构造黑洞互补性的一个反例
Constructing a counterexample to the black hole complementarity
摘要：
我们提出了一个规则的黑洞，它的内部产生一个德西特空间，然后最终被挫折成一个奇点。这是一个修改后的模型，最初是由Frolov，马尔可夫和Mukhanov提出。在我们的模型中，我们可以调整一个规则的黑洞，使其进入极端状态之前的时间远远长于信息保留时间。在此期间，可能存在一个观察者，他观察到霍金辐射的信息，自由地落入黑洞的规则中心，并最终再次遇到自由下落的信息。这样一个观测者的存在意味着互补的观点可能与规则的黑洞不一致，因此，不适合作为黑洞物理学的一般原理。
英文摘要：
We propose a regular black hole whose inside generates a de Sitter space and then is finally frustrated into a singularity. It is a modified model which was suggested originally by Frolov, Markov, and Mukhanov. In our model, we could adjust a regular black hole so that its period before going into the extreme state is much longer than the information retention time. During this period an observer could exist who observes the information of the Hawking radiation, falls freely into the regular center of the black hole, and finally meets the free-falling information again. The existence of such an observer implies that the complementary view may not be consistent with a regular black hole, and therefore, is not appropriate as a generic principle of black hole physics.
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