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- W2000563452 abstract "We investigate the self-consistent electrodynamic structure of a particle accelerator in the Crab pulsar magnetosphere on the two-dimensional poloidal plane, solving the Poisson equation for the electrostatic potential together with the Boltzmann equations for electrons, positrons, and γ-rays. If the transfield thickness of the gap is thin, the created current density becomes sub-Goldreich-Julian, giving the traditional outer-gap solution but with negligible γ-ray luminosity. As the thickness increases, the created current increases to become super-Goldreich-Julian, giving a new gap solution with substantially screened acceleration electric field in the inner part. In this case, the gap extends toward the neutron star with a small-amplitude positive acceleration field, extracting ions from the stellar surface as a space-charge-limited flow. The acceleration field is highly unscreened in the outer magnetosphere, resulting in a γ-ray spectral shape that is consistent with the observations." @default.
- W2000563452 created "2016-06-24" @default.
- W2000563452 creator A5080847519 @default.
- W2000563452 date "2006-12-01" @default.
- W2000563452 modified "2023-10-10" @default.
- W2000563452 title "Particle Accelerator in Pulsar Magnetospheres: Super‐Goldreich‐Julian Current with Ion Emission from the Neutron Star Surface" @default.
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- W2000563452 doi "https://doi.org/10.1086/508317" @default.
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