Chinese Physics Letters, 2020, Vol. 37, No. 8, Article code 087501Express Letter An Origin of Dzyaloshinskii–Moriya Interaction at Graphene-Ferromagnet Interfaces Due to the Intralayer RKKY/BR Interaction Jin Yang (杨锦)1, Jian Li (李健)1, Liangzhong Lin (林亮中)2, and Jia-Ji Zhu (朱家骥)1* Affiliations 1School of Science and Laboratory of Quantum Information Technology, Chongqing University of Posts and Telecommunications, Chongqing 400065, China 2School of Information Engineering, Zhongshan Polytechnic, Zhongshan 528400, China Received 28 June 2020; accepted 3 July 2020; published online 4 July 2020 Supported by the National Natural Science Foundation of China (Grant Nos. 11404043 and 1160041160), the Key Technology Innovations Project to Industries of Chongqing (Grant No. cstc2016zdcy-ztzx0067), and the Graduate Research Innovation Project of Chongqing (Grants No. CYS18253).
*Corresponding author. Email: zhujj@cqupt.edu.cn
Citation Text: Yang J, Li J, Lin L Z and Zhu J J 2020 Chin. Phys. Lett. 37 087501    Abstract We present a theory of both the itinerant carrier-mediated RKKY interaction and the virtual excitations-mediated Bloembergen–Rowland (BR) interaction between magnetic moments in graphene induced by proximity effect with a ferromagnetic film. It is shown that the RKKY/BR interaction consists of the Heisenberg, Ising, and Dzyaloshinskii–Moriya (DM) terms. In the case of the nearest distance, we estimate the DM term from the RKKY/BR interaction is about $0.13$ meV for the graphene/Co interface, which is consistent with the experimental result of DM interaction $0.16\pm0.05$ meV. Our calculations indicate that the intralayer RKKY/BR interaction may be a possible physical origin of the DM interaction in the graphene-ferromagnet interface. This work provides a new perspective to comprehend the DM interaction in graphene/ferromagnet systems. DOI:10.1088/0256-307X/37/8/087501 PACS:75.30.Gw, 75.70.Ak, 75.70.Cn, 75.70.Tj © 2020 Chinese Physics Society Article Text Graphene has been the superstar for its unique properties in condensed matter physics since 2004. Magnetism and magnetic phenomena in graphene are the key issues in implementing graphene-based spintronic devices. Since the intrinsic magnetism is absent in graphene, one may induce magnetism by some extrinsic strategies, for example, creating magnetic moments by introducing vacancies,[1–3] adding adatoms,[4–6] or doping magnetic impurities.[7,8] However, the feasibility of these approaches is under debate, and the experimental realizations pose tough challenges.[9–11] Therefore, the other extrinsic strategies such as edge engineering in zigzag nanoribbons,[12–14] biased bilayer graphene,[15,16] or magnetic proximity effect borrowed from adjacent magnetic materials,[17,18] receive great attention. The magnetic proximity effect could bring about the strong hybridization between the $2p_z$ orbitals of the carbon atoms with the $d$ states of the metallic substrate and the sublattice-symmetry breaking.[19] The proximity effect may also promote the enhancement of the Rashba spin-orbit coupling (RSOC)[20] and anomalous Hall effect in graphene-ferromagnetic films.[17] Between the magnetic moments borrowed from the ferromagnetic substrate, an indirect magnetic interaction emerges, which is called the Ruderman–Kittel–Kasuya–Yosida (RKKY) interaction.[21–23] The RKKY interaction is an indirect magnetic interaction mediated by itinerant electrons or holes between magnetic moments, which permits highly controllability thanks to the itinerant carriers. There have been intense researches on the RKKY interaction in graphene using various approaches like the Matsubara Green function technique,[24–26] the lattice Green function technique,[27,28] and the exact diagonalization approach.[29] Some common conclusions have been reached: (i) The RKKY interaction is a usual isotropic Heisenberg-typed interaction in graphene. (ii) The range function decays as $1/R^{3}$ with no oscillation in pristine graphene and oscillates with $1/R^{2}$ decay in doped graphene. (iii) The RKKY interaction between two magnetic moments is ferromagnetic when they are on the same sublattice and is antiferromagnetic when they are on different sublattices. The progress of the spin-orbitronics permits highly efficient electrical control of chiral spin textures—skyrmions or domain wall dynamics, and shows some exciting potential applications in spintronic memory and logic devices.