On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars
Fuente:
arXiv
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| Autore principale: | |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| Accesso online: | |
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| _version_ | 1866929343451627520 |
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| author | Jones, P B |
| author_facet | Jones, P B |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_08660 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars Jones, P B High Energy Astrophysical Phenomena 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. |
| title | On the origin of the quasi-periodic micro-pulses observed in the radio-frequency emission of some neutron stars |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2405.08660 |