Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-20T20:13:22.142Z Has data issue: false hasContentIssue false

Modes of Energy Loss from Isolated Magnetized Neutron Star

Published online by Cambridge University Press:  04 August 2017

S. Shibata*
Affiliation:
Astronomical Institute Tohoku University Sendai 980 Japan

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.

Pulsar may be regarded as a discharge tube by electron-positron pair creation. On this viewpoint we carry out two numerical calculations. The obtained magnetic field is consistent with the flow. We find that pulsars emit their rotational energy through three modes simultaneously. The three modes are (1)relativistic acceleration and following gamma-ray emission in the closed current circuit in the magnetosphere, (2)wind of the electron-positron pair plasma, and (3)dipole radiation.

Type
V. Neutron Star Physics
Copyright
Copyright © Reidel 1987