Orbital Torque: Torque Generation by Orbital Current Injection
Dongwook Go, Hyun-Woo Lee

TL;DR
This paper introduces the concept of orbital torque, generated by orbital current injection in magnetic bilayers, which can induce magnetization switching even with weak spin-orbit coupling, offering a new approach for spin-torque devices.
Contribution
It proposes a novel orbital torque mechanism in NM/FM bilayers where orbital currents induce magnetization torque without requiring strong SOC in the NM.
Findings
Orbital Hall effect can generate significant orbital currents in NMs.
Orbital torque can be comparable to spin torque even with weak SOC.
Potential for new spintronic devices using light elements with large orbital responses.
Abstract
We propose a mechanism of torque generation by injection of an orbital current, which we call . In a magnetic bilayer consisting of a nonmagnet (NM) and a ferromagnet (FM), we consider a situation where the spin-orbit coupling (SOC) is present only in the FM. Although the SOC is absent in the NM, the orbital Hall effect can arise in the NM. When the resulting orbital Hall current is injected to the FM, the SOC of the FM converts the orbital angular momentum into spin, which exerts torque to the magnetization of the FM. Remarkably, even for small SOC strength comparable to that of FMs, the orbital torque can be comparable to the spin torque induced by the spin Hall effect of the NM with strong SOC. This provides a way to experimentally probe the OHE and opens a new venue to achieving spin-torque devices based on light elements that exhibit gigantic orbital…
| same sign | opposite signs | |
| opposite signs | same sign |
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Orbital Torque: Torque Generation by Orbital Current Injection
Dongwook Go
Department of Physics, Pohang University of Science and Technology, Pohang 37673, Korea
Basic Science Research Institute, Pohang University of Science and Technology, Pohang 37673, Korea
Peter Grünberg Institut and Institute for Advanced Simulation, Forschungszentrum Jülich and JARA, 52425 Jülich, Germany
Hyun-Woo Lee
Department of Physics, Pohang University of Science and Technology, Pohang 37673, Korea
Abstract
We propose a mechanism of torque generation by injection of an orbital current, which we call orbital torque. In a magnetic bilayer consisting of a nonmagnet (NM) and a ferromagnet (FM), we consider a situation where the spin-orbit coupling (SOC) is present only in the FM. Although the SOC is absent in the NM, the orbital Hall effect can arise in the NM. When the resulting orbital Hall current is injected to the FM, the SOC of the FM converts the orbital angular momentum into spin, which exerts torque to the magnetization of the FM. Remarkably, even for small SOC strength comparable to that of FMs, the orbital torque can be comparable to the spin torque induced by the spin Hall effect of the NM with strong SOC. This provides a way to experimentally probe the OHE and opens a new venue to achieving spin-torque devices based on light elements that exhibit gigantic orbital response. Experimental implications are discussed.
Spin injection into a ferromagnet (FM) generates a spin torque (ST) on magnetic moments of the FM by the angular momentum transfer from the spin of injected conduction electrons. For ST generation, a spin current source is needed. A popular source is a nonmagnet (NM) with strong spin-orbit coupling (SOC), which exhibits sizable spin Hall effect (SHE). The ST of the SOC origin is called spin-orbit torque Pi et al. (2010); Mihai Miron et al. (2010); Miron et al. (2011a, b); Pai et al. (2012); Liu et al. (2012a, b); Kim et al. (2012); Haney et al. (2013a, b); Garello et al. (2013, 2014); Kurebayashi et al. (2014); Hayashi et al. (2014); Yu et al. (2014); Freimuth et al. (2014); Kim et al. (2017); Mahfouzi and Kioussis (2018), which has drawn considerable attention as a powerful means to electrically control magnetic configurations.