[30,31] These potential applications are based on interfacial Dzyaloshinskii–Moriya (DM) interaction which has been experimentally observed.[32] The DM interaction was first proposed for explaining the weak ferromagnetism in oxide materials[33] and is related to spin-orbit coupling.[34] Typical DM interaction exists in noncentrosymmetric bulk magnets[35,36] and at interfaces between ferromagnets and metals.[37–40] Yang et al. showed that the physical origin of interfacial DM interaction is the Rashba effect.[41,42] Indeed, several kinds of research shows that there is a large Rashba spin-orbit splitting at the graphene-ferromagnet (e.g., Ni or Co) interface,[43–45] and the RSOC could be enhanced to a giant Rashba effect by the intercalation.[46,47] However, the giant Rashba effect could also make some difference from the RKKY interaction in graphene and may result in an anisotropic coupling which consists of the DM interaction.[48] Vedmedenko et al. showed that the interfacial DM interaction attributes to an interlayer DM term from the RKKY interaction (Lévy–Fert model).[49] They also showed that the intralayer RKKY interaction is dominated by a ferromagnetic Heisenberg term. However, we will show that the RKKY interaction also contains an intralayer DM term which contributes to the interfacial DM interaction. In this Letter, we present the RKKY interaction in graphene between magnetic moments induced by proximity effect of a ferromagnetic metal. The ferromagnet provides both broken time-reversal symmetry and RSOC. Due to the RSOC resulting from the graphene-ferromagnet interface, we find that there are Heisenberg, Ising, and DM terms in the RKKY interaction rather than the usual Heisenberg-typed interaction in graphene. This DM interaction could also induce magnetic chirality and weak ferromagnetism. We also consider the Bloembergen–Rowland (BR) interaction when the Fermi energy lies across the neutral point,[50] and show that the BR interaction mainly consists of DM term and Heisenberg term in the nearest distance. We estimate the DM interaction arising from the RKKY/BR interaction to be about $0.13$ meV for the graphene-Co interface, which is consistent with the experimental result of DM interaction $0.16\pm0.05$ meV.[41] Our results indicate that the DM interaction may not be induced by the Rashba effect directly but may be induced by the Rashba effect indirectly via the BR/RKKY interaction. We also show that the RKKY interaction is nearly independent of Fermi energy in the nearest distance, and almost the same as the BR interaction. The Fermi energy hardly influences our estimate of the DM interaction. Model. We consider two magnetic moments located in graphene, which are borrowed from an adjacent ferromagnetic metal (Co or Ni films). The atomic distance of fcc Ni(111) or hcp Co(0001) planes is almost perfectly matched with the length of the basis vector of graphene, as shown in Fig. 1(a). The total Hamiltonian can be written as $ {H}={H}_{0}+{H}_{\rm int}$, where ${H_{0}}$ is the Hamiltonian of itinerant electrons in graphene with RSOC and intrinsic spin-orbit coupling (ISOC),[51,52] $$ {H}_{0}=\hbar v_{\rm F}\left({\tau}_{x}k_{x}+{\tau}_{y}k_{y}\right) +\lambda _{\rm R}\left({\tau}_{x} {\sigma}_{y}-{\tau}_{y}{\sigma}_{x}\right) +\varDelta {\tau}_{z}{\sigma}_{z},~~ \tag {1} $$ where the $\lambda_{\rm R}$ and $\varDelta$ are the RSOC and the ISOC constant, respectively, the $v_{\rm F}$ denotes the Fermi velocity of graphene, Pauli matrices of pseudospin ${\boldsymbol \tau}$ operate on A(B) sublattices, and ${\boldsymbol \sigma}$ represents Pauli matrices for real electron spin.
cpl-37-8-087501-fig1.png
Fig. 1. (a) The top-view of the crystal configurations of graphene-coated Ni or Co films, and (b) the band structure for the graphene-nickel system with $\lambda_{\rm R}=50$ meV, $\varDelta=40$ µeV. The red (blue) lines represent conduction (valence) bands, and $\uparrow$ ($\downarrow$) represents spin up (down). The spin quantum axis is perpendicular to the interface.
