On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars

P B Jones

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arXiv · 2405.08660

On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars

P B Jones

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Abstract

The linear relationship between pulsar micro-pulse widths and rotation period is consistent with the existence of a physical length L on the neutron-star surface and seen on the observer arc of transit across the polar cap. Within the ion-proton model it is the width of the minimum area of surface that can support the critical growth rate of the unstable two-beam Langmuir mode that is the source of the radio emission.

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P B Jones. 2024-05-14. On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars. https://arxiv.org/abs/2405.08660

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