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Thermodynamical Properties of Stationary,Axially Symmetric Non-Kerr Black Holes

Thermodynamical Properties of Stationary,Axially Symmetric Non-Kerr Black Holes
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摘要 The thermodynamical properties of some stationary,axially symmetric non-Kerr black holes possessing mass with multipole moments are discussed.The rotating angularvelocities of this sort of black holes are zero.There exist thermal radiations,and the temper-atures on the event horizons are constants.The existence of naked singularities stronglyinfluences the Hawking temperature at the two poles of the black holes,and enables it tovanish or diverge.It shows that the thermodynamical laws forbid this sort of naked singu-larities to appear,and go so far as to forbid this sort of black holes to form or emerge. The thermodynamical properties of some stationary,axially symmetric non- Kerr black holes possessing mass with multipole moments are discussed.The rotating angular velocities of this sort of black holes are zero.There exist thermal radiations,and the temper- atures on the event horizons are constants.The existence of naked singularities strongly influences the Hawking temperature at the two poles of the black holes,and enables it to vanish or diverge.It shows that the thermodynamical laws forbid this sort of naked singu- larities to appear,and go so far as to forbid this sort of black holes to form or emerge.
机构地区 Department of Physics
出处 《Science China Mathematics》 SCIE 1993年第9期1103-1113,共11页 中国科学:数学(英文版)
基金 Project supported by the Natioal Natural Science Foundation of China.
关键词 BLACK hole thermal radiation SINGULARITY STATIONARY SPACE-TIME black hole thermal radiation singularity stationary space-time
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