Looking Inside a Black Hole
arXiv:1309.4125 · doi:10.1088/0264-9381/31/8/082001
Abstract
The cosmic censorship conjecture posits that singularities forming to the future of a regular Cauchy surface are hidden by an event horizon. Consequently any topological structures will ultimately collapse within the horizon of a set of black holes and so no observer can actively probe them classically. We consider here a quantum analog of this problem, in which we compare the transition rates of an Unruh-DeWitt detector placed outside the horizon of an eternal BTZ black hole and its associated geon counterpart. We find the transition rates differ, with the latter being time-dependent, implying that we are indeed able to probe the structure of the singularity from outside the Killing horizon.
5 pages, 3 figures
References in corpus (2)
Cited by in corpus (24)
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