The exchange interaction between the local magnetic moments, ${\boldsymbol S}_{1}$ and ${\boldsymbol S}_{2}$, induced by proximity effect of a ferromagnet with the itinerant electron spins ${\boldsymbol \sigma}$ can be given by[51,53,54] ${H}_{\rm int}=-J({\boldsymbol \sigma}\cdot {\boldsymbol S}_{i}) \delta ({\boldsymbol r}-{\boldsymbol R}_{i})$, where $J$ denotes the strength of the $s$–$d$ exchange interaction. In the loop approximation we find the RKKY/BR interaction between two magnetic moments in the form of[53,54] $$\begin{align} {H}_{\alpha \beta}^{\rm RKKY/BR} ={}&-\dfrac{J^{2}}{\pi}\operatorname{{\rm Im}}\int_{-\infty }^{\varepsilon_{\rm F}}{d}\varepsilon {\rm Tr}\big[({\boldsymbol \sigma }\cdot {\boldsymbol S}_{1}) \\ &\times {\boldsymbol G}_{0}^{\alpha \beta}({\boldsymbol R}, \varepsilon) ({\boldsymbol \sigma}\cdot {\boldsymbol S}_{2}) {\boldsymbol G}_{0}^{\beta \alpha }(-{\boldsymbol R}, \varepsilon) \big],~~ \tag {2} \end{align} $$ where $\alpha,\beta$ are the sublattice indices, A or B, and ${\boldsymbol R}$ denotes the lattice vector between the sublattices $\beta$ and $\alpha$. Here ${\boldsymbol G}_{0}^{\alpha \beta}({\boldsymbol R,}\varepsilon) $ is the unperturbed Green function in energy-coordinate representation and $\varepsilon_{\rm F}$ is Fermi energy. Tr means a partial trace over the spin degree of freedom of itinerant Dirac electrons. The Green functions in real space can be calculated by integrating the corresponding Green functions in momentum space over the wave vector ${\boldsymbol k}$ in the vicinity of $K$ valley,[27,51] $$\begin{alignat}{1} {\boldsymbol G}_{0}^{\alpha \beta}\left(\pm {\boldsymbol R,}\varepsilon \right) =\dfrac{1}{\varOmega_{\mathrm{BZ}}}\int d^{2}ke^{\pm {i}{\boldsymbol k}\cdot {\boldsymbol R}}{\boldsymbol G}_{0}^{\alpha \beta }\left({\boldsymbol k},\varepsilon \right).~~ \tag {3} \end{alignat} $$ The ${\boldsymbol k}$-dependent Green functions, ${\boldsymbol G}_{0}\left({\boldsymbol k,}\varepsilon \right)=\left(\varepsilon+{i}\eta-{H}_{0}\right)^{-1}$, corresponding to Hamiltonian (1), can be rewritten as a $2\times2$ matrix form on the bases of different sublattices. With all the calculated on-site Green functions and site-site Green functions, the effective RKKY/BR interaction can be obtained as follows: $$\begin{align} {H}_{\alpha,\beta}^{\rm RKKY/BR} ={}&J_{\rm H}^{\alpha \beta}{\boldsymbol S}_{1}\cdot {\boldsymbol S}_{2}+J_{\rm DM}^{\alpha \beta} \left({\boldsymbol S}_{1}\times {\boldsymbol S}_{2}\right)_{y} \\ &+ J_{z}^{\alpha \beta}{S}_{1z}{S}_{2z} +J_{y}^{\alpha \beta}{S}_{1y}{S}_{2y}~~ \tag {4} \end{align} $$ To obtain the simplest expression, we rotate the $x$-axis to make sure that the angle of the position vector ${\boldsymbol R}$ with respect to the crystalline orientation vanishes. The $y$-axis is perpendicular to the $x$-axis in the plane of graphene sheet. The effective anisotropic spin-spin interaction between local moments includes Heisenberg, Ising, and DM interactions. This behavior of RKKY/BR interaction recurs in topological insulators,[53] topological semimetals,[55,56] p-doped transition-metal dichalcogenides,[57] etc. The three type terms arise from the symmetry breaking due to the RSOC and the ISOC. We list the results for two cases, i.e., the magnetic moments located on the same sublattices or the opposite sublattices, and one can see that the $y$ direction Ising term and the DM term only depend on the RSOC. This means that the Rashba effect plays a key role in realizing the DM interaction. The Ising term of the $z$ direction results from both the ISOC and the RSOC.[58] All the range functions $J_{i}^{\alpha \beta}$ of the RKKY interaction are listed in Table 1.
Table 1. The RKKY interaction range function including both of the same sublattices (AA) and the opposite sublattices (AB), where $\kappa{=}\frac{2\pi^{2}}{4\hbar^{2}v_{\rm F}^{2}\varOmega_{\rm BZ}}$, $\zeta_{\pm}{=}\sqrt {\varepsilon^{2}-\varDelta^{2}\pm2\left(\varepsilon-\varDelta \right) \lambda_{\rm R}}$, $\mathscr{J}{=}-\frac{\kappa^{2}J^{2}}{2\pi}$, $s (s^{\prime})=\mathrm{sgn} (\varepsilon\pm\lambda_{\rm R})$. ${\cal{H}}_{\nu}^{(1)}(z)$ is the Hankel function of the first kind in the order $\nu$.
