Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-26T21:37:35.610Z Has data issue: false hasContentIssue false

Tortion Influence on the Magnetic Field of Rotating Neutron Stars

Published online by Cambridge University Press:  04 August 2017

C.N. Zhang
Affiliation:
Department of Physics, Dalian Institute of Technology, Dalian, China
J.G. Shi
Affiliation:
Department of Physics, Dalian Institute of Technology, Dalian, China
F.P. Chen
Affiliation:
Department of Physics, Dalian Institute of Technology, Dalian, China

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.

Using the axisymmetric tortion tensor given by J. Nitsh in U4 gravitational gauge theory. Applying G. S. Yang and L. F. Luo's magnetic field model of neutron stars, i.e. magnetic field is originated from long-arranged neutron spin. Precession of spin coupled with tortion has been studied, indicating an influence on the magnetic field. The results show that the initial magnetic filed B made of long-arranged spin magnetic moment is at an angle of α with rotating axis, if radians, B makes a so small angle to the rotating axis at time 108 sec. that no pulses could be radiated from the neutron stars. Only when radians, the pulse radiation could be done. Based on the assumption that the orientation of the initial magnetic fields is isotropic, we can get then that only about ten percent of the rotating neutron stars radiate pulses.

Type
IV. Neutron Stellar Evolution
Copyright
Copyright © Reidel 1987