Orbital effect in the stationary axisymmetric field
Gong Tian-Xi(龚添喜)a)b) and Wang Yong-Jiu(王永久)a)†
a Institute of Physics, Hunan Normal University, Changsha 410081, China; b School of Physics, Hunan University of Science and Technology, Xiangtan 411201, China
Abstract This paper uses an elegant mathematical method to calculate the orbital effects in the axisymmetric field created by the spinning mass with electric charge and a large number of magnetic monopoles. In comparison with that in the Reissner--Nordström (R--N) field, the correction terms caused by the spinning mass decrease the advanced effect as the revolution direction of the test particle coincides with that of the Kerr field, however, the correction terms caused by the spinning charged mass increase the advance effect as the revolution direction of the test particle coincides with that of the Kerr--Newman--Kasnya (KNK) field. Generalizing the effect in the axisymmetric field, it obtains interesting results by discussing the parameters of the celestial body, these parameters provide a feasible experimental verification of the general relativity.
Received: 17 October 2007
Revised: 26 December 2007
Accepted manuscript online:
Fund: Project
supported by the National Basic Research Program of China (Grant No
2003CB716300) and Natural Science Foundation of Hunan
Province, China (Grant No 06JJ20026).
Cite this article:
Gong Tian-Xi(龚添喜) and Wang Yong-Jiu(王永久) Orbital effect in the stationary axisymmetric field 2008 Chin. Phys. B 17 2356
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