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Quantum magnetism of topologically-designed graphene nanoribbons

Xingchuan Zhu1    Huaiming Guo2 hmguo@buaa.edu.cn    Shiping Feng1 1Department of Physics, Beijing Normal University, Beijing, 100875, China 2Department of Physics, Key Laboratory of Micro-Nano Measurement-Manipulation and Physics (Ministry of Education), Beihang University, Beijing, 100191, China
Abstract

Based on the Hubbard models, quantum magnetism of topologically-designed graphene nanoribbons (GNRs) is studied using exact numerical simulations. We first study a two-band Hubbard model describing the low-energy topological bands using density matrix renormalization group (DMRG) and determinant quantum Monte Carlo (DQMC) methods. It is found the spin correlations decay quickly with the distance, and the local moment is extrapolated to zero in the presence of symmetry-breaking terms. The results show that the two-band Hubbard chain is nonmagnetic, which is in contrast to the mean-field calculation predicting a critical interaction for the magnetic transition. We then include the Hubbard interaction to the topological-designed GNRs. For large interactions, the spin correlations keep finite for all distances, and the magnetic order develops. The local moment is extrapolated to almost zero for weak interactions, and begins to increase rapidly from a critical interaction. The estimated critical value is much larger than the realistic value in graphene, and we conclude the experimentally relevant GNRs is nonmagnetic, which is consistent with the experimental results.

pacs:
71.10.Fd, 03.65.Vf, 71.10.-w,

.1 Introduction

Graphene nanoribbon (GNR) is a planer strip of graphene with extraordinary electronic and physical propertiesYazyev (2010); Son et al. (2006a); Yazyev (2013). It is first introduced as a theoretical model to study the size effect in grapheneNakada et al. (1996). Recent advance in bottom-up techniques have allowed production of atomically precise GNRs with armchair, zigzag and other sophistated edgesKimouche et al. (2015); Ruffieux et al. (2016). GNRs have potential applications in the next-generation nanoelectronics, and have been extensively investigated.

GNRs exhibit electronic properties that are not present in grapheneRuffieux et al. (2016). In the simplest form, the edges can be either armchair or zigzag. Tight binding calculations predict that zigzag GNRs are always metallic, while armchair ones can be insulating or metallic. The graphene features two inequivalent Dirac points, which are characterized by ±π\pm\pi Berry phasesCastro Neto et al. (2009). In the presence of zigzag edges, the two Dirac points are projected to different momenta of the one-dimensional (1D) Brillouin zone, and flat bands connecting them appear. The low-energy states on the flat bands are localized at the edge. The large density of states at the Fermi energy is sensitive to the electron-electron interactions, and the nanoribbon has an instability to magnetic ordering. Remarkable edge magnetism develops in the weak-coupling regime U/t<2U/t<2, where bulk magnetic order is absentSorella and Tosatti (1992); Paiva et al. (2005); Meng et al. (2010); Sorella et al. (2012). The magnetic moments form long-ranged ferromagnetic order along the zigzag edge while they are antialigned at the opposite edgeFeldner et al. (2011); Hikihara et al. (2003); Feldner et al. (2010); Luitz et al. (2011); Schmidt and Loss (2010); Golor et al. (2013); Hagymási and Legeza (2016). The opposite spin polarization along the zigzag edges opens a band gap, and the system becomes a semiconductor. Recent experiments provide direct evidence of the edge magnetismJoly et al. (2010); Magda et al. (2014). In particular, it is found that the magnetic order on zigzag edges can be stable even at room temperatureMagda et al. (2014).

The gap values of the armchair GNRs depend on width. When the number of dimer lines across the ribbon is N=3p+2N=3p+2 with pp a positive integer, the armchair GNRs are metallic. Otherwise, they are insulating with the gaps inversely proportional to the widthsSon et al. (2006b); Brey and Fertig (2006); Ezawa (2006). Recently, the topological properties of the insulating armchair GNRs are investigated, which demonstrates that different widths and end terminations lead to distinct topological phasesCao et al. (2017); Lin and Chou (2018). The topology is characterized by a 2\mathbb{Z}_{2} invariant, and is manifested by localized boundary state between two segments with different topologies. Later experiments confirming the predictions are reportedGroning et al. (2018); Rizzo et al. (2018). Furthermore, the junction states are successfully used as building block to engineer the famous Su-Schrieff-Heeger topological modelGroning et al. (2018); Rizzo et al. (2018); Su et al. (1979).

