Abstract In the spacetime of a charged spinning black hole, the distribution of particle energy levels has been studied. Near the event horizon of such a black hole a crossing of the particle energy levels exists, which leads to the occurrence of non-thermal radiation of the black hole. This quantum effect is non-thermal and also different from those of the Kerr and Kerr-Newman black holes.
Received: 17 October 2000
Revised: 23 April 2001
Accepted manuscript online:
Xie Shi-chong (谢实崇), Yang Xue-te (杨雪特), Yang Shu-zheng (杨树政), Lin Li-bin (林理彬) NON-THERMAL RADIATION FROM A NON-KERR-NEWMAN BLACK HOLE 2001 Chinese Physics 10 979
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