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Approach to a Cauchy Problem in Stability Study of the Schwarzschild Black Hole

Approach to a Cauchy Problem in Stability Study of the Schwarzschild Black Hole
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摘要 Generally, the Schwarzschild black hole is proven to be stable by two different methods: the mode-decomposition method and the integral method. We show that the integral method can only apply to the initial data vanishing at both the horizon and the spatial infinity. It can not treat the initial data only vanishing at the spatial infinity. We give an example to show the misleading information caused by the use of tortoise coordinates in the perturbation equations. Subsequently, the perturbation equations in the Schwarzschild coordinates are shown to be insuftlcient for the stability study. Generally, the Schwarzschild black hole is proven to be stable by two different methods: the mode-decomposition method and the integral method. We show that the integral method can only apply to the initial data vanishing at both the horizon and the spatial infinity. It can not treat the initial data only vanishing at the spatial infinity. We give an example to show the misleading information caused by the use of tortoise coordinates in the perturbation equations. Subsequently, the perturbation equations in the Schwarzschild coordinates are shown to be insuftlcient for the stability study.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2007年第6期1475-1478,共4页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundations of China under Grant Nos 10475013, 10373003, and 10375087, the National Key Basic Research Programme of China under Grant No 2004CB318000.
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