-centrosymmetric systems with SOC, an applied electric field can induce a nonequilibrium spin or orbital polarization—known respectively as the spin Edelstein effect and orbital Edelstein effect or Rashba-Edelstein effect [49, 51, 53]. Within linear response theory, the expectation value of an observable Ô ℓ (ℓ ∈ {x, y, z}) as a linear response to an in-plane j electric field

PE

jalong direction j ∈ {x, y} is given by ℓ ⟨ Ô ⟩ =

j χ ℓj E , where χ ℓj is the Edelstein response tensor (susceptibility). For the spin Edelstein effect, Ô ℓ = ℏσ ℓ /2 (spin operator), while for the orbital Edelstein effect, Ô ℓ = L̂ ℓ (orbital angular momentum, see below). Using the Kubo formula, χ ℓj reads as [54, 79]

χℓ j = ie me d2 k (2π)2 n ∂f n⃗k ∂ε n⃗k Oℓ nn,⃗k pj nn,⃗k iτ −1 i ntra − n̸= m f n⃗k − f m⃗k ε n⃗k − ε m⃗k Oℓ mn,⃗k pj nm,⃗k ε m⃗k − ε n⃗k + iτ −1 i nter , (5)

where n = ± is the spin band index, f n⃗k is the corresponding Fermi-Dirac distribution, τ intra (τ inter )

corresponding Fermi-Dirac distribution, τi ntra (τi nter) is the intraband (interband) lifetime, Oℓ mn,⃗k = ⟨u m⃗k | ˆ O ℓ |u n⃗k ⟩, and pj nm,⃗k = me ⟨ u n⃗k |ˆvj |u m⃗k ⟩, where ˆvj = ℏ− 1 ∂He ff,dx 2 − y2 ⃗ k /∂k j is the velocity operator. In Eq. (5), the first term reflects intraband contributions, and the

second captures interband coherence.

There are two ways to compute induced responses. One way starts from the unperturbed Hamiltonian and treats both light and in-plane fields perturbatively, requiring linear and quadratic corrections to the electric field—often cumbersome. Our simpler approach uses the dressed Hamiltonian, already incorporating CPL effects, on which we directly compute the Edelstein responses.

Our model applies only at temperatures well below the energy cutoff of the effective theory; at higher T , thermal excitations may access neglected high-energy scales. We thus focus on low T , where the approximation is valid.

thus focus on low T , where the approximation is valid. As T → 0, ∂f /∂ε → −δ(ε − µ), with µ the chemical po-

tential (tunable within spin bands, analogous to doping), yielding the intraband contribution

χi ntra ℓ j = − eτi ntra m d2 k (2π)2 n δ(ε n⃗k − µ) Oℓ nn,⃗k pj nn,⃗k .

(6)

While the atom-centered approximation is commonly employed to study the orbital Edelstein effect in bulk magnetic materials and full-band models [51, 80, 81], in few-band models—particularly two-band—the orbital moment can be expressed as [82, 83]

⃗L mn⃗k = i⟨∇⃗ k u m⃗k | × He ff,dx 2 − y2 ⃗k − ε n⃗k |∇⃗ k u n⃗k ⟩ . (7)

This formulation captures the internal angular momentum of Bloch wavepackets, which is primarily governed by the Berry curvature of the bands.

The complete spin and orbital ingredients of the Edelstein effect are presented in Appendix B.

Results and discussion.—In the following, we first consider an ideal d x 2 −y 2 altermagnet with D = 1 and weak gate-induced RSOC λ = 0.2 eV·Å. We then tune D and λ to study responses to light potentials ∆ and inplane fields (E x , E y ). Two doping levels are set by

plane fields (E , E ). Two doping levels are set by µ = ε± = ε ±,⃗k=0, the band edges at ⃗k = 0, where state

degeneracy and spin polarizations peak in the pristine phase. We note that when µ lies within spin bands, the main conclusions remain valid. We use k B T ≈ 1 meV and normalize the Edelstein susceptibility by χ 0 = e/4π 2 with natural units e = ℏ = m e = 1. Intraband and in-

with natural units e = ℏ = me = 1. Intraband and in- terband lifetimes τ −1 i ntra and τ −1 i nter are set to 0.5 eV, an ac-

ceptable value for metallic systems [49, 79], noting longer lifetimes enhance spin polarizations but do not alter qualitative trends. We also emphasize that numerical and analytical results (Appendix B) agree perfectly, thus, duplicate plots are omitted. We use ∆ > 0 for right-handed and ∆ < 0 for left-handed CPL.

