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Anisotropic Electron-Hole Excitation and Large Linear Dichroism in Two-Dimensional Ferromagnet CrSBr with In-Plane Magnetization

Tian-Xiang Qian,1,2 Ju Zhou,1,3 Tian-Yi Cai,1,111Electronic address: [email protected] and Sheng Ju1,222Electronic address: [email protected] 1 Institute of Theoretical and Applied Physics, School of Physical Science and Technology and Jiangsu Key Laboratory of Thin Film, Soochow University, Suzhou 215006, P. R. China
2 Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy
3 School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, Northern Ireland, United Kingdom
Abstract

The observation of magnetic ordering in atomically thin CrI3 and Cr2Ge2Te6 monolayers has aroused intense interest in condensed matter physics and material science. Studies of van de Waals two-dimensional (2D) magnetic materials are of both fundamental importance and application interest. In particular, exciton-enhanced magneto-optical properties revealed in CrI3 and CrBr3 monolayers have expanded the understanding of exciton physics in 2D materials. Unlike CrI3 and CrBr3 with out-of-plane magnetization, CrSBr has an in-plane magnetic moment, therefore, providing a good opportunity to study the magnetic linear dichroism and high-order magneto-optical effects. Here, based on the many-body perturbation method within density-functional theory, we have studied quasiparticle electronic structure, exciton, and optical properties in CrSBr monolayer. Strongly bounded exciton has been identified with the first bright exciton located at 1.35 eV, in good agreement with an experiment of photoluminescence (Nat. Mater. 20, 1657 (2021)). Strong contrast in the optical absorption is found between the electric fields lying along the in-plane two orthogonal directions. In accordance with a typical and realistic experimental setup, we show that the rotation angle of linear polarized light, either reflected or transmitted, could be comparable with those revealed in black phosphorene. Such large linear dichroism arises mainly from anisotropic in-plane crystal structure. The magnetic contribution from the off-diagonal component of dielectric function to the linear dichroism in CrSBr is negligible. Our findings not only have revealed excitonic effect on the optical and magneto-optical properties in 2D ferromagnet CrSBr, but also have shown its potential applications in 2D optics and optoelectronics.

I introduction

Due to strong light-matter interaction, two-dimensional (2D) materials have demonstrated potential applications in semiconductor optoelectronics and photonics [1, 2, 3, 4]. The discovery of 2D van der Waals magnets Cr2Ge2Te6 [5] and CrI3 [6] monolayer, on the other hand, has provided an additional degree of freedom, where the out-of-plane magnetization could facilitate magneto-optical Kerr and Faraday effects in ultrathin limit [7, 8]. Based on many-body perturbation theory, Wu, Cao, Li, and Louie have revealed exciton effect on the magneto-optical effects in the monolayer of CrI3 [9] and CrBr3 [10]. The Kerr rotation angle for the reflected light could reach as high as 0.9 and the Fraday angle for the transmitted light could reach as high as 0.3. Recently, another kind of 2D magnet CrSBr with in-plane magnetization has been identified [11] and fabricated [12] successfully. The bilayer system shows great contrast in the optical responses between antiferromagnetic and ferromagnetic interlayer coupling [12]. Considering the excitonic effect, such a magnetic ordering dependence of optical properties has been well explained by the many-body perturbation calculations [12]. In monolayer limit, the system shows strong photoluminescence (PL) at 1.3 eV [12]. In the meantime, the exciton-coupled coherent magnons will lead to efficient optical access to spin information [13]. In contrast to Cr2Ge2Te6 and CrI3 (CrBr3), when the magnetization in CrSBr monolayer is lying along the easy axis within the 2D plane, as demonstrated in Fig. 1, the former magneto-optical Kerr and Fraday effects, which measures rotation angle of linear polarized light, will be replaced by Schäfer-Hubert (SH) effect and Voigt effect, for reflected and transmitted lights, respectively [14]. The original purpose of this paper is to provide a comprehensive framework of excitonic effect on the optical and high-order magneto-optical properties in 2D ferromagnetic CrSBr with in-plane magnetization. Generally, when the magnetization is pointing along yy direction, it is believed that [14]

Refer to caption
Figure 1: SH and Vogit setup consisting of layers of vacuum, ferromagnetic monolayer CrSBr, substrate of semi-infinitely thick SiO2. Red arrow denotes the in-plane magnetization, which is along y axis. (b) Illustration of rotation angle and ellipticity for reflected (left panel) and transmitted (right panel) lights.
ϕSH\displaystyle\phi_{\rm SH} =θSH+iηSH\displaystyle=\theta_{\rm SH}+i\eta_{\rm SH} =iωdc(1nsub2)(n2n2)\displaystyle=\frac{-i\omega d}{c(1-n_{sub}^{2})}(n_{\parallel}^{2}-n_{\perp}^{2}) =iωdc(1nsub2)(εyyεxxεzx2εzz),\displaystyle=\frac{-i\omega d}{c(1-n_{sub}^{2})}(\varepsilon_{yy}-\varepsilon_{xx}-\frac{\varepsilon_{zx}^{2}}{\varepsilon_{zz}}), (1)

and

ϕV\displaystyle\phi_{\rm V} =θViηV\displaystyle=\theta_{\rm V}-i\eta_{\rm V} =ωd2ic(nn)\displaystyle=\frac{\omega d}{2ic}(n_{\parallel}-n_{\perp}) =ωd2ic[εyy12(εxx+εzx2εzz)12].\displaystyle=\frac{\omega d}{2ic}[\varepsilon_{yy}^{\frac{1}{2}}-(\varepsilon_{xx}+\frac{\varepsilon_{zx}^{2}}{\varepsilon_{zz}})^{\frac{1}{2}}]. (2)

Here, θSH\theta_{\rm SH} and θV\theta_{\rm V} are rotation angles, and ηSH\eta_{\rm SH} and ηV\eta_{\rm V} are ellipticities. cc is the velocity of light, nn is the complex refraction index, and ε\varepsilon is the dielectric function. ω\omega is the optical frequency, dd is the thickness of magnetic material, and subsub means the substrate. Clearly, such effects are closely related to the contrast between the dielectric properties of two in-plane diagonal components εxx\varepsilon_{xx} and εyy\varepsilon_{yy} as well as the magnitude of the off-diagonal component εzx\varepsilon_{zx} of the system of interest. Based on independent particle approximation (IPA), such effects in 2D magnets CrXY (X=S, Se, and Te; Y=Cl, Br, and I) were studied computationally [15]. For the monolayer geometry with particular 2D dielectric screening, the inherent many-body correction to the quasiparticle band structure and optical properties could not be ignored [16, 17, 18, 19, 20, 21]. A huge excitonic effect with binding energy of as large as 1 eV (two orders larger than conventional semiconductors) will modify the optical spectrum from IPA strongly. Therefore, in this paper, based on density functional theory with many-body perturbation method, i.e., GW-BSE method (G for one-particle Green’s function, W for screened Coulomb interaction, and BSE for Bethe-Salpeter equation) [22], we have studied the quasiparticle electronic structure, exciton, and optical properties in CrSBr monolayer. The first bright excitonic state is found located at 1.35 eV, in good agreement with experiment [12]. In the meantime, large linear dichroism (optical birefringence) from anisotropic in-plane crystal structure has been identified. The intrinsic magneto-optical effect from off-diagonal components of dielectric function, however, is found to be very small. CrSBr shows large difference between εxx\varepsilon_{xx} and εyy\varepsilon_{yy} which will dominate the linear dichroism, and consequently the magnitude of rotation angle θ\theta and ellipticity η\eta. It has also been revealed that excitonic effect has modified εxx\varepsilon_{xx}, εyy\varepsilon_{yy}, and εxz\varepsilon_{xz} dramatically, and consequently the linear dichroism and the high-order magneto-optical properties. When the magnetization is tuned by external perpendicular magnetic field towards out-of-plane direction, CrSBr monolayer could exhibit significant Kerr and Faraday effects, which are even larger than those in CrI3 [9] and CrBr3 [10]. Furthermore, the short lifetime of the first bright exciton suggests its potential application in infrared light-emitting. Our findings not only have revealed excitonic effect on the optical and magneto-optical properties in 2D ferromagnet CrSBr, but also have shown its potential applications in 2D optics and optoelectronics.

II computational method

Our first-principle calculations are performed using density-functional theory (DFT) as implemented in the Quantum Espresso package [23]. We use the generalized gradient approximation with Perdew-Burke-Ernzerhof (PBE) [24] and norm-conserving pseudopotentials with a plane-wave cutoff of 80 Ry [25]. The ground-state wave functions and eigenvalues are calculated within a k grid of 16×12×116\times 12\times 1. The structures are relaxed until the total forces are less than 0.01 eV/Å and the convergence criterion for total energies is set to 10510^{-5} eV. The quasiparticle band structure and excitonic properties are calculated with BerkeleyGW package [26, 27, 28, 29] (see Appendix A). We have included spin-orbit coupling with spinor GW-BSE calculations [29]. A slab model is used with vacuum layer of 15 Å along the out-of-plane direction and a truncated Coulomb interaction between CrSBr monolayer and its periodic image is adopted [30]. Here, the calculations are based on one-shot G0W0G_{0}W_{0} with generalized plasmon pole model. The mean-field wave functions and eigenvalues within PBE are chosen as the starting point for G0W0G_{0}W_{0}, as a first guess for quasiparticle wave functions and eigenvalues. For the convergence of quasiparticle energies [31], we have tested the dependence on k-grid size, number of bands, as well as dielectric cutoff. We use a coarse k grid of 16×12×116\times 12\times 1, 1080 of number of bands, and the dielectric cutoff of 20 Ry (see Appendix B). The electron-hole excitations are then calculated by solving the BSE for each exciton state and frequency-dependent complex dielectric function ε(ω)\varepsilon(\omega). For the BSE part, the fine k grid of 64×48×164\times 48\times 1 is used (see Appendix B). We use a Gaussian smearing with a broadening constant of 30 meV in optical absorbance spectrum. The number of bands for optical transitions is 6 valence and 8 conduction bands, which is sufficient to cover the span of the energies of visible light. Such kind of treatment of excited states is robust and has been applied successfully in a wide range of 2D materials [32], including graphene [33, 34, 35, 36, 37, 38, 39], graphyne [40], 2D transition metal dichalcogenides [41, 42, 43, 44, 45, 46, 47, 48, 49, 50, 51], black phosphorene [52, 53, 54, 55, 56], blue phosphorene [57, 58], violet (Hittorf’s) phosphorene [59, 60], 2D monochalcogenides [61, 62, 63], 2D GaN [64], 2D boron nitrides [65, 66, 67], and 2D magnets [9, 10, 68].

III results and discussion

Bulk CrSBr belongs to an orthorhombic structure with crystal parameters a = 3.504 Å, b = 4.738 Å, and c = 7.907 Å in the space group Pmmn (No. 59). This structure is built of monolayers of CrSBr, which are bonded through van der Waals interactions along the c-axis. For monolayer CrSBr as demonstrated in Fig. 2, it still belongs to space group Pmmn (No. 59) with an effective thickness of around 5.7 Å. The monolayer CrSBr consists of two buckled rectangular planes of CrS fused together, with both surfaces capped by Br atoms. The top view of monolayer CrSBr in Fig. 2 shows a rectangular network lattice with a = 3.537 Å and b = 4.730 Å.

Refer to caption
Figure 2: Illustration of crystal structure of 2D magnet CrSBr monolayer. Local magnetic moment at Cr atoms pointing along y axis.

Experimentally, using second-harmonic generation technique, ferromagnetic order with magnetic moment pointing along yy axis has been identified in CrSBr monolayer with a Curie temperature of TC = 146 ±\pm 2 K [69]. In the meanwhile, photoluminescence spectra show an obvious decrease at temperature between 130 K and 150 K, suggesting a phase transition therein [12]. This Curie temperature in CrSBr monolayer is therefore much higher than Cr2Ge2Te6 monolayer (@ 22 K under magnetic field of 0.075 T) [5] and CrI3 monolayer (@ 45 K) [6]. Theoretically, Cr3+ ion has a magnetic moment of 3 μB\mu_{B}, pointing along the y axis of 2D plane. When the magnetization points along x or z axis, the total energy is 0.042 meV/Cr and 0.072 meV/Cr higher, respectively. And the value along zz axis is in agreement with another theoretical result of 0.078 meV/Cr [70]. It is noted that the calculated total energy for the state with magnetization along in-plane direction is 0.025 meV/Cr lower in Cr2Ge2Te6 monolayer [7] and 0.263 meV/Cr higher in CrI3 monolayer [8] when compared with the magnetic state of out-of-plane magnetization. On the other hand, the antiferromagnetic coupling between the in-plane two Cr3+ ions is 58.86 meV/Cr higher than the ferromagnetic ground state. This result agrees with previous ground-state calculations [70]. For multilayer systems, the local magnetic moment still prefers y axis, with magnetic moment antiparallel with each other between neighboring layers [12].

As indicated by the band structure in Fig. 3, this monolayer of CrSBr is a direct band gap semiconductor with the top of valence band and the bottom of conduction band both located at Γ\Gamma point. The band gap increases a little along x direction and increases sharply along orthogonal direction, i.e., ΓY\Gamma\to\rm{Y}. Clearly, this monolayer structure shows anisotropic band dispersion. On the other hand, the two spin channels are well separated in the ferromagnetic ground state.

Refer to caption
Figure 3: PBE band structure with colors denoting the direction of spin polarization along the y axis.

