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Light with a self-torque: extreme-ultraviolet beams with time-varying orbital angular momentum

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arxiv 1901.10942 v1 pith:RIOTE5C4 submitted 2019-01-30 physics.optics

classification physics.optics
keywords beamslightself-torqueangularmomentumariseextreme-ultravioletnaturally
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Twisted light fields carrying orbital angular momentum (OAM) provide powerful capabilities for applications in optical communications, microscopy, quantum optics and microparticle rotation. Here we introduce and experimentally validate a new class of light beams, whose unique property is associated with a temporal OAM variation along a pulse: the self-torque of light. Self-torque is a phenomenon that can arise from matter-field interactions in electrodynamics and general relativity, but to date, there has been no optical analog. In particular, the self-torque of light is an inherent property, which is distinguished from the mechanical torque exerted by OAM beams when interacting with physical systems. We demonstrate that self-torqued beams in the extreme-ultraviolet (EUV) naturally arise as a necessary consequence of angular momentum conservation in non-perturbative high-order harmonic generation when driven by time-delayed pulses with different OAM. In addition, the time-dependent OAM naturally induces an azimuthal frequency chirp, which provides a signature for monitoring the self-torque of high-harmonic EUV beams. Such self-torqued EUV beams can serve as unique tools for imaging magnetic and topological excitations, for launching selective excitation of quantum matter, and for manipulating molecules and nanostructures on unprecedented time and length scales.

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Cited by 2 Pith papers

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    Hermite-Gaussian driven high harmonic generation produces tunable, self-interfering arrays of phase-locked EUV beamlets, demonstrated experimentally and by simulation, with applications to grating calibration and sing...

  2. Vortex Propagation in Orbital Angular Momentum Beams and the Effects of a Limited Aperture

    physics.optics 2025-10 conditional novelty 5.0 of 10

    For aperture-limited Gaussian vortex beams, the dark core radius at the phase-imprinting plane is set by the first Bessel root of order ell, and the distance over which the core grows follows a D^{-3/2} scaling with f...

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