A Resonant-Mode Model of Pulsar Radio Emission

Details A Resonant-Mode Model of Pulsar Radio Emission A Resonant-Mode Model of Pulsar Radio Emission

2003-10-15

arxiv.org/abs/astro-ph/0310411v1

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure. To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conference Proceedings),

Scientific paper

It 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.

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