Modeling γ and X-ray Pulsar Spectra

Details Modeling γ and X-ray Pulsar Spectra Modeling γ and X-ray Pulsar Spectra

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aps..ses..jf08t&link_type=abstract

American Physical Society, 66th Annual Meeting of the Southeastern Section of the American Physical Society November 7-9, 1999 C

Physics

Scientific paper

Since the discovery of pulsars in 1967, their emission spectra have been a source of great study. The focus of the current research is to model the high frequency component, gamma and X-ray. The model will use a dipole magnetic field that can either be aligned or not aligned with the rotation axis and the induced electic field to establish the pulsar magnetosphere. The first goal will be to use the curvature radiation photons to calculate the rate of electron-positron production and their density. With this information, further radiation processes can be included to further describe the observed spectra.

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