93 research outputs found

    An exact transverse Helmholtz equation

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    We derive an exact equation for the transverse component of the electric field propagating along a given longitudinal z direction in the presence of an isotropic refractive-index distribution n(x,y)

    The case of the oscillating party balloon: A simple toy experiment requiring a not-so-simple interpretation

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    The intriguing midair oscillations of a party balloon, which occur once its buoyancy is no longer capable of keeping it against the ceiling, is shown to require a rather sophisticated explanation in terms of variable-mass dynamics. The ubiquity of this phenomenon, the accessibility of its actual observation, and the subtlety of its analytic description provide a good opportunity for an interesting zero-cost classroom demonstration

    Vectorial nonparaxial propagation equation in the presence of a tensorial refractive-index perturbation

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    The standard scalar paraxial parabolic (FockLeontovich) propagation equation is generalized to include all-order nonparaxial corrections in the significant case of a tensorial refractive-index perturbation on a homogeneous isotropic background. In the resultant equation, each higher-order nonparaxial term (associated with diffraction in homogeneous space and scaling as the ratio between beam waist and diffraction length) possesses a counterpart (associated with the refractive-index perturbation) that allows one to preserve the vectorial nature of the problem (∇∇· E ≠ 0). The tensorial character of the refractive-index variation is shown to play a particularly relevant role whenever the tensor elements δnxz and δnyz (z is the propagation direction) are not negligible. For this case, an application to elasto-optically induced optical activity and to nonlinear propagation in the presence of the optical Kerr effect is presented

    Perfect Optical Solitons: Spatial Kerr Solitons as Exact Solutions of Maxwell's Equations

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    We prove that spatial Kerr solitons, usually obtained in the frame of nonlinear Schroedinger equation valid in the paraxial approximation, can be found in a generalized form as exact solutions of Maxwell's equations. In particular, they are shown to exist, both in the bright and dark version, as linearly polarized exactly integrable one-dimensional solitons, and to reduce to the standard paraxial form in the limit of small intensities. In the two-dimensional case, they are shown to exist as azimuthally polarized circularly symmetric dark solitons. Both one and two-dimensional dark solitons exhibit a characteristic signature in that their asymptotic intensity cannot exceed a threshold value in correspondence of which their width reaches a minimum subwavelength value.Comment: 19 pages, 11 figure. Submitted for publication on Josa

    Self-phase modulation and modal noise in optical fibers

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    The phase variations associated with the intensity-dependent part of the refractive index assume different values for the different propagation modes of an optical fiber. As a consequence, intensity fluctuations of the exciting source are converted into relative phase fluctuations, which give rise to an amplitude-dependent modal noise

    Phase conjugation by degenerate four-wave mixing and temporal coherence

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    The influence of the temporal-coherence properties of the pump and signal waves on the efficiency and the temporal fidelity of the phase-conjugation process associated with degenerate four-wave mixing is examined

    Soliton propagation in multimode optical fibers

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    Soliton propagation in a multimode optical fiber in the presence of an intensity-dependent refractive index is investigated by means of a set of nonlinear coupled equations derived in the frame of coupled-mode theory. In particular, the conditions on modal amplitudes and modal dispersion necessary for soliton existence are derived

    Electromagnetic propagation in a turbulent medium: a new approach

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    A formalism based on coupled-mode theory is presented that allows one to deduce the equations of evolution of the correlation functions of the field propagating in a turbulent medium. As a particular application, the second-order correlation function is evaluated under less stringent conditions than those usually required in the frame of optical propagation theories in random media
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