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At the end of Hawking evaporation, the horizon of a black hole enters a physical region where quantum gravity cannot be neglected.
1903
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C. Rovelli and F. Vidotto, “Planck stars,” Int. J. Mod. Phys. D
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A. Barrau, C. Rovelli, and F. Vidotto, “Fast radio bursts and white hole signals,” Physical Review D
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M. Christodoulou and C. Rovelli, “How big is a black hole?,” Physical Review D
2015
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I. Bengtsson and E. Jakobsson, “Black holes: Their large interiors,” Mod. Phys. Lett. A
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C. Rovelli and F. Vidotto, Covariant loop quantum gravity: An elementary introduction to quantum gravity and spinfoam theory · 2015
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M. Christodoulou and T. De Lorenzo, “Volume inside old black holes,” Physical Review D
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C. Rovelli and F. Vidotto, “Small black/white hole stability and dark matter,” Universe
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2019
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