Beam instability of the plasma in pulsar magnetospheres
Journal Article
·
· Astrophysics (Engl. Transl.); (United States)
The question of what beam instabilities can arise in the ultrarelativistic plasma of electrons and positrons near a pulsar is examined. It is shown that for the currently known parameters of the magnetospheric plasma of pulsars a beam instability can develop only through the hydrodynamic stage, and the beam may be smeared. Thus, the picture of
- Research Organization:
- Kharkovskii Gosudarstvennyi Universitet, Kharkov, Ukrainian SSR
- OSTI ID:
- 6236626
- Journal Information:
- Astrophysics (Engl. Transl.); (United States), Journal Name: Astrophysics (Engl. Transl.); (United States) Vol. 19; ISSN ATPYA
- Country of Publication:
- United States
- Language:
- English
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