Abstract
From protein motifs1 to black holes2, topological solitons are pervasive nonlinear excitations that are robust and can be driven by external fields3. So far, existing driving mechanisms all accelerate solitons and antisolitons in opposite directions3,4. Here we introduce a local driving mechanism for solitons that accelerates both solitons and antisolitons in the same direction instead: non-reciprocal driving. To realize this mechanism, we construct an active mechanical metamaterial consisting of non-reciprocally coupled oscillators5,6,7,8 subject to a bistable potential9,10,11,12,13,14. We find that such nonlinearity coaxes non-reciprocal excitations—so-called non-Hermitian skin waves5,6,7,8,15,16,17,18,19,20,21,22, which are typically unstable—into robust one-way (anti)solitons. We harness such non-reciprocal topological solitons by constructing an active waveguide capable of transmitting and filtering unidirectional information. Finally, we illustrate this mechanism in another class of metamaterials that shows the breaking of ‘supersymmetry’23,24 causing only antisolitons to be driven. Our observations and models demonstrate a subtle interplay between non-reciprocity and topological solitons, whereby solitons create their own driving force by locally straining the material. Beyond the scope of our study, non-reciprocal solitons might provide an efficient driving mechanism for robotic locomotion25 and could emerge in other settings, for example, quantum mechanics26,27, optics28,29,30 and soft matter31.
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Data availability
All the data supporting this study are available on the public repository https://uva-hva.gitlab.host/published-projects/non-reciprocal-topological-solitons.
Code availability
All the codes supporting this study are available on the public repository https://uva-hva.gitlab.host/published-projects/non-reciprocal-topological-solitons.
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Acknowledgements
We thank R. Hassing and K. van Nieuwland for technical support and F. van Gorp, J.-S. Caux, J. van Wezel, A. Souslov, J. Binysh and V. Vitelli for insightful discussions. We also thank S. Bouché, Q. Cai and J. Lankhorst for gathering preliminary data in the context of the MSc course ‘Project Academic Skills for Research’ they followed at the University of Amsterdam. We acknowledge funding from the European Research Council under grant agreement no. 852587 and from the Netherlands Organisation for Scientific Research under grant agreement no. VI.Vidi.213.131.3.
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C.C. and J.V. conceptualized and guided the project. J.V. and X.G. designed the samples and experiments. J.V. carried out the experiments. J.V., X.G. and C.C. carried out the numerical simulations. O.G., C.V.M. and A.S. performed the theoretical study. All authors contributed extensively to the interpretation of the data and the production of the manuscript. J.V. and C.C. wrote the main text. J.V. created the figures and videos. All authors contributed to the writing of the Methods and the Supplementary Information.
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Extended data figures and tables
Extended Data Fig. 1 Dependence of the Peierls-Nabarro barrier on the nondimensional amplitude D and initial conditions in the Frenkel-Kontorova model.
(abc) The Peierls-Nabarro barrier, regime of instability and (anti)soliton velocities as the continuum limit is approached as a function of the unnormalized non-reciprocity \(\eta \sqrt{D}\) and damping \(\Gamma \sqrt{D}\). As the discreteness parameter D becomes smaller, the line separating stable from unstable solutions approaches Γ = η as predicted for the continuum. The initial condition used corresponds to the experimentally used soliton with single lattice spacing width. In addition, the Peierls-Nabarro barrier gradually decreases and (d) eventually goes to zero, provided that the initial soliton shape also becomes less discrete49. (e) When the activation amplitude ϕ0 of the experimental initial condition is changed, the Peierls-Nabarro barrier also changes but for large enough amplitudes, it becomes constant. (f) When instead of an initial activation angle, an edge oscillator is initialized with some radial velocity \({\dot{\phi }}_{0}\), the Peierls-Nabarro barrier remains constant.
Extended Data Fig. 2 Calibration of experimental parameters.
(a) The nonlinear potential generated by the periodically spaced magnets, as measured with an Instron torsion testing machine. Red line represents the sinusoidal fit used to calibrate the magnetic potential amplitude B. (b) Instron measurement of the elastic forces experienced by a single oscillator connected to two neighboring oscillators. Red line shows the smoothed data and green dashed lines show linear fits around the two potential minima, denoting the elastic coupling strength κ. (c) Oscillation of a single oscillator elastically coupled to two neighbors, used to measure the viscous damping coefficient γ. (d) The biased potential for different amounts of bias δ. (e) The difference between the potential minima ΔV between the two uneven minima plotted versus the bias δ. A linear fit establishes the relation between the bias and δ the effective external force E it corresponds to.
Extended Data Fig. 3 Stability of the soliton.
(a) Snapshots of a soliton in the unstable regime showing the destabilization of high wavenumber modes, found numerically for η = 1.1 and Γ = 1. (b) Growth rates \({\rm{I}}{\rm{m}}(\varOmega )\) of perturbations around the soliton solution for various wavenumbers given by Eq. (9). The dotted line at \({\rm{I}}{\rm{m}}(\varOmega )\) marks the transition between decaying and growing solutions, with high wavenumbers being the first to become unstable as the threshold of stability η = Γ is crossed. (c) Dependence of \({\rm{I}}{\rm{m}}({\varOmega }_{\pm })\) on the wavenumber k for Γ = 1 and η = 0.5 (red) and η = 1.5 (blue). In the latter case, modes in the regions \({\rm{Im}}({\varOmega }_{+}) > 0\) become unstable at \(k=\pm \Gamma /\sqrt{{\eta }^{2}-{\Gamma }^{2}}\) given by the dashed lines.
Extended Data Fig. 4 Kane-Lubensky chain.
Sketch of the Kane-Lubensky chain and its notation conventions.
Extended Data Fig. 5 Insensitivity of non-reciprocal solitons to boundary conditions.
Although at a linear level, the non-Hermitian skin effect causes the energy spectrum to change radically upon changing boundary conditions, nonreciprocal solitons are insensitive to the boundary as their topological charge protects them from amplifying exponentially in space. (a) Simulation of a single Frenkel-Kontorova soliton driven by non-reciprocity (η = 1.1, Γ = 1.3, D = 1.2) under antiperiodic boundary conditions. (b) Simulation of a Frenkel-Kontorova soliton-antisoliton pair driven by non-reciprocity (η = 1.1, Γ = 1.3, D = 1.2) under periodic boundary conditions. Neither periodic, antiperiodic or the open boundary conditions used in the main text affect the stability and velocity of the (anti)soliton.
Extended Data Fig. 6 Solitons with higher topological charge.
(a) Simulation of a staircase of Frenkel-Kontorova solitons under the influence of non-reciprocity (η = 1.1, Γ = 1.3, D = 1.2). As in the single soliton case, (anti)solitons with higher topological charge travel undisturbed at the same steady state velocity.
Extended Data Fig. 7 Effect of non-reciprocal driving and damping on the collision of sine-Gordon solitons.
(a) In the absence of both driving and damping, solitons and antisolitons pass through each other without interacting. (b) For nonzero damping, soliton and antisoliton annihilate and the resulting non-topological solution dissipates away. (c) With only non-reciprocity turned on, both excitations still pass through each other unhindered but are also rendered unstable. (d) Dissipation and non-reciprocity can balance, giving rise to non-reciprocal breather solutions.
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Veenstra, J., Gamayun, O., Guo, X. et al. Non-reciprocal topological solitons in active metamaterials. Nature 627, 528–533 (2024). https://doi.org/10.1038/s41586-024-07097-6
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DOI: https://doi.org/10.1038/s41586-024-07097-6
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