TL;DR
This paper examines a semiclassical spacetime foam model with two wormhole types, exploring area quantization and entropy implications, and discusses applications to charged black holes.
Contribution
It introduces a model with Schwarzschild and Schwarzschild-Anti-de Sitter wormholes to analyze entropy and potential configuration selection.
Findings
Area quantization suggests a preference between wormhole configurations.
Application to charged black holes provides insights into their entropy.
The model offers a semiclassical approach to spacetime foam analysis.
Abstract
A simple model of spacetime foam, made by two different types of wormholes in a semiclassical approximation, is taken under examination: one type is a collection of Schwarzschild wormholes, while the other one is made by Schwarzschild-Anti-de Sitter wormholes. The area quantization related to the entropy via the Bekenstein-Hawking formula hints a possible selection between the two configurations. Application to the charged black hole are discussed.
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.