The electromagnetic field of a slowly rotating magnetized neutron star in Saa's gravitation model with torsion

Details The electromagnetic field of a slowly rotating magnetized neutron star in Saa's gravitation model with torsion The electromagnetic field of a slowly rotating magnetized neutron star in Saa's gravitation model with torsion

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cha%26a..29...20c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 29, Issue 1, p. 20-38.

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

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 ≠ 0. Therefore, we can judge whether or not torsion exists by observing the exterior electromagnetic field of the neutron star.

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