Theory of the radio emission of pulsars |
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Authors: | V S Beskin A V Gurevich Ya N Istomin |
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Institution: | (1) P.N. Lebedev Physical Institute, Academy of Sciences of the USSR, Moscow, U.S.S.R. |
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Abstract: | A consistent theory of excitation, stabilization, and propagation of electromagnetic oscillations in a relativistic one-dimensional electron-positron plasma flowing along curved magnetic field lines is presented. It is shown that in such a medium which is typical of the magnetosphere of a neutron star there exist unstable natural modes of oscillations. Nonlinear saturation of the instability leads to an effective energy conversion into transverse oscillations capable of leaving the magnetosphere of a pulsar. The polarization spectrum and the directivity pattern of generated radiation are determined. A comparison with observations has shown that the theory makes it possible to explain practically all the basic characteristics of observed pulsar radio emission. |
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