arXiv · astro-ph/9612078
Physical processes in pulsar magnetospheres and non-thermal high-frequency emission
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.
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Vladimir V. Usov. 1996-12-09. Physical processes in pulsar magnetospheres and non-thermal high-frequency emission. https://arxiv.org/abs/astro-ph/9612078
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