It should be pointed out that what we have simulated is a suspended monolayer, i.e., a single layer of CrSBr in vacuum. The strength of the Coulomb interaction in such material originates from weak dielectric screening in the 2D limit. For distances exceeding few nanometres, the screening is determined by the immediate surroundings of the material, which can be vacuum or air in the ideal case of suspended samples. Compared to MoS2 [44] and blue phosphorene [57], such unique 2D dielectric screening in CrSBr should also be anisotropic. The static screened Coulomb interaction is constructed as [44]

W𝐆𝐆(𝒒;0)=ε𝐆𝐆1(𝒒;0)v(𝒒+𝐆).W_{\rm\bf{GG^{\prime}}}({\bm{q}};0)=\varepsilon^{-1}_{\rm\bf{GG^{\prime}}}({\bm{q}};0)v({\bm{q}}+{\rm\bf{G^{\prime}}}). (3)

The effective static 2D dielectric function ε2D(q)\varepsilon_{2D}(q) could be obtained [44]

ε2D1(𝒒)=|𝒒|2πe2Lz𝐆z𝐆zW𝐆z𝐆z(𝒒),\varepsilon_{2D}^{-1}(\bm{q})=\frac{|\bm{q}|}{2\pi e^{2}L_{z}}\sum_{{\rm\bf G}_{z}{\rm\bf G^{\prime}}_{z}}W_{{\rm\bf G}_{z}{\rm\bf G^{\prime}}_{z}}(\bm{q}), (4)

where the complicated details of the screening in the out-of-plane direction zz have been integrated out. The dielectric screening in such a system obeys particular wavelength dependence. As demonstrated in Fig. 4(a), in the long-distance limit the electron-electron interacts like that in vacuum with ε=1\varepsilon=1, while within the intermediate distance, the electron-electron interaction has effective dielectric screening by the 2D materials with ε1\varepsilon\geq 1. The label “others” in Fig. 4(a) refers to the other 𝒒\bm{q} points in qq mesh which do not belong to (qxq_{x},0) or (0,qyq_{y}). For the anisotropic nature, the dielectric screening changes along different directions. To accurately access the distance-dependence of 2D dielectric screening, we have obtained ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}) through Hankel transformation of ε2D(𝒒)\varepsilon_{\rm 2D}(\bm{q}) and shown it in Fig. 4(b). Clearly, if two charges are very close together, there is not enough space for the electronic cloud to polarize, so ε2D(𝒔0)\varepsilon_{\rm 2D}(\bm{s}\rightarrow 0) == 11. On the other hand, if the two charges are very far away, the field lines connecting the charges travel mainly through the vacuum, so they are not much affected by the intrinsic dielectric environment of the quasi-2D semiconductor and ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}\rightarrow\infty) == 11. Between these two ends, ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}) is influenced by the intrinsic material property of CrSBr monolayer and is larger than 1. At finite distance 𝒔max\bm{s}_{max}, ε2D(𝒔max)\varepsilon_{\rm 2D}(\bm{s}_{max}) will exhibit its maximum. Such kind of 2D dielectric screening has also been revealed in MoS2 monolayer with 𝒔max=1.5\bm{s}_{max}=1.5 Å\rm\AA and ε2D(𝒔max)\varepsilon_{\rm 2D}(\bm{s}_{max}) = 11 [44]. For CrSBr monolayer, 𝒔max\bm{s}_{max} is little larger and ε2D(𝒔max)\varepsilon_{\rm 2D}(\bm{s}_{max}) is weaker. In the meantime, due to anisotropic crystal structure, the 2D dielectric screening in CrSBr monolayer also exhibits strong anisotropy. ε2D(𝒔max)\varepsilon_{\rm 2D}(\bm{s}_{max}) is 4.4 and 7.0 for ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}) along xx and yy axis, respectively. And corresponding 𝒔max\bm{s}_{max} is 3.0 Å\rm\AA and 4.0 Å\rm\AA, the same order with lattice constants. Interestingly, such kind of anisotropy persists to long distance. As shown in the inset of Fig. 4(b), the difference between ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}) along xx and yy axis does not vanish until 60 Å\rm\AA. So at the distance from 1 Å\rm\AA to ten times length of lattice constant, the anisotropic dielectric screening dominates Coulomb interaction in CrSBr monolayer. For 2D system, Coulomb potential could be described by the Keldysh model [17], where the potential between two charges has the form

V2D(𝒔)=πe22ρ0[H0(|𝒔|ρ0)Y0(|𝒔|ρ0)].V_{\rm 2D}(\bm{s})=\frac{\pi e^{2}}{2\rho_{0}}[H_{0}(\frac{|\bm{s}|}{\rho_{0}})-Y_{0}(\frac{|\bm{s}|}{\rho_{0}})]. (5)

Here H0H_{0} and Y0Y_{0} are, respectively, the Struve and Bessel functions of the second kind. ρ0\rho_{0} is a screening length, which is ρ0=2πα2D\rho_{0}=2\pi\alpha_{\rm 2D}, and α2D\alpha_{\rm 2D} is the 2D polarizability. Taking the 2D Fourier transform of Eq. 5 results in a dielectric function of the form

ε2D(𝒒)=1+ρ0|𝒒|.\varepsilon_{\rm 2D}(\bm{q})=1+\rho_{0}|\bm{q}|. (6)

We fit the Keldysh model to our abab initioinitio effective dielectric function at small 𝒒\bm{q}, where the Coulomb potential approaches 1/s. The 2D polarizability, however, shows large difference between orthogonal two directions. α2D\alpha_{\rm 2D} is 4.2 Å\rm\AA for 𝒒\bm{q} along xx axis and 10.4 Å\rm\AA for 𝒒\bm{q} along yy axis. Based on above discussion, in sufficiently long range from 1 Å\rm\AA to 60 Å\rm\AA, the dielectric screening in CrSBr monolayer is anisotropic.

Refer to caption
Figure 4: (a) Frequency-dependence of 2D dielectric screening in CrSBr monolayer under abab initioinitio calculation. (b) Distance-dependence of 2D dielectric screening in CrSBr monolayer under abab initioinitio calculation (solid line) and Keldysh model (dashed line). Inset of (b) shows the difference between ε2D(𝒔)\varepsilon_{\rm 2D}(\bm{s}) along yy axis and xx axis.

Due to the unique dielectric environment (monolayer 2D material suspended in vacuum or other dielectric surroundings), electron-electron and electron-hole interactions in 2D materials are much stronger than conventional bulk materials, like GaAs, Si, and so on. Therefore, dielectric screening in 2D materials is reduced compared with conventional bulk materials. With the reduced dielectric screening in 2D CrSBr monolayer, the quasiparticle correction to the electronic band structure is large. At Γ\Gamma point, the quasiparticle band gap is 2.22 eV, where the value is 0.50 eV within PBE. In Fig. 5, we have shown the direct quasiparticle band gap in the Brillouin zone. The one-dimensional nature of the lowest transition energies is obvious.

Refer to caption
Figure 5: The lowest valence to conduction band transition energy (based on quasiparticle energies).

The optical absorbance in CrSBr monolayer is further calculated and shown in Fig. 6, where the difference between two in-plane orthogonal directions is obvious. Although the main optical absorption is located at 3.01 eV, the small peak located below could catch as high as 20 % of the incident light. The optical absorption edge is located at 1.35 eV when the electric field is along y direction. For the other direction, the absorption edge is 1.73 eV. Compared with the results without the consideration of electron-hole interaction, the excitonic effect is obvious in this 2D material. In Fig. 6(c), the exciton states are demonstrated and agree with the optical spectrum well. Dark excitons are also indicated in these non-Rydberg series. Clearly, the binding energy for the first exciton state could reach as high as 1.0 eV, almost 1/3 of the quasiparticle band gap for the center of electron-hole excitations. When the electric field is rotated along the xy plane, as shown in Fig. 7 for several bright exciton states, the oscillator strength shows an anisotropic distribution.

Refer to caption
Figure 6: Anisotropic optical absorbance with electric polarization along x axis (a) and y axis (b) and corresponding exciton spectrum (c) in CrSBr monolayer. Here, green lines are for the bright excitons and the gray lines are for dark excitons. The dotted lines are for the optical absorption based on IPA. Inset shows the experiment data of PL spectrum of CrSBr monolayer under magnetic field along y axis [12].
Refer to caption
Figure 7: Optical anisotropy (absorbance amplitude) for the five excitonic states with the wavelength of 1.35 eV (918 nm), 1.66 eV (747 nm), 1.76 eV (705 nm), 1.73 eV (716 nm), and 1.99 eV (623 nm), respectively.
Refer to caption
Figure 8: Real-space plots (upper panel) of modulus squared of the exciton wave function and corresponding reciprocal-space plots (down panel) for the first eight excitons. Here, the hole (black circle) is fixed at Cr.

We now look at the character of the first eight excitons, which are all excited around the Γ\Gamma point. In Fig. 8, we show the modulus squared of the real-space exciton wave function when the hole is fixed near a Cr atom. Electron-hole pair amplitudes (the envelope functions) of low energy exciton wave functions in reciprocal space are plotted in the down panel of each figure. From these plots, the nodal structures of the envelope functions of the states are apparent. 1s1s state has only one node with the strongest transition at Γ\Gamma point. In detail, in Fig. 8(a), the character of the exciton corresponding to the first peak in the absorption spectrum (E\parallely) reflects the transitions from the top of valence band to the lowest conduction band around Γ\Gamma point. The envelope of the exciton wave function is almost azimuthally symmetric. The root-mean-square radius of the exciton in real space is around 1.4 nm. The second excitonic state is a dark exciton. It is also a 1s state and also arises from the electron-hole excitations around Γ\Gamma point, but the orbitals for the electron-hole formation are different from the first bright state. Although it has a much smaller oscillator strength, the electric polarization along y direction is much higher than that along the x direction. The next two dark excitons shown in Fig. 8(c) and (d) are 2p2p states. Bright exciton shown in Fig. 8(e) is 2s state and the exciton in Fig. 8(h) is 3d state. Together with the first state, these five states could be categorized into the series of electron-hole excitations from v1 to c1 mainly at Γ\Gamma point. This can also be judged from energy distribution in Fig. 9, where the distribution of the constituent free electron-hole pairs specified by (EvE_{v}, EcE_{c}) for selected exciton states weighted by the module squared exciton envelop function for each specific interband transition is plotted for all these eight excitonic states. Clearly, these five states have similar patterns. As shown in Appendix C, the orbitals corresponding to the electron-hole pairs are Cr dyzd_{yz} and Cr dx2y2d_{x^{2}-y^{2}} [71]. For the second and sixth excitons, it involves v1 to c2 transitions, i.e., from Cr dyzd_{yz} to Cr dx2y2d_{x^{2}-y^{2}} hybrid with S 3p3p. These transitions bring to the above mentioned dark 1s state in Fig. 8(b) and the bright 2p state in Fig. 8(f). For the exciton shown in Fig. 8(g), it involves more complicated electron-hole pairs formation (from v2 to c1 and v1 to c2 as indicated in Fig. 9(g)), and it is a dark state. Characterization of all the node structures of these excitons is summarized in Table I. Obviously, these excitons process an increased real-space extension of the wave function. The effective electron-hole interaction is therefore reduced strongly, consistent with the smaller binding energy as shown in Table I. The difference in the oscillator strength between x direction and y direction is obvious for all the exciton states.

Refer to caption
Figure 9: The distribution of free electron-hole pair with electron energy at EcE_{c} and hole energy at EvE_{v} for selected exciton states weighted by module squared exciton envelope function for each interband transitions between states |vk|\textbf{vk}\rangle and |ck|\textbf{ck}\rangle, with quasiparticle energies of EvkQPE^{\rm QP}_{vk} and EckQPE^{\rm QP}_{ck}, respectively.
Table 1: Excitonic properties of first eight excitons with excitation energy (ExctE_{xct}), exciton binding energy (EbE_{b}), and oscillator strength for electric field along xx and yy directions.
Excitons ExctE_{xct} (eV) EbE_{b} Oscillator strength
E \parallel x E \parallel y
1 1.351 0.870 1.9×1031.9\times 10^{-3} 2.3×1042.3\times 10^{4}
2 1.468 0.735 2.7×1062.7\times 10^{-6} 3.2×1043.2\times 10^{-4}
3 1.586 0.635 3.6×1023.6\times 10^{-2} 4.7×1004.7\times 10^{0}
4 1.599 0.622 2.8×1032.8\times 10^{-3} 4.1×1004.1\times 10^{0}
5 1.659 0.562 6.4×1016.4\times 10^{-1} 5.8×1035.8\times 10^{3}
6 1.665 0.556 1.2×1011.2\times 10^{-1} 4.6×1024.6\times 10^{2}
7 1.673 0.548 3.8×1043.8\times 10^{-4} 5.0×1015.0\times 10^{-1}
8 1.729 0.492 8.3×1018.3\times 10^{1} 3.8×1023.8\times 10^{2}

With the above revealed anisotropic quasiparticle electronic band structure, electron-hole excitation, and optical absorption, we continue to show the (magnetic) linear dichroism and MO SH and Vogit effects in CrSBr monolayer. The essence of a theoretical modeling of the MO effects lies in accurately accounting for the diagonal and off-diagonal frequency-dependent macroscopic dielectric functions, which have been readily available from our G0W0G_{0}W_{0}-BSE calculations with electron-hole interaction included. As verified by the agreement between our theoretical calculations and experiments of CrSBr as well as the fact that exciton effect in ferromagnetic monolayer CrI3 and CrBr3 has strongly modified its MO responses [9, 10], significantly different behaviors going beyond those from a treatment considering only transitions between non-interacting Kohn-Sham orbitals should be expected in CrSBr. To simulate the experimental setup, as demonstrated in Fig. 1, we consider CrSBr monolayer deposited on a dielectric substrate α\alpha-Al2O3, which has a wide band gap of 8.7 eV with refraction constant of 1.75 [10]. Assuming a linearly polarized incident light, we calculate the SH and Voigt signals by analyzing the polarization plane of the reflection (transmission) light, which is in general elliptically polarized with a rotation angle and an ellipticity. The detailed calculations are based on the transfer matrix method and could be found in Appendix D. In Fig. 10, we have found that the rotation angle could be larger than 10 for the reflected light. For transmitted light, the largest rotation angle is around 8. On the other hand, the revealed SH and Voigt effects dominate within the quasiparticle band gap. When the electron-hole interaction is not considered, both the amplitude and the position of the spectrum are modified significantly (see Fig. 15 in Appendix E). This verifies again the fact that it is the exciton effect that leads to the large linear dichroism in CrSBr monolayer. In addition, we can find that the off-diagonal component of dielectric function plays little role in the above revealed large linear dichroism in CrSBr, where as shown in Fig. 16 (Appendix E), θSH\theta_{\rm SH} and θV\theta_{\rm V} do not change.

Refer to caption
Figure 10: Rotation angles of (a) reflected and (b) transmitted light in CrSBr monolayer. Insets are ellipticity.

We have also performed the calculations of magneto-optical effects when spin orientation is pointing along xx and zz axis. As shown in Fig. 17 and Fig. 18 (Appendix F), absorbance spectrum and exciton states are similar to those for the state with spin orientation along yy axis. In the meantime, due to extremely small εyz\varepsilon_{yz}, the revealed rotation angle of long axis of the polarization ellipse for reflection and transmission light is still determined by the large ratio of εxx\varepsilon_{xx}/εyy\varepsilon_{yy} (see Fig. 19 in Appendix G). On the other hand, when spin orientation is tuned by external perpendicular magnetic field towards out-of-plane direction, i.e. zz axis, the magneto-optical Kerr and Faraday effects will appear in CrSBr monolayer. In this case, a linearly polarized continuous-wave light is modified by the presence of out-of-plane magnetic field when propagating through CrSBr monolayer. The left and right-circularly polarized components will propagate with different refractive index and will pick up different optical path length and absorption. Therefore, the reflected or transmitted light becomes elliptically polarized (characterized by an ellipticity η\eta), and the long axis of the polarization ellipse is rotated (characterized by a rotation angle θ\theta). The detailed theoretical calculations of rotation angles and ellipticities are shown in Appendix H. Meanwhile, as shown in Fig. 21 (Appendix H), the maximal rotation angles of Kerr and Faraday effects are 1.1 and 0.6, respectively, which are even larger than 0.9 and 0.3 in CrI3 [9] and 0.3 and 0.2 in CrBr3 [10]. Similar to the cases with in-plane magnetization, the optical spectrum has been modified significantly for the exciton effects (see Fig. 22 in Appendix H). We list the maximal rotation angles in TABLE II for different spin orientations. Therefore, for both linearly and circularly polarized light, the large phase shift facilitates the applications of CrSBr monolayer as optical polarizers and waveplates.

