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
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
