(Received 22 July 1996; accepted 18 November 1996)
The behavior of a relativistic electron
positron plasma in the pulsar magnetosphere is investigated. The equation of the motion of the magnetospheric plasma is discussed, from which it follows that, if the plasma particle radial velocity Vr > c/
(where c is the speed of light), the centrifugal acceleration changes its sign and the particle braking begins. The stability of the magnetospheric plasma with respect to the radially oriented potential perturbations is discussed and the possibility of the electrostatic field generation in this plasma along the pulsar magnetic field lines is shown. © 1997 American Institute of Physics.
| History | Received: 22 July 1996; Accepted: 18 November 1996 |
| Subject | Stars |
| PACS |
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| Keywords | pulsars; astrophysical plasma; stellar magnetism; stellar atmospheres; plasma instability; plasma magnetohydrodynamics; electric fields; relativistic plasmas |
| Doc. Type | Theoretical |
| Coden | PHPAEN |
| PII | S1070-664X(97)00403-5 |