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dc.contributor.authorStefani, Alessio
dc.contributor.authorKuhlmey, Boris
dc.contributor.authorFleming, Simon
dc.date.accessioned2021-12-22T03:40:22Z
dc.date.available2021-12-22T03:40:22Z
dc.date.issued2017en_AU
dc.identifier.urihttps://hdl.handle.net/2123/27261
dc.description.abstractGeneration and use of orbital angular momentum (OAM) of light is finding more and more interest in a wide variety of fields of photonics: communications, optical trapping, quantum optics, and many more [1]. In the investigation of such behavior, twisting of photonic crystal fibers shows interesting physical phenomena [2]. We previously reported the ability to create helical hollow fibers by mechanically twisting a tube lattice fiber made of polyurethane, the twist of which can be adjusted and reversed [3]. In this work we report how such deformation induces a mode transformation to an OAM mode, allowing a simple and tunable way to generate OAM modes. We take advantage of THz time domain spectroscopy to obtain information on both intensity and field components, and to be able to investigate how they change both in time and with frequency. The fiber here reported is 10 cm long, has a core diameter of 3 mm, it is twisted with twist rates between 0 and 62 rad/m and it is designed for frequencies 0.2 to 1.5 THz. A microscope image of the fiber is shown as inset of Fig. 1(a). The transmission spectrum of the fiber when straight and twisted was measured and is shown in Fig. 1(a). Above and below, the measured near-field images of the untwisted and twisted fiber output, respectively, are plotted for some selected frequencies in the different transmission bands. The twisted fiber in the transmission band centered at 750 GHz has a mode with a central minimum. The effect of twist on this fiber’s modes is investigated by finite-element (COMSOL) simulations by using a helical coordinate transformation [2] (Fig. 1(b)). A small amount of twist is not sufficient to perturb the guided mode. However, when sufficient twist is applied, the mode shows a singularity at its center. Increasing the twist further compromises guidance and the mode leaks into the cladding. Comparison between measurements and simulations for both mode intensity and x component of the electric field (Fig. 1(c)) confirms agreement between the two. Moreover, from the electric field it is possible to infer that the mode observed is radially polarized as the measured x-component of the output mode has a zero of electric field occurring along y. To ensure this mode possesses orbital angular momentum (which is expected because of the helicity of the fiber), the temporal evolution of the mode is examined: as the input is not a continuous wave, but a pulse, an OAM mode will have a temporal spiraling evolution. Snapshots of the temporal evolution of the mode are shown is Fig. 1(d). The mode starts from the lower-right corner and spirals to the top-left confirming the mode carries an orbital angular momentum.en_AU
dc.language.isoenen_AU
dc.publisherIEEEen_AU
dc.relation.ispartof2017 Conference on Lasers and Electro-Optics Europe & European Quantum Electronics Conference (CLEO/Europe-EQEC)en_AU
dc.rightsCopyright All Rights Reserveden_AU
dc.subjectAntiresonant fiberen_AU
dc.subjectOrbital angular momentum modesen_AU
dc.titleOrbital angular momentum modes by twisting of a hollow core antiresonant fiberen_AU
dc.typeConference paperen_AU
dc.subject.asrc0205 Optical Physicsen_AU
dc.identifier.doi10.1109/CLEOE-EQEC.2017.8086442
dc.type.pubtypeAuthor accepted manuscripten_AU
dc.relation.arcDP170103537
dc.relation.otherMarie Skłodowska-Curie Grant of the Horizon 2020 Framework Programme (H2020) (708860)
usyd.facultySeS faculties schools::Faculty of Science::School of Physicsen_AU
usyd.citation.spagePaper 8086442en_AU
workflow.metadata.onlyNoen_AU


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