arXiv is now an independent nonprofit! Learn more
License: CC BY 4.0
arXiv:2302.09514v1 [cond-mat.mtrl-sci] 19 Feb 2023

Magnetic bulk photovoltaic effect as a probe of magnetic structures of EuSn2As2\rm{EuSn_{2}As_{2}}

Hanqi Pi Affiliation: Beijing National Laboratory for Condensed Matter Physics and Institute of physics, Chinese academy of sciences, Beijing 100190, China Affiliation: University of Chinese academy of sciences, Beijing 100049, China    Shuai Zhang Affiliation: Beijing National Laboratory for Condensed Matter Physics and Institute of physics, Chinese academy of sciences, Beijing 100190, China Affiliation: University of Chinese academy of sciences, Beijing 100049, China    Hongming Weng Email: hmweng@iphy.ac.cn Affiliation: Beijing National Laboratory for Condensed Matter Physics and Institute of physics, Chinese academy of sciences, Beijing 100190, China Affiliation: University of Chinese academy of sciences, Beijing 100049, China Affiliation: Songshan Lake Materials Laboratory, Dongguan, Guangdong 523808, China
August 24, 2026
Abstract

The bulk photovoltaic effect (BPVE) is a second-order optical process in noncentrosymmetric materials that converts the light into DC currents. BPVE is classified into shift current and injection current according to the generation mechanisms, whose dependence on the polarization of light is sensitive to the spatial and time-reversal symmetry of materials. In this work, we present a comprehensive study on the BPVE response of EuSn2As2\mathrm{EuSn_{2}As_{2}} with different magnetic structures through symmetry analysis and first-principles calculation. We demonstrate that the interlayer antiferromagnetic (AFM) EuSn2As2\mathrm{EuSn_{2}As_{2}} of even-layer breaks the inversion symmetry and has the second-order optical responses. Moreover, the bilayer AFM EuSn2As2\mathrm{EuSn_{2}As_{2}} not only displays distinct BPVE responses when magnetic moments align in different directions, but also shows symmetry-related responses in two phases which have mutually perpendicular in-plane magnetic moments. Due to the dependence of BPVE responses on the polarization of light and magnetic symmetry, these magnetic structures can be distinguished by the circular polarized light with well-designed experiments. Our work demonstrates the feasibility of the BPVE response as a tool to probe the magnetic structure.

I Introduction

Nonlinear optical phenomena play an essential role in condensed matter physics to advance fundamental knowledge about materials and stimulate the development of technological applications. For instance, the second harmonic generation (SHG) has been applied to probe the electronic, magnetic and crystallographic structures of materials[1, 2, 3, 4, 5, 6, 7, 8]. The high-harmonic generation (HHG) recently has been intensively studied to reveal the electron dynamics[9], band structures[10] and topological phase transitions[11]. Among various nonlinear optical processes, the bulk photovoltaic effect (BPVE) in noncentrosymmetric materials converting light into a DC current has gained numerous interests[12, 13, 14, 15, 16, 17, 18]. As it surpasses the Shockley-Queisser limit and generates above-band-gap photovoltages, the BPVE is expected to be a replacement for the conventional solar cell[19, 20]. Besides, BPVE can be utilized to develop promising photodetectors because it does not require a bias voltage which would cause the dark current. Furthermore, due to the close relationship with geometric quantities such as Berry connection and Berry curvature[21, 22, 23], the BPVE is employed to obtain the band geometry and topology information of materials[24, 25, 26].

The photocurrent in BPVE consists of the shift current and the injection current, which are induced by the change in the charge center and group velocity of electrons during the interband transitions, respectively[27, 22]. The study on the BPVE photocurrents has been confined to nonmagnetic materials for decades[28, 29, 30, 27, 17, 31]. In systems with time-reversal symmetry (𝒯\mathcal{T}), these two currents could be distinguished by their dependence on the polarization of incident photons. While the injection current is excited only by the circular polarized light, the shift current can be generated by light regardless of polarization[27, 32]. Besides, the circular injection current alters its direction when the helicity of incident light changes while the linear shift current does not[33].

In recent years, a series of works[34, 35, 36, 32, 37] have shown the growing interests in the BPVE response of magnetic materials, which has a contrast dependence on the polarization of light compared to nonmagnetic ones. In magnetic materials where 𝒯\mathcal{T} is broken and the space-time inversion symmetry 𝒫𝒯\mathcal{PT} is preserved, shift current excited by the linear polarized light is prohibited while injection current excited by light of any polarization is allowed. It results in the linear injection current and circular shift current in the 𝒫𝒯\mathcal{PT} magnetic materials[34, 35]. Moreover, in system with neither 𝒯\mathcal{T} nor 𝒫𝒯\mathcal{PT}, both BPVE photocurrents can be induced by either linear or circular polarized light[32].

Due to the sensitivity to the crystalline symmetry and the polarization of light, BPVE responses could be employed to probe the magnetic structure of materials. We take the magnetic material EuSn2As2\mathrm{EuSn_{2}As_{2}} as an example and analyze the BPVE in three magnetic structures of EuSn2As2\mathrm{EuSn_{2}As_{2}}. The symmetry analysis demonstrates that BPVE is allowed to exist only in even-layer EuSn2As2\mathrm{EuSn_{2}As_{2}} with antiferromagnetic (AFM) order. BPVE in three AFM phases of bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} are investigated through group representation theory and first-principles calculation. The result shows that both linear injection current and circular shift current can be generated in AFM bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} with the in-plane magnetic moments, while only linear injection current exist when the magnetic moments are out of plane. Besides, the two magnetic structures with mutually perpendicular in-plane magnetic moments has the similar BPVE responses, which can be explained by the connection between their magnetic symmetry groups, namely their magnetic moments alignment is related by the C4zC_{4z} rotation. By exploiting the discrepancies among their nonlinear optical responses, we provide an experimental protocol to distinguish the magnetic structures by two circular polarized light beams with the opposite helicity.

II Results

II.1 The bulk photovoltaic effect

When illuminated by the monochromatic light 𝑬~(t)=𝑬(ω)eiωt+c.c\bm{\tilde{E}}(t)=\bm{E}(\omega)e^{-i\omega t}+\operatorname{c.c}, noncentrosymmetric materials can give rise to a DC photocurrent described by the following relation[27],

Ja=σabc(0,ω,ω)Eb(ω)Ec(ω)+σabc(0,ω,ω)Eb(ω)Ec(ω)=σabc(0,ω,ω)Eb(ω)Ec(ω)+c.c.=2σabc(0,ω,ω)Eb(ω)Ec(ω),\begin{split}J^{a}=&\sigma^{abc}(0;-\omega,\omega)E_{b}(-\omega)E_{c}(\omega)\\ +&\sigma^{abc}(0;\omega,-\omega)E_{b}(\omega)E_{c}(-\omega)\\ =&\sigma^{abc}(0;-\omega,\omega)E_{b}(-\omega)E_{c}(\omega)+\operatorname{c.c.}\\ =&2\sigma^{abc}(0;-\omega,\omega)E_{b}(-\omega)E_{c}(\omega),\end{split} (1)

where we use the intrinsic permutation symmetry of nonlinear optical coefficients to derive the final expression. Different from the photovoltaic effect in a pp-nn junction, the direct current generated in noncentrosymmetric homogeneous crystals comes from the second-order optical process and is termed as bulk photovoltaic effect (BPVE) or photogalvanic effect (PGE)[31].

