Physical processes in pulsar magnetospheres and non-thermal high-frequency emission
arXiv:astro-ph/9612078
Abstract
The energy source of a pulsar's non-thermal emission is the rotational energy loss of the neutron star. The rotational energy of the neutron star is transformed into the pulsar radiation by a long sequence of processes. The processes of this sequence are discussed.
8 pages, latex, no figures. To be published in the Proceedings of the IAU Colloquium No 160, Pulsars: Problems and Progress, Sydney, 8-12 January 1996 (invited paper)