Table 2: Comparison of magneto-optical effects for reflection and transmission lights, polarization of lights propagating in CrSBr monolayer, off-diagonal elements, and maximums of corresponding rotation angles with electron-hole interaction when spin orientation is along xx, yy, and zz axis in the energy range of 0 \sim 3 eV.
Spin orientation Magneto-optical effects Polarization Off-diagonal elements Rotation angles ()
xx SH/Voigt linear εyz\varepsilon_{yz} 11.6/8.1
yy SH/Voigt linear εxz\varepsilon_{xz} 11.6/8.1
zz Kerr/Faraday circular εxy\varepsilon_{xy} 1.1/0.6

For black phosphorene, it is noted that the ratio between the long axis and short one is 1.4 for the anisotropic crystal structure and 1.5 eV energy difference between absorption edges for the electric field along two axes could be found (see Fig. 23 in Appendix I). For comparison, it is noted that the rotational angle in black phosphorene is of similar magnitude. However, CrSBr shows two broad peaks at the energies of both infrared and red lights, whereas black phosphorene exhibits a single narrow peak in this energy window (see Fig. 24 in Appendix I). Additionally, obvious linear dichroism has been revealed experimentally in black phosphorene and its few-layers [72, 73, 74, 75]. Therefore, polarization-sensitive broadband photodetector using a CrSBr vertical p-n junction could be constructed successfully for the application in 2D semiconductor optoelectronics.

To demonstrate other potential applications in 2D semiconductor optoelectronics, we further calculate the lifetime of the first bright exciton. Using “Fermi’s golden rule”, the radiative lifetime τS(0)\tau_{S}(0) at 0 K of an exciton in state SS is derived according to [76, 77]

τS(0)=2c8πe2ES(0)AucμS2,\tau_{S}(0)=\frac{\hbar^{2}c}{8\pi e^{2}E_{S}(0)}\frac{A_{\rm{uc}}}{\mu_{S}^{2}}, (7)

where cc is the speed of light, AucA_{\rm{uc}} is the area of the unit cell, ES(0)E_{S}(0) is the energy of the exciton in state S, and μS2=(2/m2ES(0)2)(|G|p|||ΨS|2/Nk)\mu_{S}^{2}=(\hbar^{2}/m^{2}E_{S}(0)^{2})(|\left\langle G|p_{||}|\Psi_{S}\right\rangle|^{2}/N_{k}) is the square modulus of the BSE exciton transition dipole divided by the number of unit cells in this 2D system. The exciton radiative lifetime τS\left\langle\tau_{S}\right\rangle at temperature T is obtained as

τS=τS(0)34(ES(0)22MSc2)1kBT,\left\langle\tau_{S}\right\rangle=\tau_{S}(0)\frac{3}{4}(\frac{E_{S}(0)^{2}}{2M_{S}c^{2}})^{-1}k_{\rm B}T, (8)

where kBk_{\rm{B}} is Boltzmann constant, and MS=me+mhM_{S}=m_{e}^{*}+m_{h}^{*} is the exciton effective mass. The computed radiative lifetime of the first bright exciton in CrSBr monolayer at 4 and 300 K is 0.001 ns and 0.100 ns, respectively, which are even smaller than those in the conventional transition metal dichalcogenides, e.g., 0.004 ns and 0.270 ns in MoS2 [77]. In Table III, we have listed the exciton lifetime of some typical 2D semiconductors [56, 57, 59, 64, 77, 78, 79, 80, 81, 82, 83, 84, 85, 86], as well as conventional semiconductor GaInN/GaN quantum wells [87]. Clearly, such a short lifetime in CrSBr monolayer together with its direct band gap shows its advantages in infrared light-emitting applications. Moreover, as shown in Fig. 11, the strong optical absorption of CrSBr monolayer covering the whole solar spectrum as well as its optimized band gap (1.35 eV) within the Shockley-Queisser limit also suggests efficient solar energy conversion. Therefore, from gapless graphene to narrow-band-gap black phosphorene, intermediate-band-gap transition-metal dichalcogenides, and wide-band-gap semiconductors of Hittorf’s phosphorene, blue phosphorene, III-V monochalcogenides, and boron nitride, magnetic CrSBr could play an important role in infrared optoelectronics and 2D photovoltaics.

Table 3: Collection of exciton radiative lifetime τ\tau (ns) for various 2D materials. τSLT\tau_{\rm S}^{\rm LT} and τSRT\tau_{\rm S}^{\rm RT} are the computed radiative lifetimes at low temperature (\approx 4 K) and room temperature, respectively. Experimental data of τexpLT\tau_{\rm exp}^{\rm LT} and τexpRT\tau_{\rm exp}^{\rm RT} are also listed for comparison.
τSLT\tau_{\rm S}^{\rm LT} τSRT\tau_{\rm S}^{\rm RT} τexpLT\tau_{\rm exp}^{\rm LT} τexpRT\tau_{\rm exp}^{\rm RT}
CrSBr monolayer 0.001 0.100
Black phosphorus monolayer 3×1053\times 10^{-5} [56] 0.002 [56] 0.221 [78]
Hittorf’s phosphorus monolayer 0.24 [59] 18 [59]
GeS monolayer 7×1057\times 10^{-5} [56] 0.005 [56]
ReS2 monolayer 0.04 [79]
Blue phosphorus monolayer 0.003 [57] 0.24 [57]
MoS2 monolayer 0.004 [77] 0.27 [77] 0.005 [80], 0.005 [81] 0.85 [82]
MoSe2 monolayer 0.005 [77] 0.38 [77] 0.002 [83] 0.9 [84]
WS2 monolayer 0.002 [77] 0.17 [77]
WSe2 monolayer 0.004 [77] 0.29 [77] 0.002 [83], 0.004 [85] 4 [86]
2D GaN 0.6 [64]
GaInN/GaN QW 10210^{2} [87]
Refer to caption
Figure 11: Some 2D materials covering a broad spectral range, from gapless graphene to narrow-band-gap black phosphorene, intermediate-band-gap transition-metal dichalcogenides, and wide-band-gap semiconductors of Hittorf’s phosphorene, blue phosphorene, III-V monochalcogenides, and boron nitride. Squares and circles represent direct and indirect band gap semiconductors, respectively. The solar spectrum [88] and averaged absorbance (dashed red line) of light polarized along xx and yy axis in CrSBr monolayer are also shown.

IV summary

To summarize, by considering explicitly many-body effects of the electron-electron and electron-hole interactions in 2D ferromagnet CrSBr, we have demonstrated unusual large optical anisotropy in this 2D material. The inherent in-plane magnetization with the consideration of spin-orbit coupling is found to contribute little to the revealed large linear dichroism. The giant SH and Voigt effects, which are comparable with those in black phosphorene, originate from the inherent anisotropic crystal structure and coherent one-dimensional band dispersion for anisotropic electron-hole pairs excitation. Our calculation of the first exciton located at 1.35 eV agrees with a recent experiment of photoluminescence. The in-gap exciton states of either bright or dark show the diversity of electron-hole excitation in this 2D magnet. Compared with black phosphorene, the relative delocalization of exciton in k-space indicates the nature of electron-hole excitation in CrSBr is in-between Wannier-Mott type and Frenkel type. Excitonic effect has modified εxx\varepsilon_{xx}, εyy\varepsilon_{yy}, and εxz\varepsilon_{xz} dramatically, and consequently the linear dichroism and the magneto-optical properties. With out-of-plane magnetization, Kerr and Faraday effects have been revealed in CrSBr monolayer, which are even larger than those in CrI3 and CrBr3. Furthermore, the short exciton lifetime as well as the strong optical absorption covering the whole solar spectrum shows its advantages in application of light-emitting diode and solar cell. Our studies have provided a basic framework to account for the high-order magneto-optical effects in 2D magnets and also shown potential applications of CrSBr in 2D optics and optoelectronics.

Acknowledgements.
S. J. thanks Prof. Steven G. Louie and his group for their great help on BerkeleyGW method and useful discussion of exciton physics in 2D materials. This work is supported by the National Basic Research Program of China (973 Program 2019YFA0308402) and the National Natural Science Foundation of China under Grant No. 51972217. T. X. Q. and J. Z. contributed equally to this work.

Appendix A BASIC FRAMEWORK OF GW-BSE IN BERKELEYGW PACKAGE

Generally, the quasiparticle self-energies are obtained by solving the Dyson equation [26].

[122+Vion+VH+Σ(En𝐤QP)]ψn𝐤QP=En𝐤QPψn𝐤QP,\left[-\frac{1}{2}\nabla^{2}+V_{\rm ion}+V_{\rm H}+\Sigma\left(E^{\rm QP}_{n{\rm\bf{k}}}\right)\right]\psi^{\rm QP}_{n{\rm\bf{k}}}=E^{\rm QP}_{n{\rm\bf{k}}}\psi^{QP}_{n{\rm\bf{k}}}, (9)

where Σ\Sigma is the self-energy operator within the GW approximation, and En𝐤QPE^{QP}_{n{\rm\bf{k}}} and ψn𝐤QP\psi^{QP}_{n{\rm\bf{k}}} are the quasiparticle energies and wavefunctions, respectively. The self-energy operator Σ\Sigma is invoked for the quasiparticle behavior with quasiparticle energies En𝐤QPE^{\rm QP}_{n{\rm\bf{k}}} and wave functions ψn𝐤QP\psi^{\rm QP}_{n{\rm\bf{k}}}. Here, we use the many-body perturbation method with one-shot G0W0G_{0}W_{0} framework. The mean-field wave functions within DFT-PBE are used as quasiparticle wave functions and the quasiparticle energy is approached starting from DFT-PBE eigenvalue.

We first compute static polarizability based on random-phase approximation (RPA) [26]:

χ𝐆𝐆(𝐪;0)=n,n,𝐤n,𝐤|ei(𝐪+𝐆)𝐫|n,𝐤+𝐪n,𝐤+𝐪|ei(𝐪+𝐆)𝐫|n,𝐤1En𝐤+𝐪En𝐤,\chi_{\rm\bf{GG^{\prime}}}({\rm\bf{q}};0)=\sum_{n,n^{\prime},\rm\bf{k}}\langle n,{\rm\bf{k}}|e^{-i({\rm\bf{q}}+{\rm\bf{G}})\cdot{\rm\bf{r}}}|n^{\prime},{\rm\bf{k}}+{\rm\bf{q}}\rangle\langle n^{\prime},{\rm\bf{k}}+{\rm\bf{q}}|e^{i({\rm\bf{q}}+{\rm\bf{G^{\prime}}})\cdot{\rm\bf{r}}^{\prime}}|n,{\rm\bf{k}}\rangle\frac{1}{E_{n^{\prime}{\rm\bf{k}}+{\rm\bf{q}}}-E_{n{\rm\bf{k}}}}, (10)

where nn, nn^{\prime} are occupied and unoccupied band indices, 𝐤\rm\bf{k} is wave vector, 𝐪\rm\bf{q} is a vector in the first Brillouin zone, 𝐆\rm\bf{G} is a reciprocal-lattice vector, and |n,𝐤|n,\rm\bf{k}\rangle and En𝐤E_{n\rm\bf{k}} are the mean-field electronic eigenvectors and eigenvalues, respectively.

Then the dielectric matrix is constructed as [26]

ε𝐆𝐆(𝐪;0)=δ𝐆𝐆v(𝐪+𝐆)χ𝐆𝐆(𝐪;0),\varepsilon_{\rm\bf{GG^{\prime}}}({\rm\bf{q}};0)=\delta_{\rm\bf{GG^{\prime}}}-v({\rm\bf{q}}+{\rm\bf{G}})\chi_{\rm\bf{GG^{\prime}}}({\rm\bf{q}};0), (11)

with the slab-truncated Coulomb interaction included [30],

vtslab(𝐪)=4πq2(1eqxyzccos(qzzc)),v_{\rm t}^{\rm slab}({\rm\bf{q}})=\frac{4\pi}{q^{2}}\cdot\left(1-e^{-q_{xy}\cdot z_{c}}{\rm cos}(q_{z}\cdot z_{c})\right), (12)

where zcz_{c} is the truncation distance in the perpendicular direction. Such kind of treatment could guarantee the convergence of dielectric screening (“head” in ε𝐆𝐆\varepsilon_{\rm\bf{GG^{\prime}}}) to approach to unit in the long wavelength limit.

Within the generalized plasmon pole (GPP) model, the imaginary and real part inverse dielectric matrix with finite frequencies are given by [26]

Imε𝐆𝐆1(𝐪,ω)=π2Ω𝐆𝐆(𝐪)ω~𝐆𝐆(𝐪){δ[ωω~𝐆𝐆(𝐪)]δ[ω+ω~𝐆𝐆(𝐪)]},{\rm Im}\varepsilon_{\rm\bf{GG^{\prime}}}^{-1}({\rm\bf{q}},\omega)=-\frac{\pi}{2}\frac{\Omega_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})}{\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})}\left\{\delta[\omega-\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})]-\delta[\omega+\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})]\right\}, (13)

and

Reε𝐆𝐆1(𝐪,ω)=1+Ω𝐆𝐆2(𝐪)ω2ω~𝐆𝐆2(𝐪),{\rm Re}\varepsilon_{\rm\bf{GG^{\prime}}}^{-1}({\rm\bf{q}},\omega)=1+\frac{\Omega_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}{\omega^{2}-\tilde{\omega}_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}, (14)

where Ω𝐆𝐆(𝐪)\Omega_{\rm\bf{GG^{\prime}}}({\rm\bf{q}}) and ω~𝐆𝐆(𝐪)\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}}) are the effective bare plasma frequency and the GPP mode frequency defined as [26]:

Ω𝐆𝐆2(𝐪)=ωp2(𝐪+𝐆)(𝐪+𝐆)|𝐪+𝐆|2ρ(𝐆𝐆)ρ(𝟎),\Omega^{2}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})=\omega_{\rm p}^{2}\frac{({\rm\bf{q}}+{\rm\bf{G}})\cdot({\rm\bf{q}}+{\rm\bf{G^{\prime}}})}{|{\rm\bf{q}}+{\rm\bf{G}}|^{2}}\frac{\rho({\rm\bf{G}}-{\rm\bf{G^{\prime}}})}{\rho(\bf{0})}, (15)
ω~𝐆𝐆2(𝐪)=Ω𝐆𝐆2(𝐪)δ𝐆𝐆ε𝐆𝐆1(𝐪,ω=0).\tilde{\omega}_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})=\frac{\Omega_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}{\delta_{\rm\bf{GG^{\prime}}}-\varepsilon_{\rm\bf{GG^{\prime}}}^{-1}({\rm\bf{q}},\omega=0)}. (16)

Here ρ\rho is the electron charge density in reciprocal space and ωp2=4πρ(𝟎)e2/m\omega_{\rm p}^{2}=4\pi\rho({\bf 0})e^{2}/m is the classical plasma frequency.

