Formation of the Radio Profile Components of the Crab Pulsar

TL;DR

This paper models the formation of the Crab pulsar's radio profile components through induced Compton scattering, explaining observed spectral, polarization, and giant pulse features with a novel scattering-based approach.

Contribution

It introduces a new scattering model that explains the origin of various Crab pulsar profile components and their spectral and polarization properties.

Findings

Backscattered components correspond to observed interpulse and high-frequency components.

HFC1 and HFC2 are a single component split by rotational aberration.

The model explains giant pulse phenomena outside the main pulse.

Abstract

The induced Compton scattering of radio emission off the particles of the ultrarelativistic electron-positron plasma in the open field line tube of a pulsar is considered. We examine the scattering of a bright narrow radio beam into the background over a wide solid angle and specifically study the scattering in the transverse regime, which holds in a moderately strong magnetic field. Making use of the angular distribution of the scattered intensity and taking into account the effect of rotational aberration in the scattering region, we simulate the profiles of the backscattered components as applied to the Crab pulsar. It is suggested that the interpulse (IP), the high-frequency interpulse (IP') and the pair of the so-called high-frequency components (HFC1 and HFC2) result from the backward scattering of the main pulse (MP), precursor (PR) and the low-frequency component (LFC), respectively. The components of the high-frequency profiles, the IP' and HFCs, are interpreted for the first time. The HFC1 and HFC2 are argued to be a single component split by the rotational aberration close to the light cylinder. It is demonstrated that the observed spectral and polarization properties of the profile components of the Crab pulsar as well as the giant pulse phenomenon outside of the MP can be explained in terms of our model.