Phys. Rev. Lett. 101, 161301 (2008) [4 pages]Black Holes in Loop Quantum Gravity: The Complete Space-Time
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 semiclassical 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–Nordström space-time including a Cauchy horizon is suggested. This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. © 2008 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.161301
DOI:
10.1103/PhysRevLett.101.161301
PACS:
04.60.Pp, 04.20.Gz
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