Optical polarisation of the Crab pulsar: precision measurements and comparison to the radio emission

TL;DR

This study presents high-time-resolution optical polarisation measurements of the Crab pulsar, revealing detailed correlations with optical and radio light curves, and suggesting a subtle link between optical and radio emission mechanisms.

Contribution

The paper provides the first high-time-resolution optical polarisation data of the Crab pulsar, uncovering detailed correlations with radio emissions and indicating a connection between optical and radio emission processes.

Findings

Optical polarisation correlates with optical light curves.

Polarisation details relate to radio frequency light curves.

Evidence of a connection between optical and radio emissions.

Abstract

The linear polarisation of the Crab pulsar and its close environment was derived from observations with the high-speed photo-polarimeter OPTIMA at the 2.56-m Nordic Optical Telescope in the optical spectral range (400 - 750 nm). Time resolution as short as 11 microseconds, which corresponds to a phase interval of 1/3000 of the pulsar rotation, and high statistics allow the derivation of polarisation details never achieved before. The degree of optical polarisation and the position angle correlate in surprising details with the light curves at optical wavelengths and at radio frequencies of 610 and 1400 MHz. Our observations show that there exists a subtle connection between presumed non-coherent (optical) and coherent (radio) emissions. This finding supports previously detected correlations between the optical intensity of the Crab and the occurrence of giant radio pulses. Interpretation of our observations require more elaborate theoretical models than those currently available in the literature.