Pulsar giant pulse: coherent instability near light cylinder
Weiyang Wang, Jiguang Lu, Songbo Zhang, Xuelei Chen, Rui Luo and, Renxin Xu

TL;DR
This paper proposes that giant pulses from the Crab pulsar originate from plasma coherent instability near the light cylinder, producing zebra-pattern spectral structures through cyclotron-resonant interactions.
Contribution
It introduces a novel plasma instability model explaining the spectral zebra patterns in pulsar giant pulses, linking them to resonance and magnetic reconnection near the light cylinder.
Findings
Spectral bands fit by a coherent instability model.
Estimated plasma density near light cylinder: 10^{13-15} cm^{-3}.
Resonance modulates spectral structures and may produce high-energy emissions.
Abstract
Giant pulses (GPs) are extremely bright individual pulses of radio pulsar. In microbursts of Crab pulsar, which is an active GP emitter, zebra-pattern-like spectral structures are observed, which are reminiscent of the `zebra bands' that are observed in type IV solar radio flares. However, band spacing linearly increases with the band center frequency of \,GHz. In this study, we propose that the Crab pulsar GP can originate from the coherent instability of plasma near a light cylinder. Further, the growth of coherent instability can be attributed to the resonance observed between the cyclotron-resonant-excited wave and the background plasma oscillation. The particles can be injected into the closed-field line regions owing to magnetic reconnection near a light cylinder. These particles introduce a large amount of free energy that further causes cyclotron-resonant instability,…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Solar and Space Plasma Dynamics · Magnetic confinement fusion research
