Black hole horizon and space-time foam
A. G. Agnese, M. La Camera
TL;DR
This paper explores how quantum-scale space-time fluctuations near a black hole's event horizon, modeled via Brans-Dicke scalar fields, can significantly impact black hole physics.
Contribution
It introduces a novel approach using Brans-Dicke scalar fields to model Planck-scale fluctuations at black hole horizons.
Findings
Space-time foam effects are significant near black hole horizons.
Scalar field modeling reveals dramatic impacts on black hole properties.
Abstract
We introduce, by means of the Brans-Dicke scalar field, space-time fluctuations at scale comparable to Planck length near the event horizon of a black hole and examine their dramatic effects.
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
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory