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Symmetry, spin-texture, and tunable quantum geometry in a WTe2 monolayer

Li-kun Shi1 and Justin C. W. Song1,2 1Institute of High Performance Computing, Agency for Science, Technology, & Research, Singapore 138632 2Division of Physics and Applied Physics, Nanyang Technological University, Singapore 637371
Abstract

The spin orientation of electronic wavefunctions in crystals is an internal degree of freedom, typically insensitive to electrical knobs. We argue from a general symmetry analysis and a 𝐤𝐩{\bf k}\cdot{\bf p} perspective, that monolayer 1T’-WTe2 possesses a gate-activated canted spin texture that produces an electrically tunable bulk band quantum geometry. In particular, we find that due to its out-of-plane asymmetry, an applied out-of-plane electric field breaks inversion symmetry to induce both in-plane and out-of-plane electric dipoles. These in-turn generate spin-orbit coupling to lift the spin degeneracy and enable a bulk band Berry curvature and magnetic moment distribution to develop. Further, due to its low symmetry, Berry curvature and magnetic moment in 1T’-WTe2 possess a dipolar distribution in momentum space, and can lead to unconventional effects such as a current induced magnetization and quantum non-linear anomalous Hall effect. These render 1T’-WTe2 a rich two-dimensional platform for all-electrical control over quantum geometric effects.

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Structure and material property/functionality have an intimate relationship. A striking example is monolayer WTe2 where a structural change from 1T to a distorted 1T’ structure induces a topological phase transition from trivial to Z2Z_{2} topological phase Qian . Recently realized in experiment Tang ; Fei ; Wu , the distorted 1T’-WTe2 monolayer possesses a large bulk bandgap 0.055eV\sim 0.055\,{\rm eV} Tang , and helical edge modes that mediate robust edge conduction Fei ; Wu characteristic of a robust quantum spin Hall state.

Here we argue that, aside from determining the band topology, the distorted crystal structure of 1T’-WTe2 (Fig. 1a-c) also enables unusual bulk band quantum geometry and spin physics to be accessed and controlled. By developing a low energy 𝐤𝐩{\bf k}\cdot{\bf p} model from symmetry analysis we find that when an out-of-plane electric field EE_{\perp} is applied, spin-degeneracy is lifted (Fig. 1d,e) by inducing both in-plane as well as out-of-plane spin orientations (Fig. 2a,b). While in-plane spin orientations are synonymous with an out-of-plane inversion symmetry (IS) breaking, out-of-plane spin orientations are less common and typically weak Yuan . As we discuss, 1T’-WTe2 bucks this expectation: even though EE_{\perp} is out-of-plane, the non-aligned outer Te atoms (Fig. 1c) enables an in-plane electric dipole to develop and a strong out-of-plane spin orientation to be induced.

Crucially, applied EE_{\perp} induces Berry curvature as well as magnetic moment. Berry curvature value is determined by an interplay between strong atomic (spin-selective) inter-orbital mixing of the 1T’-WTe2 and EE_{\perp} induced terms, and exhibits a characteristic anisotropic distribution; magnetic moment mirrors this behavior (see Fig. A-2). While an electrically tunable Berry curvature can be readily realized in bilayer systems Xiao07 owing to a electric control over layer degree of freedom, electrical tunability in monolayer systems is considerably more difficult. Berry curvature is realizable in 1T’-WTe2 as a direct result of the asymmetric non-aligned outer Te atoms.

Further, due to the low symmetry of 1T’-WTe2 distorted crystal structure, induced Berry curvature and magnetic moment also possess an asymmetry characterized by a dipolar distribution in reciprocal space. As a result, shifts in the distribution function (e.g., induced when a dissipative charge current is flowing, 𝐣{\bf j}) enable a net Berry flux, and a net out-of-plane magnetization, MzM_{z}, to develop (Fig. 4). The latter corresponds to a direct (linear) magneto-electric effect Mz=iα~zijiM_{z}=\sum_{i}\tilde{\alpha}_{zi}j_{i} (i=x,yi=x,y), where α~zi\tilde{\alpha}_{zi} characterizes the strength of the magneto-electric effect; the former mediates a quantum nonlinear anomalous Hall effect Sodemann .

Both these are intimately tied to the low-symmetry of gated 1T’-WTe2; they do not appear in rotationally symmetric systems. They constitute striking experimental signatures of the tunable quantum geometry (induced Berry curvature and magnetic moment) of 1T’-WTe2, as well as the direct impact that its distorted structure has on its material response. Using available parameters for 1T’-WTe2, we anticipate a sizeable MzM_{z} that can be readily probed for e.g., using Kerr effect microscopy lee2017 . 1T’-WTe2 provides a compelling venue to manipulate spins and magnetic moments in a tunable two-dimensional material. Out-of-plane spin orientations are particularly useful since they may enable to couple to out-of-plane spins necessary for high-density magnetic applications MacNeil ; Kurebayashi .

Refer to caption
Figure 1: (a,b) Crystal structure for a 1T’-WTe2 monolayer possess a particularly low symmetry with (b) a single mirror plane black dashed line (primitive cell denoted by red box). (c) A net in-plane dipole moment dxd_{x} can be induced by a perpendicular electric field EE_{\perp} as a result of non-alignment of the Te atoms on the top and bottom layers. (d,e) The electronic band structure of bulk 1T’-WTe2 monolayer along kyk_{y} direction when an perpendicular electric field is applied possesses (zoom-in, e) spin split conduction and valence bands near the gap opening. Solid and dashed lines are bandstructure from six-band (SBD) and effective four-band heff(𝐤)h^{\rm eff}({\bf k}) models respectively. Parameters used: for the pristine part we used values listed in Table A-III Supp . For the electric field induced part we used αx,y=λ=δx=0\alpha_{x,y}=\lambda=\delta_{x}=0, and δz=0.025eV\delta_{z}=0.025~{\rm eV} as an illustration.

Symmetry analysis and 𝐤𝐩{\bf k}\cdot{\bf p} model — We begin by analyzing the band structure of monolayer 1T’-WTe2 in the presence of an applied out-of-plane electric field EE_{\perp} [Fig. 1(a)]. In doing so, we will employ a 𝐤𝐩{\bf k}\cdot{\bf p} method based on the underlying symmetries of the material: for e.g., mirror symmetry about the xzxz mirror plane [dashed line in Fig. 1(b)], time-reversal symmetry (TRS), and (broken) inversion symmetry (IS). For completeness, our analysis takes into account the three relevant atomic orbitals (ψ1,2,3\psi_{1,2,3}) and two spin states (,\uparrow,\downarrow) that contribute to the states near the Γ\Gamma point and the gap opening [Fig. 1(d)], as revealed by ARPES measurements Tang as well as first principles calculations Qian ; Choe ; Lin ; Xu . This produces a six-band 𝐤𝐩{\bf k}\cdot{\bf p} description (SBD), see Appendix Supp , for a detailed account of the symmetry analysis of these orbitals and spin operators and the symmetry allowed terms in the SBD description.

Importantly, while E=0E_{\perp}=0 produces a spin-degenerate bandstructure Tang ; Qian ; Choe ; Lin ; Xu , when E0E_{\perp}\neq 0 (e.g., induced by proximal gate) we find the bands become spin-split (Fig. 1d). As shown in Fig. 1d, this is particularly relevant away from the Γ\Gamma point, where the splitting becomes pronounced close to the band gap (gray shaded region, Fig. 1d,e). These are characterized by states Ψτξ\Psi_{\tau\xi} with higher (ξ=+1\xi=+1) or lower (ξ=1\xi=-1) energies as shown in Fig. 1e, and τ=±1\tau=\pm 1 correspond to the conduction and valence bands. As we will see, the splitting induced by EE_{\perp} drives a range of novel spin behavior.

At low carrier densities typical for 1T’-WTe2 devices Wu , the electronic and spin behavior is dominated by low-energy excitations around the bandgap in the four bands (Fig. 1e). In order to compactly illustrate the physics, we develop a simple effective four-band model using the basis {ψc\{\psi_{c\uparrow}, ψv\psi_{v\uparrow}, ψc\psi_{c\downarrow}, ψv}\psi_{v\downarrow}\} in the regime around the gap opening (see gray region). This is obtained by performing a Löwdin partitioning (see Supp ) of the bands in Fig. 1d and can be expressed as heff(𝐤)=h0(𝐤)+h1(𝐤)h^{\rm eff}({\bf k})=h_{0}({\bf k})+h_{1}({\bf k}). Here h0(𝐤)h_{0}({\bf k}) describes the electronic behavior in pristine 1T’-WTe2 (E=0E_{\perp}=0):

h0(𝐤)=ϵ¯𝐤+(m𝐤v𝐤+00v𝐤m𝐤0000m𝐤v𝐤00v𝐤+m𝐤),\displaystyle h_{0}({\bf k})=\bar{\epsilon}_{{\bf k}}+\left(\begin{array}[]{cccc}m_{{\bf k}}&v^{+}_{{\bf k}}&0&0\\ -v^{-}_{{\bf k}}&-m_{{\bf k}}&0&0\\ 0&0&m_{{\bf k}}&v^{-}_{{\bf k}}\\ 0&0&-v^{+}_{{\bf k}}&-m_{\bf k}\end{array}\right), (5)

where ϵ¯𝐤=(ϵc𝐤+ϵv𝐤)/2\bar{\epsilon}_{{\bf k}}=(\epsilon_{c{\bf k}}+\epsilon_{v{\bf k}})/2, m𝐤=(ϵc𝐤ϵv𝐤)/2m_{{\bf k}}=(\epsilon_{c{\bf k}}-\epsilon_{v{\bf k}})/2, v𝐤±=±vxkx+ivykyv_{{\bf k}}^{\pm}=\pm v_{x}k_{x}+iv_{y}k_{y} represents the strong spin selective atomic orbital coupling (sharing the same spin), while ϵc𝐤\epsilon_{c{\bf k}} and ϵv𝐤\epsilon_{v{\bf k}} are diagonal parts for the conduction and valence bands, capturing their energy offsets and effective masses Supp . We note that h0(𝐤)h_{0}({\bf k}) is simply a tilted Bernevig-Hughes-Zhang (BHZ) hamiltonian Bernevig that describes the spin-degenerate bands in pristine 1T’-WTe2; here the tilt arises from large effective mass differences between the conduction and valence bands (see Table. A-III Supp ).

On the other hand, h1(𝐤)=hZ(𝐤)+hR(𝐤)h_{1}({\bf k})=h_{Z}({\bf k})+h_{R}({\bf k}) captures the electric field-induced spin-orbit coupling that are allowed by symmetry

hZ(𝐤)\displaystyle h_{Z}({\bf k}) =(λkyiδz00iδzλky0000λkyiδz00iδzλky),\displaystyle=\begin{pmatrix}\lambda k_{y}&i\delta_{z}&0&0\\ -i\delta_{z}&\lambda k_{y}&0&0\\ 0&0&-\lambda k_{y}&-i\delta_{z}\\ 0&0&i\delta_{z}&-\lambda k_{y}\end{pmatrix},
hR(𝐤)\displaystyle h_{R}({\bf k}) =(00α𝐤iδx00iδxα𝐤α𝐤+iδx00iδxα𝐤+00),\displaystyle=\begin{pmatrix}0&0&\alpha_{{\bf k}}^{-}&i\delta_{x}\\ 0&0&i\delta_{x}&\alpha_{{\bf k}}^{-}\\ \alpha_{{\bf k}}^{+}&-i\delta_{x}&0&0\\ -i\delta_{x}&\alpha_{{\bf k}}^{+}&0&0\end{pmatrix}, (6)

where we have grouped the electric field-induced spin-orbit coupling terms into hZ(𝐤)h_{Z}({\bf k}) and hR(𝐤)h_{R}({\bf k}) in order to highlight the out-of-plane and in-plane spin orientations they induce respectively (see Fig. 2). Here α𝐤±=±iαxkx+αyky\alpha_{{\bf k}}^{\pm}=\pm i\alpha_{x}k_{x}+\alpha_{y}k_{y}, δx,z\delta_{x,z} are kk-independent coupling terms, and λky\lambda k_{y} is a kk-dependent that can induce out-of-plane spin orientation. We note, parenthetically, that the spin-orbit coupling terms in hZh_{Z} have sometimes been referred to as “Zeeman-like” see e.g., Ref. Yuan ; Xu so as highlight the out-of-plane spin orientation it induces; in the following, we will not use this terminology, but instead focus on their physical manifestation: its spin orientation. We emphasize that both hZ(𝐤)h_{Z}({\bf k}) and hR(𝐤)h_{R}({\bf k}) in this work physically originate from IS breaking induced by the application of the electric field, see next section for detailed discussion.

In writing Eq. (6) we have kept all symmetry allowed terms up to the linear order in kk as allowed by symmetry. We remark that the magnitudes of each of the symmetry allowed terms can be determined from experimental or first principle calculation results (see Appendix Supp for a discussion). However, before we move to specific values, we first discuss the physical origin of the coupling terms, and some possible interplays brought by these couplings.

Physical origin of out-of-plane and in-plane spin orientations — For physical clarity, we will denote hR(𝐤)h_{R}({\bf k}) and hZ(𝐤)h_{Z}({\bf k}) as spin-orbit coupling induced by out-of-plane and in-plane IS breaking, respectively. In a general sense, hR(𝐤)h_{R}({\bf k}) [or hZ(𝐤)h_{Z}({\bf k})] always couple states with opposite spins [the same spin]. As a result, these terms split the spin degeneracy and re-orient the spins of the eigenstate Ψτξ\Psi_{\tau\xi}: hRh_{R} terms create in-plane spin orientations (Fig. 2a) whereas hZh_{Z} terms align spins out-of-plane (Fig. 2b). Here spin orientations are plotted only for the right valley (ky>0k_{y}>0). For ky<0k_{y}<0, spin textures are flipped.

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Figure 2: (a,b) Schematic spin splitting and spin texture of the conduction band (near the gap) induced by an applied electric field. These can be classed as (a) In-plane spin orientation (α,δx0\alpha,\delta_{x}\neq 0, λ,δz=0\lambda,\delta_{z}=0) originating from an out-of-plane electric field EztotE_{z}^{\rm tot}, or (b) Out-of-plane spin orientation (α,δx=0\alpha,\delta_{x}=0, λ,δz0\lambda,\delta_{z}\neq 0) arising from an in-plane dipole dxd_{x}.

Their physical origins are also distinct. When a charge neutral monolayer 1T’-WTe2 is placed under EE_{\perp}, the top layer and the bottom layer Te atoms experience a charge redistribution becoming oppositely charged. This charge redistribution counteracts EE_{\perp} forming an out-of-plane dipole moment, dzd_{z} (see Fig. 1c). Crucially, because the Te atoms are not perfectly aligned, this charge redistribution also creates an in-plane electric dipole moment along the xx-direction, dxd_{x}, yielding a net induced electric dipole, 𝐝net{\bf d}_{\rm net}, that is canted (see Fig. 1c).

As a result, EE_{\perp} induces IS breaking in both zz- and xx-directions developing a nonzero zϕ(𝐫)\partial_{z}\phi({\bf r}) and xϕ(𝐫)\partial_{x}\phi({\bf r}); here ϕ(𝐫)\phi({\bf r}) is the local electro-static potential induced by EE_{\perp}. Since spin-orbit coupling arises as matrix elements of the microscopic spin-orbit interaction: H^so(𝐤)(𝐤+𝐩^/m0)𝐬×ϕ(𝐫){\hat{H}}_{\rm so}({\bf k})\sim({\bf k}+{\hat{{\bf p}}}/m_{0})\cdot{\bf s}\times\nabla\phi({\bf r}) 111see e.g., Eq. (16.1) of Ref. Bir , or Eq. (2.4) of Ref. WinklerBook , we find that spin-orbit coupling terms δx\delta_{x} and α𝐤±\alpha_{{\bf k}}^{\pm} come from the total out-of-plane electric field zϕ(𝐫)-\partial_{z}\phi({\bf r}); this constrains the terms 𝐤+𝐩^/m0{\bf k}+{\hat{{\bf p}}}/m_{0} and 𝐬{\bf s} in H^so(𝐤){\hat{H}}_{\rm so}({\bf k}) to be in-plane only. However, the charge re-distribution also enables an in-plane xϕ(𝐫)\partial_{x}\phi({\bf r}) to develop. This in-plane electric field picks out 𝐬{\bf s} in H^so(𝐤){\hat{H}}_{\rm so}({\bf k}) as the out-of-plane component szs_{z}, and 𝐤+𝐩^/m0{\bf k}+{\hat{{\bf p}}}/m_{0} as the yy-component. As a result of the in-plane xϕ(𝐫)\partial_{x}\phi({\bf r}), hZh_{Z} terms λky\lambda k_{y} and δz\delta_{z} in Eq. 6 manifest. The distorted structure of 1T’-WTe2 enables 𝐝net{\bf d}_{\rm net} that is generically canted with finite hZh_{Z} and hRh_{R} terms that co-exist. In contrast, since λky\lambda k_{y} and δz\delta_{z} result from the in-plane electric field xϕ(𝐫)\partial_{x}\phi({\bf r}), the non-distorted transition metal dichalcogenide monolayers whose atoms at top and bottom layers are aligned (e.g., MoS2) do not possess an external EE_{\perp}-induced out-of-plane spin orientations near the Γ\Gamma point (up to linear in kk).

As a further illustration of the role that low symmetry plays in 1T’-WTe2, we can also compare the spin-orbit coupling terms in hR(𝐤)h_{R}({\bf k}) allowed in 1T’-WTe2 [induced by out-of-plane IS breaking], with that of HgTe quantum wells recently discussed in the literature Tarasenko ; Rothe . For 1T’-WTe2, all terms in hR(𝐤)h_{R}({\bf k}) are allowable when an out-of-plane electric field is applied because of its very low symmetry, and that fact that angular momentum in the zz-direction is not a good quantum number. In contrast, HgTe quantum wells possess a D2dD_{2d} symmetry, [hR(𝐤)]24,(42)[h_{R}({\bf k})]_{24,(42)} is missing because its 2nd and 4th basis functions are heavy hole bands with jz=±3/2j_{z}=\pm 3/2 and the coupling between them is at least of k3k^{3} order. Only iδxi\delta_{x} and [hR(𝐤)]13,(31)[h_{R}({\bf k})]_{13,(31)} can appear, corresponding to the existence of bulk inversion asymmetry Tarasenko and structural inversion asymmetry Rothe , respectively.

Interplay between Berry curvature and the two types of spin-orbit couplings — Pristine 1T’-WTe2 possesses both IS and TRS ensuring that Berry curvature (and orbital magnetic moment) vanish exactly. As we now discuss, in 1T’-WTe2 with E0E_{\perp}\neq 0, hZh_{Z} [Eq. (6)] presents an opportunity to break in-plane IS turning on a finite Berry curvature distribution. For clarity, we will first focus on the case when λ\lambda and αx,y\alpha_{x,y} are non-zero, while setting the kk-independent terms δx,z=0\delta_{x,z}=0, and then analyse the case when δx,z0\delta_{x,z}\neq 0 later in the text.

To proceed, we first note that for pristine 1T’-WTe2 (when E=0E_{\perp}=0), the hamiltonian heff=h0(𝐤)h^{\rm eff}=h_{0}({\bf k}) in Eq. (5) possesses spin degenerate states Ψτξ\Psi_{\tau\xi}, with ξ=±1\xi=\pm 1 corresponding to ,\uparrow,\downarrow states, and spin-degenerate energy ετξ(𝐤)=ϵ¯𝐤+τΔ𝐤\varepsilon_{\tau\xi}({\bf k})=\bar{\epsilon}_{{\bf k}}+\tau\Delta_{{\bf k}} where Δ𝐤2=(vxkx)2+(vyky)2+m𝐤2\Delta_{{\bf k}}^{2}=(v_{x}k_{x})^{2}+(v_{y}k_{y})^{2}+m_{{\bf k}}^{2} is the energy difference between the conduction and valence bands. In the absence of vx,yv_{x,y}, conduction (ψτ=+1,ξ\psi_{\tau=+1,\xi}) and valence (ψτ=1,ξ\psi_{\tau=-1,\xi}) bands touch, and exhibit a gapless spectrum along Γ\Gamma-YY Muechler . However, large spin-selective atomic orbital coupling vx,yv_{x,y} in 1T’-WTe2 creates strong inter-orbital mixing (between ψc,v\psi_{c,v}) giving a large QSH gap 0.055eV\sim 0.055\,{\rm eV} Tang .

Even though the external EE_{\perp} induced spin orbit coupling [Eq. (6)] is small as compared with the intrinsic spin-selective atomic orbital coupling, α±,λv±\alpha_{\pm},\lambda\ll v_{\pm}, nevertheless, when an external electric field E0E_{\perp}\neq 0 is applied, IS is immediately broken. Specifically, we emphasize that it is in-plane IS breaking that enables a finite Berry curvature, Ωτξ(𝐤)\Omega_{\tau\xi}({\bf k}), distribution to develop. As a result, we find that λ\lambda encoding in-plane IS breaking (arising from dxd_{x}, Fig. 1c) turns on Ωτξ(𝐤)\Omega_{\tau\xi}({\bf k}). In contrast, while αx,y\alpha_{x,y} is also induced by E0E_{\perp}\neq 0 (and can also spin-split ψc,v\psi_{c,v} bands) it corresponds to an out-of-plane IS breaking, and does not lead to Ωτξ(𝐤)\Omega_{\tau\xi}({\bf k}).

Refer to caption
Figure 3: Peak Berry curvature value Ωτ=1,ξ=1(𝐤0)\Omega_{\tau=1,\xi=-1}({\bf k}_{0}) as a function of (a) kk-dependent spin-orbit coupling (α,λ)(\alpha,\lambda) where we have set δx,z=0\delta_{x,z}=0, and (b) kk-independent spin-orbit coupling (δx,δz)(\delta_{x},\delta_{z}) where we have set α,λ=0\alpha,\lambda=0. Peak values are taken at the band edge 𝐤0=(0,k0){\bf k}_{0}=(0,k_{0}) with k0=0.385Å1k_{0}=0.385~{\rm\AA ^{-1}}. Dashed lines denote equi-Berrry-curvature contours. Both (a) and (b) show that Berry curvature is pronounced only when (λ\lambda, or δz\delta_{z}) is large; this corresponds to strong in-plane inversion symmetry breaking. Parameters for the pristine part are listed in Table A-III Supp .

To see this explicitly, we first consider the case αλ\alpha\ll\lambda where out-of-plane IS breaking is much weaker than in-plane IS breaking. In this case, λ\lambda dominates h1(𝐤)h_{1}({\bf k}) and we can take α0\alpha\to 0. Therefore, heff(𝐤)=h0(𝐤)+h1(𝐤)h^{\rm eff}({\bf k})=h_{0}({\bf k})+h_{1}({\bf k}) produces a Ψτξ\Psi_{\tau\xi} bandstructure with a lifted spin-degeneracy (Fig. 1e) and energies ετξ(𝐤)=ϵ¯𝐤+τΔ𝐤+ξ|λky|\varepsilon_{\tau\xi}({\bf k})=\bar{\epsilon}_{{\bf k}}+\tau\Delta_{{\bf k}}+\xi|\lambda k_{y}|. We note that since both λ\lambda as well as spin-selective atomic orbital coupling vx,yv_{x,y} do not mix spins, Ψτξ\Psi_{\tau\xi} possess spins that purely point out of plane (Fig. 2b). Using this, we find a Berry curvature distribution Ωτξ(𝐤)=𝐤×Ψτξ(𝐤)|i𝐤|Ψτξ(𝐤)\Omega_{\tau\xi}({\bf k})=\boldsymbol{\nabla}_{{\bf k}}\times\langle\Psi_{\tau\xi}({\bf k})|i\boldsymbol{\nabla}_{{\bf k}}|\Psi_{\tau\xi}({\bf k})\rangle as

Ωτξ(0)(𝐤)=sgn(ky)τξ2vxvyΔ𝐤3(1𝐤𝐤)m𝐤.\displaystyle\Omega_{\tau\xi}^{(0)}({\bf k})={\rm sgn}(k_{y})\frac{\tau\xi}{2}\frac{v_{x}v_{y}}{\Delta_{{\bf k}}^{3}}(1-{\bf k}\cdot\nabla_{{\bf k}})m_{{\bf k}}. (7)

Strikingly, Ωτξ(0)(𝐤)\Omega_{\tau\xi}^{(0)}({\bf k}) in Eq. (7) does not depend on λ\lambda even though finite λ\lambda was required to break in-plane IS. Instead, Ωτξ(0)(𝐤)\Omega_{\tau\xi}^{(0)}({\bf k}) is solely determined by the spin-selective atomic orbital coupling vx,yv_{x,y}, and the band parameters in pristine 1T’-WTe2.

This decoupling behavior between IS breaking strength and the value of Ωτξ\Omega_{\tau\xi} persists even in the presence of finite out-of-plane IS breaking characterized by the ratios λ/α\lambda/\alpha. To see this, we note that when α\alpha is finite, h1(𝐤)h_{1}({\bf k}) starts to hybridize Ψτξ\Psi_{\tau\xi} with different spins (in the same τ\tau band). Since the intrinsic Berry curvature Ωτξ(0)(𝐤)\Omega_{\tau\xi}^{(0)}({\bf k}) for spin up and spin down states are opposite in sign, when the ξ\xi states couple (via α\alpha) the Berry curvature drops. Along the high symmetry line kx=0k_{x}=0 about which the Berry curvature is even due to the TRS and mirror symmetry in the yy-direction, the Berry curvature for the spin split bands near band edge can be expressed as Supp

Ωτξ(kx=0,ky)=λ(λ2+αy2)1/2Ωτξ(0)(kx=0,ky),\displaystyle\Omega_{\tau\xi}(k_{x}=0,k_{y})=\frac{\lambda}{(\lambda^{2}+\alpha_{y}^{2})^{1/2}}\Omega_{\tau\xi}^{(0)}(k_{x}=0,k_{y}), (8)

clearly displaying how Ωτξ(kx=0,ky)\Omega_{\tau\xi}(k_{x}=0,k_{y}) tends to the value expected in Ωτξ(0)\Omega_{\tau\xi}^{(0)} for λα\lambda\gg\alpha. In Fig. 3a, we plot the peak value of Berry curvature Ωτ=1,ξ=1\Omega_{\tau=1,\xi=-1} reproduced in a numerical evaluation of the SBD description. This verifies our above analysis that the value of Ωτξ\Omega_{\tau\xi} is bounded by the intrinsic (depends only on vx,yv_{x,y}) Ωτξ(0)\Omega_{\tau\xi}^{(0)}, and is tuned only by the ratios λ/α\lambda/\alpha, which makes equi-Berry-curvature contours to be straight lines (see Fig. 3a).

We now consider the case of δx,z0\delta_{x,z}\neq 0, while setting kk-dependent terms α,λ=0\alpha,\lambda=0. By numerically evaluating peak Berry curvature Ωτ=1,ξ=1(𝐤0)\Omega_{\tau=1,\xi=-1}({\bf k}_{0}) (see Fig. 3b), we find that the peak Berry curvature Ωτ=1,ξ=1(𝐤0)\Omega_{\tau=1,\xi=-1}({\bf k}_{0}) develops a more complicated behavior. In particular, Ωτ=1,ξ=1(𝐤0)\Omega_{\tau=1,\xi=-1}({\bf k}_{0}) is no longer bounded by the intrinsic value Ωτξ(0)\Omega_{\tau\xi}^{(0)}, and increases with δz\delta_{z} without saturation. However, similar to the previous case, out-of-plane IS breaking δx\delta_{x} alone is not able to induce a nonzero Berry curvature since it corresponds to an out-of-plane IS breaking. Large Berry curvature only appears when δz\delta_{z} is significant.

In the above, we concentrated on unveiling the (Berry curvature) features that the various symmetry allowed spin-orbit coupling terms possess. These features can in turn help to diagnose which of the (a priori symmetry-allowed) spin-orbit coupling terms dominate. We illustrate this by comparing with recent first principles calculations as well as a recent experiment Xu . In Ref. Xu , the Berry curvature of monolayer 1T’-WTe2 was investigated at different perpendicular electric fields, from 0 to around 1 V nm-1 using both first principles and a photocurrent measurement. In particular, their first principles results revealed the EE_{\perp} induced spin-splitting in the bandstructure that vanished at larger kyk_{y} away from the band edge, and a peak Berry curvature that increased with EE_{\perp}. This observation means that kk-dependent spin-orbit couplings may play only a minimal role. Further both the experiment and the first principles calculations found large Berry curvature at band edge even at small electric field shows that δz>δx\delta_{z}>\delta_{x} (see Fig. 3). Strikingly, these values of Berry curvature are close to the large intrinsic values expected from vx,yv_{x,y} and m𝐤m_{{\bf k}}. Together with Fig. 3b this indicates that the in-plane IS breaking and hZh_{Z} terms dominates, overwhelming the hRh_{R} terms. As a result, in what follows we will use the k-independent δz\delta_{z} spin-orbit coupling term to describe the EE_{\perp} induced spin texture.

Refer to caption
Figure 4: (a,b) Asymmetry in 1T’-WTe2 enable dipolar distributions of intrinsic magnetic moment (a) mintm^{\rm int} characterized by a (b) kymint\partial_{k_{y}}m^{\rm int} near the gap opening ±𝐤0=(0,±k0)\pm{\bf k}_{0}=(0,\pm k_{0}). Black curves represent the conduction band (τ=1,ξ=1\tau=1,\xi=-1), dashed lines denote the chemical potential μ\mu with gray shaded areas are the occupied states. Due to the tilt of the band dispersion, an intrinsic magnetic moment dipole arises near the gap opening, and gives rise to a non-zero current-induced magnetization MzM_{z} [see Eq. (10)]. Parameters used for the pristine part are the same as those in Fig. 1 for an illustration. (c) Schematic of a 1T’-WTe2 monolayer under a perpendicular electric field E𝐳^E_{\perp}\hat{{\bf z}} and an in-plane electric field EyE_{y}, which can give rise to intrinsic magnetization MzM_{z}. (d) Calculated intrinsic magnetization MzM_{z} induced by a current jy=10Am1j_{y}=10~{\rm A\,m^{-1}} in the yy-direction from Eq. (10), with λ,α,δx=0\lambda,\alpha,\delta_{x}=0, but varying δz=0.075eV\delta_{z}=0.075~{\rm eV} (blue), 0.05eV0.05~{\rm eV} (green), and 0.025eV0.025~{\rm eV} (red). These magnitudes for δz\delta_{z} are within reach by applying an E<1Vnm1E_{\perp}<1~\rm{V\,nm}^{-1} Xu . The MzM_{z} plotted here becomes non-zero only when the chemical potential is above the conduction band bottom (denoted by dashed lines), which is different for each of the lines. The trend from the red line to the blue line shows that a larger δz\delta_{z} (stronger in-plane IS breaking) leads to an increased intrinsic magnetic moment as well as more pronounced MzM_{z}, as illustrated in Fig. 2.

Current induced magnetization — Another closely related quantity, the (intrinsic) orbital magnetic moment mnint(𝐤)m_{n}^{\rm int}({\bf k}), also appears when in-plane IS is broken by E𝐳^E_{\perp}\hat{{\bf z}}:

mnint(𝐤)=eRennin|H/kx|nn|H/ky|nεnεn,\displaystyle m_{n}^{\rm int}({\bf k})=\frac{e}{\hbar}{\rm Re}\,\sum_{n^{\prime}\neq n}\frac{i\langle n|\partial H/\partial k_{x}|n^{\prime}\rangle\langle n^{\prime}|\partial H/\partial k_{y}|n\rangle}{\varepsilon_{n}-\varepsilon_{n^{\prime}}}, (9)

where we have written n={τξ}n=\{\tau\xi\} as a short-hand, and HH is the hamiltonian. The orbital magnetic moment comes from the self-rotation of a Bloch electron wave packet around its center of mass, and is an intrinsic property of the Bloch band Xiao , and its distribution in momentum space mimics that of the Berry curvature distribution (see Appendix Supp ).

The low-symmetry of 1T’-WTe2 enables an asymmetric distribution of of Ωn(𝐤)\Omega_{n}({\bf k}) and mn(𝐤)m_{n}({\bf k}) (see Fig. 4 a,b). This affords the opportunity to realize Berry phase effects not normally achievable in their rotational symmetric cousins. A striking example is the (linear) magneto-electric effect (ME) Mz=iαziEiM_{z}=\sum_{i}\alpha_{zi}E_{i} (i=x,yi=x,y), where the flow of an in-plane current induces an out-of-plane magnetization. While typically found in multi-ferroic materials Eerenstein where TRS and IS are explicitly broken, ME effects can arise in metals with sufficiently low symmetry (broken IS as well as broken rotational symmetry) and where the dissipation of a charge current breaks TRS Levitov . 222 We can see these from the symmetry analysis as follows: (a) in a time-reversal symmetric system Mz=iαziEiM_{z}=\sum_{i}\alpha_{zi}E_{i}, then under the symmetry operation ttt\to-t we have MzMzM_{z}\to-M_{z}, 𝐄𝐄{\bf E}\to{\bf E}, and Mz=iαziEiMz=iαziEiM_{z}=\sum_{i}\alpha_{zi}E_{i}\to-M_{z}=\sum_{i}\alpha_{zi}E_{i} which leads to αzx=αzy=0\alpha_{zx}=\alpha_{zy}=0; (b) if a system has a rotational symmetry, then under the rotation by angle θ\theta we have MzMzM_{z}\to M_{z}, ExExcosθEysinθE_{x}\to E_{x}\cos\theta-E_{y}\sin\theta, EyEsinθ+EycosθE_{y}\to E\sin\theta+E_{y}\cos\theta, and Mz=αzxEx+αzyEyMz=(αzxEx+αzyEy)cosθ+(αzyExαzxEy)sinθM_{z}=\alpha_{zx}E_{x}+\alpha_{zy}E_{y}\to M_{z}=(\alpha_{zx}E_{x}+\alpha_{zy}E_{y})\cos\theta+(\alpha_{zy}E_{x}-\alpha_{zx}E_{y})\sin\theta which leads to θ=2nπ\theta=2n\pi (n=0,1,2,n=0,1,2,\dots), i. e., rotational symmetry is not allowed for non-zero αzx\alpha_{zx} and αzy\alpha_{zy}; (c) if a system is centrosymmetric, then under the operation (x,y)(x,y)(x,y)\to(-x,-y) we have MzMzM_{z}\to M_{z}, 𝐄𝐄{\bf E}\to-{\bf E}, and Mz=iαziEiMz=iαziEiM_{z}=\sum_{i}\alpha_{zi}E_{i}\to M_{z}=-\sum_{i}\alpha_{zi}E_{i} which also requires αzx=αzy=0\alpha_{zx}=\alpha_{zy}=0. . This is termed the kinetic ME effect Levitov ; Sahin .

Indeed, the low-symmetry of 1T’-WTe2 (with E0E_{\perp}\neq 0) where only a mirror symmetry in the yy-direction remains is the largest symmetry group that hosts the kinetic ME Levitov ; Sodemann . This makes 1T’-WTe2 a natural venue to control ME.

To illustrate the kinetic ME effect in 1T’-WTe2, we first note that the magnetic moment is asymmetric, displaying a dipolar distribution (see Fig. 4a,b). This can be seen explicitly by considering kym\partial_{k_{y}}m and noting that it is displaced in relation to the bottom of the band, Fig. 4b. As a result, when an in-plane electric field shifts the distribution function, a uniform out-of-plane magnetization MzM_{z} develops:

Mz=i=x,yα~ziji,α~zi=[en,𝐤fn𝐤(0)mntot(𝐤)ki](Dii)1\displaystyle M_{z}=\sum_{i=x,y}\tilde{\alpha}_{zi}j_{i},\quad\tilde{\alpha}_{zi}=\Big{[}\frac{e}{\hbar}\sum_{n,{\bf k}}f_{n{\bf k}}^{(0)}\frac{\partial m_{n}^{\rm tot}({\bf k})}{\partial k_{i}}\Big{]}(D_{ii})^{-1} (10)

where DiiD_{ii} is the Drude weight along ii direction, fn𝐤(0)f_{n{\bf k}}^{(0)} is the equilibrium distribution function, mntot(𝐤)=mnint(𝐤)+(ge/2m0)u𝐤|sz|u𝐤m_{n}^{\rm tot}({\bf k})=m_{n}^{\rm int}({\bf k})+(ge/2m_{0})\langle u_{{\bf k}}|s_{z}|u_{{\bf k}}\rangle is the intrinsic contribution to the magnetic moment in a particular band, containing both orbital and spin contributions with sz=σz/2s_{z}=\hbar\sigma_{z}/2. For 1T’-WTe2 monolayer, we estimate g5g\sim 5 Wu ; Fei .

Importantly, Eq. (10) reflects the symmetry of the crystal. For example, magnetic moment distribution has equal magnitudes but opposite signs in the two electron pockets in the conduction band. As a result, α~zx=0\tilde{\alpha}_{zx}=0 vanishes as expected from symmetry, see above. In contrast, when in-plane electric field is applied along yy, a non-zero MzM_{z} is generated (i.e. α~zy0\tilde{\alpha}_{zy}\neq 0).

Using Eq. (10), we obtain a finite out-of-plane magnetization MzM_{z} in Fig. 4d when current is driven along the yy direction. In doing so, we used fn𝐤(0)=Θ(εn𝐤μ)f_{n{\bf k}}^{(0)}=\Theta(\varepsilon_{n{\bf k}}-\mu) with μ\mu the chemical potential, and computed the Drude weight in the usual fashion. Further, to capture the full reciprocal space distribution of the magnetic moment (including regions away from the gap opening), we used the SBD description to compute the magnetic moment distribution. Here we have concentrated on small chemical potentials so that only moments in the lowest conduction band (blue band in Fig. 1e) contribute. Since mnint(𝐤)m_{n}^{\rm int}({\bf k}) is an odd function of kyk_{y} when TRS is present, the filled bands do not contribute to ME. This reflects the fact that kinetic ME arises from a dissipative process. As a result, when the chemical potential is in the gap, α~zy=0\tilde{\alpha}_{zy}=0. However, once the system is doped into the conduction band, a non-zero ME develops, see Fig. 4d. Similar analysis also applies to the Berry curvature Ωτξ\Omega_{\tau\xi} (which exhibits a dipolar distribution), and leads to a non-linear Hall effect without applied magnetic field (see Ref. Sodemann as well as the Appendix Supp for an explicit discussion for this system).

Summary – 1T’-WTe2 with an applied out-of-plane electric field EE_{\perp}, provides a new and compelling venue to control bulk band quantum geometry. In particular, its bands exhibit a tunable Berry curvature and magnetic moment with switch-like behavior. Crucially, the low symmetry of its crystal structure enable effects not normally found in its rotationally symmetric cousins. These include striking Berry phase effects such as a current induced magnetization (ME), and a quantum non-linear Hall effect. These are particularly sensitive to orientation of in-plane electric field and the crystallographic directions. Indeed, MzM_{z} is strongest when current runs along the yy-direction; this sensitivity can be verified through measurements in a single 1T’-WTe2 sample, for e.g., using a Corbino disc geometry. Perhaps most exciting, however, is how IS broken 1T’-WTe2 enables direct and electric-field tunable access to out-of-plane magnetic degrees of freedom. Given its two-dimensional nature, 1T’-WTe2 can be stacked with other two-dimensional materials, providing a key magneto-electric component in creating magnetic van der Waals heterostructures.

Acknowledgements - We gratefully acknowledge useful conversations with Valla Fatemi, Qiong Ma, Su-Yang Xu, and Dima Pesin. This work was supported by the Singapore National Research Foundation (NRF) under NRF fellowship award NRF-NRFF2016-05 and a Nanyang Technological University Start-up grant (NTU-SUG).

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Appendix for “Symmetry, spin-texture, and tunable quantum geometry in WTe2 monolayer”

.1 Six-band 𝐤𝐩{\bf k}\cdot{\bf p} model for monolayer 1T’-WTe2

Without external fields, 1T’-WTe2 monolayers possess time-reversal (TR) symmetry and a point symmetry group P21/mP2_{1}/m that contains four symmetry operations. If we set one of the inversion center as the origin 𝒪0=(0,0,0){\cal O}_{0}=(0,0,0) in real space, the four symmetry operations are {(x,y,z),(x,y,z),(x,1/2y,z),(x,1/2+y,z)}\{(x,y,z),(-x,-y,-z),(x,1/2-y,z),(-x,1/2+y,-z)\} where 1/21/2 denotes shifting by 1/21/2 a unit cell in the yy-direction. When we shift the origin 𝒪0{\cal O}_{0} to 𝒪1=(0,1/2,0){\cal O}_{1}=(0,1/2,0), the four symmetry operations become {(x,y,z),(x,y,z),(x,1/2,z),(x,1/2,z)}\{(x,y,z),(x,-y,z),(-x,1/2,-z),(-x,-1/2,-z)\}.

Various first-principle calculations as well as expermental measurements Qian ; Tang ; Choe ; Lin showed that there are three relevant orbitals contributing to the states near the gap. Although the exact orbital compositions at the Γ\Gamma point is not clear, these orbitals at the Γ\Gamma point are consistently revealed Tang ; Choe ; Lin to be (even, odd, even) under the reflection operation in yy-direction (the orbitals are ordered with decreasing energy). Here we note that Choe et al. used a different coordinate system with xx and yy directions exchanged.

A perpendicularly applied electric field breaks symmetry operations that flip in the zz-direction and reduce the point group P21/mP2_{1}/m to group C1vC_{1v} that has only two symmetry operations {𝕀,My}\{\mathbb{I},M_{y}\} (i. e., identity and reflection about the xzxz plane that cross a Te atom). It has two real 1D irreducible representations (see Table A-I).

Aside from the spin degrees of freedom, each of the three orbitals at the Γ\Gamma point is non-degenerate and transforms according to one of the 1D irreducible representations of C1vC_{1v}. Moreover, although inversion symmetry is broken, the three orbitals remain (even, odd, even) in the yy-direction at the Γ\Gamma point. These two observations show that the three orbitals at the Γ\Gamma point transform as:

ψ11,ψ2y,ψ31,\displaystyle\psi_{1}\sim 1,\quad\psi_{2}\sim y,\quad\psi_{3}\sim 1, (A-1)

where the symbol “\sim” denotes how these functions transform under operations in C1vC_{1v}. Using {ψ1\{\psi_{1}, ψ2\psi_{2}, ψ3}\psi_{3}\} as basis, the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian near the Γ\Gamma point assumes a 3×33\times 3 form:

H(𝓚)=(H11(𝓚)H12(𝓚)H13(𝓚)H21(𝓚)H22(𝓚)H23(𝓚)H31(𝓚)H32(𝓚)H33(𝓚)),\displaystyle H(\boldsymbol{\cal K})=\left(\begin{array}[]{ccc}H^{11}(\boldsymbol{\cal K})&H^{12}(\boldsymbol{\cal K})&H^{13}(\boldsymbol{\cal K})\\ H^{21}(\boldsymbol{\cal K})&H^{22}(\boldsymbol{\cal K})&H^{23}(\boldsymbol{\cal K})\\ H^{31}(\boldsymbol{\cal K})&H^{32}(\boldsymbol{\cal K})&H^{33}(\boldsymbol{\cal K})\\ \end{array}\right), (A-5)

where Hαβ(𝓚)H^{\alpha\beta}(\boldsymbol{\cal K}) is the 2×22\times 2 (1×11\times 1) block matrix between ψ1\psi_{1} and ψ2\psi_{2} with (without) spin degree of freedom included.

In the following, we will obtain the general form of H(𝓚)H(\boldsymbol{\cal K}) from symmetry analysis. The necessary information for ψ1,2,3\psi_{1,2,3} is contained in its transformation property under group C1vC_{1v} [Eq. (A-1)]. We note that detailed orbital compositions, e. g., the weight of pp- or dd- orbital in |ψ1,2,3|\psi_{1,2,3}\rangle, does not affect the following analysis.

We will proceed by using the theory of invariants Bir ; Winkler ; Zhou which is based on the invariance of the Hamiltonian H^\hat{H} under all operations of the corresponding crystal symmetry group. When the Hamiltonian H^\hat{H} is projected to the energy bands of interest H^=α,β|ψαHαβ(𝓚)ψβ|\hat{H}=\sum_{\alpha,\beta}|\psi_{\alpha}\rangle H^{\alpha\beta}(\boldsymbol{\cal K})\langle\psi_{\beta}|, where 𝓚\boldsymbol{\cal K} denotes a tensor operator formed by combinations of wave vectors, the symmetry group constrains the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian Hαβ(𝓚)H^{\alpha\beta}(\boldsymbol{\cal K}) as follows: under an arbitrary symmetry operation gC1vg\in{C_{1v}}, the basis |ψα|\psi_{\alpha}\rangle transforms according to the irreducible representation Γα\Gamma_{\alpha}, so the invariance of the Hamiltonian under the symmetry operation gg dictates P^gH^P^g1=H^\hat{P}_{g}{\hat{H}}\hat{P}_{g}^{-1}={\hat{H}}, where P^g\hat{P}_{g} denotes the operator for symmetry operation gg. This leads to α,βψα|P^g|ψαHαβ(P^g𝓚P^g1)ψβ|P^g1|ψβ=Hαβ(𝓚)\sum_{\alpha^{\prime},\beta^{\prime}}\langle\psi_{\alpha}|\hat{P}_{g}|\psi_{\alpha^{\prime}}\rangle H^{\alpha^{\prime}\beta^{\prime}}(\hat{P}_{g}\boldsymbol{\cal K}\hat{P}_{g}^{-1})\langle\psi_{\beta^{\prime}}|\hat{P}_{g}^{-1}|\psi_{\beta}\rangle=H^{\alpha\beta}({\boldsymbol{\cal K}}), or equivalently,

𝐃α(g)Hαβ(P^g𝓚P^g1)𝐃β(g1)=Hαβ(𝓚),\displaystyle{\bf D}^{\alpha}(g)H^{\alpha\beta}(\hat{P}_{g}{\boldsymbol{\cal K}}\hat{P}_{g}^{-1}){\bf D}^{\beta}(g^{-1})\ =H^{\alpha\beta}({\boldsymbol{\cal K}}), (A-6)

where ψα|P^g|ψα=δαα𝐃α(g)\langle\psi_{\alpha}|\hat{P}_{g}|\psi_{\alpha^{\prime}}\rangle=\delta_{\alpha\alpha^{\prime}}{\bf D}^{\alpha}(g) with 𝐃α(g){\bf D}^{\alpha}(g) is the representation matrix of gg in Γα\Gamma_{\alpha} (in the 1D irreducible representation case here, 11 or 1-1), and P^g𝓚P^g1\hat{P}_{g}{\boldsymbol{\cal K}}\hat{P}_{g}^{-1} denotes the transformation of 𝓚{\boldsymbol{\cal K}} under the symmtery operation gg, e. g., if g=Myg=M_{y} and 𝓚=ky{\boldsymbol{\cal K}}=k_{y}, then P^MykyP^My1=ky\hat{P}_{M_{y}}k_{y}\hat{P}_{M_{y}}^{-1}=-k_{y}.

In constructing the 𝓚\boldsymbol{\cal K} operators, one can also take into account the spin degree of freedom, by including the spin operator 𝐬=(sx,sy,sz){\bf s}=(s_{x},s_{y},s_{z}) in the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian. Note that 𝐬{\bf s} is a pseudovector, we have sxsxs_{x}\to-s_{x}, szszs_{z}\to-s_{z}, and sysys_{y}\to s_{y} under the operation MyM_{y} Zhou , e. g., if g=Myg=M_{y} and 𝓚=kysx{\boldsymbol{\cal K}}=k_{y}s_{x}, then P^MykysxP^My1=(P^MykyP^My1)(P^MysxP^My1)=(ky)(sx)=kysx\hat{P}_{M_{y}}k_{y}s_{x}\hat{P}_{M_{y}}^{-1}=(\hat{P}_{M_{y}}k_{y}\hat{P}_{M_{y}}^{-1})(\hat{P}_{M_{y}}s_{x}\hat{P}_{M_{y}}^{-1})=(-k_{y})(-s_{x})=k_{y}s_{x}.

For general cases in which crystals have high symmetry point groups, the expression of an arbitrary block Hαβ(𝓚)H^{\alpha\beta}({\boldsymbol{\cal K}}) of the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian can be constructed in several standard procedures with the corresponding full character table Bir ; Winkler ; Zhou . In our case, however, the group C1vC_{1v} is the simplest non-trivial group that has only two symmetry operations {𝕀,My}\{\mathbb{I},M_{y}\}, and we can do the analysis just based on mirror symmetry operation MyM_{y}:

i) For blocks Hαα(𝓚)H^{\alpha\alpha}(\boldsymbol{\cal K}) (α=1,2,3\alpha=1,2,3) and H13(𝓚)H^{13}(\boldsymbol{\cal K}): since |ψαψα||\psi_{\alpha}\rangle\langle\psi_{\alpha}| (α=1,2,3\alpha=1,2,3) and |ψ1ψ3||\psi_{1}\rangle\langle\psi_{3}| are even under MyM_{y} operation, to make sure H^\hat{H} is invariant under MyM_{y} operation, then Hαα(𝓚)H^{\alpha\alpha}(\boldsymbol{\cal K}) (α=1,2,3\alpha=1,2,3) and H13(𝓚)H^{13}(\boldsymbol{\cal K}) must be composed by 𝓚\boldsymbol{\cal K} operators that are also even under MyM_{y} operation. Relevant operator combinations that are invariant under MyM_{y} operation are listed in the first row of Table A-I.

Table A-I: The character table for the group C1vC_{1v}, and corresponding operator combinations that are even (first row) and odd (second row) under MyM_{y}. s0s_{0} is the 2×22\times 2 identity matrix. Note that the prefactor ii in some of the terms guarantees TR symmetry, since ii, 𝐤{\bf k}, and 𝐬{\bf s} are odd under the TR operation. Here we only keep terms up to O(k2)O(k^{2}) in the diagonal part and O(k)O(k) in the off-diagonal part.
C1vC_{1v} 𝕀\mathbb{I} MyM_{y}   TR invariant operators
Γ1\Gamma_{1} 11 11   s0s_{0}, ikxik_{x}, kx2k_{x}^{2}, ky2k_{y}^{2}, isyis_{y}, kxsyk_{x}s_{y}, kysxk_{y}s_{x}, kyszk_{y}s_{z}
Γ2\Gamma_{2} 11 1-1   ikyik_{y}, isxis_{x}, iszis_{z}, kxsxk_{x}s_{x}, kxszk_{x}s_{z}, kysyk_{y}s_{y}

ii) For blocks H12(𝓚)H^{12}(\boldsymbol{\cal K}) and H23(𝓚)H^{23}(\boldsymbol{\cal K}): since |ψ1ψ2||\psi_{1}\rangle\langle\psi_{2}| and |ψ2ψ3||\psi_{2}\rangle\langle\psi_{3}| are odd under MyM_{y} operation, then H12(𝓚)H^{12}(\boldsymbol{\cal K}) and H23(𝓚)H^{23}(\boldsymbol{\cal K}) must be composed by 𝓚\boldsymbol{\cal K} operators that are also odd under MyM_{y} operation to ensure that H^\hat{H} is invariant under MyM_{y} operation. Relevant operator combinations that are odd under MyM_{y} are listed in the second row of Table A-I.

After obtaining the terms that transform correctly for each of the blocks, we note further constraints that trim the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian:

(1) The 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian must be Hermitian, which dictates that the invariants for a diagonal block must be Hermitian.

