Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..44..389h&link_type=abstract
Astrophysics and Space Science, vol. 44, Oct. 1976, p. 389-395.
Astronomy and Astrophysics
Astrophysics
8
Electrostatic Waves, Particle Beams, Plasma-Particle Interactions, Pulsars, Relativistic Plasmas, Stellar Models, Astrophysics, Beam Plasma Amplifiers, Density Wave Model, Wave Excitation
Scientific paper
A class of pulsar models which provide a stationary beam-plasma system as the source of radiation is considered. Since the beam-plasma system is stable near the pulsar, where the coherent curvature radiation damps the longitudinal mode, the beam-plasma system away from the star is considered so that effects of curvature radiation may be neglected. It is found that the total wave energy density may attain a significant fraction of the beam energy density, provided the beam and plasma carry away a comparable amount of energy from the star. It should be noted that the attained high wave energy density is peculiar to a relativistic beam-plasma interaction.
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