| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701023 | Chinese Astronomy and Astrophysics | 2005 | 19 Pages |
Abstract
The equations of the electromagnetic field of a slowly rotating magnetized neutron star in Saa's gravitation model with torsion are derived and their exterior solution is investigated. The following conclusions are obtained: first, there is a specific solution for the electromagnetic field when Aô = 0; second, there is no solution at all when Aô â 0. Therefore, we can judge whether or not torsion exists by observing the exterior electromagnetic field of the neutron star.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Chen Ci-xing, Zhang Jia-lü,