Physics of the pulsar magnetosphere

Physics

Scientific paper

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Stellar Physics, Pulsar Magnetospheres, Atmospheric Physics, Radio Stars, Neutron Stars, Electrodynamics, Electron-Positron Plasmas, Radio Emission, Stellar Radiation, Emission Spectra, Stellar Evolution, Star Formation, Binary Stars, Stellar Structure, Boundary Layers, Nonuniform Plasmas, Distribution Functions, Relaxation Oscillators, Stellar Rotation

Scientific paper

Theoretical treatments of radio pulsars have yielded a consistent view of the physical processes present in the magnetosphere of a neutron star, explaining the deceleration of neutron star rotation, the release of rotational energy in active regions, and the generation of plasma and directed radio emission. The present work is a methodical presentation of this theoretical framework. The ultimate physical basis for the complex processes of the pulsar magnetosphere is found to be the fast rotation of a strongly magnetized conducting body, namely the neutron star.

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