Similar to the SHE, the orbital Hall effect (OHE) allows for electrical generation of a transverse orbital current. In transition metals, for example, electron wavefunctions near atomic cores have mainly character, and superpositions such as carry the orbital angular momentum . A flow of wavepackets with such superposed wavefunctions generates an orbital current. Considering that an orbital current carries the angular momentum just like a spin current does, it is reasonable to expect that injection of an orbital current (or orbital injection in short) into a FM may generate a torque on local magnetic moments of the FM. We call such torque as orbital torque (OT), which provides an experimental way to detect the OHE. Although the OHE has not yet been experimentally verified, theoretical calculations Tanaka et al. (2008); Kontani et al. (2009) on and transition metals indicate that the orbital Hall conductivities (OHCs) of these NM’s are about an order of magnitude larger than the spin Hall conductivities (SHCs). Moreover, our recent theoretical analysis finds that the OHC can be gigantic even in materials with negligible SOC Go et al. (2018); Jo et al. (2018). Thus the OT also provides a new venue to achieving high torque efficiency in spintronic devices.
In this Letter, we investigate the theoretical idea of the OT for a NM/FM bilayer structure (Fig. 1). When an in-plane electric field is applied, both OHE and SHE arise in the NM in general Go et al. (2018); Kontani et al. (2009); Tanaka et al. (2008); Jo et al. (2018). In order to focus on the OT due to the orbital injection, we suppress the SHE by setting the SOC of the NM zero. Then only OHE is induced and a resulting torque in the FM can be identified unambiguously as the OT. We find that the OT indeed arises as long as the SOC of the FM is finite.
For a quantitative evaluation of the OT, we adopt the tight-binding description of the bilayer with atomic layer thick NM(FM) [Fig. 2(a)]. We assume both NM and FM to have the simple cubic structure. For the NM, we adopt the model that has been used previously Go et al. (2018) to illustrate the OHE without the SOC. In this model, each lattice site can host , , , and orbitals, and the orbital hydridization, which is crucial for the emergence of the OHE Go et al. (2018), arises from the symmetry-allowed nearest neighbor hoppings between and orbitals. For the FM, we adopt a trivial model; each lattice site can host , , , , and orbitals with nearest neighboring hoppings allowed. This model does not allow any orbital hybridization Cub and thus there is no OHE Go et al. (2018); Jo et al. (2018). The model is augmented by adding the SOC
[TABLE]
and the exchange coupling , where is the orbital angular momentum of character states in the FM, is the spin, and denotes the magnetization direction of the FM. Below, we focus on the case . At the interface, the nearest neighbor hoppings exist between the orbitals in the NM and the orbitals in the FM. Details of the tight-binding description are given in Ref. Sup . All parameters of the NM and FM are set to have typical energy scales of nonmagnetic and magnetic metals. In particular, we set , which is a typical SOC strength of transition metals Wang and Callaway (1974); Sunko et al. (2017); Jo et al. (2018). We emphasize that the nonzero is crucial for the OT since couples only to and there is no direct coupling between and in the Hamiltonian. Thus for the injected orbital current to generate the OT, it should be first converted to spin through and then the resulting spin can generate the torque through (Fig. 1).
Figure 2(b) shows the band structure of the NM/FM bilayer for and , where the color represents the equilibrium expectation value of the spin-orbit correlation in the FM region for each state. The correlation is negative in the lower energy range (), and positive in the higher energy range (). In the middle energy range (), states with positive and negative correlations coexist. We later demonstrate that is important for the sign of the OT.
For , we calculate the electrically generated orbital () and spin () accumulations at each atomic layer as a function of . From the Kubo formula, one obtains the expectation value ( or ) generated by , where
[TABLE]
are the intraband and interband contributions, respectively. Here, measures the local accumulation of at , where is the projection operator to the atomic layer at . In Eq. (2), is the unit charge, is the Plank constant, is the velocity operator along the direction, is the Fermi-Dirac distribution function for a periodic part of the Bloch state with its energy eigenvalue . To incorporate the effect of disorder scatterings, we phenomenologically introduce a spectral broadening , which is a room temperature scale.
