Annular gap model for multi-wavelength pulsed emission from young and millisecond pulsars

Abstract

The multi-wavelength pulsed emission from young pulsars and millisecond pulsars can be well modeled with the single-pole 3-dimension annular gap and core gap model. To distinguish our single magnetic pole model from two-pole models (e.g. outer gap model and two-pole caustic model), the convincing values of the magnetic inclination angle and the viewing angle will play a key role.

Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 3 pages, 2 figures

References in corpus (8)

• The First Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
• Two-Pole Caustic Model for High-Energy Lightcurves of Pulsars
• The inner annular Gap for pulsar radiation: gamma-ray and radio emission
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• An annular gap acceleration model for $\gamma$-ray emission of pulsars