Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T05:03:25.901Z Has data issue: false hasContentIssue false
  • English
  • Français

Synchro-Curvature Radiation and Magnetic Pair Production of Relativistic Electrons in Strong Curved Magnetic Fields

Published online by Cambridge University Press:  04 August 2017

S.-Y. An
S.-Y. An*
Affiliation:
Phys. Dept., Beijing Teachers College, Beijing, China

Extract

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.

Most of common curved magnetic fields with axial symmetry in astrophysics can be expressed in a local cylindrical coordinate system (R, φ, Z) as where HO, RO and N are real constants. It has been known that the non-zero curvature of the magnetic field lines can impose an additional pitch angle on the electrons moving in the field (1).

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 452
Copyright
Copyright © Reidel 1987