Figure 3 shows the (a) and (b) components of the resulting and for the Fermi energy . We first consider a situation when the NM and the FM are disconnected (hoppings between the NM and FM turned off). In the NM (), [white inverted triangles in Fig. 3(a)] has nonzero values of opposite signs at the opposite edges of the NM ( and 20). This result can be interpreted as the orbital accumulation at the edges due to the OHE in the NM. The OHC in the NM is for Go et al. (2018); Sup . On the other hand, [white inverted triangles in Fig. 3(b)] is absent in the NM. In the FM (), both and are zero, confirming the absence of the OHE in the FM. The spin accumulation is zero both in the NM and the FM (not shown), which is natural since the SHE is absent in both NM and FM.
Next we connect the NM and the FM (hoppings between the NM and FM turned on). Near , which is far from the NM/FM interface, [blue circles in Fig 3(a)] remains essentially unchanged. Near the interface (), on the other hand, is reduced significantly since the orbital Hall current is now injected into the FM instead of getting accumulated at the interface. The injected orbital Hall current in the FM produces not only but also [orange squares in Fig 3(a) for 10 enlarged values] due to . Moreover once becomes nonzero in the FM, the spin precesses around due to and produces as well [orange squares in Fig 3(b) for 10 enlarged values]. This precession results in oscillatory profiles of and in the FM, which resemble oscillatory spin accumulation profiles Haney et al. (2013a) in a conventional situation, where a spin current is injected into a FM to generate the ST. The oscillatory profiles of and in the FM are accompanied by similar oscillatory profiles of and . The coexistence of the spin and orbital accumulation oscillations is due to and we note that the spin and orbital oscillations are 180∘ out of phase for (Fig. 3), which we attribute to negative spin-orbit correlation at this energy [Fig. 2(b)]. By the way, the spin accumulation in the NM is due to partial reflection of the orbital Hall current at the NM/FM interface.
The torque acting on the FM can be obtained from the spin accumulation as follows,
[TABLE]
where . When the SOC of the NM is zero, arises from the orbital injection and thus the resulting amounts to the OT. Analogous to the ST, the OT can be decomposed as , where refers to the field(damping)-like component. When , and . We find that , which arises from the intraband(interband) contribution in Eq. (2), is even(odd) in , thus the field(damping)-like OT is odd(even) under sign reversal of . This is similar to the generation of the field-like and damping-like STs when a spin current polarized along direction is injected into a FM magnetized along the direction Haney et al. (2013a).
Since plays a more important role for the current-induced magnetization dynamics than Liu et al. (2012a, b), we focus on . A result for is given in Ref. Sup . Figure 4(a) shows that the ratio (orange squares) is positive for and negative for . For comparison, the ratio (blue circles) is also shown, where . Note that the relative ratio between and is negative for , and positive for . The -dependence of the relative ratio sign closely resembles the energy dependence of the spin-orbit correlation in Fig. 2(b). By combining the calculation result in Fig. 4(a) with the fact that the OHC of the NM is positive essentially for all Go et al. (2018), we find that the sign of tends to be determined by the sign of the product between the OHC of the NM and the spin-orbit correlation in the FM. Considering that determines the damping-like OT, the latter tendency may be regarded as the OT counterpart of the sign “rule" for the ST; the damping-like ST tends to be determined by the sign of the spin Hall conductivity (SHC) in the NM Liu et al. (2012a, b); Haney et al. (2013a).
Figure 4(b) shows the ratio as a function of for (purple squares) and (green squares). These two values are close to the peak positions in Fig. 4(a) (denoted by the yellow star and the red cross). For these favorable choices of , values of are and for , which is SOC energy scale for FMs. Here is the lattice constant. By increasing , they reach up to and for , which is SOC energy scale for transition metals. Note that these values for are not negligible compared to the corresponding value for the damping-like torque calculated for the Pt/Co bilayer Freimuth et al. (2010); Mahfouzi and Kioussis (2018) with the SOC strength of for Pt. Then, considering that the OHC in real materials such as V is gigantic , which is about 6 times larger than the OHC of the model used in our calculation, for real NMs may be proportionally larger and comparable to the corresponding ST value for the Pt/Co bilayer. Although quantitative predictions on require realistic calculations that take material details into account, we argue it is still reasonable to expect that the OT may be sizable for a FM with weak SOC, thus providing an alternative route to enhancing the torque efficiency.
