Black hole evaporation: a paradigm
Black hole evaporation: a paradigm
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DOI：
10.1088/0264-9381/22/16/014
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发表时间：
2005-08-21
影响因子：
3.5
通讯作者：
Bojowald, M
中科院分区：
文献类型：
--
作者：
Ashtekar, A;Bojowald, M
通过组合两组，开发了描述非微扰量子引力中黑洞蒸发的范式。详细结果：（i）使用史瓦西奇点来解决。量子几何方法和（ii）捕获和动态视界框架中黑洞的时间演化。量子几何效应介绍。对黑洞蒸发的传统时空图进行了重大修改，为恢复在黑洞形成过程中经典丢失的信息提供了一种可能的机制。该范式直接在洛伦兹体系中发展，并讨论了其可行性的必要条件。如果满足这些条件，基于时空几何的期望与量子理论结构之间的大部分紧张关系将得到解决。
A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by combining two sets. of detailed results: (i) resolution of the Schwarzschild singularity using. quantum geometry methods and (ii) time evolution of black holes in the trapping and dynamical horizon frameworks. Quantum geometry effects introduce. a major modification in the traditional spacetime diagram of black hole evaporation, providing a possible mechanism for recovery of information that is classically lost in the process of black hole formation. The paradigm is developed directly in the Lorentzian regime and necessary conditions for its viability are discussed. If these conditions are met, much of the tension between expectations based on spacetime geometry and structure of quantum theory would be resolved.