AA AB
$J_{y}^{\rm AA}=\mathscr{J} {\rm Im}\int_{-\infty }^{\varepsilon_{\rm F}}{d}\varepsilon\left(-4{\it\Gamma}_{1}^{2}\right)$ $J_{y}^{\rm AB}=\mathscr{J}{\rm Im}\int_{-\infty}^{\varepsilon_{\rm F}}{d}\varepsilon(-4{\it\Lambda}_{2} {\it\Lambda}_{3})$
$J_{z}^{\rm AA}=\mathscr{J} {\rm Im}\int_{-\infty }^{\varepsilon_{\rm F}}{d}\varepsilon\left( -4{\it\Gamma}_{3}^{2}\right)$ $J_{z}^{\rm AB}=\mathscr{J} {\rm Im}\int_{-\infty}^{\varepsilon_{\rm F}} {d}\varepsilon\left({\it\Lambda}_{2}-{\it\Lambda}_{3} \right)^{2}$
$J_{\rm DM}^{\rm AA}=\mathscr{J} {\rm Im}\int_{-\infty }^{\varepsilon_{\rm F}}{d}\varepsilon(-4{\it\Gamma}_{1}{\it\Gamma}_{2})$ $J_{\rm DM}^{\rm AB}=\mathscr{J}{\rm Im}\int_{-\infty}^{\varepsilon_{\rm F}} {d}\varepsilon(-2){\it\Lambda}_{1}\left({\it\Lambda}_{2}+{\it\Lambda}_{3} \right)$
$J_{\rm H}^{\rm AA}=\mathscr{J} {\rm Im}\int_{-\infty}^{\varepsilon_{\rm F}}{d} \varepsilon 2\left( {\it\Gamma}_{1}^{2}-{\it\Gamma}_{2}^{2}+{\it\Gamma}_{3}^{2}\right)$ $J_{\rm H}^{\rm AB}=\mathscr{J} {\rm Im}\int_{-\infty}^{\varepsilon_{\rm F}}{d}\varepsilon2\left( {\it\Lambda}_{2} {\it\Lambda}_{3}-{\it\Lambda}_{1}^{2} \right)$
${\it\Gamma}_{1}=s\zeta_{+}{\cal{H}}_{1}^{\left( 1\right) }\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right) -s^{\prime}\zeta_{-}{\cal{H}}_{1}^{\left( 1\right) }\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $ ${\it\Lambda}_{1}=s\zeta_{+}{\cal{H}}_{1}^{\left( 1\right) }\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right) +s^{\prime}\zeta_{-}{\cal{H}}_{1}^{\left( 1\right) }\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $
${\it\Gamma}_{2}=\left( \varepsilon+\lambda_{\rm R}\right) {\cal{H}}_{0}^{\left( 1\right) }\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right) +\left( \varepsilon -\lambda_{\rm R}\right) {\cal{H}}_{0}^{\left( 1\right) }\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $ ${\it\Lambda}_{2}=-\left( \varepsilon-\varDelta \right) {\cal{H}}_{0}^{(1)}\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right) +\left( \varepsilon-\varDelta \right) {\cal{H}}_{0}^{(1)}\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $
${\it\Gamma}_{3}=\left( \varDelta+\lambda_{\rm R}\right) {\cal{H}}_{0}^{\left( 1\right) }\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right) +\left( \varDelta-\lambda _{\rm R}\right) {\cal{H}}_{0}^{\left( 1\right) }\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $ ${\it\Lambda}_{3} =\left( \varepsilon+\varDelta+2\lambda_{\rm R}\right) {\cal{H}}_{2}^{\left( 1\right) }\left( \tfrac{sR\zeta_{+}}{\hbar v_{\rm F}}\right)-\left( \varepsilon+\varDelta-2\lambda_{\rm R}\right){\cal{H}}_{2}^{\left( 1\right) }\left( \tfrac{s^{\prime}R\zeta_{-}}{\hbar v_{\rm F}}\right) $
The RKKY/BR Interaction. The well-preserved linear dispersion of graphene with the RSOC and ISOC is shown in Fig. 1(b), where the splitting energy of subbands is about $2\lambda_{\rm R}$. In our calculations we used the strength of $s$–$d$ interaction $J$ about $1\,\mathrm{eV}$,[51] the Fermi velocity $10^{6}$ m/s,[59] and the ISOC of graphene sheet ${\varDelta}=40\,µ$eV.[60] We only need to discuss the case of the same sublattices when we focus on the RKKY interaction in graphene on the Ni(111) or Co(0001) films, because there are one carbon atom of the graphene unit cell that locates on top of the adjacent Co(Ni) atom and another carbon atom that locates above the hollow site, as shown in Fig. 1(a). Generally speaking, the asymptotic behavior of RKKY range functions is determined by the dimensionality of the host materials.[61] In 2D electron gas or 2D materials, the range functions decay as $1/R^{2}$ with distance $R$. We can see from Fig. 2(a) that all the terms decay as $1/R^{2}$ and conform to other 2D systems. To compare the different terms in the RKKY interaction, we plot all the four types of the RKKY range functions depending on the distance $R$ or Fermi energy $\varepsilon_{\rm F}$ in Figs. 2(a) and 2(b). We can see that the Ising term of the $z$ direction is rather weak and relatively insensible to the increase of the distance between moments, and this is because the Ising term $J_{z}$ relies mainly on the ISOC and the strength of the ISOC is low. The other terms show decaying oscillations with increasing distance, as conventional RKKY range functions behave. Figure 2(b) shows the dependence of the four terms on Fermi energy. Again the Ising term of the $z$ direction shows a relatively flat curve with increasing Fermi energy, and the other range functions show normally enhanced oscillations with the increase of Fermi energy. While the Fermi energy is cross the neutral point and the density of state drops to zero, there are no carriers in the graphene sheet. The RKKY interaction seems to vanish due to the absence of the mediated carriers. However, the virtual excitations could also offer mediated carriers, and the RKKY interaction would turn to the BR interaction.[50,53] The BR interaction, in general, exponentially decays with increasing the distance between moments and preserves all the four spin-spin interaction terms. We can see from Fig. 2(c) the perfect exponential decaying behavior of the BR interaction. The Heisenberg term falls more rapidly than the other three terms. The intensity of the Heisenberg interaction will be lower than that of the DM interaction in the distance larger than $5.7\,\mathrm{nm}$. In comparison, the intensity of the Ising interaction of the $z$ direction will be higher than that of the DM interaction in the distance larger than $12.1\,\mathrm{nm}$. When the distance approaches zero, the relative strength of two Ising terms almost vanish. However, the Heisenberg term is dominant in this case. In Fig. 2(d), we plot the RSOC dependence of the different terms in the BR interaction. We can see that the DM term and the Ising terms monotonously increase with increasing RSOC, whereas the isotropic Heisenberg interaction decreases, indicating the anisotropy of the BR interaction also arises from the RSOC.
