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    OU :: Department of Physics &

    Astronomy :: Journal Club

    Alexander Baker23rd March 2011

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    Propagation dynamics of optical

    vortices .Journal of Optical Society of America B/Volume14th3054-3065 (Nov1997).

    D. RozasDepartment of Physics, Worcester Polytechnic

    Institute, Worcester, Massachusetts.C. T. LawDepartment of Electrical Engineering and

    Computer Science, University of Wisconsin, Milwaukee.

    G. A. Swartzlander, Jr. Department of Physics, Worcester

    Polytechnic Institute, Worcester, Massachusetts.

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    University College London

    Department of Physics & Astronomy, Dr PhillipJones

    Optical Tweezers Group

    Summer project to investigate a numerical model for

    the propagation of OVs in linear and non linearmediums.

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    Contents

    Section 1: Background & Introduction Section 2: Review of definitions

    Section 3: Analytical descriptions of the propagation

    dynamics

    Section 4: Numerical and revised theoretical analysesfor special cases

    Section 5: Conclusions

    UCL Model, demonstration and findings

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    Section 1: Background

    Optical Vortex Light can be twisted like a corkscrew around its axis

    of travel, light waves at the axis cancel each other out.

    Projected ring of light.

    Topological Charge.

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    Section 1: Introduction

    Dynamics similar to hydrodynamic vortexphenomena.

    Develop intuitive understanding of OV motion.

    Describe propagation dynamics of different types of

    vortices. Applications in Optical Tweezers, Exoplanet

    detection, Quantum Computing.

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    Section 2: Definitions and Properties of

    OVs.

    Field of single

    vortex with Ansatz

    G_{bg} - Gaussianprofile.

    Compare and

    contrast two core

    functions.

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    Section 3 : Analytics Descriptions of

    the propagation dynamics.

    Scalar paraxial

    propagation, linear

    and nonlinear. Phase and intensity

    gradient

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    Section 3.1 : Gaussian beam dynamics.

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    Phase increases 2pi

    clockwise both cores.

    No rotation found

    around optical axis.

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    Section 4: Numerical analyses

    for special cases

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    Split step or beam

    propagation method.

    Linear and non linear

    terms.

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    Section 5: Conclusions

    Three factors that affect motion of optical vortices Amplitude gradient

    Phase gradient

    non linear factordepends on intensity gradient

    Contrasting differences between r and tanh corefunctions.

    Discuss 4 different cases

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    Case 1: Linear vortexLinear propagation of a vortex placed in the centre of a

    Gaussian beam.

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    Diffraction ringing

    may occur in near

    field

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    Case 2: Nonzero background gradientDisplaced vortex from the centre of the beam to location

    with non zero background gradient

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    Single tanh vortex

    expected to move in

    straight line

    propagation.

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    Case 3: Second vortexIntroduce a second vortex, trajectory affected by Gaussian

    field and field of second vortex.

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    R vortex no

    rotation.

    Pair of tanh

    vortices significant

    rotation

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    Case 3: Second vortexIntroduce a second vortex, trajectory affected by Gaussian

    field and field of second vortex.

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    Case 4: Nonlinear mediaIntroduce self-defocusing non linear medium.

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    Section 5: Conclusions

    Three factors that affect motion of optical vortices Amplitude gradient

    Phase gradient

    non linear factordepends on intensity gradient

    Contrasting differences between r and tanh corefunctions.

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    UCL Model & Findings ::

    animations

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    OU :: Department of Physics &

    Astronomy :: Journal Club

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    Appendix A : Geometry.

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    Ginzburg and

    Pitaevskii.

    Scalar paraxial

    propagation, linear

    and nonlinear.

    Hydrodynamic

    paradigms describe

    EM phenomena

    Phase and intensity

    gradient.