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Updated: Jul 4, 2026

Determination of the Excitation and Coupling Rates Between Light Emitters and Surface Plasmon Polaritons
Published on: July 21, 2018
Excitation and conversion of electromagnetic waves in pulsar magnetospheres
G Gogoberidze1, G Z Machabeli, V V Usov
1Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Leuven, Belgium.
Abstract:
We demonstrate that nonlinear decay of obliquely propagating Langmuir waves into Langmuir and Alfvén waves (L --> L' + A) is possible in a one-dimensional, highly relativistic, streaming pair plasma. Such a plasma may be in the magnetospheres of pulsars. It is shown that the characteristic frequency of generated Alfvén waves is much less than the frequency of Langmuir waves and may be consistent with the observational data on the radio emission of pulsars.
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