A Single spark model for PSR J2144$-$3933
Dipanjan Mitra, Rahul Basu, George I. Melikidze, Mihir Arjunwadkar

TL;DR
This paper explains the unique emission characteristics of PSR J2144$-$3933 using a single spark within the partially screened vacuum gap model, highlighting the role of non-dipolar magnetic fields and polar cap temperature regulation.
Contribution
It demonstrates that a single spark in the PSG model can account for the pulsar's single-component profile and emission features, emphasizing the importance of non-dipolar magnetic fields.
Findings
Single spark suffices to sustain critical temperature in PSR J2144$-$3933.
Observations support a centrally traversed emission beam by the line-of-sight.
No subpulse drifting observed, consistent with a single spark model.
Abstract
The partially screened vacuum gap model (PSG) for the inner acceleration region in normal radio pulsars, a variant of the pure vacuum gap model, attempts to account for the observed thermal X-ray emission from polar caps and the subpulse drifting timescales. We have used this model to explain the presence of death lines, and extreme location of PSR J21443933 in the diagram. This model requires maintaining the polar cap near a critical temperature and the presence of non-dipolar surface magnetic field to form the inner acceleration region. In the PSG model, thermostatic regulation is achieved by sparking discharges which are a feature of all vacuum gap models. We demonstrate that non-dipolar surface magnetic field reduces polar cap area in PSR J21443933 such that only one spark can be produced and is sufficient to sustain the critical temperature. This pulsar has a…
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