cpl-37-8-087501-fig2.png
Fig. 2. All the RKKY interaction range functions of the same sublattice versus the distance ${R}$ (a) and Fermi energy $\varepsilon_{\rm F}$ (b). (c) The BR interaction of the same sublattices depending on distance in the logarithmic coordinate. (d) The BR interaction of the same sublattices depending on RSOC in units of $\mathrm{meV}$. We set ${\varDelta}=40\,µ$eV for all cases, $\lambda_{\rm R}=50$ meV and $\varepsilon_{\rm F}=200$ meV for (a), $\lambda_{\rm R}=50$ meV and $R=8$ nm for (b), $\lambda_{\rm R}=50$ meV and $\varepsilon_{\rm F}=0$ meV for (c), $R=8$ nm, $\varepsilon_{\rm F}=0$ meV for (d).
The DM Interaction from the Intralayer RKKY/BR Interaction. Since the adjacent Co(Ni) atoms locate under the same sublattice of graphene with a distance of about 0.25 $\mathrm{nm}$,[62,63] we turn our attention to the case of $R=0.25$ nm. We can see from Fig. 3(a) that the DM term significantly depends on the RSOC, while the other three terms show insensible dependence. At the nearest distance, the isotropic Heisenberg term makes the major contribution. However, we do not care about the isotropic Heisenberg interaction which offers a usual ferromagnetic exchange interaction. We are interested in the DM interaction arising from the BR or RKKY interaction. Since the parameters of RSOC for the Co film $\lambda_R=265$ meV and for the Ni film $\lambda_R=136$ meV,[20] we can calculate the corresponding DM interaction $J_{\rm DM}=0.133$ meV for graphene/Co and $J_{\rm DM}=0.069$ meV for graphene/Ni from the BR interaction. We compare our estimate of the DM interaction with the experimental result $J_{\rm DM}=0.16\pm0.05$ meV of the graphene/Co film,[41] and the theoretical estimate is perfectly consistent with the experimental result. This coincidence indicates that the DM interaction may not be induced by the Rashba effect directly but may be induced by the Rashba effect indirectly via the BR interaction. Figure 3(b) shows that the RKKY interaction is nearly independent of Fermi energy. The RKKY interaction will be almost the same as the BR interaction even if the Fermi energy drastically increases. The corresponding DM terms from the RKKY interaction ($\varepsilon_{\rm F}=200$ meV) can be extracted as $J_{\rm DM}=0.134$ meV for graphene/Co and $J_{\rm DM}=0.069$ meV for graphene/Ni, which are almost the same as the DM interaction from the BR interaction. One reason for the inert characteristic lies in the fact that the propagating modes of the mediated carriers reduce within the nearest distance and the mediated carriers involved nearly saturate. The other reason is that the distance is too short to accumulate the angle of spin twisting and the phase changing of the itinerant carriers. How can we identify the DM interaction from the intralayer RKKY/BR interaction or from the Rashba effect directly? Since the DM interaction from the intralayer BR/RKKY interaction is always along with a Heisenberg term, we can decide theoretically both the energies of the DM term $J_{\rm DM}$ and the ferromagnetic Heisenberg term $J_{\rm H}$. If we could extract the $J_{\rm DM}$ and $J_{\rm H}$ from asymmetric spin-wave dispersion by measuring the highly resolved spin-polarized electron energy loss spectra,[64] we may verify our conclusion by comparing the theoretical value and the experimental result of the $J_{\rm DM}/J_{\rm H}$.
cpl-37-8-087501-fig3.png
Fig. 3. (a) The range functions of the BR interaction of the same sublattices depending on RSOC in units of $\mathrm{meV}$ with Fermi energy $\varepsilon_{\rm F}=0$ meV. (b) The range functions of the RKKY interaction of the same sublattices depending on Fermi energy with RSOC $\lambda_R=50$ meV. $\varDelta=40$ µeV, $R=0.25$ nm are both for (a) and (b).