Owing to the d x 2 −y 2 -wave symmetry of our model, the generation of orbital polarizations—both in-plane and out-of-plane—is negligible with and without gating or CPL, as the orbital responses to in-plane electric fields cancel out with opposite signs along different momentum directions, as confirmed by the orbital results shown in Fig. 2.

Under CPL illumination, spin polarization arises along z. We focus on the Edelstein effect to study in-plane polarizations induced by x- and y-directed electric fields. By mirror symmetry in the z direction (reflection about the plane), the in-plane Edelstein effect cannot generate z-polarization (Fig. 2), but it induces in-plane polarizations that are strongly reshaped anisotropically under combined gating and optical driving.

While we focus on the dominant off-diagonal (transverse) susceptibility components, the longitudinal components (χ xx and χ yy ) show similar behavior (dark gray and yellow curves in Fig. 2(a) and 2(b)).

Figure 2 reveals the light-induced evolution of the spin and orbital Edelstein effects as functions of the light potential ∆ in a 2D d x 2 −y 2 -wave Rashba altermagnet. In the absence of light (∆ = 0), the inherent spin textures enforce antisymmetric susceptibilities independent 4

IG. 2. Calculated spin (‘s’) and orbital (‘o’) Edelstein sus- arises from light-modified band velocities and spin tex- tures rather than virtual transitions. In particular, the induced spin polarizations along x and y, given by χx y and χy x, vanish at critical light potentials (insets of Fig. 2), depending on CPL helic- ity. From modified RSOC components in Eq. (4a), (λx , λy ) = (λ − ℏ2 ∆D mλ , λ + ℏ2 ∆D mλ ), χx y vanishes under RCPL at λx = 0, while χy x vanishes under LCPL at λy = 0. The critical light potential is then ∆±c ≈± m λ2 ℏ2 D , (10) where + and − stand for right and left light helicity, respectively. For ℏΩd ≈ 1 eV and D = 1, the criti-

χx y (∆ = 0, µ ̸= 0) = −χy x( ∆ = 0, µ ̸= 0) → ⟨ ˆ S x ⟩ = −⟨ ˆ S y ⟩ .

⟨S ⟩ and ⟨S ⟩ arise under in-plane electric fields, pro- ducing antisymmetric x- and y-polarizations. Combined

⟨ ˆ S x ⟩ ⟨ ˆ S y ⟩ = χx x χx y −χx y −χx x Ex Ey . (9)

(Fig. 2). At this value, in-plane spin polarizations switch off and then reverse due to a sign change in spin susceptibilities. The corresponding critical vector potential is

tibilities. The corresponding critical vector potential is Ac ≈ ±0.377 Å− 1 and critical field Ec0 ≈ 3.7 V/nm, in-

dependent of µ. While experimentally challenging, these values are achievable with current ultrafast lasers [84], though real setups involve losses not captured in a zerotemperature free-standing model [84, 85].

Following the analysis of the spin Edelstein components at finite doping (µ ̸ = 0) in Fig. 2, when light is present (∆ ̸ = 0), we find

χx y (∆ < 0, µ = ε− ) = − χy x( ∆ > 0, µ = ε+ ) , (11a) χx y (∆ > 0, µ = ε− ) = − χy x( ∆ < 0, µ = ε+ ) , (11b)

revealing a chiral antisymmetry between the spin-up and spin-down bands. This antisymmetry stems from inversion symmetry of spin components and light helicity acting oppositely on different spins, a phenomenon we term the chiral optical activity. This behavior is unique to altermagnets, as non-altermagnetic systems lack the pa-

altermagnets, as non-altermagneticsy
rameter D in light-modified RSOCs.

