Electronic Resource
Springer
Astrophysics and space science
145 (1988), S. 241-249
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract Radio-emission of pulsars is investigated through computer simulation. We assume that electronpositron plasma is thermal and beam particles haveγ b ≈ 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. We 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.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00642101
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