One-dimensional electric field structure of an outer gap accelerator — II. γ-ray production resulting from inverse Compton scattering
We study the structure of a stationary and axisymmetric charge-deficient region (or a potential gap) in the outer magnetosphere of a spinning neutron star. A large electric field along the magnetic field lines is created in this potential gap and accelerates migratory electrons (e−) and/or positrons...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 1999-09, Vol.308 (1), p.67-76 |
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