In summary, we have studied the long-range RKKY interaction (the short-range BR interaction) mediated by itinerant carriers (virtual excitations) in graphene between magnetic moments induced by proximity effect with a ferromagnetic film. Thanks to the giant RSOC of the graphene-ferromagnet interface, the RKKY/BR interaction consists of the Heisenberg, DM, and Ising terms. Since the adjacent atoms from a ferromagnetic substrate locate under the same sublattice of graphene, we focus on the RKKY/BR interaction on the same sublattice and find that the DM term and the Heisenberg term make the main contribution. While in the case of the nearest distance, we show the RKKY interaction that is nearly independent of the Fermi energy and is almost the same as the BR interaction. The Heisenberg and the Ising terms are also insensible to the RSOC except for the DM term. We estimate the DM term from the BR/RKKY interaction is about $0.13$ meV for the graphene/Co interface, which is consistent with the experimental result of DM interaction $0.16\pm0.05$ meV. This result indicates that the DM interaction may not be induced by the Rashba effect directly but may be induced by the Rashba effect indirectly via the intralayer BR/RKKY interaction.
References Defect-induced magnetism in grapheneRoom-temperature ferromagnetism in graphite driven by two-dimensional networks of point defectsMissing Atom as a Source of Carbon MagnetismLocalized Magnetic States in GrapheneDual origin of defect magnetism in graphene and its reversible switching by molecular dopingAtomic-scale control of graphene magnetism by using hydrogen atomsMagnetic impurities in grapheneTunable Magnetism and Half-Metallicity in Hole-Doped Monolayer GaSeRoom-Temperature Ferromagnetism of GrapheneLimits on Intrinsic Magnetism in GrapheneSpin-half paramagnetism in graphene induced by point defectsHalf-metallic graphene nanoribbonsMagnetic Correlations at Graphene Edges: Basis for Novel Spintronics DevicesRoom-temperature magnetic order on zigzag edges of narrow graphene nanoribbonsFermi liquid theory of a Fermi ringLow-Density Ferromagnetism in Biased Bilayer GrapheneProximity-Induced Ferromagnetism in Graphene Revealed by the Anomalous Hall EffectStrong interfacial exchange field in the graphene/EuS heterostructureRashba Effect in the Graphene/Ni(111) SystemProximity-induced exchange and spin-orbit effects in graphene on Ni and CoIndirect Exchange Coupling of Nuclear Magnetic Moments by Conduction ElectronsA Theory of Metallic Ferro- and Antiferromagnetism on Zener's ModelMagnetic Properties of Cu-Mn AlloysDiluted Graphene AntiferromagnetRKKY in half-filled bipartite lattices: Graphene as an exampleRKKY interaction in grapheneRKKY interaction in graphene from the lattice Green’s functionFocusing RKKY interaction by graphene P–N junctionRKKY coupling in grapheneMagnetic Domain-Wall Racetrack MemorySkyrmions on the trackThickness dependence of the interfacial Dzyaloshinskii–Moriya interaction in inversion symmetry broken systemsA thermodynamic theory of “weak” ferromagnetism of antiferromagneticsAnisotropic Superexchange Interaction and Weak FerromagnetismRole of the Dzyaloshinskii-Moriya interaction in multiferroic perovskitesMeasuring the Dzyaloshinskii–Moriya interaction in a weak ferromagnetAsymmetric magnetic domain-wall motion by the Dzyaloshinskii-Moriya interactionDirect Observation of the Dzyaloshinskii-Moriya Interaction in a Pt/Co/Ni FilmAnatomy of Dzyaloshinskii-Moriya Interaction at Co / Pt InterfacesLinear relation between Heisenberg exchange and interfacial Dzyaloshinskii–Moriya interaction in metal filmsSignificant Dzyaloshinskii–Moriya interaction at graphene–ferromagnet