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arXiv · 1306.2341

An emission mechanism explaining off-pulse emission originating in the outer magnetosphere of pulsars

Rahul Basu·Dipanjan Mitra·George I. Melikidze
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Abstract

We have examined the cyclotron resonance instability developing in the relativistic out-flowing plasma in the pulsar magnetosphere. The instability condition leads to radio emission in the sub-GHz frequency regime which is likely to be seen as off-pulse emission. Recent studies have shown the presence of off-pulse emission in long period pulsars, and we demonstrate this plasma process to be an energetically viable mechanism.

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Rahul Basu, Dipanjan Mitra, George I. Melikidze. 2013-06-10. An emission mechanism explaining off-pulse emission originating in the outer magnetosphere of pulsars. https://doi.org/10.1088/0004-637x/772/2/86

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