Chin. Phys. Lett.  2006, Vol. 23 Issue (4): 783-785    DOI:
Original Articles |
Rediscussion of the Stability Problem of the Schwarzschild Black Hole
Tian Gui-Hua
School of Science, Beijing University of Posts and Telecommunications, Beijing 100876 Academy of Mathematics and Systems Science, Chinese Academy of Sciences, Beijing 100080
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Tian Gui-Hua 2006 Chin. Phys. Lett. 23 783-785
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Abstract We use the Kruskal time coordinate T to define the initial time. By this way, the stability study naturally becomes the one connected with the two regions, i.e. the white-hole-connected region and the black-hole-connected region. The union of the two regions covers the Schwarzschild space-time (r≥2m). We also obtain the very reasonable conclusion: the white-hole-connected region is unstable and the black-hole-connected region is stable. If we take the instability with caution and seriousness, it is not unreasonable to regard that the Schwarzschild black hole might be unstable to some extent.
Keywords: 04.20.-q      04.07.Bw      97.60.-s     
Published: 01 April 2006
PACS:  04.20.-q (Classical general relativity)  
  04.07.Bw  
  97.60.-s (Late stages of stellar evolution (including black holes))  
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https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2006/V23/I4/0783
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