interfaces due to the Rashba effectReversible control of Dzyaloshinskii-Moriya interaction at the graphene/Co interface via hydrogen absorptionInterface-Induced Topological Insulator Transition in GaAs / Ge / GaAs Quantum WellsPolarization-Driven Topological Insulator Transition in a GaN / InN / GaN Quantum WellSpin splitting of Dirac fermions in aligned and rotated graphene on Ir(111)Is There a Rashba Effect in Graphene on 3 d Ferromagnets?Giant Rashba splitting in graphene due to hybridization with goldRole of Anisotropic Exchange Interactions in Determining the Properties of Spin-GlassesInterlayer Dzyaloshinskii-Moriya InteractionsNuclear Spin Exchange in Solids: Tl 203 and Tl 205 Magnetic Resonance in Thallium and Thallic OxideExchange interaction of magnetic impurities in grapheneIntrinsic and Rashba spin-orbit interactions in graphene sheetsElectrically Controllable Surface Magnetism on the Surface of Topological InsulatorsIndirect magnetic interaction mediated by Fermi arc and boundary reflection near Weyl semimetal surfaceRKKY interaction of magnetic impurities in Dirac and Weyl semimetalsRuderman-Kittel-Kasuya-Yosida interaction in Weyl semimetalsRKKY interaction and intervalley processes in p -doped transition-metal dichalcogenides SU ( 2 ) non-Abelian holonomy and dissipationless spin current in semiconductorsCyclotron resonance study of the electron and hole velocity in graphene monolayersResonance Microwave Measurements of an Intrinsic Spin-Orbit Coupling Gap in Graphene: A Possible Indication of a Topological StateHidden quantum mirage by negative refraction in semiconductor P-N junctionsStructure and Electronic Properties of Graphene Nanoislands on Co(0001)Graphene-protected iron layer on Ni(111)Asymmetric Spin-Wave Dispersion on Fe(110): Direct Evidence of the Dzyaloshinskii-Moriya Interaction
[1] Yazyev O V and Helm L 2007 Phys. Rev. B 75 125408
[2] Cervenka J, Katsnelson M I and Flipse C F J 2009 Nat. Phys. 5 840
[3] Ugeda M M, Brihuega I, Guinea F and Gómez-Rodríguez J M 2010 Phys. Rev. Lett. 104 096804
[4] Uchoa B, Kotov V N, Peres N M R and Castro Neto A H 2008 Phys. Rev. Lett. 101 026805
[5] Nair R R, Tsai I L, Sepioni M, Lehtinen O, Keinonen J, Krasheninnikov A V, Castro Neto A H, Katsnelson M I, Geim A K and Grigorieva I V 2013 Nat. Commun. 4 2010
[6] González-Herrero H, Gómez-Rodrı́guez J M, Mallet P, Moaied M, Palacios J J, Salgado C, Ugeda M M, Veuillen J Y, Yndurain F and Brihuega I 2016 Science 352 437
[7] Hu F M, Ma T, Lin H Q and Gubernatis J E 2011 Phys. Rev. B 84 075414
[8] Cao T, Li Z and Louie S G 2015 Phys. Rev. Lett. 114 236602
[9] Wang Y, Huang Y, Song Y, Zhang X Y, Ma Y F, Liang J J and Chen Y S 2009 Nano Lett. 9 220
[10] Sepioni M, Nair R R, Rablen S, Narayanan J, Tuna F, Winpenny R, Geim A K and Grigorieva I V 2010 Phys. Rev. Lett. 105 207205
[11] Nair R R, Sepioni M, Tsai I L, Lehtinen O, Keinonen J, Krasheninnikov A V, Thomson T, Geim A K and Grigorieva I V 2012 Nat. Phys. 8 199
[12] Son Y W, Cohen M L and Louie S G 2006 Nature 444 347
[13] Yazyev O V and Katsnelson M I 2008 Phys. Rev. Lett. 100 047209
[14] Magda G Z, Jin X Z, Hagymási I et al. 2014 Nature 514 608
[15] Stauber T, Peres N M R, Guinea F and Castro Neto A H 2007 Phys. Rev. B 75 115425
[16] Castro E V, Peres N M R, Stauber T and Silva N A P 2008 Phys. Rev. Lett. 100 186803
[17] Wang Z, Tang C, Sachs R, Barlas Y and Shi J 2015 Phys. Rev. Lett. 114 016603
[18] Wei P, Lee S, Lemaitre F, Pinel L, Cutaia D, Cha W, Katmis F, Zhu Y, Heiman D, Hone J, Moodera J S and Chen C T 2016 Nat. Mater. 15 711
[19] Dedkov Y S, Fonin M, Rudiger U and Laubschat C 2008 Phys. Rev. Lett. 100 107602
[20] Peralta M, Medina E and Mireles F 2019 Phys. Rev. B 99 195452
