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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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
PATH is extended with three fitted P(m_r|z) prior models combined with P(z|DM), raising host-association confidence for ASKAP FRBs while showing fainter-than-expected host magnitude distribution.
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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.