Experimental demonstration of angular momentum-dependent topological transport using a transmission line network

Novel classical wave phenomenon analogs of the quantum spin Hall effect are mostly based on the construction of pseudo-spins. Here we show that the non-trivial topology of a system can also be realized using orbital angular momentum through a coupling between the angular momentum and the wave vector. The idea is illustrated with a tight-binding model and experimentally demonstrated with a transmission line network. We show experimentally that even a very small network cluster exhibits angular momentum-dependent one-way topological edge states, and their properties can be described in terms of local Chern numbers. Our work provides a new mechanism to realize counterparts of the quantum spin Hall effect in classical waves and may offer insights for other systems. Here, the authors show that a system can exhibit angular momentum-dependent topological properties through angular-momentum-orbital coupling and provide a proof-of-principle experimental demonstration using a transmission line network.

R ecent efforts to realize classical wave topological materials have given rise to the field of topological photonics  . In order to realize the classical counterpart of the quantum Hall effect, the nontrivial band topologies are typically achieved by breaking time reversal symmetry, while the nontrivial topologies of the quantum spin Hall effect (QSHE) are usually realized through spin-orbital coupling. Due to the absence of intrinsic Kramers degeneracy in classical waves, the analogs of the QSHE are realized by constructing pseudo-spins [18][19][20][21][22][23][24][25] . Apart from polarization (spin), the angular momentum of classical waves also offers freedom to control wave 26,27 and signal propagation 28,29 . Angular momentum has been treated as a synthetic dimension and the nontrivial topologies made possible by this synthetic dimension have been explored 26,27,30 .
Here, we show that a system can exhibit angular momentumdependent topological properties through angular-momentumorbital coupling. The boundary of such a system possesses oneway edge states that are locked to the angular momentum without breaking time reversal symmetry. We also provide a proof-ofprinciple experimental demonstration using a transmission line network. We will see that local Chern numbers 31,32 can be used to characterize the topology of a small cluster of such network systems for each angular momentum subspace. For simplicity, we limit our discussion to a hexagonal network in this work, but the ideas can be easily generalized to other systems.

Results
Orbital angular momentum. In two-dimensional (2D) systems, electromagnetic waves decouple into two independent transverse electric and transverse magnetic modes whose evolution can then be represented by a scalar component as denoted by φ. Consider a cylindrical meta-atom whose eigenfield (H z or E z ) can be written as where r, θ are the polar coordinates and m denotes the orbital angular momentum. The phase distribution of such a meta-atom with angular momentum m = 1 is shown in Fig. 1a. If the angular momentum eigenmodes in the system do not interact (which is usually ensured by the rotational symmetry), the system Hamiltonian can be block-diagonalized and each block is labeled by the corresponding angular momentum eigenvalue. Meta-atoms that possess a well-defined angular momentum can be regarded as elementary building blocks of the system and they can form a lattice structure. One such lattice structure is shown pictorially in Fig. 1b, where a 2D honeycomb lattice is considered. Below we will show that periodic systems and finite-size clusters comprising such meta-atoms exhibit topological properties by introducing angular-momentum-orbital coupling.
