Speaker
Mariano Cadoni
(Istituto Nazionale di Fisica Nucleare)
Description
Quantum gravity effects are generally expected to resolve the classical singularity of the Schwarzschild black hole. In this talk we present a general approach to construct effective models for nonsingular black holes and discuss their possible observational signatures.
Primary author
Mariano Cadoni
(Istituto Nazionale di Fisica Nucleare)
