Phys. Rev. D 79, 061501(R) (2009) [5 pages]Complete single-horizon quantum corrected black hole spacetime
We show that a semiclassical polymerization of the interior of Schwarzschild black holes gives rise to a tantalizing candidate for a nonsingular, single-horizon black hole spacetime. The exterior has nonzero quantum stress energy but closely approximates the classical spacetime for macroscopic black holes. The interior exhibits a bounce at a microscopic scale and then expands indefinitely to a Kantowski-Sachs spacetime. Polymerization therefore removes the singularity and produces a scenario reminiscent of past proposals for universe creation via quantum effects inside a black hole. © 2009 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.061501
DOI:
10.1103/PhysRevD.79.061501
PACS:
04.70.Dy, 04.50.Gh, 04.60.Pp
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