Quantum Improved Schwarzschild-(A)dS and Kerr-(A)dS Space-times

Understand

We discuss quantum black holes in asymptotically safe quantum gravity with a scale identification based on the Kretschmann scalar.

• After comparing this scenario with other scale identifications, we investigate in detail the Kerr-(A)dS and Schwarzschild-(A)dS space-times.
• The global structure of these geometries is studied as well as the central curvature singularity and test particle trajectories.
• The existence of a Planck-sized, extremal, zero temperature black hole remnant guarantees a stable endpoint of the evaporation process via Hawking radiation.