Orbital effect in the stationary axisymmetric field
Wang Yong-Jiua, Gong Tian-Xib
a Institute of Physics, Hunan Normal University, Changsha 410081, China; b Institute of Physics, Hunan Normal University, Changsha 410081, China;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--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.
Received: 17 October 2007
Revised: 26 December 2007
Published: 09 July 2008
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, Wang Yong-Jiu Orbital effect in the stationary axisymmetric field 2008 Chin. Phys. B 17 2356
