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Refractive convergent plasma lenses explain extreme scattering events and pulsar scintillation

Authors

  • Ue-Li Pen,

    Corresponding author
    1. Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St George Street, Toronto M5S 3H8, Canada
      E-mail: pen@cita.utoronto.ca (U-LP); lindsay.king@utdallas.edu (LK)
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  • Lindsay King

    Corresponding author
    1. Institue of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA
    2. Department of Physics, The University of Texas at Dallas, Richardson, TX 75080, USA
      E-mail: pen@cita.utoronto.ca (U-LP); lindsay.king@utdallas.edu (LK)
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E-mail: pen@cita.utoronto.ca (U-LP); lindsay.king@utdallas.edu (LK)

ABSTRACT

We propose convergent plasma lenses, possibly from current sheets, as a generic solution to strong interstellar scattering. These lenses resolve the overpressure problem by geometric alignment as noted by Goldreich & Shridhar. Our new model further quantitatively explains properties of extreme scattering events and pulsar parabolic arcs. It makes quantitative predictions testable by VLBI on scattering events. It differs conceptually from previous models by occurring through rare, localized underdense sheets. Such sheets are thermally and kinematically stable, and could be consequences of reconnection. The apparent diffractive effects are a result of coherent interference of refractive images. We propose that these lenses can be used for precision distance determination to pulsars, enabling accurate gravity source localization.

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