The full control mechanism, combining gating, CPL, and in-plane electric fields, becomes now evident. In a nutshell, the effects of RCPL and LCPL (σ + for RCPL and σ − for LCPL) when doping spin band (σ for spin-up and −σ for spin-down) are given by the following chiral features

⟨ ˆ S x ⟩ ⟨ ˆ S y ⟩ = χx x( σ± , σ) χx y (σ± , σ) −χx y (σ∓ , −σ) −χx x( σ∓ , −σ) Ex Ey ,

(12)

enabling highly tunable in-plane spin polarizations in altermagnets. We stress that the d x 2 −y 2 -wave symmetry in altermagnets forbids out-of-plane (z) spin polarization via the Edelstein effect, which can only be induced directly by CPL.

Next, we examine how gate voltage, or gate-induced RSOC, affects spin Edelstein polarizations (Fig. 3). Susceptibilities increase with λ, enhancing polarizations.

5

FIG. 3. Calculated transverse spin susceptibilities χ xy /χ 0 (blue) and χy x/ χ0 (red) versus RSOC λ in an ideal altermag- net (D = 1) for various light potentials: ∆ = 0 (solid), +3.2 meV (dashed), and −3.2 meV (dotted). Panel (a): µ = ε− at ⃗k = 0 for the spin-down band; panel (b): µ = ε + at ⃗k = 0 for the spin-up band. Chiral optical activity from combined light and in-plane fields is independent of finite RSOC.

Without light (∆ = 0), the system retains antisymmetric spin susceptibility, χ xy = −χ yx , confirmed by solid curves in Fig. 3. Introducing CPL (∆ ̸ = 0) breaks this antisymmetry for all λ, depending on light helicity and doping.

oping. At µ = ε− (Fig. 3(a)), RCPL (∆ = +3.2 meV, dashed)

largely preserves antisymmetry, like the undriven case. In contrast, LCPL (∆ = −3.2 meV, dotted) induces pronounced anisotropy between χ xy and χ yx , showing helical light-spin coupling enhancing one spin texture. At µ = ε + (Fig. 3(b)), the effect is similar but with reversed curvature, reflecting opposite upper-band spin polarization. The susceptibility components no longer mirror each other under CPL, evidencing breakdown of response reciprocity with helicity reversal (cf. Fig. 2).

Notably, Eq. (8) implies that the crossing point at which χ xy and χ yx vanish and spin polarization is reversed, remains fixed and is not shifted by RSOC. These

observations across varying RSOC strengths reinforce our claim regarding the robustness of the chiral optical re- FIG. 4. Calculated spin susceptibilities χx y (a) and χy x (b) for doping into the spin-up band (µ = ε+ ) with weak RSOC λ = 0.2 eV·Å. For spin-down doping (µ = ε − ) , the behaviors reverse. Both components are plotted versus light potential ∆ and altermagnetism D, illustrating highly tunable CPL- induced spin polarizations and the critical phase boundary where polarizations switch. can be increased by stronger gating (Fig. 3) or purer ma- terials with smaller inverse lifetimes than 0.5 eV. For experimental setups, one can use heterostruc- tures of thin films grown epitaxially on substrates (e.g., TiO2 for RuO2 [87]) to achieve 2D-like behavior, with top/bottom gates (e.g., high-κ dielectrics) induc- ing RSOC in van der Waals heterostructures. Circularly polarized mid-infrared or terahertz pulses (Ωd ≈ 1 eV, E0 ≈ 3–5 V/nm [84]) enable Floquet engineering [88]. Spin textures and symmetry breaking can be probed via TR-ARPES, while the Edelstein effect is measurable through Hall-bar transport or spin pumping. Chiral re- sponses are accessible via MOKE or Faraday rotation near band edges [89, 90]. Despite challenges such as ma- terial quality and ultrafast timescales, recent advances demonstrate that these measurements are feasible. Summary.—We have shown that combining gating, optical driving, and in-plane electric fields enables ver- satile control of spin polarization in d-wave altermag- nets. Starting from the dressed Hamiltonian that in- cludes CPL and gating, induced in-plane responses can

rality to altermagnetic strength, we plot χx y /χ0 and χy x/ χ0 versus ∆ and D (Figs. 4(a,b)). CPL (∆ ̸= 0)

able with current laser technology. In natural units (e = ℏ = me = 1), µB = 1/2, and using ρ(µ) ≈ 1– 10 states/eV/unit cell per spin, ⟨Sz ⟩ = (1/2) ρ(µ) ∆

gives, for a ≈ 4 Å (a representative lattice constant) and ∆ = 6.5 meV, ⟨ ˆ S z ⟩ ≈ 10.4 × 10− 2 µB . (13)

