Original Articles |
|
|
|
|
Distribution Characteristics of Dirac Energy Levels in Non-Kerr Space-time |
YANG Xue-Te1;YANG Shu-Zheng2 |
1Department of Physics, Neijiang Teachers College, Neijiang 641112
2Department of Physics, Sichuan Teachers College, Nanchong 637002
|
|
Cite this article: |
YANG Xue-Te, YANG Shu-Zheng 2002 Chin. Phys. Lett. 19 1752-1754 |
|
|
Abstract The distribution of Dirac energy levels in a non-Kerr black hole space-time is related to an arbitrary set of multiple moments determined by the parameters αn. A singular point appears on the event horizon of the black hole, at which the Dirac energy levels have obvious distribution characteristics and are different from those in the space-time of the Kerr black hole.
|
Keywords:
04.70.-s
95.10.Ce
|
|
Published: 01 December 2002
|
|
PACS: |
04.70.-s
|
(Physics of black holes)
|
|
95.10.Ce
|
(Celestial mechanics (including n-body problems))
|
|
|
|
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|