Gravitomagnetism in the Kerr-Newman-Taub-NUT spacetime

被引:53
作者
Bini, D [1 ]
Cherubini, C
Jantzen, RT
Mashhoon, B
机构
[1] CNR, Ist Applicaz Calcado M Picone, I-00161 Rome, Italy
[2] Univ Rome, Int Ctr Relativist Astrophys, I-00185 Rome, Italy
[3] Villanova Univ, Dept Math Sci, Villanova, PA 19085 USA
[4] Univ Salerno, Dipartimento Fis ER Caianiello, I-84081 Baronissi, Italy
[5] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
[6] Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA
关键词
D O I
10.1088/0264-9381/20/3/305
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the motion of test particles and electromagnetic waves in the Kerr-Newman-Taub-NUT spacetime in order to elucidate some of the effects associated with the gravitomagnetic monopole moment of the source. In particular, we determine in the linear approximation the contribution of this monopole to the gravitational time delay and the rotation of the plane of the polarization of electromagnetic waves. Moreover, we consider 'spherical' orbits of uncharged test particles in the Kerr-Taub-NUT spacetime and discuss the modification of the Wilkins orbits due to the presence of the gravitomagnetic monopole.
引用
收藏
页码:457 / 468
页数:12
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