The investigation of a relativistic electron beam dynamics in the pulsar magnetosphere is given. The equation of motion of the magnetospheric plasma particles is discussed. As it turned out, if the particle radial velocity Vr > c/√2 (where c is the speed of light), centrifugal acceleration changes its sign and the particle braking begins. Also 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 the pulsar magnetosphere plasma along the magnetic field lines is shown.
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机译:给出了对脉冲星磁层中相对论电子束动力学的研究。讨论了磁层等离子体粒子的运动方程。事实证明,如果粒子径向速度Vr> c /√2(其中c是光速),则离心加速度会改变其符号,并且粒子制动开始。还讨论了磁层等离子体相对于径向取向的电势扰动的稳定性,并显示了沿磁场线在脉冲星磁层等离子体中产生静电场的可能性。
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