Faraday conversion in magnetar winds explains the range of observed FRB circular polarization and yields constraints on near-source wind parameters from Stokes data.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Repeating FRBs show Gaussian-distributed intrinsic PAs with no periodicity, explained by stochastic magnetospheric axis wandering in an extended rotating vector model.
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.
citing papers explorer
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Constraining the near-source relativistic wind medium using Fast Radio Burst circular polarization data
Faraday conversion in magnetar winds explains the range of observed FRB circular polarization and yields constraints on near-source wind parameters from Stokes data.
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Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts
Repeating FRBs show Gaussian-distributed intrinsic PAs with no periodicity, explained by stochastic magnetospheric axis wandering in an extended rotating vector model.
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Searching for links between energetic millisecond pulsars and repeating fast radio bursts
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.