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Black holes in loop quantum gravity: the complete space-time
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We consider the quantization of the complete extension of the Schwarzschild space-time using spherically symmetric loop quantum gravity. We find an exact solution corresponding to the semi-classical theory. The singularity is eliminated but the space-time still contains a horizon. Although the solution is known partially numerically and therefore a proper global analysis is not possible, a global structure akin to a singularity-free Reissner--Nordstr\"om space-time including a Cauchy horizon is suggested.
Forward citations
Cited by 3 Pith papers
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