Using the form of the above frequency-dependent dielectric function, the self-energy operator Σ\rm\Sigma is solved in two parts, Σ=ΣSEX+ΣCOH\rm\Sigma=\Sigma_{SEX}+\Sigma_{COH}, where ΣSEX\rm\Sigma_{SEX} is the screened exchange operator and ΣCOH\rm\Sigma_{COH} is the Coulomb-hole operator as [26]

n,𝐤|ΣSEX(E)|n,𝐤=n1occ𝐪,𝐆,𝐆n,𝐤|ei(𝐪+𝐆)𝐫|n1,𝐤𝐪n1,𝐤𝐪|ei(𝐪+𝐆)𝐫|n,𝐤\displaystyle\langle n,{\rm\bf{k}}|{\rm\Sigma_{SEX}}(E)|n^{\prime},{\rm\bf{k}}\rangle=-\sum_{n_{1}}^{\rm occ}\sum_{\rm\bf{q,G,G^{\prime}}}\langle n,{\rm\bf{k}}|e^{i({\rm\bf{q}}+{\rm\bf{G}})\cdot{\rm\bf{r}}}|n_{1},{\rm\bf{k}}-{\rm\bf{q}}\rangle\langle n_{1},{\rm\bf{k}}-{\rm\bf{q}}|e^{-i({\rm\bf{q}}+{\rm\bf{G^{\prime}}})\cdot{\rm\bf{r^{\prime}}}}|n^{\prime},{\rm\bf{k}}\rangle (17)
×(1+Ω𝐆𝐆2(𝐪)(EEn1𝐤𝐪)2ω~𝐆𝐆2(𝐪))v(𝐪+𝐆),\displaystyle\times\left(1+\frac{\Omega_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}{(E-E_{n_{1}{\rm\bf{k-q}}})^{2}-\tilde{\omega}_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}\right)v({\rm\bf{q+G^{\prime}}}),

and

n,𝐤|ΣCOH(E)|n,𝐤=n1𝐪,𝐆,𝐆n,𝐤|ei(𝐪+𝐆)𝐫|n1,𝐤𝐪n1,𝐤𝐪|ei(𝐪+𝐆)𝐫|n,𝐤\displaystyle\langle n,{\rm\bf{k}}|{\rm\Sigma_{COH}}(E)|n^{\prime},{\rm\bf{k}}\rangle=\sum_{n_{1}}\sum_{\rm\bf{q,G,G^{\prime}}}\langle n,{\rm\bf{k}}|e^{i({\rm\bf{q}}+{\rm\bf{G}})\cdot{\rm\bf{r}}}|n_{1},{\rm\bf{k}}-{\rm\bf{q}}\rangle\langle n_{1},{\rm\bf{k}}-{\rm\bf{q}}|e^{-i({\rm\bf{q}}+{\rm\bf{G^{\prime}}})\cdot{\rm\bf{r^{\prime}}}}|n^{\prime},{\rm\bf{k}}\rangle (18)
×12Ω𝐆𝐆2(𝐪)ω~𝐆𝐆(𝐪)[EEn1𝐤𝐪ω~𝐆𝐆(𝐪)]v(𝐪+𝐆).\displaystyle\times\frac{1}{2}\frac{\Omega_{\rm\bf{GG^{\prime}}}^{2}({\rm\bf{q}})}{\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})[E-E_{n_{1}{\rm\bf{k-q}}}-\tilde{\omega}_{\rm\bf{GG^{\prime}}}({\rm\bf{q}})]}v({\rm\bf{q+G^{\prime}}}).

With the above obtained quasiparticle energies and static dielectric screening from RPA, the electron-hole excitations are then calculated by solving the BSE for each exciton state S [27]:

(Ec𝐤QPEv𝐤QP)Avc𝐤S+vc𝐤vc𝐤|Keh|vc𝐤Avc𝐤S=ΩSAvc𝐤S,\left(E^{\rm QP}_{c{\rm\bf{k}}}-E^{\rm QP}_{v{\rm\bf{k}}}\right)A^{S}_{vc{\rm\bf{k}}}+\sum_{v^{\prime}c^{\prime}{\rm\bf{k}}^{\prime}}\left\langle vc{\rm\bf{k}}\left|K^{\rm eh}\right|v^{\prime}c^{\prime}{\rm\bf{k}}^{\prime}\right\rangle A^{S}_{v^{\prime}c^{\prime}{\rm\bf{k^{\prime}}}}={\Omega}^{S}A^{S}_{vc{\rm\bf{k}}}, (19)

where Avc𝐤SA^{S}_{vc{\rm\bf{k}}} is the exciton wavefunction, ΩS\Omega^{S} is the excitation energy, and KehK^{\rm eh} is the electron-hole interaction kernel.

The kernel contains two terms, a screened direct interaction and a bare exchange interaction, Keh=Kd+KxK^{\rm eh}=K^{\rm d}+K^{\rm x}, defined as [27]:

vc𝐤|Kd|vc𝐤=𝐆𝐆c,𝐤+𝐪|ei(𝐪+𝐆)𝐫|c,𝐤W𝐆𝐆(𝐪;0)v,𝐤|ei(𝐪+𝐆)𝐫|v,𝐤+𝐪,\left\langle vc{\rm\bf{k}}\left|K^{\rm d}\right|v^{\prime}c^{\prime}{\rm\bf{k}}^{\prime}\right\rangle=\sum_{\rm\bf{GG^{\prime}}}\langle c,{\rm\bf{k+q}}|e^{-i({\rm\bf{q}}+{\rm\bf{G}})\cdot{\rm\bf{r}}}|c^{\prime},{\rm\bf{k}}\rangle W_{\rm\bf{GG^{\prime}}}({\rm\bf{q}};0)\langle v^{\prime},{\rm\bf{k}}|e^{i({\rm\bf{q}}+{\rm\bf{G^{\prime}}})\cdot{\rm\bf{r}}}|v,{\rm\bf{k+q}}\rangle, (20)

and

vc𝐤|Kx|vc𝐤=𝐆𝐆c,𝐤+𝐪|ei(𝐪+𝐆)𝐫|v,𝐤δ𝐆𝐆v(𝐪+𝐆)v,𝐤|ei(𝐪+𝐆)𝐫|c,𝐤+𝐪.\left\langle vc{\rm\bf{k}}\left|K^{\rm x}\right|v^{\prime}c^{\prime}{\rm\bf{k}}^{\prime}\right\rangle=\sum_{\rm\bf{GG^{\prime}}}\langle c,{\rm\bf{k+q}}|e^{-i({\rm\bf{q}}+{\rm\bf{G}})\cdot{\rm\bf{r}}}|v,{\rm\bf{k}}\rangle\delta_{\rm\bf{GG^{\prime}}}v({\rm\bf{q}}+{\rm\bf{G}})\langle v^{\prime},{\rm\bf{k}}|e^{i({\rm\bf{q}}+{\rm\bf{G^{\prime}}})\cdot{\rm\bf{r}}}|c^{\prime},{\rm\bf{k+q}}\rangle. (21)

Finally, we obtain the imaginary parts of frequency-dependent complex dielectric function ε2(ω)\varepsilon_{2}(\omega) as [27]

ε2(ω)=16π2e2ω2S|𝐞0|𝐯|S|2δ(ωΩS),\varepsilon_{2}(\omega)=\frac{16\pi^{2}e^{2}}{\omega^{2}}\sum_{S}\left|{\rm\bf{e}}\cdot\left\langle 0|{\rm\bf{v}}|S\right\rangle\right|^{2}\delta\left(\omega-\Omega^{S}\right), (22)

where 𝐯\rm\bf{v} is the velocity operator and 𝐞\rm\bf{e} is the polarization of the incoming light. Here, we use absorbance 𝒜\mathcal{A} of 2D materials to measure their optical properties, which is expressed as [62]

𝒜(ω)=1eα(ω)d=1eωε2dc,\mathcal{A}(\omega)=1-e^{-\alpha(\omega)d}=1-e^{-\frac{\omega\varepsilon_{2}d}{\hbar c}}, (23)

where α\alpha is the absorption coefficient, d is the thickness of the simulation cell along the direction perpendicular to the layer, ε2\varepsilon_{2} is the imaginary part of the dielectric function, and ω\omega is the photon energy, respectively.

Appendix B CONVERGENCE OF G0W0G_{0}W_{0}-BSE CALCULATIONS OF CrSBr MONOLAYER

In Fig. 12, we show the convergence of quasiparticle energies in CrSBr with respect to (a) the scale of kk grid (coarse grid), (b) the number of bands, and (c) the dielectric cutoff. It is noted that fine sampling is necessary to capture the rapid variation in screening at small wave vectors and the fine features in the exciton wave functions, which are tightly localized in k space. In Fig. 13, besides the RPA dielectric function, we show the convergence of exciton energy in CrSBr with respect to the scale of kk grid (fine grid).

Refer to caption
Figure 12: Convergence of the quasiparticle (G0W0G_{0}W_{0}) band gap at three high symmetry kk points with respect to the scale of coarse k grid (a), number of bands (b), and dielectric cutoff energy (εcutoff\varepsilon_{\rm cutoff}) (c). In (a), we use a εcutoff\varepsilon_{\rm cutoff} of 20 Ry and 1080 bands; in (b), we use a k grid of 16×12×116\times 12\times 1 and 1080 bands; and in (c), we use a εcutoff\varepsilon_{\rm cutoff} of 20 Ry and a k grid of 16×12×116\times 12\times 1. With the above consideration, we use a 16×12×116\times 12\times 1 k grid, a εcutoff\varepsilon_{\rm cutoff} of 20 Ry, and 1080 (20 times larger) bands for our G0W0G_{0}W_{0} calculations.
Refer to caption
Figure 13: Convergence of the energy of the 1s exciton state in BSE calculations with respect to the scale of the fine k grids: including 32×24×132\times 24\times 1, 60×60×160\times 60\times 1, 48×36×148\times 36\times 1, and 64×48×164\times 48\times 1. With the above consideration, we use a 64×48×164\times 48\times 1 k grid in our BSE calculations.

Appendix C MAXIMUM LOCALIZED WANNIER ORBITALS IN CRSBR

Using Wannier90 [71], the orbital-decomposed band structure (PBE level) is shown in Fig. 14.

Refer to caption
Figure 14: The up panel shows the orbital-decomposed band structure (DFT-PBE level) of CrSBr from maximum localized Wannier orbitals using Wannier90 [71]. The partial charge at Γ\Gamma point is shown in the down panel.

Appendix D CALCULATIONS OF LINEAR DICHROISM (OPTICAL BIREFRIGENCE) AND SCHAFER-HUBERT AND VOIGT EFFECTS

As shown in Fig. 1, considering the in-plane magnetization along y axis (𝑩=B𝒆^𝒚\bm{B}=B\bm{\hat{e}_{y}}), the dielectric tensor is expressed as:

𝜺(ω,𝑩)=(εxx(ω,𝑩)0εxz(ω,𝑩)0εyy(ω,𝑩)0εxz(ω,𝑩)0εzz(ω,𝑩)).\bm{\varepsilon}(\omega,\bm{B})=\begin{pmatrix}\varepsilon_{xx}(\omega,\bm{B})&0&\varepsilon_{xz}(\omega,\bm{B})\\ 0&\varepsilon_{yy}(\omega,\bm{B})&0\\ -\varepsilon_{xz}(\omega,\bm{B})&0&\varepsilon_{zz}(\omega,\bm{B})\\ \end{pmatrix}. (24)

The Fresnel equation for the propagation of electromagnetic wave is given by:

[n2𝑰𝜺𝒏:𝒏]𝑬=0.[n^{2}\bm{I}-\bm{\varepsilon}-\bm{n}:\bm{n}]\cdot\bm{E}=0. (25)

For normal incidence, the complex refractory index n is:

𝒏=c𝒌ω=ckω𝒆^𝒛.\bm{n}=\frac{c\bm{k}}{\omega}=\frac{ck}{\omega}\bm{\hat{e}_{z}}. (26)

By solving the above Fresnel equations, we get the normal modes as the \parallel and \perp for linearly polarized plane waves which are parallel and perpendicular to 𝒆^𝒚\bm{\hat{e}_{y}} (magnetization direction), with distinct refractive indices:

n2(ω,B𝒆^𝒚)=εyy(ω,B𝒆^𝒚),n^{2}_{\parallel}(\omega,B\bm{\hat{e}_{y}})=\varepsilon_{yy}(\omega,B\bm{\hat{e}_{y}}), (27)

and

n2(ω,B𝒆^𝒚)=εxx(ω,B𝒆^𝒚)+εxz2(ω,B𝒆^𝒚)εzz(ω,B𝒆^𝒚).n^{2}_{\perp}(\omega,B\bm{\hat{e}_{y}})=\varepsilon_{xx}(\omega,B\bm{\hat{e}_{y}})+\frac{\varepsilon_{xz}^{2}(\omega,B\bm{\hat{e}_{y}})}{\varepsilon_{zz}(\omega,B\bm{\hat{e}_{y}})}. (28)

To mathematically describe how an electromagnetic wave interacts with such stratified and anisotropic media, we adopt a 4x4 formalism involving the in-plane components of both electric (Ex,Ey)(E_{x},E_{y}) and magnetic fields (Bx,By)(B_{x},B_{y}). We consider a monolayer material magnetized along the +y+y direction, and the second layer is vacuum. Within each layer (ll = 0, 1, 2), we choose the four eigenmodes of light as follows:𝒆^𝟏(𝒍)=𝒆^𝟐(𝒍)=𝒆^𝒙,𝒆^𝟑(𝒍)=𝒆^𝟒(𝒍)=𝒆^𝒚\,\bm{\hat{e}^{(l)}_{1}}=\bm{\hat{e}^{(l)}_{2}}=\bm{\hat{e}_{x}},\,\bm{\hat{e}^{(l)}_{3}}=\bm{\hat{e}^{(l)}_{4}}=\bm{\hat{e}_{y}}, with the corresponding refractive indices:n1(l)=n2(l)=n(l),n3(l)=n4(l)=n(l)\,n^{(l)}_{1}=-n^{(l)}_{2}=n^{(l)}_{\perp},\,n^{(l)}_{3}=-n^{(l)}_{4}=n^{(l)}_{\parallel}. The electric and magnetic fields of light in the first and second layers are given by:

𝑬(l)=j=14E0j(l)𝒆^j(l)exp{i[kj(l)(zzl1)ωt]},\bm{E}^{(l)}=\sum_{j=1}^{4}E^{(l)}_{0j}\bm{\hat{e}}^{(l)}_{j}\exp\{i[k^{(l)}_{j}(z-z_{l-1})-\omega t]\}, (29)

and

c𝑩(l)=j=14E0j(l)𝒃j(l)exp{i[kj(l)(zzl1)ωt]},c\bm{B}^{(l)}=\sum_{j=1}^{4}E^{(l)}_{0j}\bm{b}^{(l)}_{j}\exp\{i[k^{(l)}_{j}(z-z_{l-1})-\omega t]\}, (30)

with 𝒃j(l)=nj(l)𝒆^z×𝒆^j(l)\bm{b}^{(l)}_{j}=n^{(l)}_{j}\bm{\hat{e}}_{z}\times\bm{\hat{e}}^{(l)}_{j}. The electric and magnetic fields of light in the zeroth layer are given by,

𝑬(0)=j=14E0j(0)𝒆^j(0)exp{i[kj(0)(zz0)ωt]},\bm{E}^{(0)}=\sum_{j=1}^{4}E^{(0)}_{0j}\bm{\hat{e}}^{(0)}_{j}\exp\{i[k^{(0)}_{j}(z-z_{0})-\omega t]\}, (31)

and

c𝑩(0)=j=14E0j(0)𝒃j(0)exp{i[kj(0)(zz0)ωt]}.c\bm{B}^{(0)}=\sum_{j=1}^{4}E^{(0)}_{0j}\bm{b}^{(0)}_{j}\exp\{i[k^{(0)}_{j}(z-z_{0})-\omega t]\}. (32)