Tight-binding model. To put our idea in context, we first consider a simple tight-binding model which is periodic in the xy plane. A meta-atom which exhibits well-defined angular momentum eigenmodes can be realized with a discrete set of N nodes (illustrated in Fig. 1c) uniformly spaced in a ring, where N is the total number of nodes. These nodes have the same wave amplitude and the phase of the j-th node is j2πm/N. These nodes need not lie on the xy plane and in fact they will be stacked in the z direction in the following discussion. Hence, Fig. 1c should be regarded as their projected positions on a plane. Such a ring of nodes can obviously exhibit N different values of angular momentum. When N = 1 or 2, the subspace of each angular momentum still possesses time reversal symmetry. For a system with time reversal symmetry to exhibit nontrivial topology, N must be larger than 2. A discretized example for m = 1 and N = 3 is shown in Fig. 1d. Similarly, a hexagonal lattice of metaatoms with angular momentum m = 1 in Fig. 1b can be represented by discretized nodes as shown in Fig. 1e. For illustration purpose, we label each node with a layer number and the honeycomb lattice in Fig. 1e Fig. 1 Realization of angular-momentum-orbital coupling in 2D honeycomb lattices. a Phase distribution of a mode with angular momentum m = 1. b A honeycomb lattice with sites exhibiting non-zero angular momentum. c A discrete set of N point nodes, where each carries a different phase, can emulate a mode with non-zero angular momentum. d A minimum of three nodes is needed to create a nontrivial topology. e A discretized version of the honeycomb lattice in (b), with each site carrying three nodes. The three nodes need not lie geometrically on the same plane. f An exemplary connection which exhibits nontrivial angular-momentum-orbital coupling. Here a layer represents the lattice structure formed by the nodes with the same sequence number j (as shown in (c)) of different loops on each lattice site. Black spheres represent nodes. The bonds in blue and yellow indicate intralayer and interlayer couplings, respectively. g An N = 3 example. The 'head-to-tail' connection here means layer 1 is connected to layer 3 via the same connections as those shown in (f). The loop formed by the nodes A 1 , A 2 and A 3 (B 1 , B 2 and B 3 ) represents the meta-atom on the sublattice A (B) form a honeycomb lattice with the same hopping strength as shown in Fig. 1f with the bonds in blue. The black spheres in Fig. 1f represent the nodes which are assumed to be identical and hence the on-site energies are all set to zero. Each honeycomb lattice consists of two sublattices and hence there are 2N nodes in each unit cell.
We now proceed to introduce the angular-momentum-orbital coupling. Such couplings essentially help distinguish different angular momentums and hence modes with different angular momentum eigenvalues experience different synthetic gauge fields. One such coupling is shown by the bonds in yellow in Fig. 1f. Such a coupling introduces a chiral coupling to the AA stacked honeycomb lattice. We note that chiral coupling has been used in constructing Weyl semimetals 33,34 . The angular momentum is preserved as long as the couplings between layers j and j + 1 (layers N and 1 when j = N) are the same for arbitrary values of j. Interlayer coupling is introduced between the first layer and the N-th layer to preserve the angular momentum, i.e., the N-th layer is connected from head to tail to the first layer. The schematic of the tight-binding model for N = 3 is presented in Fig. 1g. In this N = 3 example, the nodes A 1 , A 2 and A 3 stacked along the z-axis constitute one meta-atom on the sublattice A and the nodes B 1 , B 2 and B 3 form another meta-atom on sublattice B.
As discussed before, the system Hamiltonian can be blockdiagonalized with each block having a different angular momentum. We define the angular momentum basis as where |j〉 in the summation denotes the original basis for the nodes in the j-th layer. In the angular momentum basis, the Hamiltonian with N = 3 can be block-diagonalized and each angular momentum block can be written as (see Supplementary Note 1 for more details) where k = (k x , k y ) is the Bloch wavevector, σ 0 is the 2 × 2 identity matrix, σ x , σ y and σ z are the Pauli matrices, and where a is the distance between nearest sublattices. Here t 1 and t 2 denote the interlayer and intralayer hopping strength as represented by the bonds in yellow and blue in Fig. 1f, respectively. In a system with time reversal symmetry, such as the one we are considering, t 1 and t 2 are both real numbers. The first two terms in Eq. (3) are the same as those in the tightbinding model of graphene 35 , which is not surprising as we have a honeycomb lattice. The last two terms in Eq. (3) represent the angular-momentum-orbital coupling, which depends explicitly on the angular momentum. The third term introduces a global energy shift only, and so it does not change the topology of the band structure. The last term introduces an angular momentumdependent mass term which lifts the Dirac cone degeneracy at K and K' for non-zero m. To see this more clearly, we expand the Hamiltonian around K 0; 4π=3 as follows: where τ = 1 for the K point and τ = −1 for the K' point, p= (p x , p y ) is momentum measured from the K or K' point. The last term in Eq. (5) represents the angular-momentum-orbital coupling which is similar to the spin-orbital coupling 36,37 . There is, however, a sector with m = 0 where the mass term vanishes, wherein the bands are degenerate at the K (K') point as guaranteed by time reversal symmetry. Although the whole system is invariant under time reversal, the band topology of the m = ±1 sectors can still be nontrivial as each sector on its own is not time reversal invariant.
