Abstract

In dissipationless linear media, spatial disorder induces Anderson localization of matter, light, and sound waves. The addition of nonlinearity causes interaction between the eigenmodes, which results in a slow wave diffusion. We go beyond the dissipationless limit of Anderson arrays and consider nonlinear disordered systems that are subjected to the dissipative losses and energy pumping. We show that the Anderson modes of the disordered Ginsburg-Landau lattice possess specific excitation thresholds with respect to the pumping strength. When pumping is increased above the threshold for the band-edge modes, the lattice dynamics yields an attractor in the form of a stable multi-peak pattern. The Anderson attractor is the result of a joint action by the pumping-induced mode excitation, nonlinearity-induced mode interactions, and dissipative stabilization. The regimes of Anderson attractors can be potentially realized with polariton condensates lattices, active waveguide or cavity-QED arrays.

Highlights

  • In dissipationless linear media, spatial disorder induces Anderson localization of matter, light, and sound waves

  • We show that the Anderson modes of the disordered Ginsburg-Landau lattice possess specific excitation thresholds with respect to the pumping strength

  • Anderson localization in active disordered systems is a combined effect produced by the energy pumping, dissipation and nonlinearity

Read more

Summary

OPEN Anderson attractors in active arrays

The recent pioneering theoretical and experimental studies have already demonstrated a rich nonlinear dynamics of traveling and immobile gap solitons in periodic 1D condensate center arrays[40,47], and further stretched to spatially quasiperiodic structures to uncover the fractal energy spectrum[41]. These advances naturally lead to the question of Anderson localization in active arrays, where pumping and dissipation join the old players, nonlinearity and disorder. We show that the increase of pumping beyond the delocalization threshold leads to a multi-mode chaos followed by cluster synchronization

Results
The dynamics of the
Discussion
Additional Information

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.