So far we have assumed the SOC is absent in the NM. Now we consider a situation where not only the FM but also the NM have the SOC. Thus the model Hamiltonian for the NM now includes
[TABLE]
where is the SOC parameter in the NM. Since character states do not carry the orbital angular momentum, in Eq. (S72) acts only on character states. Due to , the NM exhibits SHE, as well as the OHE. Thus, on top of the OT, injection of the spin Hall current into the FM generates the ST. It is known that OHE and SHE occur in the same(opposite) direction if is positive(negative) at Tanaka et al. (2008); Kontani et al. (2009); Go et al. (2018). Thus, when at , which is a case for Ni, the OT and ST add up if and cancel each other if . This situation becomes the opposite when , as in Gd. The result is summarized in Table 1, which is supported by our numerical calculation Sup . This implies that the total torque may go even beyond the level expected from the theoretical value for the SHC of a NM, as in recent experiments Zhu et al. (2018); Du et al. (2018) When the OT and ST cancel each other, the total torque may even exhibit the opposite sign compared to the sign expected from the SHC of the NM. For example, Ta and W exhibit the opposite signs of the OHC and SHC Tanaka et al. (2008).
Unfortunately, the OT and ST exhibit qualitatively similar behavior, thus disentangling the OT from the ST is challenging. The orbital and spin operator transform in the same way for symmetry operations, i.e. both OT and ST exhibit the same angular dependence. Nonetheless, the OT and ST are expected to exhibit different quantitative features. One characteristic feature of the OT is its strong correlation with as demonstrated in Figs. 3 and 4(b). This suggests that the OT can be probed through material variation of a FM. This is in stark contrast to the ST, where the a role of the FM is less important. We expect that alloying a FM with heavy elements would not only increase the OT since the conversion from the orbital to spin becomes more efficient but also provide a way to systematically tune the spin-orbit correlation of the FM FM_ .
Another distinct feature of the OT compared to the ST is its dependence on the interface crystallinity. For the orbital injection across the interface, it must occur through orbital hybridizations at the NM/FM interface. In the tight-binding model in Fig. 2(a), and hybridizations are crucial for transferring Sup . Thus even spin-conserving interface scatterings can result in orbital relaxation, making the orbital transparency more sensitive to the interface crystallinity than the spin transparency. Particularly, when the NM and FM elements tend to be mixed, the OT will be suppressed since the atomic ordering of the NM and FM atoms disappears at the interface ato .
When the NM/FM bilayer consists only of light elements with weak SOC, the total torque is dominated by the OT as in Fig. 1, which is advantageous for unambiguously quantifying the OT. In the past, unexpectedly large torque was measured in samples containing Cr Du et al. (2014); Qu et al. (2015) and Py Miao et al. (2013); Tsukahara et al. (2014) in spite of small SOC of these elements. These results may be related to the OT, which requires further investigation. Finally, we remark that the orbital angular momentum can be generated not only by the OHE but also by the interfacial Rashba-type states Go et al. (2017); Chen et al. (2018), which may be related to sizable field-like torque measured in Py/(Cu)/ structure Emori et al. (2016).
Acknowledgements.
We acknowledge Daegeun Jo, Junyeon Kim, YoshiChika Otani, Jan-Philipp Hanke, Frank Freimuth, Yuriy Mokrousov, and Kyung-Jin Lee for insightful discussions. D. G. and H.-W. L. were supported by the SSTF (Grant No. BA-1501-07).
