Pulsar polarization: a partial-coherence model

TL;DR

This paper introduces a partial-coherence model to explain complex polarization features in radio pulsars, including frequency evolution, polarization angle deviations, and circular polarization, enhancing understanding of pulsar emission mechanisms.

Contribution

The paper presents a novel partial-coherence model that explains observed polarization phenomena in pulsars and provides insights into their emission and propagation processes.

Findings

Model explains polarization frequency evolution

Accounts for deviations in polarization angle

Reproduces features of circular polarization

Abstract

The population of radio pulsars is observed to demonstrate certain polarization properties not explained by the conventional picture of pulsar polarization, namely frequency evolution of polarization, deviations of the linear polarization angle from a curve of geometric origins and the presence of features in the circular polarization. We present the partial-coherence model as a way to explain the co-occurrence of these features and to provide an origin for circular polarization in radio pulsar profiles. We describe the mathematics of the model and demonstrate how it can explain these observed features, both on a population level and for the idiosyncrasies of individual pulsars. The partial coherence model can account for complex polarization behaviour, enabling improved access to information about pulsar geometries. We discuss the scientific implications of this for our understanding of pulsar radio emission and propagation.