Restoring µB and lattice units, for weak gating (λ = 0.2 eV·Å), in-plane fields (Ex , Ey ) = (1, 1) V/nm, and |∆| ≈ 6.5 meV, we find ⟨ ˆ S x ⟩ ≈ 4.32 × 10− 2 µB , ⟨ ˆ S y ⟩ ≈ 9.6 × 10− 2 µB . (14)

6 be computed directly, avoiding complex perturbative corrections. Optical driving generates out-of-plane polarization, while in-plane fields induce in-plane polarizations via the Edelstein effect, all within experimentally accessible ranges. This multi-field approach allows highly tunable and switchable spin polarizations in all directions. Additionally, we find that selective doping of spin bands produces chiral optical activity, which highlights a feature unique to altermagnets. Our results provide a practical route for complete spin control in altermagnets, paving the way for advanced spintronic applications.

Acknowledgments.—M.Y. gratefully acknowledges the hospitality of the Max Planck Institute for the Physics of Complex Systems and of Uppsala University during his visit, where parts of this work were carried out. M.Y. was supported by the Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Contract No. DE-FG02-08ER46542 for the formal developments, the analytical/numerical work, and the writing of the manuscript. J.L. was supported by the Research Council of Norway through its Centres of Excellence funding scheme Grant No. 262633 and Grant No. 353894. M. Berritta and P.M.O. acknowledge support by the Swedish Research Council (VR), the German Research Foundation (Deutsche Forschungsgemeinschaft) through CRC/TRR 227 “Ultrafast Spin Dynamics” (project MF, project-ID: 328545488), and the K. and

A. Wallenberg Foundation (Grants No. 2022.0079 and

2023.0336). Part of the calculations were supported by the National Academic Infrastructure for Supercomputing in Sweden (NAISS) at NSC Linköping, funded by VR through Grant No. 2022-06725. M. Bukov was funded by the European Union (ERC, QuSimCtrl, 101113633). L. Š. acknowledges funding from the ERC Starting Grant No. 101165122.

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End Matter

Appendix A: Time-dependent Hamiltonian.—In this Appendix, we provide the time-dependent Rashba Hamiltonians in the minimal coupling regime:

HR ,d x 2 − y2 ⃗k− e ℏ ⃗A(t) (t) = ℏ2 (k2x + k2y ) 2me σ0 + ℏ2 D(k2x − k2y ) 2me σz + λ (kx σy − ky σx ) + ℏ2 2 me e2 A2d ℏ2 − 2 e Ad ℏ (kx sin(Ωd t ) + ky cos(Ωd t )) σ0 + ℏ2 β 2 me − e2 A2d ℏ2 cos(2Ωd t ) − 2 e Ad ℏ (kx sin(Ωd t ) − ky cos(Ωd t )) σz − λ e Ad ℏ (sin(Ωd t )σy − cos(Ωd t )σx ) , (15a) HR ,dx y ⃗k− e ℏ ⃗A(t)( t) = ℏ2 (k2x + k2y ) 2me σ0 + ℏ2 D kx ky me σz + λ (kx σy − ky σx ) + ℏ2 β me e2 A2d 2ℏ2 sin(2 Ωd t) − e Ad ℏ (kx cos(Ωd t ) + ky sin(Ωd t )) σz −λ e Ad ℏ (sin(Ωd t )σy − cos(Ωd t )σx ) (kx σy − ky σx ) (15b) Using HF0 = 1 T T 0 HR ⃗k− e ℏ ⃗A(t)( t)dt and HF± 1 = 1 T T 0 HR ⃗k− e ℏ ⃗A(t)( t)e± iΩd t dt, the zeroth-order HF0 and first-order HF± 1 Floquet terms are obtained. Finally, in the van Vleck expansion He ff ⃗k ≈ HF0 + [HF− 1, HF+ 1] ℏΩd , the effetive time-independent

Hamiltonian is calculated.