Transmission line network. We proceed to implement the above tight-binding model with a transmission line network [38][39][40][41] , which provides the flexibility to realize the "head to tail" connection. The transmission lines here are coaxial cables which can be regarded as one-dimensional waveguides. These coaxial cables are then connected at nodes to form a network, which is described by a set of equations as follows 38: Here, ψ j is the voltage at the j-th node, l jk is the length of the cable connecting nodes j and k, and with ω, c 0 and ε being the angular frequency, the speed of light in vacuum and the relative permittivity of the dielectric medium in the coaxial cables, respectively. This network equation is equivalent to a tight-binding model with an on-site term À P k cothðgl jk Þ and a hopping term 1/sinh(gl jk ). The connecting nodes can be regarded as the discrete nodes considered previously and a cable provides coupling between two nodes. The coupling coefficient depends on the frequency, length and permittivity of the cable. More mathematical details about the calculations of transmission line network can be found in Supplementary Note 2. The network topology provides the flexibility to connect the first layer back to the third layer and hence realize the Hamiltonian in Eq. (3). We note that although the hopping here depends on the frequency, this frequency dependence does not change the topology of the system. The idea discussed here can also be extended to other waveguide networks.
Bulk band and angular momentum-dependent one-way edge states. To show that the transmission line network exhibits the basic characters of the tight-binding model, we solve Eq. (6) numerically and plot the band structures in Fig. 2a, b with m = 0 and m = 1, respectively. The coaxial cables are connected in the way shown in Fig. 1g and periodic boundary conditions are applied in the in-plane directions. The lengths of intralayer and interlayer cables are taken to be a = 0.43 m and b = 2.06 m, respectively. The wave speed inside the cable is assumed to be 0.66c (the same as experimentally measured results). For simplicity, the loss in the cable is ignored for now. The band structures in Fig. 2a, b are quite similar to those of the tightbinding model as shown in Supplementary Fig. 1a, b and Supplementary Note 1. The band structure of m = −1 is the same as that of m = 1. For m = 0, the Dirac point appears at the K point as predicted by the tight-binding Hamiltonian where there is no σ z term. For m = 1, a band gap emerges between two bulk bands. Our system is C 6 invariant and the angular momentum-dependent Chern number of each band can be obtained using the rotational eigenvalues at high symmetry points 42,43 . The Chern number of each m = 1 band is labeled in Fig. 2b (the Chern numbers have opposite signs when m = −1). We can see that a nontrivial band gap exists from 31 MHz to 36.3 MHz. We also show the projected band structure along the x direction (y direction) of the m = 1 sector with the armchair (zigzag) boundaries in Fig. 2c (Fig. 2d), where the gray area represents the projection of bulk bands, and the red and blue curves represent the edge states localized at the upper (right) and lower (left) boundaries of a strip, respectively. The existence of these one-way edge states verifies once again the nontrivial topology of the band structure for the m = 1 sector.
Angular momentum-dependent local Chern number. The Chern number in Fig. 2 is obtained by considering an infinite system. Next, we explore the topological property of a finite-size cluster. We consider a sample which is of finite size in the xy plane while the "head to tail" connection is kept such that the angular momentum remains well defined. To study the topological characteristics of a finite-size structure, we adopt the concept of the local Chern number 31,32 , which is defined by the antisymmetric product of the projection operators: where P ¼ P f f c ju f ihu f j is the projection operator which adds up all the eigenstates |u f 〉 below a cutoff frequency f c , and P jk ¼ hx j jPjx k i is the spatial relation between sites x j and x k . These sites lie in three different sectors (labeled A, B and C in the counterclockwise direction) of the circular computational domain (see left panel of Fig. 3a). The cutoff frequency f c is set to 31 MHz, which is the lower band edge frequency of the nontrivial band gap. Figure 3a shows a top view of the finite size 9 × 9 lattice with the computational domain at the center. Each sector (A, B or C) covers 120°and the computational domain is a circle with radius r. For the sites on the boundaries between two sectors, we distribute them to the adjacent sector in the clockwise direction. The value of ν as defined in Eq. (7) for