The armchair GNRs have no edge states, and the critical interaction to antiferromagnetism is similar to that of bulk graphene. In the topologically-designed GNRs, there are zigzag-edge segments at the boundary, which suggests the possibility of magnetic ordering at weak interactions. While the mean-field (MF) calculation finds a critical interaction smaller than that of bulk system (Uc=2.23tU_{c}=2.23t)Sorella and Tosatti (1992), it is still larger than the realistic value in graphene, and supports that the experimentally realized structures are nonmagnetic. Since the quantum fluctuation is strong in two dimensions, it is very necessary to perform an exact numerical study of the effect of interactions, and validate the absence of the magnetism.

In the manuscript, we study quantum magnetism of topologically-designed GNRs based on the Hubbard models using exact numerical simulations. We first derive a two-band model for the low-energy topological bands, and study the corresponding 1D Hubbard model using DMRG and DQMC methods. It is found the spin correlations decay quickly with the distance, and the local moment is extrapolated to zero in the presence of symmetry-breaking terms. The results show that the two-band Hubbard chain is nonmagnetic. We then include the Hubbard interaction to the topological-designed GNRs, and calculate the spin correlations and the local moments in the presence of symmetry-breaking terms. We find the magnetic order develops from a critical interaction, which is much larger than the realistic value in graphene. We conclude the experimentally relevant GNRs is nonmagnetic, which is consistent with the experimental results.

Refer to caption
Figure 1: (a) Schematic structure of a pristine 7-AGNR. (b) The geometry of a topologically-designed GNR based on the pristine 7-AGNR. In (a) the pristine 7-AGNR with a zigzag termination is a 1D topological insulator, and the wavefunction of the zero boundary mode is plotted (red filled circles with the radius denoting the wavefunction amplitude). In (b) we also show the wavefunction of the designed topological band, which is mainly distributed on the two outmost sites of each zigzag shoulder. The unit cell is enclosed by green dashed lines, which have 14(48)14(48) sites in (a)[(b)].

.2 The model and method

We consider a nearest-neighbor (NN) tight-binding Hamiltonian on a topologically-designed GNR with the geometry shown in Fig. 1,

H0=ljσtcjσclσ,H_{0}=-\sum_{\langle lj\rangle\sigma}tc^{\dagger}_{j\sigma}c^{\phantom{{\dagger}}}_{l\sigma}, (1)

where cjσc_{j\sigma} and cjσc^{{\dagger}}_{j\sigma} are the annihilation and creation operators at site jj with spin σ=,\sigma=\uparrow,\downarrow. The hopping amplitudes between the NN sites ll and jj are tt, which is about 3eV3~{}eV in graphene.

The geometry in Fig. 1(b) is obtained by adding small segments with zigzag edges periodically on the pristine armchair GNR with the width N=7N=7 (77-AGNR). The resulting geometry is a superlattice of alternating unit cells of 77-AGNR and 99-AGNR. The topological property of the 7(9)7(9)-AGNR composed of such unit cells [see shaded region in Fig. 1(b)] is described by a Z2Z_{2} invariant: Z2=1±(1)W3+W+122Z_{2}=\frac{1\pm(-1)^{\lfloor\frac{W}{3}\rfloor+\lfloor\frac{W+1}{2}\rfloor}}{2}, where x\lfloor x\rfloor is the floor function and the sign is negative (positive) for W=7(9)W=7(9)Cao et al. (2017). The Z2Z_{2} value is 0(1)0(1) for 7(9)7(9)-AGNR, and the topological and trivial unit cells alternate along the chain. Thus the localized boundary states between adjacent unit cells may form low-energy dispersing bands in the gap.

Performing Fourier transformation, the Hamiltonian in Eq.(1) becomes H0=𝐤ψ𝐤(𝐤)ψ𝐤H_{0}=\sum_{\bf k}\psi^{\dagger}_{\bf k}{\cal H}({\bf k})\psi_{\bf k}, where the basis is ψ𝐤=(c1,𝐤,c2,𝐤,,cNs,𝐤)T\psi_{\bf k}=(c_{1,{\bf k}},c_{2,{\bf k}},...,c_{N_{s},{\bf k}})^{T} (NsN_{s} is the number of sites in a unit cell), and (𝐤){\cal H}({\bf k}) is the NsN_{s}-by-NsN_{s} Hamiltonian matrix in the momentum space. By diagonalizing (𝐤){\cal H}({\bf k}), the band structures are directly obtained, and are shown in Fig. 2. Figure 2(a) shows the band structure of the pristine 77-AGNR for comparison, which has been known to be a semiconductor with the gap size about 0.5t0.5t. By including small segments, two new dispersing bands appear in the gap[see Fig. 2(b)], and their wave functions mainly distribute on the zigzag sites of the small segments.