Appendix B : Spin, orbital, and momentum operators.—In this Appendix, we outline the complete set of ingredients required to evaluate the spin and orbital Edelstein response functions, formulated as follows:

Sx ±±,⃗k = ± ℏ 2 sin θ⃗ k cos ϕ⃗ k , Sy ±±,⃗k = ± ℏ 2 sin θ⃗ k sin ϕ⃗ k , Sz ±±,⃗k = ± ℏ 2 cos θ⃗ k , (16a) px ±±,⃗k = ℏkx ∓ λx me ℏ sin θ⃗ k cos ϕ⃗ k ± ℏDkx cos θ⃗ k , (16b) py ±±,⃗k = ℏky ± λy me ℏ sin θ⃗ k sin ϕ⃗ k ∓ ℏDky cos θ⃗ k , pz ±±,⃗k = 0 , (16c) Sx ±∓,⃗k = ℏ 2 cos2 (θ⃗ k /2)e± iϕ⃗ k − sin2 (θ⃗ k /2)e∓ iϕ⃗ k , (16d) Sy ±∓,⃗k = ∓iℏ 2 sin2 (θ⃗ k /2)e∓ iϕ⃗ k + cos2 (θ⃗ k /2)e± iϕ⃗ k , Sz ±∓,⃗k = − ℏ 2 sin θ⃗ k , (16e) px ±∓,⃗k = − λx m e ℏ cos2 (θ⃗ k /2)e± iϕ⃗ k − sin2 (θ⃗ k /2)e∓ iϕ⃗ k − ℏDkx sin θ⃗ k , (16f) py ±∓,⃗k = ∓ i λy me ℏ cos2 (θ⃗ k /2)e± iϕ⃗ k + sin2 (θ⃗ k /2)e∓ iϕ⃗ k + ℏDky sin θ⃗ k , pz ±∓,⃗k = 0 , (16g)

where

cos θ⃗ k = dz (⃗k ) d(⃗k ) , tan ϕ⃗ k = dy (⃗k ) dx ( ⃗k ) ,

(17)

10

stemming from the Hamiltonian He ff,dx 2 − y2 ⃗k = d0 ( k) σ0 + ⃗d(⃗k ) · ⃗σ in Eq. (4a) with eigenenergies ε ±⃗k = d0 ( k) ± | ⃗ d (⃗k )| and eigenstates |u +⃗k ⟩ = cos θ⃗ k 2 e− iϕ⃗ k sin θ⃗ k 2 , |u −⃗k ⟩ = − sin θ⃗ k 2 e− iϕ⃗ k cos θ⃗ k 2 . (18)

Moreover, in two dimensions, the orbital magnetic moment m ℓmn⃗k = µ B L ℓmn⃗k , with µ B = eℏ/(2m e ) as the Bohr magneton and ℓ ∈ {x, y, z}, connects to the Berry curvature Ω ℓmn ( ⃗k). Notably, within the model under consideration, interband transitions do not contribute to the orbital Edelstein effect due to the vanishing of off-diagonal matrix elements: ⟨u ± ⃗k |u ∓ ⃗k ⟩ = 0. Thus, for m = n intraband contributions, we write

Lℓ nn⃗k = − e ℏµB ε n⃗k Ωℓn n( ⃗k ) , Ωℓn n( ⃗k ) = n ϵα βℓ 2 ⃗d(⃗k ) · ∂k α ⃗d(⃗k ) × ∂k β ⃗d(⃗k ) | ⃗ d (⃗k )|3 ,

(19)

where ϵ αβℓ is the Levi-Civita tensor. As there is no k z term in the Hamiltonian, we have L xnn⃗k = L y ⃗ = 0, yielding nn k an angular momentum (in dimensionless units) only along the z-direction:

Lz nn⃗k = n e ε n⃗k λx λy ℏ2 D(k2x − k2y ) 2 me − ∆ 2ℏµB d2x ( ⃗k ) + d2y (⃗k ) + d2z (⃗k ) 3 /2 . (20)