Relativistic single-particle scattering cross sections for strong electromagnetic waves in strongly magnetized plasma are computed for arbitrary polarization and angle, showing strong suppression and sub-unity optical depth for quasi-parallel propagation.
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astro-ph.HE 2years
2026 2verdicts
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Reanalysis of pulsar data shows polarization angles in PSRs B1133+16 and B2016+28 follow great-circle geodesics on the Poincare sphere due to mode transitions.
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Scattering of Strong Radio Waves by Particles in Strongly Magnetized Plasmas and Implications for Fast Radio Bursts
Relativistic single-particle scattering cross sections for strong electromagnetic waves in strongly magnetized plasma are computed for arbitrary polarization and angle, showing strong suppression and sub-unity optical depth for quasi-parallel propagation.
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Polarization Angle Geodesics in PSRs B1133+16 and B2016+28
Reanalysis of pulsar data shows polarization angles in PSRs B1133+16 and B2016+28 follow great-circle geodesics on the Poincare sphere due to mode transitions.