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
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
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.
(Late stages of stellar evolution (including black holes))
引用本文:
Tian Gui-Hua. Rediscussion of the Stability Problem of the Schwarzschild Black Hole[J]. 中国物理快报, 2006, 23(4): 783-785.
Tian Gui-Hua. Rediscussion of the Stability Problem of the Schwarzschild Black Hole. Chin. Phys. Lett., 2006, 23(4): 783-785.
2006, Vol. 23 