Since the two low-energy bands in Fig. 2(b) are isolated from other bands, an effective model for them can be constructed using maximally localized Wannier functionsMarzari et al. (2012), which is a 1D chain containing hoppings of different ranges. The main contribution is from the NN ones, and the corresponding hopping amplitudes are t1=0.1493tt_{1}=0.1493t and t2=0.1824tt_{2}=-0.1824t, respectively. It is found that the low-energy two bands are fitted quite well only using the above NN hoppings (see Fig. 2). Thus the designed GNR realizes an effective 1D tight-binding model analog to the famous Su-Schrieffer-Heeger one.

Refer to caption
Figure 2: The band structures for (a) the pristine 7-AGNR, and (b) the topologically-designed GNR based on the pristine 7-AGNR. In (b), the two bands near the Fermi energy are well fitted using a 1D chain with alternating hopping amplitudes t1=0.1493tt_{1}=0.1493t and t2=0.1824tt_{2}=-0.1824t (orange open circles).

It has been known that the pristine 77-AGNR supports a topological phase. The topological invariant depends on the shape of its termination, and the zigzag termination yields a nontrivial topological invariant. It is also desirable to know the topological class of the above topologically-designed GNR. The 1D topological property is characterized by the Berry phaseGuo and Shen (2011); Guo et al. (2012); Wang and Zhang (2014); Resta (1994); Xiao et al. (2010),

γ=iψk|ddk|ψk𝑑k,\displaystyle\gamma=i\oint\langle\psi_{k}|\frac{d}{dk}|\psi_{k}\rangle dk, (2)

where kk varying from 0 to 2π2\pi is the wave vector, and ψk\psi_{k} is the periodic part of the Bloch wave function corresponding to kk. The Berry phase of the Hamiltonian Eq.(1) on the geometry shown in Fig. 2 has a nontrivial value π\pi, corresponding to which a pair of zero boundary modes appear under open boundary condition.

To study the magnetic property of the topologically-designed GNR, we consider the Hubbard interaction, which writes as,

HU=iU(ni12)(ni12),H_{U}=\sum_{i}U(n_{i\uparrow}-\frac{1}{2})(n_{i\downarrow}-\frac{1}{2}), (3)

where niσ=ciσciσn_{i\sigma}=c^{\dagger}_{i\sigma}c_{i\sigma} is the number operator of fermion and UU is the strength of the on-site interaction. In the following discussions, we include the Hubbard term into both the Hamiltonian in Eq.(1) and the two-band effective model, and study the induced magnetism.

The interacting Hamiltonian is solved numerically by means of the DQMC and DMRG methodsWhite et al. (1989); Hirsch (1985); White (1992). In the DQMC approach, one decouples the on-site interaction term through the introduction of an auxiliary Hubbard-Stratonovich field (HSF). The fermions are integrated out analytically, and then the integral over the HSF is performed stochastically. The only errors are those associated with the statistical sampling, the finite spatial lattice and inverse temperature discretization. All are well-controlled in the sense that they can be systematically reduced as needed, and further eliminated by appropriate extrapolations. The DMRG method is most efficient for the ground state of 1D systemsBauer et al. (2011). We use it to solve the effective model directly at zero temperature. In the following calculations, we focus on half-filled bands, when the DQMC method is free of the infamous ‘minus-sign problem’.

