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Particle Acceleration in Spherical Wave Fields

Published online by Cambridge University Press:  27 September 2017

K. O. Thielheim
K. O. Thielheim*
Affiliation:
Institut für Reine und Angewandte Kernphysik, Abteilung Mathematische Physik, Universität Kiel

Extract

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A magnet rotating in vacuo with its vector of angular velocity ω perpendicular to its vector of magnetic dipole moment μ is able to act as a particle accelerator. The dynamic features involved may be relevant for the understanding of rotating magnetized neutron stars as cosmic accelerators (Thielheim 1989) and may be useful for the designing of new mechanisms for accelerating devices.

Type
Part III Magnetospheric models
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 109 - 111
Copyright
Copyright © United States Naval Observatory 1992