Pulsar Magnetosphere Radiation Processes

Details Pulsar Magnetosphere Radiation Processes Pulsar Magnetosphere Radiation Processes

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..dmp.d6094t&link_type=abstract

American Physical Society, 2002 Division of Atomic, Molecular and Optical , abstract #D6.094

Physics

Scientific paper

Our results offer the possibility that certain neutron stars can undergo spontaneous magnetization. We use a simple potential to describe the nucleon-nucleon interaction. From these calculations, we derive the internal and external electromagnetic field. The external magnetic field structure is not a simple dipole even in the non-rotating case. Pulsar spectra are produced based on this model, which includes curvature radiation, inverse Compton scattering and relativistic Bremsstrahlung radiation processes.

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