4D Weyl Anomaly and Diversity of the Interior Structure of Quantum Black Hole
Pei-Ming Ho, Hikaru Kawai, Henry Liao, Yuki Yokokura

TL;DR
This paper investigates the interior geometries of 4D quantum black holes using semi-classical Einstein equations with Weyl anomaly, revealing diverse structures that relate to black hole entropy.
Contribution
It introduces a non-perturbative analysis of interior black hole geometries considering Weyl anomaly, showing a variety of possible structures without horizons or singularities.
Findings
Identifies four types of asymptotic interior behaviors.
Derives a class of geometries with diverse structures.
Connects the number of interior patterns to Bekenstein-Hawking entropy.
Abstract
We study the interior metric of 4D spherically symmetric static black holes by using the semi-classical Einstein equation and find a consistent class of geometries with large curvatures. We approximate the matter fields by conformal fields and consider the contribution of the 4D Weyl anomaly, giving a state-independent constraint. Combining this with an equation of state yields an equation that determines the interior geometry completely. We explore the solution space of the equation in a non-perturbative manner for . First, we find four types of asymptotic behaviors and examine the general features of the solutions. Then, by imposing physical conditions, we obtain approximately a general class of interior geometries: various combinations of dilute and dense structures without a horizon or singularity. This represents the diversity of the interior structure. Finally, we show that…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
