The Effective Theory of Quantum Black Holes

Abstract

We explore the quantum nature of black holes by introducing an effective framework that takes into account deviations from the classical results. The approach is based on introducing quantum corrections to the classical Schwarzschild geometry in a way that is consistent with the physical scales of the black hole and its classical symmetries. This is achieved by organizing the quantum corrections in inverse powers of a physical distance. By solving the system in a self-consistent way we show that the derived physical quantities, such as event horizons, temperature and entropy can be expressed in a well defined expansion in the inverse powers of the black hole mass. The approach captures the general form of the quantum corrections to black hole physics without requiring to commit to a specific model of quantum gravity.

Revised version matching the published one

References in corpus (6)

• Dynamical renormalization of black-hole spacetimes
• Non-local quantum effects in cosmology 1: Quantum memory, non-local FLRW equations and singularity avoidance
• Non-Local Gravity Cosmology: an Overview
• Sifting quantum black holes through the principle of least action
• Gravitational waves in non-local gravity
• Marginally Deformed Starobinsky Gravity

Cited by in corpus (5)

• Quasinormal modes and gray-body factors of regular black holes in asymptotically safe gravity
• Traces of quantum gravitational correction at third-order curvature through the black hole shadow and particle deflection at the weak field limit
• Spacetime-curvature induced uncertainty principle: linking the large-structure global effects to the local black hole physics
• Entanglement entropy in quantum black holes
• Positivity Conditions for Generalised Schwarzschild Space-Times