.1 A. Tight-Binding Model
The tight-binding model for a magnetic bilayer presented in the Letter is composed of a nonmagnet (NM) and a ferromagnet (FM). The numbers of layers for the NM and the FM are and , respectively. We assume the simple cubic structure for both NM and FM with only nearest neighbor hoppings allowed. We also assume that the layer is periodic in and directions, and the layers are stacked along direction. Thus, the NM is located from to and the FM is located from to (in unit of the lattice spacing ), and we use the Bloch theorem for and directions by introducing the crystal momentum . The total Hamiltonian is formally written as
[TABLE]
where is the Hamiltonian for a two-dimensional NM(FM) layer, is the hopping between nearest NM(FM) layers, and is the interface hopping between the last NM layer () and the first FM layer ().
.1.1 1. NM
We assume the NM hosts orbitals at each site, which was introduced in Ref. Go et al. (2018). Writing the Hamiltonian in a finite film structure is straightforward as follows. The Hamiltonian within each two-dimensional NM layer consists of the kinetic energy and spin-orbit coupling (SOC) parts:
[TABLE]
First, the kinetic part is
[TABLE]
where
[TABLE]
and is an identity operator in the spin space. Here, the basis states are
[TABLE]
where is a Wannier function localized at the Bravais lattice with its orbital character and spin , which is defined in a layer located at . For the Wannier states, , are onsite energies for and orbitals, and , , are the nearest hopping amplitudes between orbitals, between orbitals via bonding, and between and orbitals, respectively. Second, the SOC part is
[TABLE]
where is the spin operator and is the orbital angular momentum (OAM) operator in orbital space. Here, is the strength of the SOC in the NM. The OAM operator is explicitly expressed in a matrix representation
[TABLE]
with , , and orbital Wannier functions. Finally, the interlayer coupling between neighboring NM layers is described as
[TABLE]
where the basis states for the row and column are and , respectively, for .
.1.2 2. FM
In the FM, we assume there are orbitals at each site. The Hamiltonian within each two-dimensional layer is
[TABLE]
where each term describes kinetic energy, SOC, and exchange interaction with magnetization, respectively. The kinetic energy term is
[TABLE]
where
[TABLE]
Here, is the onsite energy of the orbital, and , , are nearest neighbor hoppings between orbitals via , , bondings, respectively. The basis states are defined similarly as Eq. (S19) but for orbital Wannier functions. The SOC term is
[TABLE]
where is the SOC strength. Here, is the OAM operator in orbital space, whose matrix representation is written as
[TABLE]
where the basis states are , , , , orbital Wannier functions. The exchange interaction is
[TABLE]
where is the strength of the exchange interaction, and is the direction of the magnetization. We assume in the calculation. The interlayer coupling between neighboring FM layers is
[TABLE]
where the basis for the row and column are and , respectively, for .
.1.3 3. Interface
At the interface, there are hoppings between the last NM layer () and the first FM layer (), which are expressed in
[TABLE]
where the basis for the row and column are and , respectively. Here, is the nearest neighbor hopping between and orbitals via hoppings. We neglect the hopping from a orbital in the NM to orbitals in the FM, since the orbital does not carry the OAM, thus not affecting the orbital injection.
.1.4 4. Parameter Setting
For the tight-binding model defined above, parameters which we used for the calculation in Figs. 2 and 3 of the Letter are set as
[TABLE]
for the NM,
[TABLE]
for the FM, and
[TABLE]
for the interface. All parameters are expressed in unit of .
.2 B. Spatial Profiles of the Orbital and Spin Hall Currents
Linear responses of the orbital and spin Hall currents are evaluated using the Kubo formula as follows:
[TABLE]
where
[TABLE]
is the spin/orbital ( or ) current operator defined in a layer at . Here, is the projection operator to a layer at . The velocity operator along the direction is defined as
[TABLE]
Figure S1 shows spatial profiles of the orbital and spin Hall currents obtained from the tight-binding model introduced in Sec. .1. The parameters are set as Eqs. (S66)-(S68), and the numbers of the NM and FM layers are and . For this calculation, we set the Fermi energy as . We find that the orbital Hall conductivity in the NM region is more than . In the FM region, part of the orbital Hall current is injected, which is converted to the spin current by the SOC of the FM [Eq (S35)]. We also find the spin current in the NM region, which is decaying from the interface. This is because reflected current from the interface becomes spin-polarized. The decay is due to finite spectral broadening in Eq. (S69).