To study the magnetic behavior, we measure the local moment mjz=Sjzm^{z}_{j}=\langle S^{z}_{j}\rangle with Sjz=12(njnj)S^{z}_{j}=\frac{1}{2}(n_{j\uparrow}-n_{j\downarrow}). Since the original Hamiltonian preserves the SU(2)SU(2) symmetry, a symmetry-breaking term should be included to induce the magnetism. We break the symmetry of the magnetic phase to zz-axis by adding an alternating Zeeman term HB=jBj(njnj)H_{B}=\sum_{j}B_{j}(n_{j\uparrow}-n_{j\downarrow}) with Bj=±BB_{j}=\pm B depending on the sublattices. The value of the local moment is extrapolated to the limit B=0B=0, and a nonzero value marks the existence of the magnetism. The equal-time spin correlation function is also calculated, which is given by

cspin(𝐢)=S𝐣+𝐢zS𝐣z+12(S𝐣+𝐢+S𝐣+S𝐣+𝐢S𝐣+),c_{spin}({\bf i})=\langle S^{z}_{{\bf j+i}}S^{z}_{{\bf j}}+\frac{1}{2}(S^{+}_{{\bf j+i}}S^{-}_{{\bf j}}+S^{-}_{{\bf j+i}}S^{+}_{{\bf j}})\rangle, (4)

where the spin raising and lowing operators are S𝐣+=c𝐣c𝐣,S𝐣=c𝐣c𝐣S^{+}_{\bf j}=c^{\dagger}_{\bf j\uparrow}c_{\bf j\downarrow},S^{-}_{\bf j}=c^{\dagger}_{\bf j\downarrow}c_{\bf j\uparrow}, respectively.

I Magnetism of the effective model for the topologically-designed GNRs

We first study the magnetic property based on the effective two-band Hubbard model, which writes as,

Heff=jσ(tjcjσcj+1σ+H.c.)+HU,H_{eff}=-\sum_{j\sigma}(t_{j}c^{\dagger}_{j\sigma}c^{\phantom{{\dagger}}}_{j+1\sigma}+H.c.)+H_{U}, (5)

where tj=t1(t2)t_{j}=t_{1}(t_{2}) for jj in A(B)A(B) sublattice. It is helpful to perform a MF analysis. In the MF approximation, the interaction term in Eq.(5) is decoupled as,

nini=nini+nininini.n_{i\uparrow}n_{i\downarrow}=\langle n_{i\downarrow}\rangle n_{i\uparrow}+\langle n_{i\uparrow}\rangle n_{i\downarrow}-\langle n_{i\downarrow}\rangle\langle n_{i\uparrow}\rangle. (6)

To incorporate an antiferromagnetism order, we write

ni,A=12+mA,ni,A=12mA\displaystyle\langle n_{i\uparrow,A}\rangle=\frac{1}{2}+m_{A},\langle n_{i\downarrow,A}\rangle=\frac{1}{2}-m_{A} (7)
ni,B=12mB,ni,B=12+mB.\displaystyle\langle n_{i\uparrow,B}\rangle=\frac{1}{2}-m_{B},\langle n_{i\downarrow,B}\rangle=\frac{1}{2}+m_{B}.

Then the Hubbard term becomes,

Uinini=E0+\displaystyle U\sum_{i}n_{i\uparrow}n_{i\downarrow}=E_{0}+ (8)
iA(mAni+mAni)+iB(mBnimBni),\displaystyle\sum_{i\in A}(-m_{A}n_{i\uparrow}+m_{A}n_{i\downarrow})+\sum_{i\in B}(m_{B}n_{i\uparrow}-m_{B}n_{i\downarrow}),

where E0=14NU+NU2(mA2+mB2)E_{0}=\frac{1}{4}NU+\frac{NU}{2}(m^{2}_{A}+m^{2}_{B}) (NN is the total number of the sites). The MF Hamiltonian writes as,

mfσ(k)=\displaystyle{\cal H}^{\sigma}_{mf}({k})= (σmAt1+t2eikt1+t2eik±σmB)\displaystyle\left(\begin{array}[]{cc}\mp\sigma m_{A}&t_{1}+t_{2}e^{-ik}\\ t_{1}+t_{2}e^{ik}&\pm\sigma m_{B}\end{array}\right) (11)

where σ=1(1)\sigma=1(-1) represents up (down) spin. For a uniform antiferromagnetic order, we suppose mA=mB=mm_{A}=m_{B}=m. The energy spectrum is directly obtained by diagonalizing the above Hamiltonian, which is ±Ek\pm E_{k} with Ek=(Um)2+(t2sink)2+(t1+t2cosk)2E_{k}=\sqrt{(Um)^{2}+(t_{2}\sin k)^{2}+(t_{1}+t_{2}\cos k)^{2}} (the dispersion is degenerate for both spin copies). Minimizing the free energy F=2kEk+E0F=-2\sum_{k}E_{k}+E_{0}, the self-consistent equation for the order parameter mm is 1=UNk1Ek1=\frac{U}{N}\sum_{k}\frac{1}{E_{k}}.

