Physical processes in pulsar magnetospheres and non-thermal high-frequency emission

Details Physical processes in pulsar magnetospheres and non-thermal high-frequency emission Physical processes in pulsar magnetospheres and non-thermal high-frequency emission

1996-12-09

arxiv.org/abs/astro-ph/9612078v1

Astronomy and Astrophysics

Astrophysics

8 pages, latex, no figures. To be published in the Proceedings of the IAU Colloquium No 160, Pulsars: Problems and Progress, S

Scientific paper

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.

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