Polar cap region and plasma drift in pulsars
Andrzej Szary, Joeri van Leeuwen

TL;DR
This paper compares two models of plasma drift in pulsar polar caps, demonstrating that the modified carousel model aligns with physical laws and offers new insights into plasma behavior and subpulse drifting.
Contribution
It introduces a comprehensive analysis of drift models in axisymmetric pulsar polar caps, favoring the modified carousel model over the lagging behind corotation model.
Findings
The lagging behind corotation model is inconsistent with Faraday's law.
The modified carousel model aligns with Faraday's law and explains plasma drift.
Electric fields between discharges are not fully screened, affecting plasma movement.
Abstract
Pulsars often display systematic variations in the position and/or intensity of the subpulses, the components that comprise each single pulse. Although the drift of these subpulses was observed in the early years of pulsar research, and their potential for understanding the elusive emission mechanism was quickly recognised, there is still no consensus on the cause of the drift. We explore the electrodynamics of two recently proposed or refined drift models: one where plasma lags behind corotation, connecting the drift with the rotational pole; and another where plasma drifts around the electric potential extremum of the polar cap. Generally, these are different locations, resulting in different drift behaviours, that can be tested with observations. In this study, however, we specifically examine these models in the axisymmetric case, where the physics is well understood. This approach…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Sensor Technology · Magnetic confinement fusion research