Figure 3 shows the self-consistent order parameter as a function of UU. The value of the order parameter mm is zero for small interactions and the 1D chain is nonmagnetic. From a critical interaction, we have a finite self-consistent solution for mm, implying the magnetism develops in the system. As UU is increased, mm also increases and the magnetism is strengthened. As shown in Fig.3, the curve dmdU\frac{dm}{dU} tends to be divergent at the critical interaction, from which we get Uc=0.29tU_{c}=0.29t.

Refer to caption
Figure 3: The MF order parameter mm as a function of UU based on: (a) the effective topological bands; (b) the topologically-designed GNR. Differentiating mm with respect to UU, we have the critical interaction (a) Uc=0.29tU_{c}=0.29t and (b) Uc=1.66tU_{c}=1.66t.

While the MF study provides a qualitative understanding of the magnetic behavior, the quantum fluctuation is strong in 1D, and the MF approximation may be not accurate. So we next perform exact numerical simulations on the Hubbard model in Eq.(5). The equal-time spin correlation function of the ground state is calculated using DMRG, and the result at U=4tU=4t is shown in Fig. 4. The spin correlations decay with the distance, and the signs of their values are alternating, implying the correlations are antiferromagnetic. In log plot, the curve for each sublattice slightly deviates from a straight line, suggesting that the decay is slightly slower than an exponential law. It has been known that the antiferromagnetic correlation is critical for a homogeneous Hubbard chainPaiva and dos Santos (2000). The difference may be due to the 1D chain with alternating hopping amplitudes has a gapped spectrum. The spin correlations at finite temperatures are also obtained using DQMC. In Fig. 5, we plot the spin correlation between the NN sites as a function of temperature. It shows that the curves become saturated at low temperatures, and the values steadily tend to those obtained with DMRG at zero temperature. The consistence further validates the accuracies of both methods. As the interactions are strengthened, the spin correlations also increase.

Refer to caption
Figure 4: The equal-time spin correlation as a function of distance at U=4tU=4t. Insets are the log plots for the left (b) and right (c) parts. The 1D lattice has 4040 sites.
Refer to caption
Figure 5: The equal-time spin correlation function between the NN sites connected by the bonds with the hopping amplitude (a) t1t_{1} and (b) t2t_{2}. The lattice size is the same as that of Fig. 4.

Next we study the spontaneous-symmetry-breaking magnetism. Figure 6 (a) shows the local moment as a function of temperature under a small symmetry-breaking term B=0.1B=0.1. When the temperature is lowered, the thermal fluctuation is reduced and the local moment increases. Near the lowest temperatures T=0.05T=0.05, accessed by our DQMC simulations, the value of mm begins to be saturated. The saturated values are in good agreement with those from the DMRG method. It is noted that the case of U=0U=0 also becomes a magnet with m0.1m\sim 0.1, which is a natural result of the inclusion of a staggered Zeeman term. An extrapolation to B=0B=0 is necessary to know the intrinsic magnetic property of the system. We carry out DMRG simulations with several different BB and the data are shown in Fig. 6(b). They are well fitted using y=a(1ebx)y=a(1-e^{-bx}), a function exponentially rising to maximum. So as large as U=4tU=4t, the extrapolated local moment is zero, and the long-ranged antiferromagnetic order is absent in a strictly 1D system. It is in great contrast to the MF theory, where the antiferromagnetism develops above a critical interaction through a first-order phase transition.

Refer to caption
Figure 6: (a) The local moment mm as a function of temperature for several values of UU. The pinning Zeeman field is along the zz-axis with the strength B=0.1B=0.1. (b) The local moment mm as a function of BB. Solid curves are from the fitting function y=a(1ebx)y=a(1-e^{-bx}). Open (solid) symbols in both figures represent DQMC (DMRG) results. The lattice size is the same as that of Fig. 4.

