Static Black Holes With Back Reaction From Vacuum Energy

Abstract

We study spherically symmetric static solutions to the semi-classical Einstein equation sourced by the vacuum energy of quantum fields in the curved space-time of the same solution. We found solutions that are small deformations of the Schwarzschild metric for distant observers, but without horizon. Instead of being a robust feature of objects with high densities, the horizon is sensitive to the energy-momentum tensor in the near-horizon region.

40 pages, 14 figures. v2: 43 pages, minor modifications, references added

References in corpus (12)

• The fuzzball proposal for black holes
• A Primer for Black Hole Quantum Physics
• Gravity solutions for the D1-D5 system with angular momentum
• Fate of gravitational collapse in semiclassical gravity
• Observation of Incipient Black Holes and the Information Loss Problem
• Backreaction of Hawking Radiation on a Gravitationally Collapsing Star I: Black Holes?
• Phenomenological Description of the Interior of the Schwarzschild Black Hole
• Do event horizons exist?
• Asymptotic Black Holes
• Cosmon Lumps and Horizonless Black Holes
• Horizon avoidance in spherically-symmetric collapse
• Generalized Virasoro anomaly for dilaton coupled theories

Cited by in corpus (27)

• Phenomenological aspects of black holes beyond general relativity
• The quantum fate of black hole horizons
• Schwarzschild geometry counterpart in semiclassical gravity
• Semiclassical constant-density spheres in a regularized Polyakov approximation
• Quantum corrections to the Schwarzschild metric from vacuum polarization
• Static Black Hole and Vacuum Energy: Thin Shell and Incompressible Fluid
• Black Hole as a Quantum Field Configuration
• Ultracompact horizonless objects in order-reduced semiclassical gravity
• On the Near-Horizon Geometry of an Evaporating Black Hole
• Reissner-Nordström geometry counterpart in semiclassical gravity
• An Analytic Description of Semi-Classical Black-Hole Geometry
• Back Reaction of 4D Conformal Fields on Static Geometry
• Quantum-corrected geometry of horizon vicinity
• Islands in Non-Minimal Dilaton Gravity: Exploring Effective Theories for Black Hole Evaporation
• Asymptotically flat vacuum solutions in order-reduced semiclassical gravity
• Entanglement entropy and vacuum states in Schwarzschild geometry
• Firewall From Effective Field Theory
• Unveiling horizons in quantum critical collapse
• Singularity resolution in spherically reduced 2D semiclassical gravity with negative central charge
• Quantum Critical Collapse Abhors a Naked Singularity
• Dynamical evolution and stability of quantum corrected Schwarzschild black holes in semiclassical gravity
• Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity
• An Ultra-compact Object from Semi-classical Gravity
• Imprints of quantum vacuum fluctuations on the gravitational field of a spherical mass
• Macroscopic backreaction of the trace anomaly on classical vacuum backgrounds
• Dynamical wormholes
• Trace anomaly contributions to semi-classical wormhole geometries