The stable problem in the Rindler space-time

Tian Gui-hua; Shi-kun Wang; Shuquan Zhong

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The stable problem in the Rindler space-time

Tian Gui-hua·Shi-kun Wang·Shuquan Zhong

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Abstract

We carefully study the stable problem of the Rindler space time by the scalar wave perturbation. Using the two different coordinate systems, the scalar wave equation is investigated. The results are different in these two cases. They are analyzed and compared in detail. The conclusions are: (a) the Rindler space time as a whole is not stable; (b) the Rindler space time could exist stably only as a part of the Minkowski space time, and the Minkowski space time could be a real entity independently; (c) there are some defects for the scalar wave equation written by the Rindler coordinates, and it is unsuitable for investigation of the stable properties of the Rindler space time. All these results might shed some lights on the stable properties of the Schwarzschild black hole. It is natural and not unreasonable for one to infer that: (a) perhaps the Regge-Wheeler equation is not sufficient to decide the stable properties; (b) the Schwarzschild black hole as a whole might be really unstable; (c) the Kruskal space time is stable and can exist as a real physical entity ; whereas the Schwarzschild black hole could occur only as part of the Kruskal space time.

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Tian Gui-hua, Shi-kun Wang, Shuquan Zhong. 2006-08-09. The stable problem in the Rindler space-time. https://arxiv.org/abs/gr-qc/0608045

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