Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-26T04:23:48.006Z Has data issue: false hasContentIssue false

The structure of the pulsar magnetosphere via particle simulation with GRAPE

Published online by Cambridge University Press:  20 March 2013

Shinpei Shibata*
Affiliation:
Department of Physics, Yamagata University, Kojirakwa, Yamagata, Japan email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

It is shown with a particle simulation that the outer gap can be reproduced under a few simple assumptions. The simulation includes just the first principles, namely Maxwell's equations, a relativistic equation of motion with radiation drag, and electron-positron pair creation. We also suggest that the Y-point (the open-close boundary in the equator) is likely to be a place of heating and acceleration of plasma, and therefore it would cause high-energy emission. The dead zone along the separatrix of the oppositely directed current is found in the middle latitude region, which separates the outer gap and the polar cap accelerators.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

Cheng, A., Ruderman, M., & Sutherland, P., 1976, ApJ, 203, 209Google Scholar
Holloway, N. J. 1973, Nat. Phys. Sci., 246, 6Google Scholar
Timokhin, A. N. 2010, Mon. Not. R. astron. Soc., 408, 2092Google Scholar
Umizaki, M. & Shibata, S. 2010, Pub. Astr. Soc Japan, 62, 131Google Scholar
Uzdensky, D. A., 2004, ApJ, 603, 652CrossRefGoogle Scholar
Wada, T. & Shibata, S., 2007, Mon. Not. R. astron. Soc., 376, 1460Google Scholar
Wada, T. & Shibata, S., 2011, Mon. Not. R. astron. Soc., 418, 612CrossRefGoogle Scholar
Yuki, S. & Shibata, S., 2012, Pub. Astr Soc. Japan, 64, 43Google Scholar