The requirement of the continuity of the tangential field components at the interfaces connects the field amplitudes E0j(l)E^{(l)}_{0j} between two neighboring layers. The dynamical matrix within each layer is given by a block-diagonal form:

𝑫(l)\displaystyle\bm{D}^{(l)} =(𝒆^1(l)𝒆^x𝒆^2(l)𝒆^x𝒆^3(l)𝒆^x𝒆^4(l)𝒆^x𝒃^1(l)𝒆^y𝒃^2(l)𝒆^y𝒃^3(l)𝒆^y𝒃^4(l)𝒆^y𝒆^1(l)𝒆^y𝒆^2(l)𝒆^y𝒆^3(l)𝒆^y𝒆^4(l)𝒆^y𝒃^1(l)𝒆^x𝒃^2(l)𝒆^x𝒃^3(l)𝒆^x𝒃^4(l)𝒆^x)\displaystyle=\begin{pmatrix}\bm{\hat{e}}^{(l)}_{1}\cdot\bm{\hat{e}}_{x}&\bm{\hat{e}}^{(l)}_{2}\cdot\bm{\hat{e}}_{x}&\bm{\hat{e}}^{(l)}_{3}\cdot\bm{\hat{e}}_{x}&\bm{\hat{e}}^{(l)}_{4}\cdot\bm{\hat{e}}_{x}\\ \bm{\hat{b}}^{(l)}_{1}\cdot\bm{\hat{e}}_{y}&\bm{\hat{b}}^{(l)}_{2}\cdot\bm{\hat{e}}_{y}&\bm{\hat{b}}^{(l)}_{3}\cdot\bm{\hat{e}}_{y}&\bm{\hat{b}}^{(l)}_{4}\cdot\bm{\hat{e}}_{y}\\ \bm{\hat{e}}^{(l)}_{1}\cdot\bm{\hat{e}}_{y}&\bm{\hat{e}}^{(l)}_{2}\cdot\bm{\hat{e}}_{y}&\bm{\hat{e}}^{(l)}_{3}\cdot\bm{\hat{e}}_{y}&\bm{\hat{e}}^{(l)}_{4}\cdot\bm{\hat{e}}_{y}\\ \bm{\hat{b}}^{(l)}_{1}\cdot\bm{\hat{e}}_{x}&\bm{\hat{b}}^{(l)}_{2}\cdot\bm{\hat{e}}_{x}&\bm{\hat{b}}^{(l)}_{3}\cdot\bm{\hat{e}}_{x}&\bm{\hat{b}}^{(l)}_{4}\cdot\bm{\hat{e}}_{x}\\ \end{pmatrix} (33)
=(1100n(l)n(l)00001100n(l)n(l)).\displaystyle=\begin{pmatrix}1&1&0&0\\ n^{(l)}_{\perp}&-n^{(l)}_{\perp}&0&0\\ 0&0&1&1\\ 0&0&-n^{(l)}_{\parallel}&n^{(l)}_{\parallel}\\ \end{pmatrix}.

The propagation matrix is defined as a diagonal matrix:

𝑷(1)=(eiδ0000eiδ0000eiδ0000eiδ),\bm{P}^{(1)}=\begin{pmatrix}e^{i\delta_{\perp}}&0&0&0\\ 0&e^{-i\delta_{\perp}}&0&0\\ 0&0&e^{i\delta_{\parallel}}&0\\ 0&0&0&e^{-i\delta_{\parallel}}\\ \end{pmatrix}, (34)

where δ=ωcn\delta_{\perp}=\frac{\omega}{c}n_{\perp}, δ=ωcn\delta_{\parallel}=\frac{\omega}{c}n_{\parallel}, and dd is the thickness of layer 1, i.e. monolayer CrSBr.

In this two-interface setup, 𝑬0(0)\bm{E}^{(0)}_{0} and 𝑬0(2)\bm{E}^{(2)}_{0} are related by the transfer matrix 𝑴c\bm{M}_{c} in the basis of linearly polarized lights:

𝑬0(2)=𝑴c𝑬0(0)=[𝑫(2)]1𝑫(1)𝑷(1)[𝑫(1)]1𝑫(0)𝑬0(0).\bm{E}^{(2)}_{0}=\bm{M}_{c}\bm{E}^{(0)}_{0}=[\bm{D}^{(2)}]^{-1}\bm{D}^{(1)}\bm{P}^{(1)}[\bm{D}^{(1)}]^{-1}\bm{D}^{(0)}\bm{E}^{(0)}_{0}. (35)

𝑴c\bm{M}_{c} has a simple block-diagonal form:

𝑴c=(𝑴00𝑴),\bm{M}_{c}=\begin{pmatrix}\bm{M}_{\perp}&0\\ 0&\bm{M}_{\parallel}\\ \end{pmatrix}, (36)
𝑴=1t21t10(eiδ+eiδr21r10eiδr10+eiδr21eiδr21+eiδr10eiδr21r10+eiδ),\bm{M}_{\perp}=\frac{1}{t^{\perp}_{21}t^{\perp}_{10}}\begin{pmatrix}e^{i\delta_{\perp}}+e^{-i\delta_{\perp}}r^{\perp}_{21}r^{\perp}_{10}&e^{i\delta_{\perp}}r^{\perp}_{10}+e^{-i\delta_{\perp}}r^{\perp}_{21}\\ e^{i\delta_{\perp}}r^{\perp}_{21}+e^{-i\delta_{\perp}}r^{\perp}_{10}&e^{i\delta_{\perp}}r^{\perp}_{21}r^{\perp}_{10}+e^{-i\delta_{\perp}}\\ \end{pmatrix}, (37)

where rmnr_{mn} and tmnt_{mn} are the Fresnel coefficients of the interface from the mth layer to the nth layer. And 𝑴\bm{M}_{\parallel} has the same form. In the left and right layers, we adopt a basis transformation from the linearly polarized light (𝒆^x\bm{\hat{e}}_{x},𝒆^y\bm{\hat{e}}_{y}) to the light (𝒆^a\bm{\hat{e}}_{a},𝒆^b\bm{\hat{e}}_{b}) with 𝒆^a=12(𝒆^x+𝒆^y)\bm{\hat{e}}_{a}=\frac{1}{\sqrt{2}}(\bm{\hat{e}}_{x}+\bm{\hat{e}}_{y}) and 𝒆^b=12(𝒆^x+𝒆^y)\bm{\hat{e}}_{b}=\frac{1}{\sqrt{2}}(-\bm{\hat{e}}_{x}+\bm{\hat{e}}_{y}). 𝒆^1(l)=𝒆^2(l)=𝒆^a\bm{\hat{e}}^{(l)}_{1}=\bm{\hat{e}}^{(l)}_{2}=\bm{\hat{e}}_{a}, 𝒆^3(l)=𝒆^4(l)=𝒆^b\bm{\hat{e}}^{(l)}_{3}=\bm{\hat{e}}^{(l)}_{4}=\bm{\hat{e}}_{b}, and n1(l)=n2(l)=n3(l)=n4(l)=n(l)n^{(l)}_{1}=-n^{(l)}_{2}=n^{(l)}_{3}=-n^{(l)}_{4}=n^{(l)}, for ll == 0, 22. This new basis of linearly polarized plane waves is denoted as {a,a,b,b}\{a\rightarrow,a\leftarrow,b\rightarrow,b\leftarrow\}. In this basis of linearly polarized lights, the electric field amplitudes in the left and right layer are related by transfer matrix MM:

(E0a(2)E0a(2)E0b(2)E0b(2))=𝑴(E0a(0)E0a(0)E0b(0)E0b(0))\begin{pmatrix}E^{(2)}_{0a\rightarrow}\\ E^{(2)}_{0a\leftarrow}\\ E^{(2)}_{0b\rightarrow}\\ E^{(2)}_{0b\leftarrow}\\ \end{pmatrix}=\bm{M}\begin{pmatrix}E^{(0)}_{0a\rightarrow}\\ E^{(0)}_{0a\leftarrow}\\ E^{(0)}_{0b\rightarrow}\\ E^{(0)}_{0b\leftarrow}\\ \end{pmatrix} (38)
𝑴=12(𝑴+𝑴𝑴+𝑴𝑴+𝑴𝑴+𝑴).\bm{M}=\frac{1}{2}\begin{pmatrix}\bm{M}_{\perp}+\bm{M}_{\parallel}&-\bm{M}_{\perp}+\bm{M}_{\parallel}\\ -\bm{M}_{\perp}+\bm{M}_{\parallel}&\bm{M}_{\perp}+\bm{M}_{\parallel}\\ \end{pmatrix}. (39)

Because the angle of electric field of incident light and the direction of magnetization (+y+y) is 4545^{\circ}, E0b(2)=0E^{(2)}_{0b\leftarrow}=0. In addition, there are no reflecting lights from the zeroth medium (semi-infinite substrate) to CrSBr, which means E0a(0)=E0b(0)=0E^{(0)}_{0a\rightarrow}=E^{(0)}_{0b\rightarrow}=0. With these two conditions, by calculating Eq. D15, we can get:

tssE0a(0)E0a(2)=𝑴44𝑴22𝑴44𝑴24𝑴42t_{ss}\equiv\frac{E^{(0)}_{0a\leftarrow}}{E^{(2)}_{0a\leftarrow}}=\frac{\bm{M}_{44}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (40)
tspE0b(0)E0a(2)=𝑴42𝑴22𝑴44𝑴24𝑴42t_{sp}\equiv\frac{E^{(0)}_{0b\leftarrow}}{E^{(2)}_{0a\leftarrow}}=\frac{-\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (41)
rssE0a(0)E0a(2)=𝑴12𝑴44𝑴14𝑴42𝑴22𝑴44𝑴24𝑴42r_{ss}\equiv\frac{E^{(0)}_{0a\rightarrow}}{E^{(2)}_{0a\leftarrow}}=\frac{\bm{M}_{12}\bm{M}_{44}-\bm{M}_{14}\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (42)
rspE0b(0)E0a(2)=𝑴32𝑴44𝑴34𝑴42𝑴22𝑴44𝑴24𝑴42r_{sp}\equiv\frac{E^{(0)}_{0b\rightarrow}}{E^{(2)}_{0a\leftarrow}}=\frac{\bm{M}_{32}\bm{M}_{44}-\bm{M}_{34}\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (43)

The SH signals for the reflected (right-moving) electric field E(2)=E0a(2)𝒆^a+E0b(2)𝒆^bE^{(2)}_{\rightarrow}=E^{(2)}_{0a\rightarrow}\bm{\hat{e}}_{a}+E^{(2)}_{0b\rightarrow}\bm{\hat{e}}_{b} are expressed as:

tan2θSH=2|rsprss|cos(argrsprss)1|rsprss|2,\tan 2\theta_{\rm{SH}}=\frac{2|\frac{r_{sp}}{r_{ss}}|\cos(\arg\frac{r_{sp}}{r_{ss}})}{1-|\frac{r_{sp}}{r_{ss}}|^{2}}, (44)
sin2ηSH=2|rsprss|sin(argrsprss)1+|rsprss|2,\sin 2\eta_{\rm{SH}}=\frac{2|\frac{r_{sp}}{r_{ss}}|\sin(\arg\frac{r_{sp}}{r_{ss}})}{1+|\frac{r_{sp}}{r_{ss}}|^{2}}, (45)

Similarly, the Voigt signals for the transmitted (left-moving) electric field E(0)=E0a(0)𝒆^a+E0b(0)𝒆^bE^{(0)}_{\leftarrow}=E^{(0)}_{0a\leftarrow}\bm{\hat{e}}_{a}+E^{(0)}_{0b\leftarrow}\bm{\hat{e}}_{b} are expressed as:

tan2θV=2|tsptss|cos(argtsptss)1|tsptss|2,\tan 2\theta_{\rm{V}}=\frac{2|\frac{t_{sp}}{t_{ss}}|\cos(\arg\frac{t_{sp}}{t_{ss}})}{1-|\frac{t_{sp}}{t_{ss}}|^{2}}, (46)
sin2ηV=2|tsptss|sin(argtsptss)1+|tsptss|2.\sin 2\eta_{\rm{V}}=\frac{2|\frac{t_{sp}}{t_{ss}}|\sin(\arg\frac{t_{sp}}{t_{ss}})}{1+|\frac{t_{sp}}{t_{ss}}|^{2}}. (47)

In this work, we rescale the calculated dielectric function in a slab model by the thickness of a monolayer material:

εαα=1+ld(ε~αα1),\varepsilon_{\alpha\alpha}=1+\frac{l}{d}(\tilde{\varepsilon}_{\alpha\alpha}-1), (48)

and

εαβ=ldε~αβ,\varepsilon_{\alpha\beta}=\frac{l}{d}\tilde{\varepsilon}_{\alpha\beta}, (49)

where ll and dd are thicknesses of the slab model along the out-of-plane direction and monolayer material, and ε~αα\tilde{\varepsilon}_{\alpha\alpha} and ε~αβ\tilde{\varepsilon}_{\alpha\beta} are calculated dielectric functions in the BerkeleyGW package.

ε~αα\tilde{\varepsilon}_{\alpha\alpha} and ε~αβ\tilde{\varepsilon}_{\alpha\beta} can be expressed as follows:

Im[εαα(ω)]=π2ε0NkVS1ΩS2|0|j^pα|S|2[δ(ωΩS)],{\rm Im}[\varepsilon_{\alpha\alpha}(\omega)]=\frac{\pi\hbar^{2}}{\varepsilon_{0}N_{k}V}\sum_{S}\frac{1}{\Omega^{2}_{S}}|\langle 0|\hat{j}^{\alpha}_{p}|S\rangle|^{2}\left[\delta(\hbar\omega-\Omega_{S})\right], (50)
Re[εαα(ω)]=2ε0NkVS1ΩS2|0|j^pα|S|2[1ωΩS],{\rm Re}[\varepsilon_{\alpha\alpha}(\omega)]=-\frac{\hbar^{2}}{\varepsilon_{0}N_{k}V}\sum_{S}\frac{1}{\Omega^{2}_{S}}|\langle 0|\hat{j}^{\alpha}_{p}|S\rangle|^{2}\left[\frac{1}{\hbar\omega-\Omega_{S}}\right], (51)

and

Im[εαβ(ω)]=i2ε0NkVS1ΩS2[0|j^pα|SS|j^pβ|0ωΩS],{\rm Im}[\varepsilon_{\alpha\beta}(\omega)]=\frac{i\hbar^{2}}{\varepsilon_{0}N_{k}V}\sum_{S}\frac{1}{\Omega^{2}_{S}}\left[\frac{\langle 0|\hat{j}^{\alpha}_{p}|S\rangle\langle S|\hat{j}^{\beta}_{p}|0\rangle}{\hbar\omega-\Omega_{S}}\right], (52)
Re[εαβ(ω)]=iπ2ε0NkV\displaystyle{\rm Re}[\varepsilon_{\alpha\beta}(\omega)]=\frac{i\pi\hbar^{2}}{\varepsilon_{0}N_{k}V} S1ΩS2[0|j^pα|SS|j^pβ|0δ(ωΩS)],\displaystyle\sum_{S}\frac{1}{\Omega^{2}_{S}}[\langle 0|\hat{j}^{\alpha}_{p}|S\rangle\langle S|\hat{j}^{\beta}_{p}|0\rangle\delta(\hbar\omega-\Omega_{S})], (53)

where NkN_{k} is the number of k-points, VV is the volume of a unit cell, 𝒋^𝒑=e𝒗^\bm{\hat{j}_{p}}=-e\bm{\hat{v}}, and 0|j^pα|S=cv𝒌Acv𝒌Sv𝒌|j^pα|c𝒌\langle 0|\hat{j}^{\alpha}_{p}|S\rangle=\sum_{cv\bm{k}}A^{S}_{cv\bm{k}}\langle v\bm{k}|\hat{j}^{\alpha}_{p}|c\bm{k}\rangle.