As the photocurrent is a real quantity and Eb(ω)=Eb(ω)E_{b}(-\omega)=E_{b}^{*}(\omega), we take the complex conjugate of (1) and obtain [σabc(0,ω,ω)]=σacb(0,ω,ω)\left[\sigma^{abc}(0;-\omega,\omega)\right]^{*}=\sigma^{acb}(0;-\omega,\omega). Therefore, the real/imaginary part of σabc(0,ω,ω)\sigma^{abc}(0;-\omega,\omega) is symmetric/antisymmetric to the exchange of the latter two index,

Reσabc(0,ω,ω)=Reσacb(0,ω,ω)\displaystyle\operatorname{Re}\sigma^{abc}(0;-\omega,\omega)=\operatorname{Re}\sigma^{acb}(0;-\omega,\omega) (2)
Imσabc(0,ω,ω)=Imσacb(0,ω,ω),\displaystyle\operatorname{Im}\sigma^{abc}(0;-\omega,\omega)=-\operatorname{Im}\sigma^{acb}(0;-\omega,\omega),

We denote Reσ(0,ω,ω)\operatorname{Re}\sigma(0;-\omega,\omega) as σL\sigma_{L} and iImσ(0,ω,ω)i\operatorname{Im}\sigma(0;-\omega,\omega) as iσCi\sigma_{C}. With this notation, the definition of BPVE (1) can be reformulated as[24, 38],

Ja=2\displaystyle J^{a}=2 σLabcEbEc+2iσCad[𝑬×𝑬]d.\displaystyle\sigma_{L}^{abc}E^{*}_{b}E_{c}+2i\sigma_{C}^{ad}[\bm{E^{*}\times E}]_{d}. (3)

Because 𝑬×𝑬\bm{E^{*}\times E} is required to be imaginary, the photocurrent described by σC\sigma_{C} can only be contributed by the circular polarized light and is called the circular photogalvanic effect (CPGE). On the contrary, PGE described by σL\sigma_{L} is called the linear photogalvanic effect (LPGE). Nonetheless, LPGE can be generated under the illumination of either linear or cicular polarized light. Moreover, because the change of helicity of circular polarized light is equivalent to the exchange of 𝑬\bm{E^{*}} and 𝑬\bm{E}, the photocurrent of CPGE will alter its direction when the circular polarized light reverses its helicity while the LPGE does not[31].

Within the framework of perturbation theory and only considering the interband transitions, we can obtain the expression of BPVE described by the following two parts[39, 40, 27],

dJinjectadt\displaystyle\frac{dJ^{a}_{\text{inject}}}{dt} =2ηinjectabc(0,ω,ω)Eb(ω)Ec(ω)\displaystyle=2\eta_{\text{inject}}^{abc}\left(0;-\omega,\omega\right)E_{b}\left(-\omega\right)E_{c}\left(\omega\right) (4)
=2e3π2nm𝒌Δmnarnmbrmncfnmδ(ωmnω)\displaystyle=-\frac{2e^{3}\pi}{\hbar^{2}}\sum_{nm\bm{k}}\Delta_{mn}^{a}r_{nm}^{b}r_{mn}^{c}f_{nm}\delta\left(\omega_{mn}-\omega\right)
×Eb(ω)Ec(ω)\displaystyle\times E_{b}\left(-\omega\right)E_{c}\left(\omega\right)
Jshifta\displaystyle J^{a}_{\text{shift}} =2σshiftabc(0,ω,ω)Eb(ω)Ec(ω)\displaystyle=2\sigma_{\text{shift}}^{abc}\left(0;-\omega,\omega\right)E_{b}\left(-\omega\right)E_{c}\left(\omega\right) (5)
=ie3π2nm𝒌fnm[(rmnc);karnmb(rnmb);karmnc]\displaystyle=-\frac{ie^{3}\pi}{\hbar^{2}}\sum_{nm\bm{k}}f_{nm}\left[\left(r_{mn}^{c}\right)_{;k^{a}}r_{nm}^{b}-\left(r_{nm}^{b}\right)_{;k^{a}}r_{mn}^{c}\right]
×δ(ωmnω)Eb(ω)Ec(ω)\displaystyle\times\delta(\omega_{mn}-\omega)E_{b}\left(-\omega\right)E_{c}\left(\omega\right)
=e3π2nm𝒌fnmrnmbrmnc(mn;acnm;ab)\displaystyle=-\frac{e^{3}\pi}{\hbar^{2}}\sum_{nm\bm{k}}f_{nm}r_{nm}^{b}r_{mn}^{c}\left(\mathcal{R}_{mn;a}^{c}-\mathcal{R}_{nm;a}^{b}\right)
×δ(ωmnω)Eb(ω)Ec(ω),\displaystyle\times\delta(\omega_{mn}-\omega)E_{b}\left(-\omega\right)E_{c}\left(\omega\right),

where Δmnavmavna\Delta_{mn}^{a}\equiv v_{m}^{a}-v_{n}^{a} and ωmnEmEn\hbar\omega_{mn}\equiv E_{m}-E_{n} denotes the group velocity along aa and eigen-energy difference between band mm and nn, respectively. rnmb=un𝒌|ikb|un𝒌r_{nm}^{b}=\left\langle u_{n\bm{k}}\right|i\partial_{k^{b}}\left|u_{n\bm{k}}\right\rangle is the transition dipole moment along bb between band mm and nn where |un𝒌\left|u_{n\bm{k}}\right\rangle is the periodic part of Bloch wavefunction[41]. fnf_{n} is the Fermi-Dirac distribution of band nn and fnmfnfmf_{nm}\equiv f_{n}-f_{m}. (rmnc);kaarmncirmnc(AmmaAnna)\left(r_{mn}^{c}\right)_{;k^{a}}\equiv{\partial_{a}r^{c}_{mn}}-ir^{c}_{mn}\left({A}^{a}_{mm}-A^{a}_{nn}\right) is the generalized derivative and Anna=un𝒌|ika|un𝒌A_{nn}^{a}=\left\langle u_{n\bm{k}}\right|i\partial_{k^{a}}\left|u_{n\bm{k}}\right\rangle is the Abelian Berry connection. mn;acilnrmncka+AmmaAnna\mathcal{R}_{mn;a}^{c}\equiv i\frac{\partial\ln r_{mn}^{c}}{\partial_{k^{a}}}+A^{a}_{mm}-A^{a}_{nn} is the shift vector indicating the change of electron position in real space when transiting from band nn to mm. Note that we adopt the definition of shift vector in Ref.[32] which is different the one in nonmagnetic systems[27, 29, 35].

We could see that (4) describes a DC current generated from the change of electron group velocity that grows linearly with time. In real materials, however, the photocurrent will saturate after a time τ\tau because of the impurities, defects, and other scattering mechanisms. Therefore, the photocurrent in (4) is named injection current. Similarly, the DC current in (5) originating from the change of electron position in real space is called shift current. According to their dependence on the polarization of light as mentioned above, the two photocurrents can be further classified into linear/circular injection current and linear/circular shift current. We obtain the corresponding response coefficients by separating the real and imaginary part of ηinject\eta_{\text{inject}} and σshift\sigma_{\text{shift}},

2ηLIabc(0,ω,ω)=\displaystyle 2\eta^{abc}_{\text{LI}}(0;-\omega,\omega)= e3π2nm𝒌fnmΔmna{rnmb,rmnc}\displaystyle-\frac{e^{3}\pi}{\hbar^{2}}\sum_{nm\bm{k}}f_{nm}\Delta_{mn}^{a}\left\{r_{nm}^{b},r_{mn}^{c}\right\} (6)
×δ(ωmnω)\displaystyle\times\delta\left(\omega_{mn}-\omega\right)
2ηCI abc(0,ω,ω)=\displaystyle 2\eta^{abc}_{\text{CI }}(0;-\omega,\omega)= ie3π2nm𝒌fnmΔmna[rnmb,rmnc]\displaystyle\frac{ie^{3}\pi}{\hbar^{2}}\sum_{nm\bm{k}}f_{nm}\Delta_{mn}^{a}\left[r_{nm}^{b},r_{mn}^{c}\right]
×δ(ωmnω)\displaystyle\times\delta\left(\omega_{mn}-\omega\right)
2σLSabc(0,ω,ω)=\displaystyle 2\sigma^{abc}_{\text{LS}}(0;-\omega,\omega)= ie3π22nm𝒌fnm{(rmnc);ka,rnmb}\displaystyle-\frac{ie^{3}\pi}{2\hbar^{2}}\sum_{nm\bm{k}}f_{nm}\left\{\left(r_{mn}^{c}\right)_{;k^{a}},r_{nm}^{b}\right\} (7)
×[δ(ωmnω)δ(ωmn+ω)]\displaystyle\times\left[\delta\left(\omega_{mn}-\omega\right)-\delta\left(\omega_{mn}+\omega\right)\right]
2σCSabc(0,ω,ω)=\displaystyle 2\sigma^{abc}_{\text{CS}}(0;-\omega,\omega)= e3π22nm𝒌fnm[(rmnc);ka,rnmb]\displaystyle-\frac{e^{3}\pi}{2\hbar^{2}}\sum_{nm\bm{k}}f_{nm}\left[\left(r_{mn}^{c}\right)_{;k^{a}},r_{nm}^{b}\right]
×[δ(ωmnω)δ(ωmn+ω)],\displaystyle\times\left[\delta\left(\omega_{mn}-\omega\right)-\delta\left(\omega_{mn}+\omega\right)\right],

where we have used the relations

(rnmb)=rmnb,[(rmnb);ka]=(rnmb);ka,\left(r_{nm}^{b}\right)^{*}=r_{mn}^{b},\quad\left[\left(r_{mn}^{b}\right)_{;k^{a}}\right]^{*}=\left(r_{nm}^{b}\right)_{;k^{a}}, (8)

and defined the commutators and anticommutators,

{rnmb,rmnc}\displaystyle\left\{r_{nm}^{b},r_{mn}^{c}\right\} (rnmbrmnc+rnmcrmnb)\displaystyle\equiv\left(r_{nm}^{b}r_{mn}^{c}+r_{nm}^{c}r_{mn}^{b}\right) (9)
[rnmb,rmnc]\displaystyle\left[r_{nm}^{b},r_{mn}^{c}\right] (rnmbrmncrnmcrmnb)\displaystyle\equiv\left(r_{nm}^{b}r_{mn}^{c}-r_{nm}^{c}r_{mn}^{b}\right)
{(rmnc);ka,rnmb}\displaystyle\left\{\left(r_{mn}^{c}\right)_{;k^{a}},r_{nm}^{b}\right\} [(rmnc);karnmb+(rmnb);karnmc]\displaystyle\equiv\left[\left(r_{mn}^{c}\right)_{;k^{a}}r_{nm}^{b}+\left(r_{mn}^{b}\right)_{;k^{a}}r_{nm}^{c}\right]
[(rmnc);ka,rnmb]\displaystyle\left[\left(r_{mn}^{c}\right)_{;k^{a}},r_{nm}^{b}\right] [(rmnc);karnmb(rmnb);karnmc].\displaystyle\equiv\left[\left(r_{mn}^{c}\right)_{;k^{a}}r_{nm}^{b}-\left(r_{mn}^{b}\right)_{;k^{a}}r_{nm}^{c}\right].

They are the same with the expressions in Ref.[35].

Under the spatial symmetry operations, response coefficients in (6) and (7) obey the same transformation rule as a third-rank tensor and thus vanish in systems with the spatial inversion symmetry 𝒫\mathcal{P}. As the Neumann’s principle breaks down in the dynamic processes such as the transport phenomenon[42], the transformation rule of response tensors under 𝒯\mathcal{T} can not be acquired by applying 𝒯\mathcal{T} to the relevant physical quantities, i.e., electric current 𝑱\bm{J} and electric field 𝑬\bm{E}. However, we can obtain the transformation rule of ηinject\eta_{\text{inject}} and σshift\sigma_{\text{shift}} from their expressions (6,7). In systems with time-reversal symmetry, 𝒓mn(𝒌)=𝒓nm(𝒌)\bm{r}_{mn}(\bm{k})=\bm{r}_{nm}(-\bm{k}) and (𝒓mn);𝒌(𝒌)=(𝒓nm);𝒌(𝒌)\left(\bm{r}_{mn}\right)_{;\bm{k}}(\bm{k})=\left(\bm{r}_{nm}\right)_{;\bm{k}}(\bm{-k}). Therefore, the circular shift and linear injection current vanish in nonmagnetic system with 𝒯\mathcal{T}, while the linear shift and circular injection current are allowed to exist. In the noncentrosymmetric magnetic systems with preserved combined 𝒫𝒯\mathcal{PT} symmetry, the linear shift and circular injection current vanish while the other two photocurrents, namely circular shift and linear injection current, exist[32]. In the next section, we take EuSn2As2\mathrm{EuSn_{2}As_{2}} as an example to analyze the BPVE responses in magnetic structures with symmetry analysis and first-principles calculation.

II.2 Crystal structure and symmetry analysis of bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}}

The bulk EuSn2As2\mathrm{EuSn_{2}As_{2}} has a layered structure and belongs to space group R3¯mR\overline{3}m. Every layer component is composed of a trigonal Eu layer sandwiched by two SnAs layers. EuSn2As2\mathrm{EuSn_{2}As_{2}} was found to be an axion insulator in the A-type AFM phase belonging to magnetic space group (MSG) R3¯mR\overline{3}m^{\prime} and a strong topological insulator in the paramagnetic phase [43]. BPVE is prohibited in the two phases because they both have 𝒫\mathcal{P} with the inversion center on Eu atoms. When we confine the EuSn2As2\mathrm{EuSn_{2}As_{2}} to have a collinear magnetic structure, only the even-layer EuSn2As2\mathrm{EuSn_{2}As_{2}} in the A-type AFM phase breaks 𝒫\mathcal{P} and is able to generate BPVE photocurrents.

Refer to caption
Figure 1: (a-b) The crystal and magnetic stucture of bilayer AFM-zz EuSn2As2\mathrm{EuSn_{2}As_{2}}. The crystal axes aa is along the xx direction in the Cartesian coordinate system. (c) The Brillouin zone of bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}}.
Refer to caption
Figure 2: (a) The band structures of bilayer AFM-zz EuSn2As2\mathrm{EuSn_{2}As_{2}} with spin-orbit coupling (SOC) calculated with first-principles calculation (black) and tight-binding Hamiltonian based on the Wannier functions (red). The red, blue and green arrows marked the interband contributions to peaks in (b-c) centering at 0.33 eV, 0.37 eV and 0.55 eV, respectively. (b) The linear injection responses ηLI\eta_{\text{LI}} in AFM-zz phase. (c) The linear injection responses ηLI\eta_{\text{LI}} in AFM-x/yx/y phases. (d) The circular shift responses σCS\sigma_{\text{CS}} in AFM-x/yx/y phases.

We consider three AFM structures of the bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} with the magnetic moments along the x^\hat{x} (AFM-xx), y^\hat{y} (AFM-yy), and z^\hat{z} (AFM-zz) directions. The nonvanishing independent components of the BPVE response tensors in those magnetic structures can be obtained by utilizing their properties under 𝒯\mathcal{T} and the irreducible representations (IRREPs) of the crystalline point group (CPG). For instance, the crystal structure of bilayer AFM-zz EuSn2As2\mathrm{EuSn_{2}As_{2}} is illustrated in Fig. 1(a), where the magnetic moments break 𝒫\mathcal{P} but preserve 𝒫𝒯\mathcal{PT}. It belongs to the magnetic point group (MPG) 3¯m\overline{3}^{\prime}m^{\prime}, ={,2C3,3C2,𝒫𝒯,2S6𝒯,3σd𝒯}\mathcal{M}=\left\{\mathcal{I},2C_{3},3C_{2},\mathcal{PT},2S_{6}\mathcal{T},3\sigma_{d}\mathcal{T}\right\}, which can be decomposed into two forms, =D3(D3dD3)𝒯\mathcal{M}=D_{3}\oplus\left(D_{3d}-D_{3}\right)\mathcal{T} and =D3{,𝒫𝒯}\mathcal{M}=D_{3}\otimes\{\mathcal{I},\mathcal{PT}\}. As σCI\sigma_{\text{CI}} and ηLS\eta_{\text{LS}} are invariant under 𝒯\mathcal{T}, the effect of 𝒯\mathcal{T} is equivalent to the identity operation and we can acquire their nonvanishing independent components by analyzing the IRREPs and generators of CPG D3dD_{3d}. The 𝒫\mathcal{P} in D3dD_{3d} prohibits the existence of σCI\sigma_{\text{CI}} and ηLS\eta_{\text{LS}}, being consistent with the former conclusion that the linear shift and circular injection current vanish in systems with 𝒫𝒯\mathcal{PT}. Similarly, we can analyze σCS\sigma_{\text{CS}} and ηLI\eta_{\text{LI}} with IRREPs of CPG D3D_{3} due to their invariance under 𝒫𝒯\mathcal{PT}. As the bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} is a quasi-2D material, we focus on the in-plane responses. Take the electric current 𝑱\bm{J} as an example, we only concern the JxJ_{x} and JyJ_{y} components that transform as EE in D3D_{3} as illustrated in Table 1. Table 1 presents the IRREPs of group D3D_{3} and characters of the second-rank tensor for the group elements[44]. As σCS\sigma_{\text{CS}} (ηLI\eta_{\text{LI}}) relates a polar vector 𝑱\bm{J} and an asymmetric (symmetric) second-order tensor [𝑬𝑬]asym[\bm{EE^{*}}]_{\text{asym}} ([𝑬𝑬]sym[\bm{EE^{*}}]_{\text{sym}}), we obtain the representation of σCS\sigma_{\text{CS}} (ηLI\eta_{\text{LI}}) and decompose it into the direct sum of irreducible representations as followings,

ΓσCS=ΓJΓ(EE)asym=E,ΓηLI=ΓJΓ(EE)sym=A1A22E.\begin{split}&\Gamma_{\sigma_{\text{CS}}}=\Gamma_{J}\otimes\Gamma_{(EE^{*})_{\text{asym}}}=E,\\ &\Gamma_{\eta_{\text{LI}}}=\Gamma_{J}\otimes\Gamma_{(EE^{*})_{\text{sym}}}=A_{1}\oplus A_{2}\oplus 2E.\end{split} (10)

Because ΓηLI\Gamma_{\eta_{\text{LI}}} includes one identity representation, there is one nonvanishing independent component in ηLI{\eta_{\text{LI}}}. Utilizing the symmetry confinement of generators, C2xC_{2x} and C3zC_{3z}, we obtain the nonvanishing independent components, i.e., ηLIxxx=ηLIxyy=ηLIyxy-\eta_{\text{LI}}^{xxx}=\eta_{\text{LI}}^{xyy}=\eta_{\text{LI}}^{yxy}. On the contrary, the decomposition of ΓσCS\Gamma_{\sigma_{\text{CS}}} without the identity representation indicates that the circular shift response vanishes in the bilayer AFM-zz EuSn2As2\mathrm{EuSn_{2}As_{2}}.

D3D_{3} EE 2C32C_{3} 3C23C_{2} basis function
A1A_{1} 1 1 1
A2A_{2} 1 1 -1 z,Rzz,\ R_{z}
EE 2 -1 0 (x,y),(Rx,Ry)(x,y),\ (R_{x},R_{y})
Γ(EE)sym\Gamma_{(EE^{\star})_{\text{sym}}} 3 0 1
Γ(EE)asym\Gamma_{(EE^{\star})_{\text{asym}}} 1 1 -1
Table 1: Characters for irreducible representations of group D3D_{3} and characters of the symmetric and asymmetric second-rank tensor for group elements.
Refer to caption
Figure 3: The distribution of the group velocity difference Δmnx(𝐤)\Delta_{mn}^{x}(\mathbf{k}) and Δmny(𝐤)\Delta_{mn}^{y}(\mathbf{k}) in the BZ of (a,d) AFM-xx , (b,e) AFM-yy and (c,f) AFM-zz structures .

We can analyze the BPVE response in bilayer AFM-xx and AFM-yy EuSn2As2\mathrm{EuSn_{2}As_{2}} through the similar scheme. The bilayer AFM-xx EuSn2As2\mathrm{EuSn_{2}As_{2}} belongs to MPG 2/m2^{\prime}/m that can be decomposed into =Cs(C2hCs)𝒯\mathcal{M}=C_{s}\oplus\left(C_{2h}-C_{s}\right)\mathcal{T} and =Cs{,𝒫𝒯}\mathcal{M}=C_{s}\otimes\{\mathcal{I},\mathcal{PT}\}, while the AFM-yy phase belongs to the MPG 2/m2/m^{\prime} that can be decomposed into =C2(C2hC2)𝒯\mathcal{M}=C_{2}\oplus\left(C_{2h}-C_{2}\right)\mathcal{T} and =C2{,𝒫𝒯}\mathcal{M}=C_{2}\otimes\{\mathcal{I},\mathcal{PT}\}. The character tables for the mentioned CPGs and detailed analysis can be found in Supplementary Material. In AFM-xx and AFM-yy phases, σCI\sigma_{\text{CI}} and ηLS\eta_{\text{LS}} are still prohibited. However, the lowered symmetry resulted from the in-plane magnetic moments lead to more BPVE responses. To be more specific, the breakdown of C3zC_{3z} symmetry not only gives rise to the violation of equivalence relations among in-plane components, i.e., xxx=xyy=yxy-xxx=xyy=yxy, yyy=xxy=yxx-yyy=xxy=yxx, but also allows for the existence of in-plane circular shift current, i.e., σCSxxy{\sigma^{xxy}_{\text{CS}}} in AFM-xx and σCSyxy{\sigma^{yxy}_{\text{CS}}} in AFM-yy.

The distinct BPVE response in different MSG helps us detect the magnetic structure of EuSn2As2\mathrm{EuSn_{2}As_{2}}. First of all, as the nonvanishing second-order optical responses only exists in even-layer AFM EuSn2As2\mathrm{EuSn_{2}As_{2}}, we could easily distinguish it from odd number layer structures. Secondly, because the circular shift current only exist in AFM-xx and AFM-yy phases and it reverses direction when the incident circular polarized light changes helicity, we can measure the difference between response currents of circular polarized light with opposite helicity, JJ\vec{J}_{\circlearrowleft}-\vec{J}_{\circlearrowright}, to distinguish them from the AFM-zz phase. Finally, we could differentiate the AFM-xx and AFM-yy phase by a beam of light regardless of the polarization. When illuminated by linear polarized light with polarization along xx or yy direction, the response photocurrent flows perpendicular to the magnetic moments due to the nonzero ηLIyxx,yyy\eta_{\mathrm{LI}}^{yxx,yyy} and ηLIxxx,xyy\eta_{\mathrm{LI}}^{xxx,xyy} in the AFM-xx and AFM-yy phase, respectively. When illuminated by circular polarized light propagating in z^\hat{z} direction, the response photocurrent flows parallel to the magnetic moments due to the nonzero ηLIxxy,σCSxxy\eta_{\mathrm{LI}}^{xxy},{\sigma^{xxy}_{\text{CS}}} and ηLIyxy,σCSyxy\eta_{\mathrm{LI}}^{yxy},{\sigma^{yxy}_{\text{CS}}} in the AFM-xx and AFM-yy phase, respectively.

II.3 First-principles calculation of BPVE in bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}}

We obtain the band structures of the bilayer AFM-x/y/zx/y/z EuSn2As2\mathrm{EuSn_{2}As_{2}} by first-principles calculation as shown in Fig.2(a) and Fig.S1(a,b). They have similar electronic structures with a narrow bandgap of 15 meV, indicating that the direction of magnetic moments has negligibly small influence on the band structure but has direct constrain on their BPVE responses. The linear injecton responses of the three magnetic phases are presented in Fig.2(b-c). As discussed before, there are three nonvanishing components of ηLI\eta_{\mathrm{LI}} in AFM-zz phase, which are supposed to share the same magnitude and only differ by a sign. The little inconsistancy shown in Fig.2(b) is attributed to the violation of symmetry in generating Wannier functions. On the contrary, the three components in AFM-x/yx/y phases are independent as demonstrated in Fig.2(c) due to the absence of C3zC_{3z}. Furthermore, EuSn2As2\mathrm{EuSn_{2}As_{2}} in AFM-x/yx/y phases display stronger linear injection response. Fig.2(d) shows the circular shift response in AFM-x/yx/y phase, which is absent in AFM-zz phase because of the relations (xxx=xyy=yxy,yyy=yxx=xxy-xxx=xyy=yxy,-yyy=yxx=xxy) required by C3zC_{3z} and the antisymmetric property of circular shift conductivity to the last two indices.

Refer to caption
Figure 4: The distribution of quantum metric gmnbc(𝐤)g_{mn}^{bc}(\mathbf{k}) in the BZ of (a,d,g) AFM-xx, (b,e,h) AFM-yy, and (c,f,i) AFM-zz structures.

From Fig.2(c-d), we notice that there is a connection between BPVE responses in AFM-xx and AFM-yy phase, i.e., ηyyyAFM-x=ηxxxAFM-y\eta_{yyy}^{\text{AFM-x}}=-\eta_{xxx}^{\text{AFM-y}}, ηxxyAFM-x=ηyxyAFM-y\eta_{xxy}^{\text{AFM-x}}=-\eta_{yxy}^{\text{AFM-y}} , ηyxxAFM-x=ηxyyAFM-y\eta_{yxx}^{\text{AFM-x}}=-\eta_{xyy}^{\text{AFM-y}} and σxxyAFM-x=σyxyAFM-y\sigma_{xxy}^{\text{AFM-x}}=\sigma_{yxy}^{\text{AFM-y}}, with minor differences resulted from the little violated symmetry in generating the Wannier functions and the tiny magnetic anisotropy. We attribute it to be a consequence required by symmetry rather than a coincidence. As the bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} is a quasi-2D material, the effect of MxM_{x} in MSG P2/mP2^{\prime}/m is identical to C2yC_{2y} when constranied in the xyx-y plane. Therefore, the MSG P2/mP2/m^{\prime} of AFM-yy phase can be transformed into the MSG P2/mP2^{\prime}/m of AFM-xx phase when transformed under C4zC_{4z}. Applied with C4zC_{4z}, we obtain (xy)=(0110)(xy)\left(\begin{matrix}x^{\prime}\\ y^{\prime}\\ \end{matrix}\right)=\left(\begin{matrix}0&1\\ -1&0\\ \end{matrix}\right)\left(\begin{matrix}x\\ y\\ \end{matrix}\right) and transform ηxxxAFM-y\eta_{xxx}^{\text{AFM-y}} to ηyyyAFM-x-\eta_{y^{\prime}y^{\prime}y^{\prime}}^{\text{AFM-x}} and σyxyAFM-y\sigma_{yxy}^{\text{AFM-y}} to σxyxAFM-x=σxxyAFM-x-\sigma_{x^{\prime}y^{\prime}x^{\prime}}^{\text{AFM-x}}=\sigma_{x^{\prime}x^{\prime}y^{\prime}}^{\text{AFM-x}}. However, the system has no C4zC_{4z} rotation symmetry but tiny magnetic anisotropy in xx and yy direction. This magnetic anisotropy might be identified in the difference between ηLI\eta_{LI} and σCS\sigma_{CS} in Fig.2(c) if the numerical error in calculations can be reduced enough, e.g., the generated Wannier functions can preserve symmetry exactly.

Symmetry operation
AFM-x AFM-y/z
Quantitiy C2x𝒯C_{2x}\mathcal{T} MxM_{x} C2xC_{2x} Mx𝒯M_{x}\mathcal{T}
Δmnx(kx,ky)\Delta_{mn}^{x}(k_{x},k_{y}) Δmnx(kx,ky)-\Delta_{mn}^{x}(-k_{x},k_{y}) Δmnx(kx,ky)-\Delta_{mn}^{x}(-k_{x},k_{y}) Δmnx(kx,ky)\Delta_{mn}^{x}(k_{x},-k_{y}) Δmnx(kx,ky)\Delta_{mn}^{x}(k_{x},-k_{y})
Δmny(kx,ky)\Delta_{mn}^{y}(k_{x},k_{y}) Δmny(kx,ky)\Delta_{mn}^{y}(-k_{x},k_{y}) Δmny(kx,ky)\Delta_{mn}^{y}(-k_{x},k_{y}) Δmny(kx,ky)-\Delta_{mn}^{y}(k_{x},-k_{y}) Δmny(kx,ky)-\Delta_{mn}^{y}(k_{x},-k_{y})
gmnxx(kx,ky)g_{mn}^{xx}(k_{x},k_{y}) gmnxx(kx,ky)g_{mn}^{xx}(-k_{x},k_{y}) gmnxx(kx,ky)g_{mn}^{xx}(-k_{x},k_{y}) gmnxx(kx,ky)g_{mn}^{xx}(k_{x},-k_{y}) gmnxx(kx,ky)g_{mn}^{xx}(k_{x},-k_{y})
gmnxy(kx,ky)g_{mn}^{xy}(k_{x},k_{y}) gmnxy(kx,ky)-g_{mn}^{xy}(-k_{x},k_{y}) gmnxy(kx,ky)-g_{mn}^{xy}(-k_{x},k_{y}) gmnxy(kx,ky)-g_{mn}^{xy}(k_{x},-k_{y}) gmnxy(kx,ky)-g_{mn}^{xy}(k_{x},-k_{y})
gmnyy(kx,ky)g_{mn}^{yy}(k_{x},k_{y}) gmnyy(kx,ky)g_{mn}^{yy}(-k_{x},k_{y}) gmnyy(kx,ky)g_{mn}^{yy}(-k_{x},k_{y}) gmnyy(kx,ky)g_{mn}^{yy}(k_{x},-k_{y}) gmnyy(kx,ky)g_{mn}^{yy}(k_{x},-k_{y})
Table 2: Transformation of group velocity difference Δmna(𝐤){\Delta}^{a}_{mn}(\mathbf{k}) and quantum metric gmnbc(𝐤)g_{mn}^{bc}(\mathbf{k}) under C2xC_{2x}, C2x𝒯C_{2x}\mathcal{T}, MxM_{x} and Mx𝒯M_{x}\mathcal{T}.

The integrand of ηLI\eta_{\mathrm{LI}} can be decomposed into three terms as shown in (6), i.e., the k-resolved group velocity difference Δmna(𝐤)\Delta_{mn}^{a}(\mathbf{k}), quantum metric 2gmnbc(𝐤){rmnb(𝐤),rnmc(𝐤)}g_{mn}^{bc}(\mathbf{k})\equiv\{r_{mn}^{b}(\mathbf{k}),r_{nm}^{c}(\mathbf{k})\}[32, 45], and joint density of states (JDOS) δ(ωnm(𝐤)ω)\delta(\omega_{nm}(\mathbf{k})-\omega). The distribution of Δmna(𝐤)\Delta_{mn}^{a}(\mathbf{k}) and gmnbc(𝐤)g_{mn}^{bc}(\mathbf{k}) in three magnetic structures are shown in Fig.3 and Fig.4, respectively, which follow the constrains of symmerty. For instance, C2xC_{2x} and Mx𝒯M_{x}\mathcal{T} in AFM-y/zy/z confine Δmnx(𝐤)\Delta_{mn}^{x}(\mathbf{k}) and gmnxx,yy(𝐤)g_{mn}^{xx,yy}(\mathbf{k}) to be symmetric about kyk_{y} axis, while Δmny(𝐤)\Delta_{mn}^{y}(\mathbf{k}) and gmnxy(𝐤)g_{mn}^{xy}(\mathbf{k}) are confined to be antisymmetric about kyk_{y} axis. These properties require ηLIyyy,xxy,yxx\eta_{LI}^{yyy,xxy,yxx} to vanish in AFM-y/zy/z structures, which is consistent with above symmetry analysis and calculation results. More details about the transformation of quantities under symmetrical operations can be found in Table.2. Furthermore, Δmna(𝐤)\Delta_{mn}^{a}(\mathbf{k}) in the three magnetic structures are similar to each other while gmnab(𝐤)g_{mn}^{ab}(\mathbf{k}) are quite different, verifying above conclusion that the alignment of magnetic moments has small influence on the band structure but greatly changes the geometrical properties of wave functions as reflected in the nonlinear optical responses.

The distribution of these quantities in BZ can offer us further information about the BPVE responses. Noticing that there are four peaks at 0.024, 0.33, 0.37 and 0.55 eV in linear injection responses as shown in Fig.2(b-c), we can figure out the corresponding interband transitions in the Brillouin zone according to the energy conservation required by δ(ωnmω)\delta(\omega_{nm}-\omega). As illustrated in Fig.2(a), the red, blue and green arrows marked the interband contributions to peaks centering at 0.33 eV, 0.37 eV and 0.55 eV, respectively. They locate around Γ\Gamma point in ΓK\Gamma-K and ΓM\Gamma-M directions. Besides, interband transition at 0.024 eV is right at Γ\Gamma. The photocurrent peaks at 0.024 eV, 0.37 eV and 0.55 eV coincide with the peaks in JDOS at the same photon energy position as shown in Fig.S2, while the photocurrent peak at 0.33 eV has no corresponding peak in JDOS. We think this peak is mostly contributed by the large values of quantum metric gmnbc(𝐤)g_{mn}^{bc}(\mathbf{k}) in ΓK\Gamma-K direction from the interband transition marked by the red arrows in Fig.2(a).

III Computational Details

The band structures are calculated using the Quantum ESPRESSO (QE) simulation package[46, 47] with the generalized gradient approximation of Perdew-Burke-Ernzerhof exchange-correlation potential[48] in PSLIBRARY[49]. The self-consistent calculations are carried out on a 11×\times11×\times1 Monkhorst-Pack k-mesh with the plane-wave function cutoff set to 150 Ry. A vacuum region of about 15 Å along the z direction is adopted to eliminate the artificial layer interactions. Due to the existence of Eu-4f orbitals, we apply a Hubbard U correction with parameter U4f=UJ=5.0eV\emph{U}_{4f}=\emph{U-J}=5.0\ \mathrm{eV}. The maximally-localized Wannier functions[50, 51, 52] are generated using p orbital Sn, p orbital of As, f orbital of Eu. With the tight-binding Hamiltonian constructed from these Wannier functions, we calculate the optical responses with modified code of the WANNIER90 package[53]. The calculation is performed on the 1500×1500×1 k-mesh and the convergence has been tested.

IV Conclusion

In summary, we demonstrate that the BPVE photocurrents can be classified into linear/circular shift current and linear/circular injection current by analyzing their dependences on the polarization of incident light and generating mechanism. Taking bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} in three AFM structures as an example, we analyze the BPVE responses constrained by the magnetic symmetry through group representation theory and first-principles calculation. The results show that AFM-zz structure has only linear injection currents while AFM-x/yx/y structures have the linear injection and circular shift currents and the currents flow in perpendicular direction when illuminated by light. We design a protocol to distinguish the magnetic structures of even-layer EuSn2As2\mathrm{EuSn_{2}As_{2}} in experiments, which can be generalised to materials with similar MPGs. Moreover, we illustrate that the geometric quantity has a crucial role in the BPVE responses, which can guide us to find the ideal materials for practical applications.

Acknowledgements.
We acknowledge the discussion with Jiacheng Gao and Yi Jiang. This work was supported by the Ministry of Science and Technology of China (Grants No. 2018YFA0305700 and No. 2022YFA1403800), the National Natural Science Foundation of China (Grants No. 11925408, No. 11921004, and No. 12188101), the Chinese Academy of Sciences (Grant No. XDB33000000) and the Informatization Plan of the Chinese Academy of Sciences (Grant No. CAS WX2021SF-0102), and the Condensed Matter Physics Data Center, CAS.

References

  • [1] P. Němec, M. Fiebig, T. Kampfrath, and A. V. Kimel, Nature Physics 14, 229 (2018).
  • [2] Z. Sun, Y. Yi, T. Song, G. Clark, B. Huang, Y. Shan, S. Wu, D. Huang, C. Gao, Z. Chen, et al., Nature 572, 497 (2019).
  • [3] M. Fiebig, V. V. Pavlov, and R. V. Pisarev, JOSA B 22, 96 (2005).
  • [4] Y. Li, Y. Rao, K. F. Mak, Y. You, S. Wang, C. R. Dean, and T. F. Heinz, Nano letters 13, 3329 (2013).
  • [5] C. Heide, Y. Kobayashi, D. R. Baykusheva, D. Jain, J. A. Sobota, M. Hashimoto, P. S. Kirchmann, S. Oh, T. F. Heinz, D. A. Reis, et al., Nature Photonics 16, 620 (2022).
  • [6] G. Vampa, T. Hammond, N. Thiré, B. Schmidt, F. Légaré, C. McDonald, T. Brabec, D. Klug, and P. Corkum, Physical review letters 115, 193603 (2015).
  • [7] T. T. Luu and H. J. Wörner, Nature communications 9, 1 (2018).
  • [8] S. A. Denev, T. T. Lummen, E. Barnes, A. Kumar, and V. Gopalan, Journal of the American Ceramic Society 94, 2699 (2011).
  • [9] R. Silva, I. V. Blinov, A. N. Rubtsov, O. Smirnova, and M. Ivanov, Nature Photonics 12, 266 (2018).
  • [10] Y.-Y. Lv, J. Xu, S. Han, C. Zhang, Y. Han, J. Zhou, S.-H. Yao, X.-P. Liu, M.-H. Lu, H. Weng, et al., Nature Communications 12, 6437 (2021).
  • [11] C. Qian, C. Yu, S. Jiang, T. Zhang, J. Gao, S. Shi, H. Pi, H. Weng, and R. Lu, Physical Review X 12, 021030 (2022).
  • [12] V. I. Belinicher and B. I. Sturman, Soviet Physics Uspekhi 23, 199 (1980).
  • [13] R. von Baltz and W. Kraut, Physical Review B 23, 5590 (1981).
  • [14] V. Fridkin, Crystallography Reports 46, 654 (2001).
  • [15] J. E. Moore and J. Orenstein, Physical review letters 105, 026805 (2010).
  • [16] F. Nastos and J. Sipe, Physical Review B 74, 035201 (2006).
  • [17] Q. Xu, Y. Zhang, K. Koepernik, W. Shi, J. van den Brink, C. Felser, and Y. Sun, npj Computational Materials 6, 1 (2020).
  • [18] Z. Ni, K. Wang, Y. Zhang, O. Pozo, B. Xu, X. Han, K. Manna, J. Paglione, C. Felser, A. G. Grushin, et al., Nature communications 12, 1 (2021).
  • [19] L. Z. Tan, F. Zheng, S. M. Young, F. Wang, S. Liu, and A. M. Rappe, Npj Computational Materials 2, 1 (2016).
  • [20] A. M. Cook, B. M Fregoso, F. De Juan, S. Coh, and J. E. Moore, Nature communications 8, 1 (2017).
  • [21] T. Morimoto and N. Nagaosa, Science advances 2, e1501524 (2016).
  • [22] N. Nagaosa and T. Morimoto, Advanced Materials 29, 1603345 (2017).
  • [23] J. Orenstein, J. Moore, T. Morimoto, D. Torchinsky, J. Harter, and D. Hsieh, Annual Review of Condensed Matter Physics 12, 247 (2021).
  • [24] F. de Juan, A. G. Grushin, T. Morimoto, and J. E. Moore, Nature communications 8, 1 (2017).
  • [25] Q. Ma, S.-Y. Xu, C.-K. Chan, C.-L. Zhang, G. Chang, Y. Lin, W. Xie, T. Palacios, H. Lin, S. Jia, et al., Nature Physics 13, 842 (2017).
  • [26] C.-K. Chan, N. H. Lindner, G. Refael, and P. A. Lee, Physical Review B 95, 041104 (2017).
  • [27] J. Sipe and A. Shkrebtii, Physical Review B 61, 5337 (2000).
  • [28] S. M. Young and A. M. Rappe, Physical review letters 109, 116601 (2012).
  • [29] L. Z. Tan and A. M. Rappe, Physical review letters 116, 237402 (2016).
  • [30] L. Wu, S. Patankar, T. Morimoto, N. L. Nair, E. Thewalt, A. Little, J. G. Analytis, J. E. Moore, and J. Orenstein, Nature Physics 13, 350 (2017).
  • [31] B. I. Sturman and V. M. Fridkin, The photovoltaic and photorefractive effects in noncentrosymmetric materials (Routledge, 2021).
  • [32] J. Ahn, G.-Y. Guo, and N. Nagaosa, Physical Review X 10, 041041 (2020).
  • [33] H. Wang and X. Qian, Science advances 5, eaav9743 (2019).
  • [34] Y. Zhang, T. Holder, H. Ishizuka, F. de Juan, N. Nagaosa, C. Felser, and B. Yan, Nature communications 10, 1 (2019).
  • [35] H. Wang and X. Qian, NPJ Computational Materials 6, 1 (2020).
  • [36] T. Holder, D. Kaplan, and B. Yan, Physical Review Research 2, 033100 (2020).
  • [37] H. Watanabe and Y. Yanase, Physical Review X 11, 011001 (2021).
  • [38] D. Rees, B. Lu, Y. Sun, K. Manna, R. Özgür, S. Subedi, H. Borrmann, C. Felser, J. Orenstein, and D. H. Torchinsky, Physical review letters 127, 157405 (2021).
  • [39] J. Sipe and E. Ghahramani, Physical Review B 48, 11705 (1993).
  • [40] C. Aversa and J. Sipe, Physical Review B 52, 14636 (1995).
  • [41] E. Blount, in Solid state physics (Elsevier, 1962), vol. 13, pp. 305–373.
  • [42] R. R. Birss, Reports on Progress in Physics 26, 307 (1963).
  • [43] H. Li, S.-Y. Gao, S.-F. Duan, Y.-F. Xu, K.-J. Zhu, S.-J. Tian, J.-C. Gao, W.-H. Fan, Z.-C. Rao, J.-R. Huang, et al., Physical Review X 9, 041039 (2019).
  • [44] M. Lax, Symmetry principles in solid state and molecular physics (Courier Corporation, 2001).
  • [45] J. Ahn, G.-Y. Guo, N. Nagaosa, and A. Vishwanath, Nature Physics 18, 290 (2022).
  • [46] P. Giannozzi, S. Baroni, N. Bonini, M. Calandra, R. Car, C. Cavazzoni, D. Ceresoli, G. L. Chiarotti, M. Cococcioni, I. Dabo, et al., Journal of physics: Condensed matter 21, 395502 (2009).
  • [47] P. Giannozzi, O. Andreussi, T. Brumme, O. Bunau, M. B. Nardelli, M. Calandra, R. Car, C. Cavazzoni, D. Ceresoli, M. Cococcioni, et al., Journal of physics: Condensed matter 29, 465901 (2017).
  • [48] J. P. Perdew, K. Burke, and M. Ernzerhof, Physical review letters 77, 3865 (1996).
  • [49] A. Dal Corso, Computational Materials Science 95, 337 (2014).
  • [50] N. Marzari and D. Vanderbilt, Physical review B 56, 12847 (1997).
  • [51] I. Souza, N. Marzari, and D. Vanderbilt, Physical Review B 65, 035109 (2001).
  • [52] N. Marzari, A. A. Mostofi, J. R. Yates, I. Souza, and D. Vanderbilt, Reviews of Modern Physics 84, 1419 (2012).
  • [53] A. A. Mostofi, J. R. Yates, G. Pizzi, Y.-S. Lee, I. Souza, D. Vanderbilt, and N. Marzari, Computer Physics Communications 185, 2309 (2014).

Appendix A Band structures of the AFM-x/yx/y structures and JDOS.

Refer to caption
Figure S1: The band structures of bilayer EuSn2As2\mathrm{EuSn_{2}As_{2}} with spin-orbit coupling (SOC) calculated with VASP (black) and tight-binding Hamiltonian based on the Wannier functions (red) in (a) AFM-xx phase and (b) AFM-yy phase.
Figure S2: The joint density of states of three magnetic structures.

Appendix B Symmetry analysis and character tables of the AFM-xx and AFM-yy phases

AFM-xx phase

The bilayer AFM-xx EuSn2As2\mathrm{EuSn_{2}As_{2}} belongs to MPG 2/m2^{\prime}/m that can be decomposed into =Cs(C2hCs)𝒯\mathcal{M}=C_{s}\oplus\left(C_{2h}-C_{s}\right)\mathcal{T} and =Cs{,𝒫𝒯}\mathcal{M}=C_{s}\otimes\{\mathcal{I},\mathcal{PT}\}. The representation of σCS\sigma_{\text{CS}} and ηLI\eta_{\text{LI}} are given below according to Table. S1. As there are one and three identity representations in ΓσCS\Gamma_{\sigma_{\text{CS}}} and ΓηLI\Gamma_{\eta_{\text{LI}}}, respectively, we can find out the nonvanishing independent components are σCSxxy\sigma_{\text{CS}}^{xxy} and ηLIyyy,ηLIyxx,ηLIxxy\eta_{\text{LI}}^{yyy},\eta_{\text{LI}}^{yxx},\eta_{\text{LI}}^{xxy}.

ΓσCS=ΓJΓ(EE)asym=A1A2,ΓηLI=ΓJΓ(EE)sym=3A13A2.\begin{split}&\Gamma_{\sigma_{\text{CS}}}=\Gamma_{J}\otimes\Gamma_{(EE^{\star})_{\text{asym}}}=A_{1}\oplus A_{2},\\ &\Gamma_{\eta_{\text{LI}}}=\Gamma_{J}\otimes\Gamma_{(EE^{\star})_{\text{sym}}}=3A_{1}\oplus 3A_{2}.\end{split} (S1)

AFM-yy phase

The AFM-yy phase belongs to the MPG 2/m2/m^{\prime} that can be decomposed into =C2(C2hC2)𝒯\mathcal{M}=C_{2}\oplus\left(C_{2h}-C_{2}\right)\mathcal{T} and =C2{,𝒫𝒯}\mathcal{M}=C_{2}\otimes\{\mathcal{I},\mathcal{PT}\}. The representation of σCS\sigma_{\text{CS}} and ηLI\eta_{\text{LI}} are given below according to Table. S2. As there are one and three identity representations in ΓσCS\Gamma_{\sigma_{\text{CS}}} and ΓηLI\Gamma_{\eta_{\text{LI}}}, respectively, we can find out the nonvanishing independent components are σCSyxy\sigma_{\text{CS}}^{yxy} and ηLIyxy,ηLIxyy,ηLIxxx\eta_{\text{LI}}^{yxy},\eta_{\text{LI}}^{xyy},\eta_{\text{LI}}^{xxx}.

ΓσCS=ΓJΓ(EE)asym=A1A2,ΓηLI=ΓJΓ(EE)sym=3A13A2.\begin{split}&\Gamma_{\sigma_{\text{CS}}}=\Gamma_{J}\otimes\Gamma_{(EE^{\star})_{\text{asym}}}=A_{1}\oplus A_{2},\\ &\Gamma_{\eta_{\text{LI}}}=\Gamma_{J}\otimes\Gamma_{(EE^{\star})_{\text{sym}}}=3A_{1}\oplus 3A_{2}.\end{split} (S2)
CsC_{s} EE MxM_{x} basis function
A1A_{1} 1 1 z,y,Rxz,\ y,\ R_{x}
A2A_{2} 1 -1 x,Rz,Ryx,\ R_{z},\ R_{y}
Γ(EE)sym\Gamma_{(EE^{\star})_{\text{sym}}} 3 1
Γ(EE)asym\Gamma_{(EE^{\star})_{\text{asym}}} 1 -1
Table S1: Characters for irreducible representations of group CsC_{s} and characters of a polar vector, a symmetric second-rank tensor and an asymmetric second-rank tensor.
C2C_{2} EE C2xC_{2x} basis function
A1A_{1} 1 1 x,Rxx,\ R_{x}
A2A_{2} 1 -1 y,z,Ry,Rzy,\ z,\ R_{y},\ R_{z}
Γ(EE)sym\Gamma_{(EE^{\star})_{\text{sym}}} 3 1
Γ(EE)asym\Gamma_{(EE^{\star})_{\text{asym}}} 1 -1
Table S2: Characters for irreducible representations of group C2C_{2} and characters of a polar vector, a symmetric second-rank tensor and an asymmetric second-rank tensor.