Titlebook: Dissipative Solitons; Nail Akhmediev,Adrian Ankiewicz Book 2005 Springer-Verlag Berlin Heidelberg 2005 Absorption.Dissipative systems.Lase

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https://doi.org/10.1007/978-94-015-9421-9linear coupling in conjunction with the cubic Kerr nonlinearity and chromatic dispersion leads to the formation of attracting soliton states, i.e. dissipative solitons. A review of each model is given with an evaluation of its merit and mode-locking features.

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The Convergence of Scientific Knowledgecomplex discrete diffraction, as well as Bloch oscillations, arising from the linear properties of such systems. Subsequently, using a generic cubic-quintic nonlinearity, we identify self-localized dissipative discrete soliton solutions, and study their characteristics.

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Dissipative Solitons in the Complex Ginzburg-Landau and Swift-Hohenberg Equations,olitons form a new paradigm for the investigation of phenomena involving stable structures in nonlinear systems far from equilibrium. We consider those aspects of the problem that can be studied on the basis of a qualitative analysis of nonlinear systems.

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Dissipative Solitons in Pattern-Forming Nonlinear Optical Systems: Cavity Solitons and Feedback SolWe consider such phenomena in driven optical cavities containing a nonlinear medium (cavity solitons) and rather similar phenomena (feedback solitons) where a driven nonlinear optical medium is in front of a single feedback mirror. The history, theory, experimental status, and potential application of such solitons are reviewed.

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Ettore Lanzarone,Francesca Ievaolitons form a new paradigm for the investigation of phenomena involving stable structures in nonlinear systems far from equilibrium. We consider those aspects of the problem that can be studied on the basis of a qualitative analysis of nonlinear systems.

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https://doi.org/10.1007/978-3-642-82348-0magneto-optic medium is . = ε. [ε·. + . ×.], where ε is the relative permittivity that exists in the absence of an applied magnetic field, ε. is the permittivity of the free space, . ∝ .(.) is called the gyration vector, and the function . (.) involves the applied magnetic field .. The vector . × .

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