.3 C. Correlation between and : Fermi Energy Dependence
Figure S2(a) shows Fermi energy dependence of for and , where or . This contribution is even under the sign reversal of , and arises from the intraband contribution [Eq. (2a) of the Letter]. While sign and magnitude vary depending on , the signs of and are opposite in the lower energy range () and same in the upper energy range (). The -dependence of the sign of the relative ratio between and strikingly resembles the energy dependence of the spin-orbit correlation in Fig. 2(b).
However, the variation of [Fig. S2(a)] differs from the variation of [Fig. 4(a)]. A reason for such difference is due to the fact that while arises from the intraband contribution for the states at the Fermi surface [Eq. 2(a)] arises from the interband contribution for the states in the Fermi sea [Eq. 2(b)]. However, for each state in the band structure, they have strong correlations. To demonstrate this point, we present in Fig. S2(b) a plot of , which corresponds to the contribution within the energy slice near . By comparing this with [Fig. S2(a)], we find strong resemblance for both orbital and spin over the whole range of , except that their relative signs are opposite.
.4 D. Spin-Orbit Coupling Dependence
Figure S3 shows Fermi energy dependences of (a) , (b) , (c) , and (d) for different values of . First, remains almost invariant under the increase of [Fig. S3(a)]. This is expected because , which results from the orbital Hall effect (OHE) in the NM, is not affected by the SOC of the FM. On the other hand, the rest three quantities exhibit monotonic increase as becomes larger within the range [Figs. S3(b), S3(c), and S3(d)]. The monotonic increase of [Fig. S3(b)] is understandable because is directly converted from the by the SOC in the FM. Also, since results from the precession of by the exchange interaction in the FM [Eq. (S53)], monotonic increase of the with follows that of [Fig. S3(d)]. On the other hand, since the precession of the spin is coupled to the orbital by the SOC in the FM, is proportional to . Thus, also increases monotonically with increasing [Fig. S3(c)].
In Fig. 4(b), the SOC dependence of , which is proportional to , is shown for fixed Fermi energies and . In Fig. S3(d), we find that monotonically increases with at and . Although the magnitude of the peak monotonically increases, the peak position may change at some Fermi energy, i.e. at . At such Fermi energy, may exhibit nonmonotonic behavior. This is due to modification of the band structure with increasing .
.5 E. Orbital Torque versus Spin Torque
.5.1 1. NM SOC included
When the SOC in the NM is nonzero, the spin Hall effect (SHE) follows the OHE Go et al. (2018) thus orbital torque (OT) and spin torque (ST) coexist. Relative sign of the OT and ST is determined by the spin-orbit correlations in the NM and in the FM as summarized in Table I of the Letter. In this section, we demonstrate this point from the numerical calculation by setting finite SOC strength in the NM:
[TABLE]
Except for , the rest of the parameters are set equal to Eqs. (S66), (S67), and (S68). Figure S4 displays the band structure shown in lines and (a) and (b) shown in colors. In the NM, is positive in the upper energy range ( near the -point and near the -point) and negative in the lower energy range ( near the -point and near the -point) in general [Fig. S4(a)]. Note that this is essentially the same as Fig. 2(b) of Ref. Go et al. (2018) because all the parameters in the NM regions are set equal to those used in Ref. Go et al. (2018). Meanwhile, in Fig. S4(b) is almost the same as Fig. 2(b) of the Letter.
In order to differentiate the OT and ST contributions to , we calculate electric field response of [Eq. (2) of the Letter] by setting SOC strength parameters in the NM and FM by (i) , , and (ii) , . Note that the sign of is reversed in (ii). This reversal is motivated by the fact that it reverses the sign of the OT while it does not affect the sign of the ST. By this way, the band structure is barely affected and also the sign of the for the case (ii) becomes opposite to that for the case (i). Thus, we define the OT and ST contributions as
[TABLE]
such that . Therefore, we calculate and from the Kubo formula in Eq. (2) of the Letter, and extract the OT and ST contributions by Eq. (S73) for , where and [Fig. S4]. Thus, the OT and ST contributions are expected to have the same sign.
