A Resonant-Mode Model of Pulsar Radio Emission

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dc.creatorYoung, Matthew D. T.
dc.date2003-10-15
dc.date.accessioned2026-07-07T02:10:27Z
dc.date.available2026-07-07T02:10:27Z
dc.descriptionIt is argued that the polar gap and flux tube in the pulsar magnetosphere act as a resonant cavity/waveguide system which is excited by oscillations in the primary beam current and accelerating potential. The modes will be converted, probably scattered, to produce radio beams in the frequency range of those observed.
dc.description4 pages, 1 figure. To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo and B. M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0310411
dc.identifierhttp://arxiv.org/abs/astro-ph/0310411
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6745
dc.subjectAstrophysics
dc.titleA Resonant-Mode Model of Pulsar Radio Emission
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