II Magnetism of topologically-designed GNRs

Next we study the experimentally relevant topological-designed GNRs, which usually contain several unit cells. We first perform a MF analysis, and decouple the Hubbard term in the same channel described in Eq. (8),

nini=nini+nininini\displaystyle n_{i\uparrow}n_{i\downarrow}=\langle n_{i\downarrow}\rangle n_{i\uparrow}+\langle n_{i\uparrow}\rangle n_{i\downarrow}-\langle n_{i\downarrow}\rangle\langle n_{i\uparrow}\rangle (12)
=mini+mini+14+mi2,\displaystyle=-m_{i}n_{i\uparrow}+m_{i}n_{i\downarrow}+\frac{1}{4}+m^{2}_{i},

where the average density on each site writes as ni()=12±min_{i\uparrow(\downarrow)}=\frac{1}{2}\pm m_{i}. We obtain the following MF Hamiltonian,

Hmf\displaystyle H_{mf} =\displaystyle= ljσtcjσclσ+Ui(mini+mini)\displaystyle-\sum_{\langle lj\rangle\sigma}tc^{\dagger}_{j\sigma}c^{\phantom{{\dagger}}}_{l\sigma}+U\sum_{i}(-m_{i}n_{i\uparrow}+m_{i}n_{i\downarrow})
+\displaystyle+ 14NU+UNnsimi2,\displaystyle\frac{1}{4}NU+\frac{UN}{n_{s}}\sum_{i}m^{2}_{i},

where NN is the total number of sites, and each unit cell has ns=48n_{s}=48 sites. Minimizing the free energy FF with respect to mim_{i}, we obtain a set of self-consistently equations mi=ns2UNFmim_{i}=-\frac{n_{s}}{2UN}\frac{\partial F}{\partial m_{i}} (i=1,,nsi=1,...,n_{s}). The order parameters mim_{i} are self-consistent solved, and the result is shown in Fig. 3(b). The order parameters become nonzero from a critical interaction Uc=1.66tU_{c}=1.66t, from which the magnetism develops in the ribbon.

Refer to caption
Figure 7: The spin correlations on a lattice containing three unit cells (144144 sites) for several values of UU. The star marks the reference site, and the radius of the circles denote the values of the spin correlations. The crosses mark the sites with too large values or error bars.

Then the interactions are exactly dealt with using the DQMC method. Figure 7 shows the spin correlations on a lattice containing three unit cells for several values of UU. Their values grow as the interactions are increased, implying the interactions strengthen the spin correlations. We plot the values at U=4U=4 as functions of the indexes of the sites and the distances along several typical directions. As shown in Fig. 8, the spin correlations keep finite for all distances in the range of the lattice, implying the magnetism develops for large interactions.

Refer to caption
Figure 8: (a), The spin correlation as a function of the indexes of the sites. (b), The spin correlation as a function of the distances along several typical directions. Here the interaction is U=4tU=4t. The lattice size is the same as that of Fig. 7.
Refer to caption
Figure 9: (a) The local moment mm as a function of BB. Solid curves are from the fitting formula y=c+a(1ebx)y=c+a(1-e^{-bx}). (b) The extrapolated local moment as a function of UU. Here the temperature is T=0.05tT=0.05t. The lattice size is the same as that of Fig. 7.

Next we study the intrinsic magnetism of the system by extrapolating a symmetry-breaking term to its vanishing limit. As shown in Fig. 9(a), the local moment as a function of BB is best fitted using an exponentially-increasing formula y=c+a(1ebx)y=c+a(1-e^{-bx}). The extrapolated local moments are almost vanishing for weak interactions, and then increase rapidly from a critical interaction. The behavior is consistent with the MF approximation. The critical interaction estimated is between 2t2t and 3t3t, which is larger than the MF one. Since the realistic value of the Hubbard interaction in graphene is about tt, the experimentally relevant GNRs should be nonmagnetic, which is consistent with the experimental resultsGroning et al. (2018); Rizzo et al. (2018).

III Conclusions

Quantum magnetism of topologically-designed GNRs is studied based on the Hubbard models using exact numerical simulations. We first study a two-band Hubbard model describing the low-energy topological bands using DMRG and DQMC methods, and show that it is nonmagnetic. We then include the Hubbard interaction to the topological-designed GNRs, and find the local moments develop from a critical interaction between 2t2t and 3t3t. Compared to the realistic value in graphene, we conclude that the experimentally relevant GNRs are nonmagnetic, which is consistent with the experimental results.

IV Acknowledgments

The work is supported by the National Key Research and Development Program of China under Grant No. 2016YFA0300304, and NSFC under Grant Nos. 11774019, 11574032 and 11734002.

References