We propose a complex Ginzburg-Landau equation (CGLE) with localized linear gain as a two-dimensional model for pattern formation proceeding via spontaneous breaking of the axial symmetry. Starting from steady-state solutions produced by an extended variational approximation, simulations of the CGLE generate a vast class of robust solitary structures. These are varieties of asymmetric rotating vortices carrying the topological charge (TC), and four-to ten-pointed revolving stars, whose angular momentum is decoupled from the TC. The fourand five-pointed stars feature a cyclic change of their structure in the course of the rotation.
We discuss differences between the variational approach to solitons and the accessible soliton approximaion in a highly nonlocal nonlinear medium. We compare results of both approximations by considering the same system of equations in the same spatial region, under the same boundary conditions. We also compare these approximations with the numerical solution of the equations. We find that the variational highly nonlocal approximation provides more accurate results and as such is more appropriate solution than the accessible soliton approximation. The accessible soliton model offers a radical simplification in the treatment of highly nonlocal nonlinear media, with easy comprehension and convenient parallels to quantum harmonic oscillator, however with a hefty price tag: a systematic numerical discrepancy of up to 100% with the numerical results.
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