Pulsar polarization: a partial-coherence model

Journal article

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.

Authors: Oswald, LS; Karastergiou, A; Johnston, S

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: Oxford University Press
• Journal: Monthly Notices of the Royal Astronomical Society
• Volume: 525
• Issue: 1
• Pages: 840–853
• Publication date: 2023-08-27
• Acceptance date: 2023-07-21
• DOI: 10.1093/mnras/stad2271
• EISSN: 1365-2966
• ISSN: 0035-8711
• Language: English
• Keywords: pulsars: individual: PSR J0820–1350; pulsars: general; pulsars: individual: PSR J0134–2937; polarization; pulsars: individual: PSR J1157–6224