(2) Terms containing both 𝐤{\bf k} and 𝐬{\bf s} are matrix elements of the microscopic spin-orbit interaction H^so(𝐤)𝐤[𝐬×V(𝐫)]{\hat{H}}_{\rm so}({\bf k})\sim{\bf k}\cdot[{\bf s}\times\nabla V({\bf r})] in H^\hat{H} thus terms kxsxk_{x}s_{x} and kysyk_{y}s_{y} will not appear.

(3) For our purposes of estimating the Berry curvature and orbital magnetic moments in the main text, we can neglect the H13H^{13} block. This is because |ψ1|\psi_{1}\rangle and |ψ3|\psi_{3}\rangle are energetically far away from each other (0.5\gtrsim 0.5 eV) and their couplings only have small contributions to Berry curvature and orbital magnetic moment for the conduction bands. Although H13H^{13} block contributes to optical transitions 0.5\gtrsim 0.5 eV, this is beyond our current scope.

The above three considerations trim/eliminate the terms {ikx,isy,kxsx,kysy}\{ik_{x},is_{y},k_{x}s_{x},k_{y}s_{y}\}. For remaining terms, we group them into terms induced by the applied perpendicular electric field, and those that are present in pristine 1T’-WTe2. To do so we perform the following symmetry analysis: when the electric field is not present, inversion symmetry about the inversion center 𝒪0{\cal O}_{0} is recovered, and the operation (x,1/2,z)(-x,1/2,-z) about 𝒪1{\cal O}_{1} becomes a symmetry operation again. Under the operation (x,1/2,z)(-x,1/2,-z), there is no flip in the yy-direction while (kx,ky)(kx,ky)(k_{x},k_{y})\to(-k_{x},k_{y}) and (sx,sy,sz)(sx,sy,sz)(s_{x},s_{y},s_{z})\to(-s_{x},s_{y},-s_{z}). We can see that terms {isx,isz,kxsy,kysx,kysz}\{is_{x},is_{z},k_{x}s_{y},k_{y}s_{x},k_{y}s_{z}\} change sign under this new operation, i. e., they are not invariant under the original symmetry group P21/mP2_{1}/m and can appear only when the perpendicular electric field is applied.

Table A-II: Terms that can appear for 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian blocks. The prefactor ii in some of the terms guarantees TR symmetry, since ii, 𝐤{\bf k}, and 𝐬{\bf s} are odd under the TR operation. s0s_{0} is the 2×22\times 2 identity matrix. Similar to above, we kept terms up to O(k2)O(k^{2}) in the diagonal part and O(k)O(k) in the off-diagonal part.
Hαα(𝓚)H^{\alpha\alpha}(\boldsymbol{\cal K}) H12(𝓚)H^{12}(\boldsymbol{\cal K}), H23(𝓚)H^{23}(\boldsymbol{\cal K})
with or w/o Ez^E{\hat{z}} s0s_{0}, kx2s0k_{x}^{2}s_{0}, ky2s0k_{y}^{2}s_{0} ikys0ik_{y}s_{0}, kxszk_{x}s_{z}
with Ez^E{\hat{z}} kyszk_{y}s_{z}; kxsyk_{x}s_{y}, kysxk_{y}s_{x} iszis_{z}; isxis_{x}

After trimming, classification, and analyzing the physical origin of the terms induced by electric field, we now obtain the general form of the 𝐤𝐩{\bf k}\cdot{\bf p} Hamiltonian (see Table A-II).

Refer to caption
Figure A-1: Energy dispersion near the Fermi surface from the model Eq. (A-13), with an overall band gap 0.055 eV Tang , indicated by the dashed line) (solid lines). Data (dots) extracted from Ref. Qian ; Xu . The parameters for the model are listed in Table A-III.

First we use a least squares fitting to extract coefficients of these invariant operators from known band structure, either from experimental measurements or numerical calculations. From the first principle calculation result Qian ; Xu , we obtained the Hamiltonian H0(𝐤)H_{0}({\bf k}) when there is no external fields. We find

H0(𝐤)=(ϵ10v1+0000ϵ10v100v10ϵ20v3+00v1+0ϵ20v300v30ϵ30000v3+0ϵ3).\displaystyle H_{0}({\bf k})=\left(\begin{array}[]{cccccc}\epsilon_{1}&0&v_{1}^{+}&0&0&0\\ 0&\epsilon_{1}&0&v_{1}^{-}&0&0\\ -v_{1}^{-}&0&\epsilon_{2}&0&v_{3}^{+}&0\\ 0&-v_{1}^{+}&0&\epsilon_{2}&0&v_{3}^{-}\\ 0&0&-v_{3}^{-}&0&\epsilon_{3}&0\\ 0&0&0&-v_{3}^{+}&0&\epsilon_{3}\end{array}\right). (A-13)

where ϵi=ci,0+ci,xkx2+ci,yky2\epsilon_{i}=c_{i,0}+c_{i,x}k_{x}^{2}+c_{i,y}k_{y}^{2}, and vi±=±vi,xkx+ivi,ykyv_{i}^{\pm}=\pm v_{i,x}k_{x}+iv_{i,y}k_{y}. The dispersion is plotted in Fig. A-1, with parameters listed in Table A-III.

Table A-III: Least squares fitted 𝐤𝐩{\bf k}\cdot{\bf p} parameters for a 1T’-WTe2 monolayer without external fields from Ref. Qian ; Xu , with an overall band gap 0.055 eV.
Parameter Value Unit Parameter Value Unit
c1,0c_{1,0} 1.01.0 eV
c2,0c_{2,0} 0 eV
c3,0c_{3,0} 0.4-0.4 eV
c1,xc_{1,x} 11.25-11.25 eV Å2 c1,yc_{1,y} 6.90-6.90 eV Å2
c2,xc_{2,x} 0.27-0.27 eV Å2 c2,yc_{2,y} 1.08-1.08 eV Å2
c3,xc_{3,x} 0.82-0.82 eV Å2 c3,yc_{3,y} 0.990.99 eV Å2
v1,xv_{1,x} 1.711.71 eV Å v1,yv_{1,y} 0.480.48 eV Å
v3,xv_{3,x} 0.480.48 eV Å v3,yv_{3,y} 0.48-0.48 eV Å

The additional terms that are induced by the applied perpendicular electric field EE_{\perp} makes the full Hamiltonian H(𝐤)=H0(𝐤)+H1(𝐤)H({\bf k})=H_{0}({\bf k})+H_{1}({\bf k}), with

H1(𝐤)=(λ1kyα1iδ1,ziδ1,x00α1+λ1kyiδ1,xiδ1,z00iδ1,ziδ1,xλ2kyα2iδ3,ziδ3,xiδ1,xiδ1,zα2+λ2kyiδ3,xiδ3,z00iδ3,ziδ3,xλ3kyα300iδ3,xiδ3,zα3+λ3ky),\displaystyle H_{1}({\bf k})=\left(\begin{array}[]{cccccc}\lambda_{1}k_{y}&\alpha_{1}^{-}&i\delta_{1,z}&i\delta_{1,x}&0&0\\ \alpha_{1}^{+}&-\lambda_{1}k_{y}&i\delta_{1,x}&-i\delta_{1,z}&0&0\\ -i\delta_{1,z}&-i\delta_{1,x}&\lambda_{2}k_{y}&\alpha_{2}^{-}&i\delta_{3,z}&i\delta_{3,x}\\ -i\delta_{1,x}&i\delta_{1,z}&\alpha_{2}^{+}&-\lambda_{2}k_{y}&i\delta_{3,x}&-i\delta_{3,z}\\ 0&0&-i\delta_{3,z}&-i\delta_{3,x}&\lambda_{3}k_{y}&\alpha_{3}^{-}\\ 0&0&-i\delta_{3,x}&i\delta_{3,z}&\alpha_{3}^{+}&-\lambda_{3}k_{y}\end{array}\right), (A-20)

where αi±=±iαi,xkx+αi,yky\alpha_{i}^{\pm}=\pm i\alpha_{i,x}k_{x}+\alpha_{i,y}k_{y} is the commonly seen spin-orbit coupling for ii-th orbital (this is sometimes referred to as “Rashba” spin texture), λiky\lambda_{i}k_{y} is a spin splitting from in-plane IS breaking, and δi,x\delta_{i,x} and δi,z\delta_{i,z} are kk-independent inter-band couplings, see main text for discussion of physical origin.

.2 4×44\times 4 model near the band gap

To obtain the effective 4×44\times 4 Hamiltonian near the band gap, we consider the energy eigenvalue equation

(hquuhd)(ψqψd)=ε(ψqψd),\displaystyle\left(\begin{array}[]{cc}h_{q}&u\\ u^{\dagger}&h_{d}\end{array}\right)\left(\begin{array}[]{c}\psi_{q}\\ \psi_{d}\end{array}\right)=\varepsilon\left(\begin{array}[]{c}\psi_{q}\\ \psi_{d}\end{array}\right), (A-27)

where hqh_{q} (hdh_{d}) is the 4×44\times 4 (2×22\times 2) diagonal block from the original 6×66\times 6 Hamiltonian, and ψq\psi_{q} (ψd\psi_{d}) is the corresponding four (two) component state vector, and uu is the 4×24\times 2 matrix couples hqh_{q} and hdh_{d}.

The second row of Eq. (A-27) allows ψd\psi_{d} to be written in terms of ψq\psi_{q}:

ψd=(εhd)1uψq.\displaystyle\psi_{d}=(\varepsilon-h_{d})^{-1}u^{\dagger}\psi_{q}. (A-28)

Substituting this into the first row of Eq. (A-27) gives an effective eigen equation solely for the ψq\psi_{q} components:

[hq+u(εhd)1u]ψq=εψq.\displaystyle\left[h_{q}+u(\varepsilon-h_{d})^{-1}u^{\dagger}\right]\psi_{q}=\varepsilon\psi_{q}. (A-29)

Performing the standard expansion in small ε\varepsilon as well as rotation procedure Winkler , we obtain the effective Hamiltonian near the band gap as

h~q=𝒮1/2(hquhd1u)𝒮1/2,𝒮=1+uhd2u,\displaystyle\tilde{h}_{q}={\cal S}^{-1/2}(h_{q}-uh_{d}^{-1}u^{\dagger}){\cal S}^{-1/2},\quad{\cal S}=1+uh_{d}^{-2}u^{\dagger}, (A-30)

valid when ε\varepsilon is small, and we have used the rotated basis ψ=𝒮1/2ψq\psi={\cal S}^{1/2}\psi_{q}.