[21] Ruderman M A and Kittel C 1954 Phys. Rev. 96 99
[22] Kasuya T 1956 Prog. Theor. Phys. 16 45
[23] Yosida K 1957 Phys. Rev. 106 893
[24] Brey L, Fertig H A and Das Sarma S 2007 Phys. Rev. Lett. 99 116802
[25] Saremi S 2007 Phys. Rev. B 76 184430
[26] Kogan E 2011 Phys. Rev. B 84 115119
[27] Sherafati M and Satpathy S 2011 Phys. Rev. B 83 165425
[28] Zhang S H, Zhu J J, Yang W and Chang K 2017 2D Mater. 4 035005
[29] Black-Schaffer A M 2010 Phys. Rev. B 81 205416
[30] Parkin S S P, Hayashi M and Thomas L 2008 Science 320 190
[31] Fert A, Cros V and Sampaio J 2013 Nat. Nanotechnol. 8 152
[32] Cho J, Kim N H, Lee S, Kim J S, Lavrijsen R, Solignac A, Yin Y, Han D S, van Hoof N J J, Swagten H J M, Koopmans B and You C Y 2015 Nat. Commun. 6 7635
[33] Dzyaloshinsky I 1958 J. Phys. Chem. Solids 4 241
[34] Moriya T 1960 Phys. Rev. 120 91
[35] Sergienko I A and Dagotto E 2006 Phys. Rev. B 73 094434
[36] Dmitrienko V E, Ovchinnikova E N, Collins S P, Nisbet G, Beutier G, Kvashnin Y O, Mazurenko V V, Lichtenstein A I and Katsnelson M I 2014 Nat. Phys. 10 202
[37] Je S G, Kim D H, Yoo S C, Min B C, Lee K J and Choe S B 2013 Phys. Rev. B 88 214401
[38] Di K, Zhang V L, Lim H S, Ng S C, Kuok M H, Yu J, Yoon J, Qiu X and Yang H 2015 Phys. Rev. Lett. 114 047201
[39] Yang H, Thiaville A, Rohart S, Fert A and Chshiev M 2015 Phys. Rev. Lett. 115 267210
[40] Nembach H T, Shaw J M, Weiler M, Jue E and Silva T J 2015 Nat. Phys. 11 825
[41] Yang H X, Chen G, Cotta A A C, N'Diaye A T, Nikolaev S A, Soares E A, Macedo W A A, Liu K, Schmid A K, Fert A and Chshiev M 2018 Nat. Mater. 17 605
[42] Yang B, Cui Q, Liang J, Chshiev M and Yang H 2020 Phys. Rev. B 101 014406
[43] Zhang D, Lou W, Miao M, Zhang S C and Chang K 2013 Phys. Rev. Lett. 111 156402
[44] Miao M S, Yan Q, Van de Walle C G, Lou W K, Li L L and Chang K 2012 Phys. Rev. Lett. 109 186803
[45] Marchenko D, Sánchez-Barriga J, Scholz M R, Rader O and Varykhalov A 2013 Phys. Rev. B 87 115426
[46] Rader O, Varykhalov A, Sánchez-Barriga J, Marchenko D, Rybkin A and Shikin A M 2009 Phys. Rev. Lett. 102 057602
[47] Marchenko D, Varykhalov A, Scholz M R, Bihlmayer G, Rashba E I, Rybkin A, Shikin A M and Rader O 2012 Nat. Commun. 3 1232
[48] Fert A and Levy P M 1980 Phys. Rev. Lett. 44 1538
[49] Vedmedenko E Y, Riego P, Arregi J A and Berger A 2019 Phys. Rev. Lett. 122 257202
[50] Bloembergen N and Rowland T J 1955 Phys. Rev. 97 1679
[51] Dugaev V K, Litvinov V I and Barnas J 2006 Phys. Rev. B 74 224438
[52] Min H, Hill J E, Sinitsyn N A, Sahu B R, Kleinman L and MacDonald A H 2006 Phys. Rev. B 74 165310
[53] Zhu J J, Yao D X, Zhang S C and Chang K 2011 Phys. Rev. Lett. 106 097201
[54] Duan H J, Zheng S H, Fu P H, Wang R Q, Liu J F, Wang G H and Yang M 2018 New J. Phys. 20 103008
[55] Chang H R, Zhou J, Wang S X, Shan W Y and Xiao D 2015 Phys. Rev. B 92 241103
[56] Hosseini M V and Askari M 2015 Phys. Rev. B 92 224435
[57] Mastrogiuseppe D, Sandler N and Ulloa S E 2014 Phys. Rev. B 90 161403
[58] Murakami S, Nagosa N and Zhang S C 2004 Phys. Rev. B 69 235206
[59] Deacon R S, Chuang K C, Nicholas R J, Novoselov K S and Geim A K 2007 Phys. Rev. B 76 081406
[60] Sichau J, Prada M, Anlauf T, Lyon T J, Bosnjak B, Tiemann L and Blick R H 2019 Phys. Rev. Lett. 122 046403
[61] Zhang S H, Zhu J J, Yang W, Lin H Q and Chang K 2016 Phys. Rev. B 94 085408
[62] Eom D, Prezzi D, Rim K T, Zhou H, Lefenfeld M, Xiao S, Nuckolls C, Hybertsen M S, Heinz T F and Flynn G W 2009 Nano Lett. 9 2844
[63] Dedkov Y S, Fonin M, Rudiger U and Laubschat C 2008 Appl. Phys. Lett. 93 022509
[64] Zakeri K, Zhang Y, Prokop J, Chuang T H, Sakr N, Tang W X and Kirschner J 2010 Phys. Rev. Lett. 104 137203