Quantum Gravity effects near the null black hole singularity
Alfio Bonanno, Martin Reuter
Abstract
The structure of the Cauchy Horizon singularity of a black hole formed in a generic collapse is studied by means of a renormalization group equation for quantum gravity. It is shown that during the early evolution of the Cauchy Horizon the increase of the mass function is damped when quantum fluctuations of the metric are taken into account.
Create a lesson
Related papers
Spiral galaxy spacetime in extended scalar-tensor-Gauss-Bonnet gravity coupled to nonlinear electrodynamics
Pedro Cañate
Quasinormal modes of rotating black holes with ultralight scalar fields
Leif Lui, Adrian Ka-Wai Chung
Probing black holes extremality bounds with non-extensive entropies
Javier Cancino, Roberto Santos-Silva, Pablo Carlos López Vázquez et al.
Finite-Time Bounds on Conformal Vacuum Energy Relaxation in Scalar-Tensor Gravity
Yousef Bisabr
Boundary-induced corrections to the response of an Unruh-DeWitt detector outside a compact star with Robin surface conditions
Nodirbek Anarboev, Javlonbek Khasanov, Javlon Rayimbaev et al.
Primordial Graviton Entanglement in Quasicrystalline Inflation
Jiro Soda