Following the above analysis, we now derive the 4×44\times 4 model for the pristine part. From Eq. (A-13) we have

hq=(ϵ10v1+00ϵ10v1v10ϵ200v1+0ϵ2),\displaystyle h_{q}=\left(\begin{array}[]{cccc}\epsilon_{1}&0&v_{1}^{+}&0\\ 0&\epsilon_{1}&0&v_{1}^{-}\\ -v_{1}^{-}&0&\epsilon_{2}&0\\ 0&-v_{1}^{+}&0&\epsilon_{2}\end{array}\right), (A-35)
u=(00v3+0000v3),\displaystyle u^{\dagger}=\left(\begin{array}[]{cccc}0&0&v_{3}^{+}&0\\ 0&0&0&v_{3}^{-}\\ \end{array}\right), (A-38)

and

hd=(ϵ300ϵ3),\displaystyle h_{d}=\left(\begin{array}[]{cc}\epsilon_{3}&0\\ 0&\epsilon_{3}\end{array}\right), (A-41)

where ϵi=ci,0+ci,xkx2+ci,yky2\epsilon_{i}=c_{i,0}+c_{i,x}k_{x}^{2}+c_{i,y}k_{y}^{2}, and vi±=±vi,xkx+ivi,ykyv_{i}^{\pm}=\pm v_{i,x}k_{x}+iv_{i,y}k_{y}. Using hdh_{d} and uu above, we have

h~q=(ϵc0v+00ϵc0vv0ϵv00v+0ϵv),\displaystyle\tilde{h}_{q}=\left(\begin{array}[]{cccc}\epsilon_{c}&0&v^{+}&0\\ 0&\epsilon_{c}&0&v^{-}\\ -v^{-}&0&\epsilon_{v}&0\\ 0&-v^{+}&0&\epsilon_{v}\end{array}\right), (A-46)

where ϵc=ϵ1\epsilon_{c}=\epsilon_{1}, and

ϵv=11+rϵ2r1+rϵ3,v=11+rv1.\displaystyle\epsilon_{v}=\frac{1}{1+r}\epsilon_{2}-\frac{r}{1+r}\epsilon_{3},\quad v=\sqrt{\frac{1}{1+r}}\,v_{1}. (A-47)

Here the kk-dependent ratio rr is

r=(v3,xkx)2+(v3,yky)2ϵ32,\displaystyle r=\frac{(v_{3,x}k_{x})^{2}+(v_{3,y}k_{y})^{2}}{\epsilon_{3}^{2}}, (A-48)

which controls the renormalization of ϵ2\epsilon_{2} and v1v_{1}. It becomes zero when v3=0v_{3}=0, i. e., when ψ2\psi_{2} and ψ3\psi_{3} do not couple with each other, r=0r=0 and there is no renormalization. We note that the form of this pristine part in Eq. (A-46) is consistent with the model proposed in Ref. Qian ; for a full discussion see the section “Unitary transformation and form of Hamiltonian” below.

If we re-order the basis to {ψc\{\psi_{c\uparrow}, ψv\psi_{v\uparrow}; ψc\psi_{c\downarrow}, ψv}\psi_{v\downarrow}\}, this gives the BHZ-type pristine part,

h0=ϵ¯+(mv+00vm0000mv00v+m),\displaystyle h_{0}=\bar{\epsilon}+\left(\begin{array}[]{cccc}m&v^{+}&0&0\\ -v^{-}&-m&0&0\\ 0&0&m&v^{-}\\ 0&0&-v^{+}&-m\end{array}\right), (A-53)

where ϵ¯=(ϵc+ϵv)/2\bar{\epsilon}=(\epsilon_{c}+\epsilon_{v})/2, m=(ϵcϵv)/2m=(\epsilon_{c}-\epsilon_{v})/2. Together with the electric field induced part (neglecting the far away ψ3\psi_{3} band),

h1=(λkyiδzαiδxiδzλkyiδxαα+iδxλkyiδziδxα+iδzλky),\displaystyle h_{1}=\left(\begin{array}[]{cccc}\lambda k_{y}&i\delta_{z}&\alpha^{-}&i\delta_{x}\\ -i\delta_{z}&\lambda k_{y}&i\delta_{x}&\alpha^{-}\\ \alpha^{+}&-i\delta_{x}&-\lambda k_{y}&-i\delta_{z}\\ -i\delta_{x}&\alpha^{+}&i\delta_{z}&-\lambda k_{y}\end{array}\right), (A-58)

we obatined the 4×44\times 4 effective hamiltonian near the gap opening

heff=h0+h1.\displaystyle h^{\rm eff}=h_{0}+h_{1}. (A-59)

When focusing on the dispersions and Berry curvatures near the gap opening, we find a convenient estimate for vv:

v=11+r0v1,r0=r(𝐤0),\displaystyle v=\sqrt{\frac{1}{1+r_{0}}}\,v_{1},\quad r_{0}=r({\bf k}_{0}), (A-60)

where 𝐤0=(0,k0){\bf k}_{0}=(0,k_{0}) is the position of the band edge with k0=0.385Å1k_{0}=0.385~{\rm\AA ^{-1}}. By doing this, we obtained the dispersion and a Berry curvature distribution which agree well with the six band model near the gap opening (see solid and dashed lines in Fig. 1d and Fig. 1e for comparison).

.3 Berry curvature at the band edge from 4×44\times 4 model
(δx,z=0\delta_{x,z}=0 case)

Using the 4×44\times 4 band model [see Eq. (5) and Eq. (6) of the main text] to describe 1T’-WTe2, we can express its Berry curvature near the band edge analytically.

Without the electric field induced part h1h_{1}, the BHZ-type pristine part h0h_{0} can be viewed as two decoupled 2×22\times 2 blocks: spin-up block hh_{\uparrow} and spin-down block hh_{\downarrow}. The two blocks form a time-reversal pair

h(𝐤)=h(𝐤)=ϵ¯𝐤+(m𝐤v𝐤+v𝐤m𝐤),\displaystyle h_{\uparrow}({\bf k})=h_{\downarrow}^{*}(-{\bf k})=\bar{\epsilon}_{{\bf k}}+\left(\begin{array}[]{cc}m_{{\bf k}}&v_{{\bf k}}^{+}\\ -v_{{\bf k}}^{-}&-m_{{\bf k}}\end{array}\right), (A-63)

where v𝐤±=±vxkx+ivykyv_{{\bf k}}^{\pm}=\pm v_{x}k_{x}+iv_{y}k_{y}. The two 2×22\times 2 blocks share the same dispersion relation and are spin-degenerate:

ετ(0)(𝐤)=ϵ¯𝐤±τΔ𝐤,Δ𝐤=(vxkx)2+(vyky)2+m𝐤2,\displaystyle\varepsilon_{\tau\uparrow\hskip-1.22911pt\downarrow}^{(0)}({\bf k})=\bar{\epsilon}_{{\bf k}}\pm\tau\Delta_{{\bf k}},\quad\Delta_{{\bf k}}=\sqrt{(v_{x}k_{x})^{2}+(v_{y}k_{y})^{2}+m_{{\bf k}}^{2}}, (A-64)

with the corresponding eigenstates:

ψτ(0)(𝐤)(m𝐤+τΔ𝐤,v𝐤,0,0)T,\displaystyle\psi_{\tau\uparrow}^{(0)}({\bf k})\sim(m_{{\bf k}}+\tau\Delta_{{\bf k}},-v_{{\bf k}}^{-},0,0)^{T},
ψτ(0)(𝐤)(0,0,m𝐤+τΔ𝐤,v𝐤+)T,\displaystyle\psi_{\tau\downarrow}^{(0)}({\bf k})\sim(0,0,m_{{\bf k}}+\tau\Delta_{{\bf k}},-v_{{\bf k}}^{+})^{T}, (A-65)

where τ=±\tau=\pm denotes conduction or valence band, and 2Δ𝐤2\Delta_{{\bf k}} is the energy difference between the conduction and valence bands.

When an external perpendicular electric field is applied and if the spin-orbit couplings induced by the field is much weaker than the atomic spin-orbit couplings (αx,y,λvx,y\alpha_{x,y},\lambda\ll v_{x,y}), we then treat h1(𝐤)h_{1}({\bf k}) as a small perturbation to the pristine part h0(𝐤)h_{0}({\bf k}). We first note that for non-zero α\alpha, and within the framework of degenerate perturbation (i.e. neglecting states that are far away in energy), h1(𝐤)h_{1}({\bf k}) hybridizes the unperturbed spin up state ψτ(0)(𝐤)\psi_{\tau\uparrow}^{(0)}({\bf k}) and spin down state ψτ(0)(𝐤)\psi_{\tau\downarrow}^{(0)}({\bf k}) in the same band τ\tau into spin split states ψτξ(𝐤)\psi_{\tau\xi}({\bf k}), with higher (ξ=+1\xi=+1) or lower (ξ=1\xi=-1) energies:

ψτξ(𝐤)=cτξ(𝐤)ψτ(0)(𝐤)+cτξ(𝐤)ψτ(0)(𝐤).\displaystyle\psi_{\tau\xi}({\bf k})=c_{\tau\uparrow}^{\xi}({\bf k})\psi_{\tau\uparrow}^{(0)}({\bf k})+c_{\tau\downarrow}^{\xi}({\bf k})\psi_{\tau\downarrow}^{(0)}({\bf k}). (A-66)

Interestingly, in the αλ,δz\alpha\ll\lambda,\delta_{z} limit, the unperturbed spin up state ψτ(0)(𝐤)\psi_{\tau\uparrow}^{(0)}({\bf k}) and spin down state ψτ(0)(𝐤)\psi_{\tau\downarrow}^{(0)}({\bf k}) do not hybridize with each other. Even so, their degeneracies are lifted by λky\lambda k_{y}:

ψτ±(𝐤)=ψτ(0)(𝐤),ετξ(𝐤)=ϵ¯𝐤+τΔ𝐤+ξ|λky|.\displaystyle\psi_{\tau\pm}({\bf k})=\psi_{\tau\uparrow\hskip-1.22911pt\downarrow}^{(0)}({\bf k}),\quad\varepsilon_{\tau\xi}({\bf k})=\bar{\epsilon}_{{\bf k}}+\tau\Delta_{{\bf k}}+\xi\left|\lambda k_{y}\right|. (A-67)

The Berry curvatures for these non-degenerate states ψτξ\psi_{\tau\xi} are well defined and read

Ωτξ(0)(𝐤)=sgn(ky)τξ2vxvyΔ𝐤3(1𝐤)m𝐤.\displaystyle\Omega_{\tau\xi}^{(0)}({\bf k})={\rm sgn}(k_{y})\frac{\tau\xi}{2}\frac{v_{x}v_{y}}{\Delta_{{\bf k}}^{3}}(1-{\bf k}\cdot\nabla)m_{{\bf k}}. (A-68)

When αλ\alpha\sim\lambda, spin up state ψτ(0)(𝐤)\psi_{\tau\uparrow}^{(0)}({\bf k}) and spin down state ψτ(0)(𝐤)\psi_{\tau\downarrow}^{(0)}({\bf k}) start to hybridize to form the spin split states ψτξ\psi_{\tau\xi}. The Berry curvature amplitudes for these hybridized states ψτξ(𝐤)\psi_{\tau\xi}({\bf k}) are smaller than that of ψτ(0)(𝐤)\psi_{\tau\uparrow\hskip-1.22911pt\downarrow}^{(0)}({\bf k}) because the spin up and spin down states have opposite Berry curvatures.

