Distribution Characteristics of Dirac Energy Levels in Non-Kerr Space-time

Chin. Phys. Lett.

2002, Vol. 19

Issue (12): 1752-1754 DOI:

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

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YANG Xue-Te, YANG Shu-Zheng 2002 Chin. Phys. Lett. 19 1752-1754

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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 α_n. 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))

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y2002/V19/I12/01752

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