- URN to cite this document:
- urn:nbn:de:bvb:355-epub-544366
- DOI to cite this document:
- 10.5283/epub.54436
Abstract
In this paper, we continue the analysis of the effective model of quantum Schwarzschild black holes recently proposed by some of the authors in [1,2]. In the resulting quantum-corrected spacetime the central singularity is resolved by a black-to-white hole bounce, quantum effects become relevant at a unique mass-independent curvature scale, while they become negligible in the low curvature ...
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