中国物理B ›› 2008, Vol. 17 ›› Issue (7): 2356-2360.doi: 10.1088/1674-1056/17/7/006

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Orbital effect in the stationary axisymmetric field

王永久1, 龚添喜2   

  1. (1)Institute of Physics, Hunan Normal University, Changsha 410081, China; (2)Institute of Physics, Hunan Normal University, Changsha 410081, China;School of Physics, Hunan University of Science and Technology, Xiangtan 411201, China
  • 收稿日期:2007-10-17 修回日期:2007-12-26 出版日期:2008-07-09 发布日期:2008-07-09
  • 基金资助:
    Project supported by the National Basic Research Program of China (Grant No 2003CB716300) and Natural Science Foundation of Hunan Province, China (Grant No 06JJ20026).

Orbital effect in the stationary axisymmetric field

Gong Tian-Xi(龚添喜)a)b) and Wang Yong-Jiu(王永久)a)†   

  1. a Institute of Physics, Hunan Normal University, Changsha 410081, China; b School of Physics, Hunan University of Science and Technology, Xiangtan 411201, China
  • Received:2007-10-17 Revised:2007-12-26 Online:2008-07-09 Published:2008-07-09
  • Supported by:
    Project supported by the National Basic Research Program of China (Grant No 2003CB716300) and Natural Science Foundation of Hunan Province, China (Grant No 06JJ20026).

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摘要： 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--Nordstr\"om (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.

关键词: general relativity, gravitational effect, space--time metric

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.

Key words: general relativity, gravitational effect, space--time metric

中图分类号:  (Spacetime topology, causal structure, spinor structure)

  • 04.20.Gz
04.20.Jb (Exact solutions) 04.25.-g (Approximation methods; equations of motion)