such a chosen computational domain is taken as the local Chern number at the center of this circular region. The radius r of this computational region will affect the value of ν. To explore this dependence, we plot the ν − r curve in the right panel of Fig. 3a for the 9 × 9 sample shown in the left panel, where the center of the circle is fixed at the center of the sample. From the results shown in Fig. 2b, we expect the local Chern number to be −1 (1) for m = 1 (m = −1). We can see that ν goes to zero when r is too small or too large compared with the sample size, but when the radius takes intermediate values, the result converges to −1 (1) for m = 1 (m = −1), consistent with the Chern numbers calculated under periodic boundary conditions. In the following calculation, the radii of the computational region are set to 2.3a and 5a for the 3 × 3 and 9 × 9 samples, respectively. By solving Eq. (6), we obtain the eigen-spectrum for m = 1 as shown in the left panel of Fig. 3b, where each black dashed line corresponds to the frequency of an eigenstate. The local Chern number ν as a function of the cutoff frequency (the summation is taken over all of the eigenstates below this frequency) is shown in the middle panel of Fig. 3b when the center of the sample is taken as the center of the computational region. We see that there is a wide spectral range where ν is almost −1. This spectral range starts from about 31 MHz and ends near 36 MHz, which coincides with the lower and upper edges of the nontrivial band gap as determined by the band structure calculation. We next set the cutoff frequency to 31 MHz (marked by the red dotted line in the left panel of Fig. 3b), and calculate ν as a function of the center position of the computational region. The corresponding results are shown in the right panel of Fig. 3b. We see that except for the boundary region where the blue color is a lighter shade, other parts exhibit a local Chern number close to −1. Such a nontrivial local topological property persists even when the sample size decreases to 3 × 3 as shown in Fig. 3c. Once again, the left, middle and right panels show the eigen-spectrum, local Chern number at the center, and local Chern number as a function of position, respectively. Here the cutoff frequency is also chosen as 31 MHz.
Experimental demonstration of the topological transport. Due to the nontrivial topological property of the m = ±1 subspace and the existence of the local Chern number, finite-size samples should have angular momentum-dependent one-way edge states. The robustness of these one-way edge states against defects and sharp corners are numerically investigated in Supplementary  Figs. 3 and 4 and Supplementary Note 3. Due to the complexity of the connected network, we work with a small sample. As shown in the previous section, the nontrivial topology should be manifested in the transmission spectra even for a 3 × 3 sample. The experimental sample is shown in Fig. 4a. Figure 4b shows the connectors in our system. One node (left hand side of the panel) consists of four cross connectors (upper-right) and three straight connectors (lower-right), connecting intralayer, interlayer and measurement cables. In our experiments, we use two cables of the same type (RG58C/U type; https://hkcn.rs-online.com/ web/p/thin-ethernet-cable/5218436/?sra=pstk) but with different lengths as shown in Fig. 4c. The one for interlayer connections is around 2.00 m long; the one for intralayer connections is around 0.37 m long. The details of how to connect cables with nodes can be seen from the hexagonal network formed by the connectors and cables as shown in Fig. 4d.
To show the robustness of the one-way edge states using simulations, we introduce a defect as shown in Fig. 5a. In the 7 × 7 sample, the defect is introduced by removing all the interlayer cables in the three unit cells highlighted in red color. We note such a defect preserves the angular momentum. The simulated transmission spectra of this larger sample for m = 1 with and without the defect are shown in Fig. 5b with the red and black curves. The transmission spectra are almost the same in the nontrivial gap region (gray region), while they differ outside the gap region. As the cables in the experiments have some intrinsic loss, we also add intrinsic loss obtained from fitting the experimental data to the numerical simulation (see Methods and Supplementary Fig. 5). The loss in the cable used in the experiment is rather small, and g ≈ ik−1/2L, where k ¼ ω ffiffiffi ffi ε′ p =c 0 and absorption length L = ε′/kε″ with ε′ and ε″ being the real and imaginary parts of the relative permittivity. In this study, the absorption length of our cables is measured to be L ≅ 338 × f −0.6123 , where L is in meters (m), and f is in MHz.
