Stability of a beam-plasma system against the excitation of the longitudinal mode around pulsars

Details Stability of a beam-plasma system against the excitation of the longitudinal mode around pulsars Stability of a beam-plasma system against the excitation of the longitudinal mode around pulsars

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..223h&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 1, 1976, pt. 1, p. 223-225.

Astronomy and Astrophysics

Astrophysics

15

Electron Beams, Plasma-Particle Interactions, Pulsars, Radio Emission, Systems Stability, Electrostatic Waves, Polar Caps, Stellar Radiation, Wave Excitation

Scientific paper

The possibility of radio wave emission from the beam-plasma system around pulsars is investigated. The indirect generation of radio waves by first exciting the longitudinal mode is found unlikely, because the beam-plasma system is stable against the excitation of such a mode around the pulsar polar caps. This may be understood if we realize that the rate of excitation of the longitudinal mode is likely to be much less than the coherent curvature-radiation loss rate at any level of excitation.

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