Speaker
Carlo Rovelli
(Centre de Physique Théorique (CPT))
Description
Quantum gravitational phenomena dominate the physics of a black hole in the past of a high curvature spacelike surface. Because of the backreaction of the evaporation, this surface crosses the horizon. I describe a recent line of investigation on the possible evolution compatible with nonperturbative quantum gravity, and in particular I illustrate what can be predicted using loop quantum gravity.
External references
- 23050133
- 7cfc3241-c973-45cc-8fc5-6d19f9e680ad
- c9e89ca1-0ee2-417d-a498-50a50d64392b
