4.7 Article

Evidence for scattering of curvature radiation in radio pulsar profiles

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 522, Issue 1, Pages 1480-1490

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stad1101

Keywords

polarization; radiation mechanisms: non-thermal; pulsars: general; pulsars: individual: PSR J1012+5307; pulsars: individual: PSR B1642-03; pulsars: individual: PSR B1700-32 (PSR J1703-3241)

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Radio pulsars display unexplained phenomena in their pulse profiles, such as the core-cone structure and frequency evolution. The author proposes that these phenomena can be explained through the geometric properties of inverse Compton scattering. The observed bifurcated components can be interpreted as magnified microbeams of curvature radiation that have been upshifted in frequency and preserved in width by beam-copying scattering.
Radio pulsars exhibit several unexplained phenomena, in particular the average pulse profiles with the apparent core-cone structure and interesting frequency evolution. I show that they can be interpreted through essential geometric properties of the inverse Compton scattering. If the scattering occurs in a dipolar magnetosphere and the mean free path is long, a nested cone structure is expected with the cone size ratio of two-thirds, which is consistent with observations. Being a discontinuous process, the scattering is consistent with the discrete altitude structure of emission rings, as derived from aberration-retardation effects. Assuming that the upscattered signal is the curvature radiation (CR), one can interpret the observed bifurcated components (BCs) as a magnified microbeam of CR: the BCs are wide low-frequency CR microbeams that have been upshifted in frequency with their width preserved by beam-copying scattering in divergent magnetic field. The large flux of BCs is partly caused by compression of the full emitted spectrum into the narrow observed bandwidth, which explains why the frequency-resolved BCs have the frequency-integrated shape. The wide low-frequency microbeams can encompass large magnetospheric volumes, which considerably abates the requirements of the energy needed for coherency. The properties of BCs thus suggest that the observed modulated radio flux is strongly affected by the scattering-driven blueshift and spectral compression. The relativistic beaming formula (1/& gamma;) is not always applicable, in the sense that it may not be directly applied to some blueshifted profile features.

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