Appendix E CALCULATIONS OF SH AND VOIGT EFFECTS IN CRSBR

In Fig. 15, we have shown the calculated results without the consideration of electron-hole interaction, i.e., under independent particle approximation. In Fig. 16, we have compared the results with and without the inclusion of off-diagonal components of dielectric function from BSE.

Refer to caption
Figure 15: Rotation angles of (a) reflected and (b) transmitted light in CrSBr monolayer without the inclusion of electron-hole interactions. Insets are the corresponding ellipticities.
Refer to caption
Figure 16: Comparison of rotation angles for both (a) reflected and (b) transmitted lights in CrSBr monolayer between the situations with and without the inclusion of off-diagonal component εxz\varepsilon_{xz}.

Appendix F ABSORBANCE AND EXCITON SPECTRUM WITH SPIN ORIENTATION ALONG X AND Z AXIS

In Fig. 17 and Fig. 18, we have shown the anisotropic optical absorbance and exciton spectrum in CrSBr monolayer for states with spin orientation along xx axis and zz axis, respectively. Optical absorbance and exciton spectrum for the state with spin orientation along xx axis are similar with those for the state with spin orientation along zz axis.

Refer to caption
Figure 17: Anisotropic optical absorbance in CrSBr monolayer with spin orientation along xx axis for the electric polarization along x (a) and y (b) directions, respectively. (c) Exciton spectrum.
Refer to caption
Figure 18: Anisotropic optical absorbance in CrSBr monolayer with spin orientation along zz for the electric polarization along x (a) and y (b) directions, respectively. (c) Exciton spectrum.

Appendix G COMPARISON OF ROTATION ANGLES OF SH AND VOIGT EFFECTS FOR THE STATES WITH SPIN ORIENTATION ALONG X AND Y AXIS

In Fig. 19, we have compared rotation angles for states with spin orientation along xx and yy axis. It is obvious that rotation angles for the state with spin orientation along xx axis are nearly unchanged compared with those for the state with spin orientation along yy axis.

Refer to caption
Figure 19: Rotation angles of (a) reflected and (b) transmitted light in CrSBr monolayer for states with spin orientation along xx (blue) and yy (red) axis considering electron-hole interactions.

Appendix H CALCULATIONS OF KERR AND FARADAY EFFECTS IN CRSBR WITH OUT-OF-PLANE MAGNETIZATION

Refer to caption
Figure 20: Illustration of crystal structure of 2D magnet CrSBr monolayer with out-of-plane magnetization.

In 2D magnets, the in-plane spin orientation could be tuned to out-of-plane direction by external perpendicular magnetic field. As shown in Fig. 20, here we consider the out-of-plane magnetization along z axis (𝑩=B𝒆^𝒛\bm{B}=B\bm{\hat{e}_{z}}). For an isotropic system the dielectric tensor is expressed as:

𝜺(ω,𝑩)=(εxx(ω,𝑩)εxy(ω,𝑩)0εxy(ω,𝑩)εxx(ω,𝑩)000εzz(ω,𝑩)).\bm{\varepsilon}(\omega,\bm{B})=\begin{pmatrix}\varepsilon_{xx}(\omega,\bm{B})&\varepsilon_{xy}(\omega,\bm{B})&0\\ -\varepsilon_{xy}(\omega,\bm{B})&\varepsilon_{xx}(\omega,\bm{B})&0\\ 0&0&\varepsilon_{zz}(\omega,\bm{B})\\ \end{pmatrix}. (54)

The Fresnel equation for the propagation of electromagnetic wave is given by:

[n2𝑰𝜺𝒏:𝒏]𝑬=0.[n^{2}\bm{I}-\bm{\varepsilon}-\bm{n}:\bm{n}]\cdot\bm{E}=0. (55)

For normal incidence, the complex refractory index n is:

𝒏=c𝒌ω=ckω𝒆^𝒛.\bm{n}=\frac{c\bm{k}}{\omega}=\frac{ck}{\omega}\bm{\hat{e}_{z}}. (56)

By solving the above Fresnel equations, we get the normal modes as the σ+\sigma^{+} and σ\sigma^{-} for circularly polarized plane waves, with distinct refractive indices:

n±2(ω,B𝒆^𝒛)=εxx(ω,B𝒆^𝒛)±iεxy(ω,B𝒆^𝒛),n^{2}_{\pm}(\omega,B\bm{\hat{e}_{z}})=\varepsilon_{xx}(\omega,B\bm{\hat{e}_{z}})\pm i\varepsilon_{xy}(\omega,B\bm{\hat{e}_{z}}), (57)

For an anisotropic system, the distinct refractive indices are:

n±2(ω,B𝒆^𝒛)=ε0(ω,B𝒆^𝒛)±iεxy(ω,B𝒆^𝒛),n^{2}_{\pm}(\omega,B\bm{\hat{e}_{z}})=\varepsilon_{0}(\omega,B\bm{\hat{e}_{z}})\pm i\varepsilon_{xy}(\omega,B\bm{\hat{e}_{z}}), (58)
ε0(ω,B𝒆^𝒛)=εxx(ω,B𝒆^𝒛)+εyy(ω,B𝒆^𝒛)2.\varepsilon_{0}(\omega,B\bm{\hat{e}_{z}})=\frac{\varepsilon_{xx}(\omega,B\bm{\hat{e}_{z}})+\varepsilon_{yy}(\omega,B\bm{\hat{e}_{z}})}{2}. (59)

To mathematically describe how an electromagnetic wave interacts with such stratified and anisotropic media, we adopt a 4x4 formalism involving the in-plane components of both electric (Ex,Ey)(E_{x},E_{y}) and magnetic fields (Bx,By)(B_{x},B_{y}). We consider a monolayer material magnetized along the +z+z direction, and the second layer is vacuum. Within each layer (ll = 0, 1, 2), we choose the four eigenmodes of light as follows:𝒆^𝟏(𝒍)=𝒆^𝟐(𝒍)=𝒆^+,𝒆^𝟑(𝒍)=𝒆^𝟒(𝒍)=𝒆^\,\bm{\hat{e}^{(l)}_{1}}=\bm{\hat{e}^{(l)}_{2}}=\bm{\hat{e}_{+}},\,\bm{\hat{e}^{(l)}_{3}}=\bm{\hat{e}^{(l)}_{4}}=\bm{\hat{e}_{-}}, with the corresponding refractive indices:n1(l)=n2(l)=n+(l),n3(l)=n4(l)=n(l)\,n^{(l)}_{1}=-n^{(l)}_{2}=n^{(l)}_{+},\,n^{(l)}_{3}=-n^{(l)}_{4}=n^{(l)}_{-}. The electric and magnetic fields of light in the first and second layers are given by:

𝑬(l)=j=14E0j(l)𝒆^j(l)exp{i[kj(l)(zzl1)ωt]},\bm{E}^{(l)}=\sum_{j=1}^{4}E^{(l)}_{0j}\bm{\hat{e}}^{(l)}_{j}\exp\{i[k^{(l)}_{j}(z-z_{l-1})-\omega t]\}, (60)

and

c𝑩(l)=j=14E0j(l)𝒃j(l)exp{i[kj(l)(zzl1)ωt]},c\bm{B}^{(l)}=\sum_{j=1}^{4}E^{(l)}_{0j}\bm{b}^{(l)}_{j}\exp\{i[k^{(l)}_{j}(z-z_{l-1})-\omega t]\}, (61)

with 𝒃j(l)=nj(l)𝒆^z×𝒆^j(l)\bm{b}^{(l)}_{j}=n^{(l)}_{j}\bm{\hat{e}}_{z}\times\bm{\hat{e}}^{(l)}_{j}. The electric and magnetic fields of light in the zeroth layer are given by,

𝑬(0)=j=14E0j(0)𝒆^j(0)exp{i[kj(0)(zz0)ωt]},\bm{E}^{(0)}=\sum_{j=1}^{4}E^{(0)}_{0j}\bm{\hat{e}}^{(0)}_{j}\exp\{i[k^{(0)}_{j}(z-z_{0})-\omega t]\}, (62)

and

c𝑩(0)=j=14E0j(0)𝒃j(0)exp{i[kj(0)(zz0)ωt]}.c\bm{B}^{(0)}=\sum_{j=1}^{4}E^{(0)}_{0j}\bm{b}^{(0)}_{j}\exp\{i[k^{(0)}_{j}(z-z_{0})-\omega t]\}. (63)

The requirement of the continuity of the tangential field components at the interfaces connects the field amplitudes E0j(l)E^{(l)}_{0j} between two neighboring layers. The dynamical matrix within each layer is given by a block-diagonal form:

𝑫(l)\displaystyle\bm{D}^{(l)} =(𝒆^1(l)𝒆^+𝒆^2(l)𝒆^+𝒆^3(l)𝒆^+𝒆^4(l)𝒆^+𝒃^1(l)𝒆^+𝒃^2(l)𝒆^+𝒃^3(l)𝒆^+𝒃^4(l)𝒆^+𝒆^1(l)𝒆^𝒆^2(l)𝒆^𝒆^3(l)𝒆^𝒆^4(l)𝒆^𝒃^1(l)𝒆^𝒃^2(l)𝒆^𝒃^3(l)𝒆^𝒃^4(l)𝒆^)\displaystyle=\begin{pmatrix}\bm{\hat{e}}^{(l)}_{1}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{e}}^{(l)}_{2}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{e}}^{(l)}_{3}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{e}}^{(l)}_{4}\cdot\bm{\hat{e}}_{+}^{*}\\ \bm{\hat{b}}^{(l)}_{1}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{b}}^{(l)}_{2}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{b}}^{(l)}_{3}\cdot\bm{\hat{e}}_{+}^{*}&\bm{\hat{b}}^{(l)}_{4}\cdot\bm{\hat{e}}_{+}^{*}\\ \bm{\hat{e}}^{(l)}_{1}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{e}}^{(l)}_{2}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{e}}^{(l)}_{3}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{e}}^{(l)}_{4}\cdot\bm{\hat{e}}_{-}^{*}\\ \bm{\hat{b}}^{(l)}_{1}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{b}}^{(l)}_{2}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{b}}^{(l)}_{3}\cdot\bm{\hat{e}}_{-}^{*}&\bm{\hat{b}}^{(l)}_{4}\cdot\bm{\hat{e}}_{-}^{*}\\ \end{pmatrix} (64)
=(1100in+(l)in+(l)00001100in(l)in(l)).\displaystyle=\begin{pmatrix}1&1&0&0\\ -in^{(l)}_{+}&in^{(l)}_{+}&0&0\\ 0&0&1&1\\ 0&0&in^{(l)}_{-}&-in^{(l)}_{-}\\ \end{pmatrix}.

The propagation matrix is defined as a diagonal matrix:

𝑷(1)=(eiδ+0000eiδ+0000eiδ0000eiδ),\bm{P}^{(1)}=\begin{pmatrix}e^{i\delta_{+}}&0&0&0\\ 0&e^{-i\delta_{+}}&0&0\\ 0&0&e^{i\delta_{-}}&0\\ 0&0&0&e^{-i\delta_{-}}\\ \end{pmatrix}, (65)

where δ+=ωcn+\delta_{+}=\frac{\omega}{c}n_{+}, δ=ωcn\delta_{-}=\frac{\omega}{c}n_{-}, and dd is the thickness of layer 1, i.e. monolayer CrSBr.

In this two-interface setup, 𝑬0(0)\bm{E}^{(0)}_{0} and 𝑬0(2)\bm{E}^{(2)}_{0} are related by the transfer matrix 𝑴c\bm{M}_{c} in the basis of linearly polarized lights:

𝑬0(2)=𝑴c𝑬0(0)=[𝑫(2)]1𝑫(1)𝑷(1)[𝑫(1)]1𝑫(0)𝑬0(0).\bm{E}^{(2)}_{0}=\bm{M}_{c}\bm{E}^{(0)}_{0}=[\bm{D}^{(2)}]^{-1}\bm{D}^{(1)}\bm{P}^{(1)}[\bm{D}^{(1)}]^{-1}\bm{D}^{(0)}\bm{E}^{(0)}_{0}. (66)

𝑴c\bm{M}_{c} has a simple block-diagonal form:

𝑴c=(𝑴+00𝑴),\bm{M}_{c}=\begin{pmatrix}\bm{M}_{+}&0\\ 0&\bm{M}_{-}\\ \end{pmatrix}, (67)
𝑴+=1t21+t10+(eiδ++eiδ+r21+r10+eiδ+r10++eiδ+r21+eiδ+r21++eiδ+r10+eiδ+r21+r10++eiδ+),\bm{M}_{+}=\frac{1}{t^{+}_{21}t^{+}_{10}}\begin{pmatrix}e^{i\delta_{+}}+e^{-i\delta_{+}}r^{+}_{21}r^{+}_{10}&e^{i\delta_{+}}r^{+}_{10}+e^{-i\delta_{+}}r^{+}_{21}\\ e^{i\delta_{+}}r^{+}_{21}+e^{-i\delta_{+}}r^{+}_{10}&e^{i\delta_{+}}r^{+}_{21}r^{+}_{10}+e^{-i\delta_{+}}\\ \end{pmatrix}, (68)

where rmnr_{mn} and tmnt_{mn} are the Fresnel coefficients of the interface from the mth layer to the nth layer. And 𝑴\bm{M}_{-} has the same form. In the left and right layers, we adopt a basis transformation from the circularly polarized light (𝒆^+\bm{\hat{e}}_{+},𝒆^\bm{\hat{e}}_{-}) with 𝒆^+=12(𝒆^x+i𝒆^y)\bm{\hat{e}}_{+}=-\frac{1}{\sqrt{2}}(\bm{\hat{e}}_{x}+i\bm{\hat{e}}_{y}) and 𝒆^=12(𝒆^xi𝒆^y)\bm{\hat{e}}_{-}=\frac{1}{\sqrt{2}}(\bm{\hat{e}}_{x}-i\bm{\hat{e}}_{y}) to the light (𝒆^x\bm{\hat{e}}_{x},𝒆^y\bm{\hat{e}}_{y}). 𝒆^1(l)=𝒆^2(l)=𝒆^x\bm{\hat{e}}^{(l)}_{1}=\bm{\hat{e}}^{(l)}_{2}=\bm{\hat{e}}_{x}, 𝒆^3(l)=𝒆^4(l)=𝒆^y\bm{\hat{e}}^{(l)}_{3}=\bm{\hat{e}}^{(l)}_{4}=\bm{\hat{e}}_{y}, and n1(l)=n2(l)=n3(l)=n4(l)=n(l)n^{(l)}_{1}=-n^{(l)}_{2}=n^{(l)}_{3}=-n^{(l)}_{4}=n^{(l)}, for ll == 0, 22. This new basis of linearly polarized plane waves is denoted as {x,x,y,y}\{x\rightarrow,x\leftarrow,y\rightarrow,y\leftarrow\}. In this basis of linearly polarized lights, the electric field amplitudes in the left and right layer are related by transfer matrix MM:

(E0x(2)E0x(2)E0y(2)E0y(2))=𝑴(E0x(0)E0x(0)E0y(0)E0y(0))\begin{pmatrix}E^{(2)}_{0x\rightarrow}\\ E^{(2)}_{0x\leftarrow}\\ E^{(2)}_{0y\rightarrow}\\ E^{(2)}_{0y\leftarrow}\\ \end{pmatrix}=\bm{M}\begin{pmatrix}E^{(0)}_{0x\rightarrow}\\ E^{(0)}_{0x\leftarrow}\\ E^{(0)}_{0y\rightarrow}\\ E^{(0)}_{0y\leftarrow}\\ \end{pmatrix} (69)
𝑴=12(𝑴++𝑴i(𝑴+𝑴)i(𝑴+𝑴)𝑴++𝑴).\bm{M}=\frac{1}{2}\begin{pmatrix}\bm{M}_{+}+\bm{M}_{-}&-i(\bm{M}_{+}-\bm{M}_{-})\\ i(\bm{M}_{+}-\bm{M}_{-})&\bm{M}_{+}+\bm{M}_{-}\\ \end{pmatrix}. (70)

Because the electric field of incident light is along the direction of magnetization (+z+z), E0y(2)=0E^{(2)}_{0y\leftarrow}=0. In addition, there are no reflecting lights from the zeroth medium (semi-infinite substrate) to CrSBr, which means E0x(0)=E0y(0)=0E^{(0)}_{0x\rightarrow}=E^{(0)}_{0y\rightarrow}=0. With these two conditions, by calculating Eq. G16, we can get:

tssE0x(0)E0x(2)=𝑴44𝑴22𝑴44𝑴24𝑴42t_{ss}\equiv\frac{E^{(0)}_{0x\leftarrow}}{E^{(2)}_{0x\leftarrow}}=\frac{\bm{M}_{44}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (71)
tspE0y(0)E0x(2)=𝑴42𝑴22𝑴44𝑴24𝑴42t_{sp}\equiv\frac{E^{(0)}_{0y\leftarrow}}{E^{(2)}_{0x\leftarrow}}=\frac{-\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (72)
rssE0x(0)E0x(2)=𝑴12𝑴44𝑴14𝑴42𝑴22𝑴44𝑴24𝑴42r_{ss}\equiv\frac{E^{(0)}_{0x\rightarrow}}{E^{(2)}_{0x\leftarrow}}=\frac{\bm{M}_{12}\bm{M}_{44}-\bm{M}_{14}\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (73)
rspE0y(0)E0x(2)=𝑴32𝑴44𝑴34𝑴42𝑴22𝑴44𝑴24𝑴42r_{sp}\equiv\frac{E^{(0)}_{0y\rightarrow}}{E^{(2)}_{0x\leftarrow}}=\frac{\bm{M}_{32}\bm{M}_{44}-\bm{M}_{34}\bm{M}_{42}}{\bm{M}_{22}\bm{M}_{44}-\bm{M}_{24}\bm{M}_{42}} (74)

The Kerr signals for the reflected (right-moving) electric field E(2)=E0x(2)𝒆^x+E0y(2)𝒆^yE^{(2)}_{\rightarrow}=E^{(2)}_{0x\rightarrow}\bm{\hat{e}}_{x}+E^{(2)}_{0y\rightarrow}\bm{\hat{e}}_{y} are expressed as:

tan2θK=2|rsprss|cos(argrsprss)1|rsprss|2,\tan 2\theta_{\rm{K}}=\frac{2|\frac{r_{sp}}{r_{ss}}|\cos(\arg\frac{r_{sp}}{r_{ss}})}{1-|\frac{r_{sp}}{r_{ss}}|^{2}}, (75)
sin2ηK=2|rsprss|sin(argrsprss)1+|rsprss|2,\sin 2\eta_{\rm{K}}=\frac{2|\frac{r_{sp}}{r_{ss}}|\sin(\arg\frac{r_{sp}}{r_{ss}})}{1+|\frac{r_{sp}}{r_{ss}}|^{2}}, (76)

Similarly, the Faraday signals for the transmitted (left-moving) electric field E(0)=E0x(0)𝒆^x+E0y(0)𝒆^yE^{(0)}_{\leftarrow}=E^{(0)}_{0x\leftarrow}\bm{\hat{e}}_{x}+E^{(0)}_{0y\leftarrow}\bm{\hat{e}}_{y} are expressed as:

tan2θF=2|tsptss|cos(argtsptss)1|tsptss|2,\tan 2\theta_{\rm{F}}=\frac{2|\frac{t_{sp}}{t_{ss}}|\cos(\arg\frac{t_{sp}}{t_{ss}})}{1-|\frac{t_{sp}}{t_{ss}}|^{2}}, (77)
sin2ηF=2|tsptss|sin(argtsptss)1+|tsptss|2.\sin 2\eta_{\rm{F}}=\frac{2|\frac{t_{sp}}{t_{ss}}|\sin(\arg\frac{t_{sp}}{t_{ss}})}{1+|\frac{t_{sp}}{t_{ss}}|^{2}}. (78)

Based on the above derivation, in Fig. 21, we have shown rotation angles and ellipticities of Kerr and Faraday effects considering electron-hole interaction. The maximal rotation angles of Kerr and Faraday effects are 1.1 and 0.6, respectively, which are larger than 0.9 and 0.3 in CrI3 [9] and 0.3 and 0.2 in CrBr3 [10]. Compared with Fig. 22, both the amplitude and the position of the spectrum are modified significantly for excitonic effect. This verifies the fact that it is excitonic effect that enhances the Kerr and Faraday effects in CrSBr monolayer.

Refer to caption
Figure 21: Magneto-optical Kerr and Faraday effects: Rotation angles of (a) reflected and (b) transmitted light in CrSBr monolayer for the state with spin orientation along zz axis considering electron-hole interactions. Insets are the corresponding ellipticities.
Refer to caption
Figure 22: Magneto-optical Kerr and Faraday effects: Rotation angles of (a) reflected and (b) transmitted light in CrSBr monolayer for the state with spin orientation along zz axis without the inclusion of electron-hole interactions. Insets are the corresponding ellipticities.

Appendix I G0W0G_{0}W_{0}-BSE CALCULATIONS OF OPTICAL PROPERTIES IN BLACK PHOSPHORENE

In Fig. 23, we have shown the anisotropic optical absorption spectrum and exciton states (within G0W0G_{0}W_{0}-BSE framework) for black phosphorene. We use the norm-conserving PBE pseudopotentials with a plane-wave cutoff of 80 Ry. For the G0W0G_{0}W_{0} part, we use a coarse k grid of 18×12×118\times 12\times 1, 500 empty bands (5 valence bands), and the dielectric cutoff of 10 Ry. For the BSE part, a fine k grid of 72×48×172\times 48\times 1 is used. A Gaussian smearing with a broadening constant of 30 meV is used in optical absorption spectrum. The number of bands for optical transitions is 4 for both valence and conduction bands, which is sufficient to cover the span of the visible light. The lattice constants are 3.303 Å for a and 4.625 Å for b. In Fig. 24, we show the linear dichroism for both reflected and transmitted light with rotation angle and ellipticity.

Refer to caption
Figure 23: Anisotropic optical absorbance in black phosphorene monolayer for the electric polarization along x (a) and y (b) directions, respectively. (c) Exciton spectrum. Both optical spectra with and without the consideration of electron-hole interaction are presented. Inset of (a) is the crystal structure of black phosphorene and the gray lines are for dark excitons.
Refer to caption
Figure 24: Rotation angles (a) and ellipticities (b) in black phosphorene.

References

  • [1] F. Xia, H. Wang, D. Xiao, M. Dubey, and A. Ramasubramaniam, Two-dimensional material nanophotonics, Nat. Photonics 8, 899 (2014).
  • [2] K. F. Mak and J. Shan, Photonics and optoelectronics of 2D semiconductor transition metal dichalcogenides, Nat. Photonics 10, 216 (2016).
  • [3] Z. Sun, A. Martinez, and F. Wang, Optical modulators with 2D layered materials, Nat. Photonics 10, 227 (2016).
  • [4] N. P. Wilson, W. Yao, J. Shan, and X. Xu, Excitons and emergent quantum phenomena in stacked 2D semiconductors, Nature 599, 383 (2021).
  • [5] C. Gong, L. Li, Z. Li, H. Ji, A. Stern, Y. Xia, T. Cao, W. Bao, C. Wang, Y. Wang, Z. Q. Qiu, R. J. Cava, S. G. Louie, J. Xia, and X. Zhang, Discovery of intrinsic ferromagnetism in two-dimensional van der Waals crystals, Nature (London) 546, 265 (2017).
  • [6] B. Huang, G. Clark, E. Navarro-Moratalla, D. R. Klein, R. Cheng, K. L. Seyler, D. Zhong, E. Schmidgall, M. A. McGuire, D. H. Cobden, W. Yao, D. Xiao, P. Jarillo-Herrero, and X. Xu, Layer-dependent ferromagnetism in a van der Waals crystal down to the monolayer limit, Nature (London) 546, 270 (2017).
  • [7] Y. Fang, S. Wu, Z. Z. Zhu, and G. Y. Guo, Large magneto-optical effects and magnetic anisotropy energy in two-dimensional Cr2Ge2Te6, Phys. Rev. B 98, 125416 (2018).
  • [8] V. K. Gudelli and G. Y. Guo, Magnetism and magneto-optical effects in bulk and few-layer CrI3: a theoretical GGA+U study, New J. Phys. 21, 053012 (2019).
  • [9] M. Wu, Z. Li, T. Cao, and S. G. Louie, Physical origin of giant excitonic and magneto-optical responses in two-dimensional ferromagnetic insulators, Nat. Comm. 10, 2371 (2019).
  • [10] M. Wu, Z. Li, and S. G. Louie, Optical and magneto-optical properties of ferromagnetic monolayer CrBr3: A first-principles GW and GW plus Bethe-Salpeter equation study, Phys. Rev. Mater. 6, 014008 (2022).
  • [11] N. Mounet, N. Mounet, M. Gibertini, P. Schwaller, D. Campi, A. Merkys, A. Marrazzo, T. Sohier, I. E. Castelli, A. Cepellotti, G. Pizzi, and N. Marzari, Two-dimensional materials from high-throughput computational exfoliation of experimentally known compounds, Nat. Nanotechnol. 13, 246 (2018).
  • [12] N. P. Wilson, K. Lee, J. Cenker, K. Xie, A. H. Dismukes, E. J. Telford, J. Fonseca, S. Sivakumar, C. Dean, T. Cao, X. Roy, X. Xu, and X. Zhu, Interlayer electronic coupling on demand in a 2D magnetic semiconductor, Nat. Mater. 20, 1657 (2021).
  • [13] Y. J. Bae, J. Wang, A. Scheie, J. Xu, D. G. Chica, G. M. Diederich, J. Cenker, M. E. Ziebel, Y. Bai, H. Ren, C. R. Dean, M. Delor, X. Xu, X. Roy, A. D. Kent, and X. Zhu, Exciton-coupled coherent magnons in a 2D semiconductor, Nature 609, 282 (2022).
  • [14] N. Tesařová, T. Ostatnický, V. Novák, K. Olejník, J. Šubrt, H. Reichlová, C. T. Ellis, A. Mukherjee, J. Lee, G. M. Sipahi, J. Sinova, J. Hamrle, T. Jungwirth, P. Němec, J. Černe, and K. Výborný, Systematic study of magnetic linear dichroism and birefringence in (Ga,Mn)As, Phys. Rev. B 89, 085203 (2014).
  • [15] X. Yang, P. Yang, X. Zhou, W. Feng, and Y. Yao, First- and second-order magneto-optical effects and intrinsically anomalous transport in the two-dimensional van der Waals layered magnets CrXY (X=S, Se, Te; Y=Cl, Br, I), Phys. Rev. B 106, 054408 (2022).
  • [16] M. L. Cohen and S. G. Louie, Fundamentals of Condensed Matter Physics (Cambridge U.P., Cambridge, 2016).
  • [17] L. V. Keldysh, Coulomb interaction in thin semiconductor and semimetal films, JETP Lett. 29, 658 (1979).
  • [18] P. Cudazzo, I. V. Tokatly, and A. Rubio, Dielectric screening in two-dimensional insulators: Implications for excitonic and impurity states in graphane, Phys. Rev. B 84, 085406 (2011).
  • [19] T. C. Berkelbach, M. S. Hybertsen, and D. R. Reichman, Theory of neutral and charged excitons in monolayer transition metal dichalcogenides, Phys. Rev. B 88, 045318 (2013).
  • [20] A. S. Rodin, A. Carvalho, and A. H. Castro Neto, Excitons in anisotropic two-dimensional semiconducting crystals, Phys. Rev. B 90, 075429 (2014).
  • [21] T. Olsen, S. Latini, F. Rasmussen, and K. S. Thygesen, Simple Screened Hydrogen Model of Excitons in Two-Dimensional Materials, Phys. Rev. Lett. 116, 056401 (2016).
  • [22] G. Onida, L. Reining, and A. Rubio, Electronic excitations: density-functional versus many-body Green’s function approaches, Rev. Mod. Phys. 74, 601 (2002).
  • [23] P. Giannozzi, S. Baroni, N. Bonini, M. Calandra, R. Car, C. Cavazzoni, D. Ceresoli, G. L. Chiarotti, M. Cococcioni, I. Dabo, A. D. Corso, S. de Gironcoli, S. Fabris, G. Fratesi, R. Gebauer, U. Gerstmann, C. Gougoussis, A. Kokalj, M. Lazzeri, L. Martin-Samos, N. Marzari, F. Mauri, R. Mazzarello, S. Paolini, A. Pasquarello, L. Paulatto, C. Sbraccia, S. Scandolo, G. Sclauzero, A. P. Seitsonen, A. Smogunov, P. Umari, and R. M. Wentzcovitch, QUANTUM ESPRESSO: a modular and open-source software project for quantum simulations of materials, J. Phys.: Condens. Matter 21, 395502 (2009).
  • [24] J. P. Perdew, K. Burke, and M. Ernzerhof, Generalized Gradient Approximation Made Simple, Phys. Rev. Lett. 77, 3865 (1996).
  • [25] D. R. Hamann, Optimized norm-conserving Vanderbilt pseudopotentials, Phys. Rev. B 88, 085117 (2013).
  • [26] M. S. Hybertsen and S. G. Louie, Electron correlation in semiconductors and insulators: Band gaps and quasiparticle energies, Phys. Rev. B 34, 5390 (1986).
  • [27] M. Rohlfing and S. G. Louie, Electron-hole excitations and optical spectra from first principles, Phys. Rev. B 62, 4927 (2000).
  • [28] J. Deslippe, G. Samzonidze, D. A. Strubbe, M. Jain, M. L. Cohen, and S. G. Louie, BerkeleyGW: A massively parallel computer package for the calculation of the quasiparticle and optical properties of materials and nanostructures, Comput. Phys. Commun. 183, 1269 (2012).
  • [29] B. A. Barker, J. Deslippe, J. Lischner, M. Jain, O. V. Yazyev, D. A. Strubbe, and S. G. Louie, Spinor GW/Bethe-Salpeter calculations in BerkeleyGW: Implementation, symmetries, benchmarking, and performance, Phys. Rev. B 106, 115127 (2022).
  • [30] S. Ismail-Beigi, Truncation of periodic image interactions for confined systems, Phys. Rev. B 73, 233103 (2006).
  • [31] B. C. Shih, Y. Xue, P. Zhang, M. L. Cohen, and S. G. Louie, Quasiparticle Band Gap of ZnO: High Accuracy from the Conventional G0W0G^{0}W^{0} Approach, Phys. Rev. Lett. 105, 146401 (2010).
  • [32] K. Xie, X. Li, and T. Cao, Theory and ab initio calculation of optically excited states-recent advances in 2D materials, Adv. Mater. 19, 04306 (2019).
  • [33] L. Yang, J. Deslippe, C. H. Park, M. L. Cohen, and S. G. Louie, Excitonic Effects on the Optical Response of Graphene and Bilayer Graphene, Phys. Rev. Lett. 103, 186802 (2009).
  • [34] C. H. Park and S. G. Louie, Tunable excitons in biased bilayer graphene, Nano Lett. 10, 426 (2010).
  • [35] L. Yang, First-principles study of the optical absorption spectra of electrically gated bilayer graphene, Phys. Rev. B 81, 155445 (2010).
  • [36] L. Yang, Excitons in intrinsic and bilayer graphene, Phys. Rev. B 83, 085405 (2011).
  • [37] Y. Liang and L. Yang, Quasiparticle energy and optical excitations of gated bilayer graphene, Phys. Rev. B 86, 205423 (2012).
  • [38] Y. Liang, R. Soklaski, S. Huang, M. W. Graham, R. Havener, J. Park, and L. Yang, Strongly bound excitons in gapless two-dimensional structures, Phys. Rev. B 90, 115418 (2014).
  • [39] T. Cao, M. Wu, and S. G. Louie, Unifying Optical Selection Rules for Excitons in Two Dimensions: Band Topology and Winding Numbers, Phys. Rev. Lett. 120, 087402 (2018).
  • [40] S. Huang, Y. Liang, and L. Yang, Exciton spectra in two-dimensional graphene derivatives, Phys. Rev. B 88, 075441 (2013).
  • [41] D. Y. Qiu, F. H. da Jornada, and S. G. Louie, Optical Spectrum of MoS2: Many-Body Effects and Diversity of Exciton States, Phys. Rev. Lett. 111, 216805 (2013).
  • [42] R. Soklaski, Y. Liang, and L. Yang, Temperature effect on optical spectra of monolayer molybdenum disulfide, Appl. Phys. Lett. 104, 193110 (2014).
  • [43] D. Y. Qiu, T. Cao, and S. G. Louie, Nonanalyticity, Valley Quantum Phases, and Lightlike Exciton Dispersion in Monolayer Transition Metal Dichalcogenides: Theory and First-Principles Calculations, Phys. Rev. Lett. 115, 176801 (2015).
  • [44] D. Y. Qiu, F. H. da Jornada, and S. G. Louie, Screening and many-body effects in two-dimensional crystals: monolayer MoS2{\mathrm{MoS}}_{2}, Phys. Rev. B 93, 235435 (2016).
  • [45] W. Song and L. Yang, Quasiparticle band gaps and optical spectra of strained monolayer transition-metal dichalcogenides, Phys. Rev. B 96, 235441 (2017).
  • [46] M. H. Naik and M. Jain, Origin of layer dependence in band structures of two-dimensional materials, Phys. Rev. B 95, 165125 (2017).
  • [47] S. Gao, L. Yang, and C. D. Spataru, Interlayer coupling and gate-tunable excitons in transition metal dichalcogenide heterostructures, Nano Lett. 17, 7809 (2017).
  • [48] M. H. Naik and M. Jain, Substrate screening effects on the quasiparticle band gap and defect charge transition levels in MoS2, Phys. Rev. Mater. 2, 084002 (2018).
  • [49] S. Refaely-Abramson, D. Y. Qiu, S. G. Louie, and J. B. Neaton, Defect-Induced Modification of Low-Lying Excitons and Valley Selectivity in Monolayer Transition Metal Dichalcogenides, Phys. Rev. Lett. 121, 167402 (2018).
  • [50] X. Lu, X. Li, and L. Yang, Modulated interlayer exciton properties in a two-dimensional moiré crystal, Phys. Rev. B 100, 155416 (2019).
  • [51] M. H. Naik, E. C. Regan, Z. Zhang, Y. H. Chan, Z. Li, D. Wang, Y. Yoon, C. S. Ong, W. Zhao, S. Zhao, M. I. B. Utama, B. Gao, X. Wei, M. Sayyad, K. Yumigeta, K. Watanabe, T. Taniguchi, S. Tongay, F. H. da Jornada, F. Wang, and S. G. Louie, Intralayer charge-transfer moiré excitons in van der Waals superlattices, Nature 609, 52 (2022).
  • [52] V. Tran, R. Soklaski, Y. Liang, and L. Yang, Layer-controlled band gap and anisotropic excitons in few-layer black phosphorus, Phys. Rev. B 89, 235319 (2014).
  • [53] V. Tran, R. Fei, and L. Yang, Quasiparticle energies, excitons, and optical spectra of few-layer black phosphorus, 2D Mater. 2, 044014 (2015).
  • [54] D. Y. Qiu, F. H. da Jornada, and S. G. Louie, Environmental screening effects in 2D materials: renormalization of the bandgap, electronic structure, and optical spectra of few-layer black phosphorus, Nano Lett. 17, 4706 (2017).
  • [55] T. Cao, Z. Li, D. Y. Qiu, and S. G. Louie, Gate switchable transport and optical anisotropy in 90 twisted bilayer black phosphorus, Nano Lett. 16, 5542 (2016).
  • [56] Y. Chen and S. Y. Quek, Tunable bright interlayer excitons in few-layer black phosphorus based van der Waals heterostructures, 2D Mater. 5, 045031 (2018).
  • [57] J. Zhou, T. Y. Cai, and S. Ju, Unusual strain dependence of quasiparticle electronic structure, exciton, and optical properties in blue phosphorene, Phys. Rev. Appl. 15, 024045 (2021).
  • [58] J. Zhou, T. Y. Cai, and S. Ju, Quasiparticle band structure, exciton, and optical properties of few-layer blue phosphorus, Phys. Rev. B 104, 245401 (2021).
  • [59] J. Zhou, T. Y. Cai, and S. Ju, Anisotropic exciton excitations and optical properties of Hittorf’s phosphorene, Phys. Rev. Res. 2, 033288 (2020).
  • [60] J. Zhou, T. Y. Cai, and S. Ju, Giant Stark effect in Hittorf’s phosphorene, Phys. Rev. Appl. 17, 054047 (2022).
  • [61] G. Antonius, D. Y. Qiu, and S. G. Louie, Orbital symmetry and the optical response of single-layer MX monochalcogenides, Nano Lett. 18, 1925 (2018).
  • [62] G. Shi and E. Kioupakis, Anisotropic spin transport and strong visible-light absorbance in few-layer SnSe and GeSe, Nano Lett. 15, 6926 (2015).
  • [63] Y. H. Chan, D. Y. Qiu, F. H. da Jornada, and S. G. Louie, Giant exciton-enhanced shift currents and direct current conduction with subbandgap photo excitations produced by many-electron interactions, Proc. Natl. Acad. Sci. U.S.A. 118, e1906938118 (2021).
  • [64] N. Sanders, D. Bayerl, G. Shi, K. A. Mengle, and E. Kioupakis, Electronic and optical properties of two-dimensional GaN from first-principles, Nano Lett. 17, 7345 (2017).
  • [65] X. Blase, A. Rubio, S. G. Louie, and M. L. Cohen, Quasiparticle band structure of bulk hexagonal boron nitride and related systems, Phys. Rev. B 51, 6868 (1995).
  • [66] K. A. Mengle and E. Kioupakis, Impact of the stacking sequence on the bandgap and luminescence properties of bulk, bilayer, and monolayer hexagonal boron nitride, APL Mater. 7, 021106 (2019).
  • [67] F. Zhang, C. S. Ong, J. W. Ruan, M. Wu, X. Q. Shi, Z. K. Tang, and S. G. Louie, Intervalley Excitonic Hybridization, Optical Selection Rules, and Imperfect Circular Dichroism in Monolayer hh-BN, Phys. Rev. Lett. 128, 047402 (2022).
  • [68] L. Zhu and L. Yang, Quasiparticle energies and excitonic effects of chromium trichloride: From two dimensions to bulk, Phys. Rev. B 101, 245401 (2020).
  • [69] K. Lee, A. H. Dismukes, E. J. Telford, R. A. Wiscons, J. Wang, X. Xu, C. Nuckolls, C. R. Dean, X. Roy, and X. Zhu, Magnetic order and symmetry in the 2D semiconductor CrSBr, Nano Lett. 21, 3511 (2021).
  • [70] K. Yang, G. Wang, L. Liu, D. Lu, and H. Wu, Triaxial magnetic anisotropy in the two-dimensional ferromagnetic semiconductor CrSBr, Phys. Rev. B 104, 144416 (2021).
  • [71] G. Pizzi, V. Vitale, R. Arita, S. Blügel, F. Freimuth, G. Géranton, M. Gibertini, D. Gresch, C. Johnson, T. Koretsune, J. Ibañez-Azpiroz, H. Lee, J. Lihm, D. Marchand, A. Marrazzo, Y. Mokrousov, J. I. Mustafa, Y. Nohara, Y. Nomura, L. Paulatto, S. Poncé, T. Ponweiser, J. Qiao, F. Thöle, S. S. Tsirkin, M. Wierzbowska, N. Marzari, D. Vanderbilt, I. Souza, A. A. Mostofi, and J. R. Yates, Wannier90 as a community code: New features and applications, J. Phys.: Condens. Matter 32, 165902 (2020).
  • [72] R. Schuster, J. Trinckauf, C. Habenicht, M. Knupfer, and B. Büchner, Anisotropic Particle-Hole Excitations in Black Phosphorus, Phys. Rev. Lett. 115, 026404 (2015).
  • [73] X. Wang, A. M. Jones, K. L. Seyler, V. Tran, Y. Jia, H. Zhao, H. Wang, L. Yang, X. Xu, and F. Xia, Highly anisotropic and robust excitons in monolayer black phosphorus, Nat. Nanotechnol. 10, 517 (2015).
  • [74] H. Yuan, X. Liu, F. Afshinmanesh, W. Li, G. Xu, J. Sun, B. Lian, A. G. Curto, G. Ye, Y. Hikita, Z. Shen, S. C. Zhang, X. Chen, M. Brongersma, H. Y. Hwang, and Y. Cui, Polarization-sensitive broadband photodetector using a black phosphorus vertical p-n junction, Nat. Nanotechnol. 10, 707 (2015).
  • [75] L. Li, J. Kim, C. Jin, G. J. Ye, D. Y. Qiu, F. H. da Jornada, Z. Shi, L. Chen, Z. Zhang, F. Yang, K. Watanabe, T. Taniguchi, W. Ren, S. G. Louie, X. H. Chen, Y. Zhang, and F. Wang, Direct observation of the layer-dependent electronic structure in phosphorene, Nat. Nanotechnol. 12, 21 (2017).
  • [76] C. D. Spataru, S. Ismail-Beigi, R. B. Capaz, and S. G. Louie, Theory and Ab Initio Calculation of Radiative Lifetime of Excitons in Semiconducting Carbon Nanotubes, Phys. Rev. Lett. 95, 247402 (2005).
  • [77] M. Palummo, M. Bernardi, and J. C. Grossman, Exciton radiative lifetimes in two-dimensional transition metal dichalcogenides, Nano Lett. 15, 2794 (2015).
  • [78] J. Yang, R. Xu, J. Pei, Y. W. Myint, F. Wang, Z. Wang, S. Zhang, Z. Yu, and Y. Lu, Optical tuning of exciton and trion emissions in monolayer phosphorene, Light: Sci. Appl. 4, e312 (2015).
  • [79] Q. Cui, J. He, Z. Bellus Matthew, M. Mirzokarimov, T. Hofmann, H.-Y. Chiu, M. Antonik, D. He, Y. Wang, and H. Zhao, Small 11, 5565 (2015).
  • [80] T. Korn, S. Heydrich, M. Hirmer, J. Schmutzler, and C. Schüller, Low-temperature photocarrier dynamics in monolayer MoS2, Appl. Phys. Lett. 99, 102109 (2011).
  • [81] D. Lagarde, L. Bouet, X. Marie, C. R. Zhu, B. L. Liu, T. Amand, P. H. Tan, and B. Urbaszek, Carrier and Polarization Dynamics in Monolayer MoS2, Phys. Rev. Lett. 112, 047401 (2014).
  • [82] H. Shi, R. Yan, S. Bertolazzi, J. Brivio, B. Gao, A. Kis, D. Jena, H. G. Xing, and L. Huang, Exciton dynamics in suspended monolayer and few-layer MoS2 2D crystals, ACS Nano 7, 1072 (2013).
  • [83] C. Robert, D. Lagarde, F. Cadiz, G. Wang, B. Lassagne, T. Amand, A. Balocchi, P. Renucci, S. Tongay, B. Urbaszek, and X. Marie, Exciton radiative lifetime in transition metal dichalcogenide monolayers, Phys. Rev. B 93, 205423 (2016).
  • [84] N. Kumar, Q. Cui, F. Ceballos, D. He, Y. Wang, and H. Zhao, Exciton-exciton annihilation in MoSe2 monolayers, Phys. Rev. B 89, 125427 (2014).
  • [85] G. Wang, L. Bouet, D. Lagarde, M. Vidal, A. Balocchi, T. Amand, X. Marie, and B. Urbaszek, Valley dynamics probed through charged and neutral exciton emission in monolayer WSe2, Phys. Rev. B 90, 075413 (2014).
  • [86] S. Mouri, Y. Miyauchi, M. Toh, W. Zhao, G. Eda, and K. Matsuda, Nonlinear photoluminescence in atomically thin layered WSe2 arising from diffusion-assisted exciton-exciton annihilation, Phys. Rev. B 90, 155449 (2014).
  • [87] T. Langer, A. Chernikov, D. Kalincev, M. Gerhard, H. Bremers, U. Rossow, M. Koch, and A. Hangleiter, Room temperature excitonic recombination in GaInN/GaN quantum wells, Appl. Phys. Lett. 103, 202106 (2013).
  • [88] AM 1.5 G solar spectrum from http://rredc.nrel.gov/solar/spectra/am1.5.