The general form of the Berry curvature Ωτξ(𝐤)\Omega_{\tau\xi}({\bf k}) for ψτξ(𝐤)\psi_{\tau\xi}({\bf k}) is complicated. Fortunately, along kx=0k_{x}=0 about which the Berry curvature is even, i. e., Ω(kx,ky)=Ω(kx,ky)\Omega(k_{x},k_{y})=\Omega(-k_{x},k_{y}), which comes from the TRS and the mirror symmetry in the yy-direction, its analytical form is greatly simplified:

Ωτξ(0,ky)\displaystyle\Omega_{\tau\xi}(0,k_{y}) =|cτξ|2Ωτ(0)(0,ky)+|cτξ|2Ωτ(0)(0,ky)\displaystyle=|c_{\tau\uparrow}^{\xi}|^{2}\Omega_{\tau\uparrow}^{(0)}(0,k_{y})+|c_{\tau\downarrow}^{\xi}|^{2}\Omega_{\tau\downarrow}^{(0)}(0,k_{y})
=(|cτξ|2|cτξ|2)Ωτ(0)(0,ky).\displaystyle=\left(|c_{\tau\uparrow}^{\xi}|^{2}-|c_{\tau\downarrow}^{\xi}|^{2}\right)\Omega_{\tau\uparrow}^{(0)}(0,k_{y}). (A-69)

where cτξc_{\tau\uparrow}^{\xi} and cτξc_{\tau\downarrow}^{\xi} satisfy

|cτξ|2|cτξ|2=τξλsgn(ky)(αy2+λ2)1/2.\displaystyle|c_{\tau\uparrow}^{\xi}|^{2}-|c_{\tau\downarrow}^{\xi}|^{2}=\tau\xi\,\frac{\lambda\,{\rm sgn}(k_{y})}{(\alpha_{y}^{2}+\lambda^{2})^{1/2}}. (A-70)

With this, the Berry curvature Ωτξ(𝐤)\Omega_{\tau\xi}({\bf k}) at the band edge 𝐤=(kx=0,ky){\bf k}^{\prime}=(k_{x}=0,k_{y}) is

Ωτ±(𝐤)\displaystyle\Omega_{\tau\pm}({\bf k}^{\prime}) =λsgn(ky)(λ2+αy2)1/2τξ2vxvyΔ𝐤3(1𝐤)m𝐤\displaystyle=\frac{\lambda{\rm sgn}(k_{y})}{(\lambda^{2}+\alpha_{y}^{2})^{1/2}}\frac{\tau\xi}{2}\frac{v_{x}v_{y}}{\Delta_{{\bf k}^{\prime}}^{3}}(1-{\bf k}^{\prime}\cdot\nabla)m_{{\bf k}^{\prime}}
=λ(λ2+αy2)1/2Ωτ(0)(𝐤).\displaystyle=\frac{\lambda}{(\lambda^{2}+\alpha_{y}^{2})^{1/2}}\Omega_{\tau\uparrow\hskip-1.22911pt\downarrow}^{(0)}({\bf k}^{\prime}). (A-71)

.4 Berry curvature and magnetic moment distribution
(λ=αx,y=δx=0\lambda=\alpha_{x,y}=\delta_{x}=0, δz0\delta_{z}\neq 0 case)

Here we show the anisotropic Berry curvature and magnetic moment distribution in kk-space away from the gap opening, using the six band description (SBD) we developed (see Fig. A-2). The formula for calculating Berry curvature and moment distribution are

Ωn(𝐤)=2Rennin|H/kx|nn|H/ky|n(εnεn)2,\displaystyle\Omega_{n}({\bf k})=2{\rm Re}\,\sum_{n^{\prime}\neq n}\frac{i\langle n|\partial H/\partial k_{x}|n^{\prime}\rangle\langle n^{\prime}|\partial H/\partial k_{y}|n\rangle}{(\varepsilon_{n}-\varepsilon_{n^{\prime}})^{2}}, (A-72)
mnint(𝐤)=eRennin|H/kx|nn|H/ky|nεnεn,\displaystyle m_{n}^{\rm int}({\bf k})=\frac{e}{\hbar}{\rm Re}\,\sum_{n^{\prime}\neq n}\frac{i\langle n|\partial H/\partial k_{x}|n^{\prime}\rangle\langle n^{\prime}|\partial H/\partial k_{y}|n\rangle}{\varepsilon_{n}-\varepsilon_{n^{\prime}}}, (A-73)

where n={τξ}n=\{\tau\xi\} is the short-hand form, and HH is the full six band hamiltonian.

Refer to caption
Figure A-2: a,b Berry curvature and magnetic moment distribution for the spin split conduction band with lower energy in kk-space. Parameters for the pristine part H0H_{0} are listed in Table A-III, while for H1H_{1} we used α,λ,δx=0\alpha,\lambda,\delta_{x}=0, and δz=0.025eV\delta_{z}=0.025~{\rm eV}.

.5 Non-linear anomalous Hall effect

Just as mnint(𝐤)m_{n}^{\rm int}({\bf k}) discussed in the main text gives rise to ME, Ωn(𝐤)\Omega_{n}({\bf k}) in the bands enable 1T’-WTe2 to exhibit a quantum non-linear Hall effect at zero magnetic field. This can be seen under general symmetry considerations Sodemann . For the convenience of the reader, we outline this symmetry analysis for a 2D system that only has in-plane mirror symmetry (e.g., 1T’-WTe2). The non-linear Hall current can be written as ja=χabbEbEbj_{a}=\chi_{abb}E_{b}E_{b} (a,b=x,ya,b=x,y). Under the operation (x,y)(x,y)(x,y)\to(x,-y), we have (jx,jy)(jx,jy)(j_{x},j_{y})\to(j_{x},-j_{y}) and (Ex,Ey)(Ex,Ey)(E_{x},E_{y})\to(E_{x},-E_{y}). This allows a non-zero χxyy\chi_{xyy} (while χyxx\chi_{yxx} vanishes). Under an in-plane DC electric field, χxyy\chi_{xyy} can be obtained using Sodemann

χxyy\displaystyle\chi_{xyy} =τ2e32n,𝐤fn𝐤(0)kyΩn(𝐤),\displaystyle=\frac{\tau}{2}\frac{e^{3}}{\hbar^{2}}\sum_{n,{\bf k}}\,f_{n{\bf k}}^{(0)}\,\partial_{k_{y}}\Omega_{n}({\bf k}), (A-74)

where τ\tau is the transport scattering time. Similar to Eq. (10) above, Ωn(𝐤)\Omega_{n}({\bf k}) is an odd function of kyk_{y} [see Fig. A-2(a)]. As a result, nonzero χabb\chi_{abb} only occurs when a=xa=x and b=yb=y: only electric field along yy induces a non-linear Hall effect along xx. When 𝐄{\bf E} is parallel to the xx-direction, the nonlinear Hall effect (as well as the kinetic ME effect) vanishes.

To illustrate the quantum non-linear Hall effect, we numerically integrate Eq. (A-74) to obtain a finite non-linear Hall current conductivity χxyy\chi_{xyy} in Fig. A-3b using a scattering time τ=50fs\tau=50~{\rm fs}. Similar to MzM_{z} in the main text, we used the SBD description in order to capture the full reciprocal space distribution of the Berry curvature. This non-linear Hall conductivity can be probed in a conventional Hall bar measurement (Fig. A-3) and provides a fully electrical way of mapping the Berry curvature (dipole).

Refer to caption
Figure A-3: a Schematic of a 1T’-WTe2 monolayer under a perpendicular electric field E𝐳^E_{\perp}\hat{{\bf z}} and an in-plane electric field EyE_{y}, which can give rise to a non-linear Hall current jxj_{x}. (b) Calculated non-linear Hall conductivity χxyy\chi_{xyy} (blue) from Eq. (A-74) using τ=50fs\tau=50~{\rm fs}. Parameters used for the pristine part are the same as those in Fig. 1; for the electric field induced part we used α,λ,δx=0\alpha,\lambda,\delta_{x}=0, and δz=0.075eV\delta_{z}=0.075~{\rm eV} (blue), 0.05eV0.05~{\rm eV} (green), and 0.025eV0.025~{\rm eV} (red).

.6 Unitary transformation and form of Hamiltonian

We note that the model in the supplement of Ref. Qian is equivalent to our model for the pristine part. For the convenience of the reader, we reproduce the four band hamiltonian in Ref. Qian as

HF=(ϵc0ivxkxvyky0ϵcvykyivxkxivxkxvykyϵv0vykyivxkx0ϵv).\displaystyle H_{F}=\left(\begin{array}[]{cccc}\epsilon_{c}&0&-iv_{x}k_{x}&v_{y}k_{y}\\ 0&\epsilon_{c}&v_{y}k_{y}&-iv_{x}k_{x}\\ iv_{x}k_{x}&v_{y}k_{y}&\epsilon_{v}&0\\ v_{y}k_{y}&iv_{x}k_{x}&0&\epsilon_{v}\end{array}\right). (A-79)

To see the equivalence, we use the unitary transformation

U=12(1100110000ii00ii).\displaystyle U=\frac{1}{\sqrt{2}}\left(\begin{array}[]{cccc}1&1&0&0\\ 1&-1&0&0\\ 0&0&i&i\\ 0&0&i&-i\end{array}\right). (A-84)

Applying the unitary transformation, we have

UHFU=h~q,\displaystyle U^{\dagger}H_{F}U=\tilde{h}_{q}, (A-85)

reproducing Eq. (A-46).