Computational approach to the radio-emission of pulsars

Details Computational approach to the radio-emission of pulsars Computational approach to the radio-emission of pulsars

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.145..241c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 145, no. 2, June 1988, p. 241-249.

Statistics

Computation

Computational Astrophysics, Electron-Positron Plasmas, Pulsars, Radio Emission, Beam Plasma Amplifiers, Electromagnetic Radiation, Electrostatic Waves, Power Spectra, Radio Frequencies, Relativistic Velocity

Scientific paper

Radio-emission of pulsars is investigated through computer simulation. The authors assume that electron-positron plasma is thermal and beam particles have γb ≈ 50 in the plasma rest frame. The main purpose of this study is to search for unstable electromagnetic waves which may be caused by beam-plasma interactions. The authors obtain the dominant waves in the range of radio frequencies in the observer frame. The results show that transverse electromagnetic waves grow rapidly, while electrostatic waves have very slow growth.

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