Due to the complexity of the connected network, we implement a small sample in the experiment. Figure 5c shows the in-plane lattice structure of the experimental sample in Fig. 4a and the interlayer coupling is the same as that shown in Fig. 1g. The parameters of the lattice are the same as those in Fig. 2. We also add three additional cables to each layer in the upperright corner (indicated by the red line) as a defect to test the oneway property of the edge states (more experimental details can be found in Methods). The experimental transmission spectra of the system for m = 1 with and without the defect are shown in Fig. 5d with the red and black curves, where the gray region denotes the nontrivial gap region. It can be seen that inside the nontrivial gap region, the transmission spectra are almost the same, while they differ for frequencies below the gap region. We note here that as the scattering of the defect is due to the additional cables placed outside the sample, its influence on the bulk states is limited. As such, the difference between the two experimental transmission spectra is rather small above the band gap region. As a comparison, the defect shown in Fig. 5a is inserted deeply into the inside of the sample, and so it will affect the propagating of the states outside the band gap more conspicuously than the defect shown in Fig. 5c. We also measure the field distribution of the edge state excitation as additional evidence of the existence and robustness of the one-way edge states. Figure Fig. 8a-d). We also measure the field patterns for m = 0. The wave propagates at 33.7 MHz inside the bulk band ( Supplementary Fig. 7a) but is reflected at 49.2 MHz which falls inside the band gap ( Supplementary Fig. 7b). For m = 0, we do not observe any nontrivial edge states at any frequency as it is topologically trivial.

Discussion
We have demonstrated that angular momentum can provide an additional degree of freedom to control the topology of a system through coupling with orbital momentum. Such an idea is illustrated with a tight-binding model and experimentally verified with a transmission line network. The well-defined angular momentum-dependent local Chern number shows that the topological properties persist even for a very small cluster, as was realized experimentally. We experimentally realized the N = 3 case but samples with higher values of N can be constructed and in principle each angular momentum subspace can carry a different topology. Our idea can be generalized to other waveguide network systems and is not limited to the discretized tightbinding model.

Methods
Experimental materials. The cables we use have intrinsic loss, whose values are calibrated experimentally. Due to the intrinsic loss, the wave amplitude along the propagation direction will attenuate at the rate of exp(−x/2L), where x is the propagation distance and L is the absorption length. The absorption length is frequency dependent and can be described by an empirical relation L ≅ αf −β in the frequency range of our experiments 38 . Here f represents frequency in MHz, and α and β are constants determined from fitting the experimental data. In Supplementary Fig. 5a, we show the log of the field amplitudes at different frequencies as functions of cable lengths, and their linear fitting gives the absorption length at each frequency. The log of the absorption lengths are then shown in Supplementary Fig. 5b (as dots) and are fitted to obtain α = 338m and β = 0.6123. The wave speed of this cable is 0.66c, and its frequency dependence can be safely ignored, especially as the loss is quite low. As evidence, the imaginary part of the relative permittivity at 30 MHz is estimated to be about 0.06, which is much smaller than the real part at approximately 2.3.
Experimental details. In the experiment, we measure the property inside each angular momentum sector only, which can be ensured if the source only excites the angular momentum of that sector. In Supplementary Fig. 6a, we show one such setup for N = 3, where m in the equation determines the angular momentum to excite. Taking advantage of the superposition principle, we excite each layer separately and then add up the amplitudes (the phase delay due to the angular momentum is included) to obtain the field distribution. In the case where only one angular momentum sector is excited, the field amplitudes of the layers differ only by a phase factor. Hence, in all the plots of field distributions, we only show the field amplitude of one layer. Due to the presence of the connectors, the length of the cables used is slightly shorter than the actual distance between two nodes. To obtain the actual distance between two nodes, we use the connection as shown in Supplementary Fig. 6b. Same as before, we only show the connection within one layer. The interlayer connections are the same as before and periodic boundary conditions are applied to the left and right boundaries. The source is at the node at the upper edge and we measure the transmission at the node at the lower edge as shown in Supplementary  Fig. 6b. In such a setup, we actually excite the band along the k x = 0 direction as highlighted in red in Supplementary Fig. 6c. The extra length added due to the presence of the connectors is the same for all cables. The blue curve in the left panel of Supplementary Fig. 6d shows the experimentally measured transmission spectrum, while the red curve represents the numerically calculated transmission spectrum with the extra length being 0.06 m. These two transmission spectra match quite well. The right panel of Supplementary Fig. 6d shows the corresponding band structure of m = 1 along the k x = 0 direction. Due to the limited size of the sample used in the experiment, the transmission inside the band gap (gray region) is shallow but can still be seen clearly. In Supplementary Fig. 6d, we also show the numerically calculated transmission spectrum with 20 unit cells along the y direction with the cyan curve. Here, we increase the magnitude of the signal by five times. With more unit cells, the band gap frequencies continue to show no transmittance as expected. The transmission amplitude also decreases and the spectrum becomes smoother due to the intrinsic loss in the cable.