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Chapter 11 - Discrete Solitons

A periodic array of optical waveguides creates a novel kind of device in which new types of spatial solitons can be generated and studied experimentally. The properties of spatially localized modes in a waveguide array are usually analyzed in the framework of a set of coupled-mode equations, each equation representing the soliton amplitude in a specific waveguide, but coupled to the neighboring waveguides. Such a coupled set of equations is referred to as the discrete nonlinear Schrödinger (NLS) equation, and its localized solutions are known as discrete solitons. A similar approach for studying discrete spatial solitons in solid-state physics is known as the tight-binding approximation. In the context of an optical waveguide array, this approximation corresponds to the assumption that the fundamental modes in all waveguides are only weakly coupled. The solitoncentered inside a single waveguide is stable because it corresponds to the minimum of the Hamiltonian. If the discrete soliton is forced to move sideways, it has to jumpfrom one waveguide to the next, passing from a stable to an unstable configuration. Thedifference between the Hamiltonians in the two cases—the so-called Peierls-Nabarropotential—accounts for the resistance that the soliton has to overcome during transverse propagation. This potential increases as the input power level increases. As a result, the soliton becomes localized to a single waveguide and is effectively decoupled from the rest of the array.

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Chapter 1 - Introduction

This chapter provides an overview of optical solitons by emphasizing on the physical principles and the simplest theoretical model based on the cubic nonlinear SchröSdinger (NLS) equation and its generalizations. The term “solitary wave” or “solitons” is used to reflect the particle-like nature of solitary waves that remained intact even after mutual collisions. In the context of nonlinear optics, solitons are classified as being either temporal or spatial, depending on whether the confinement of light occurs in time or space during wave propagation. Temporal solitons represent optical pulses that maintain their shape, whereas spatial solitons represent self-guided beams that remain confined in the transverse directions orthogonal to the direction of propagation. Both types of solitons evolve from a nonlinear change in the refractive index of an optical material induced by the light intensity — a phenomenon known as the optical Kerr effect in the field of nonlinear optics. The intensity dependence of the refractive index leads to spatial self-focusing (or self-defocusing) and temporal self-phase modulation (SPM)- the two major nonlinear effects that are responsible for the formation of optical solitons. The scalar NLS equation applies for both temporal and spatial aspects of wave Propagation It is derived on the basis of quite general assumptions about the dispersive (and diffractive) effects and the nonlinear properties of physical systems.

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Chapter 6 - Two-Dimensional Solitons

The fundamental physical mechanism behind the transverse instability induced by the self-focusing of soliton stripes is similar to the mechanism governing the self-focusing and modulation instabilities of small-amplitude, quasi-harmonic, wave packets.The instability occurs when transverse modulations on the wave front of a planar solitonstripe decrease the local value of the soliton energy. Two analytical methods can be used for studying the transverse instability of solitons, namely, ray-optics approach and linear stability analysis. The ray -optics approach is based on the assumption that a transversely modulatedplane wave remains locally close to its steady-state profile, so each individual segment of the wave evolves along an individual ray used for analyzing the self-focusinginstabilities of a soliton stripe. It makes use of a linear eigenvalue problem that is obtained by linearizing the (2 + 1)-dimensional NLS equation near the exactone-dimensional soliton solution. Because two-dimensional spatial solitons are unstable in a Kerr medium, the soliton interaction and spiraling can be observed only in non-Kerr media. The interaction can bemodeled theoretically either by using an NLS equation with saturable nonlinearity or by employing the cubic-quintic NLS equation. If the two-dimensional spatial solitons are treated as “effective particles” their interaction potential can be calculated by using the collective-coordinate approach.

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