Resolving Black Holes singularities in Analytic infinite derivative theories of gravity

In my talk I will show that Analytic infinite derivative gravity in any dimension represents the most general gravity action ever needed to extract propagator around maximally symmetric spacetimes. Moving on, I will show that such a theory is geodesically complete leading to the resolution of the Black Hole singularities. Thus singular blackholes (Schwarzschild as an example) can be understood as non-singular compact objects still with a horizon, whose core is governed by the mass and the effective scale of the non-locality.