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

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 va...

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Bibliographic Details
Published inarXiv.org
Main Authors Du, YuanJie, Qiao, GuoJun
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 22.10.2012
Subjects
Annular gaps
Emission
Inclination angle
Magnetic poles
Millisecond pulsars
Physics - High Energy Astrophysical Phenomena
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Summary: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.
ISSN:2331-8422
DOI:10.48550/arxiv.1210.5801