Mechanism of giant pulses in radio pulsars

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Pulsars, Radiative Transfer, Magnetospheric Electromagnetic Wave Propagation, Stellar Atmospheres, Electromagnetic Wave Polarisation, Pulsars, Radiative Transfer, Scattering, Emission, Absorption, And Scattering Of Electromagnetic Radiation, Radiation Mechanisms, Polarization

Scientific paper

Giant radio pulses are explained in terms of induced Compton scattering by the secondary plasma particles in pulsar magnetosphere. This process can account for the energetics and statistics of giant pulses as well as for their substructure at nanosecond timescales. The mechanism suggested predicts strong polarization of giant radiation in the plane of the ambient magnetic field.

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