In Fig. S5(a), spatial profile of is shown in the NM region () and the FM region (). The OT contribution (orange squares) is similar to the result of when [Fig. 3(a) of the Letter]. On the other hand, the ST contribution (cyan diamonds) exhibits a standard behavior of the SHE; the spin is accumulated at the boundary. Near , sign of is negative, which implies that the OHE and SHE occurs in the opposite directions. In the absence of the FM, is positive near (not sown). However, due to presence of the FM attached, is reduced near , which is injected to the FM. We find that the signs of the OT and ST contributions are same in the FM region. This is expected from the spin-orbit correlations of states near and from the fact that results from the intraband contribution at the Fermi surface [Eq. (2a)]. When is injected to the FM, it precesses along the magnetization by the exchange interaction, regardless of whether it is the OT or ST contribution. In the Kubo formula calculation, is captured by the interband contribution in the Fermi sea [Eq. (2b) of the Letter]. Nevertheless, we find that the signs of the OT and ST contributions are same in the FM region [Fig. S5(b)], which is because all the states below satisfy and .
.5.2 2. NM SOC included, FM onsite changed
The result shown in the previous subsection considers the case when the sign of the OT and ST is same. In this subsection, we present a result in another regime where the OT and ST have the opposite signs. To achieve this, we shift the onsite energy of orbitals in the FM by setting
[TABLE]
which is lower than the original system by [Eq. (S67)]. The rest of the parameters are unchanged. The spin-orbit correlations in the NM and FM are shown on top of the band structure in Figs. S6(a) and S6(b), respectively. Now near , but , thus we expect the opposite signs for the OT and ST. From the same method [Eq. (S73)], we calculate the electric field responses of the OT and ST contributions. Figures S7(a) and S7(b) show the results for and , respectively. We find the signs of the OT and ST contributions are opposite in both cases. The result for [Fig. S7(b)], which is the interband contribution from the Fermi sea, is understood as the following. Although there are many FM bands with below , the hotspots for the OHE and SHE in the NM is concentrated in the energy range Go et al. (2018) thus the torque contribution from the FM bands with is negligible and the major contribution is from the states in an energy range .
.6 F. Role of the Interface Hoppings for the Orbital Torque
In this section, we demonstrate crucial role of the interface hoppings for the OT. For the orbital injection from the NM to the FM in the tight-binding model presented in the Letter, the orbital information in the orbitals in the NM should be transferred to the orbitals in the FM. At the interface, two types of hoppings are crucial for this:
[TABLE]
Once a state carrying finite OAM, for example, is induced in the NM, the interface hoppings in Eq. (S75) can generate a state that also carries net OAM.
Thus, the relative sign of and is crucial, by which the OT changes the sign. In the tight-binding model used in the Letter, we assume the same sign for and [Eq. (S68)]. In order to demonstrate this effect, we present calculation results for and in Figs. S8(a) and S8(b), respectively, by assuming
[TABLE]
which is to be compared with Fig. 3 of the Letter. We find that is unchanged near , which is away from the interface. However, near the interface () and in the FM region (), the sign of the in Fig. S8(a) is opposite to that in Fig. 3(a) of the Letter. As a consequence, , which is converted from the injected orbital angular momentum, also changes the sign [Fig. S8(a)]. Since precesses along the magnetization by the exchange interaction and follows by the SOC in the FM, the signs of and in Fig. S8(b) are flipped compared to Fig. 3(b) of the Letter.
Therefore, the interface crystallinity is crucial for the generation of the OT. In dirty interface, the interface hoppings, such as Eq. (S75), are randomized, and this reduces the magnitude of the OT. On the other hand, the spin injection is not affected by the relative sign of the interface hoppings, thus the ST is less susceptible to the interface crystallinity.
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