Scattering of Low-Frequency Radiation by a Gyrating Electron
S. A. Petrova

TL;DR
This paper analyzes how low-frequency electromagnetic waves scatter off gyrating electrons in magnetic fields, revealing effects on radio wave polarization, intensity, and potential high-energy emission in pulsar environments.
Contribution
It provides a detailed analysis of low-frequency wave scattering by gyrating electrons, highlighting its significance in pulsar radio wave behavior and high-energy emission mechanisms.
Findings
Scattering transfers low-frequency photons to high harmonics of gyrofrequency.
Total scattering cross-section is much larger than for stationary particles.
Scattering can influence pulsar radio spectrum and contribute to high-energy emissions.
Abstract
The scattering of electromagnetic radiation by the particle gyrating in an external magnetic field is considered. Particular attention is paid to the low-frequency case, when the frequencies of incident radiation are much less than the electron gyrofrequency. The spectral and polarization features of the scattering cross-section are analyzed in detail. It is found that the scattering transfers the low-frequency photons to high harmonics of the gyrofrequency, into the range of the synchrotron emission of the electron. The total scattering cross-section appears much larger than that for the particle at rest. The problem studied is directly applicable to the radio wave scattering in the magnetosphere of a pulsar. The particles acquire relativistic rotational energies as a result of resonant absorption of the high-frequency radio waves and concurrently scatter the low-frequency radio waves,…
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