Beyond Einstein's Horizon: Gravitational Condensates and Black Hole Interiors in the Effective Theory of Gravity
Emil Mottola

TL;DR
This paper proposes an effective field theory of quantum gravity that resolves black hole singularities and explains dark energy through gravitational condensates influenced by quantum matter anomalies.
Contribution
It introduces a novel EFT framework incorporating conformal anomalies and a 3-form gauge field to produce non-singular black hole interiors and variable dark energy.
Findings
Non-singular black hole interiors predicted
A gravitational condensate star replaces the event horizon
Testable predictions for gravitational waves and cosmology
Abstract
Two of the most fundamental problems at the nexus of Einstein's classical General Relativity (GR) and Quantum Field Theory (QFT) are: (1) complete gravitational collapse, presumed in classical GR to lead to a Black Hole (BH) horizon and interior singularity, which generate a number of paradoxes for quantum theory; and (2) the origin and magnitude of the cosmological dark energy driving the accelerated expansion of the Universe. In this Snowmass white paper it is proposed that these twin puzzles on disparate scales are related, and that their resolution depends upon taking full account of the conformal anomaly of quantum matter in gravitational fields. The topological term in the anomaly leads naturally to the introduction of an abelian -form gauge field, whose field strength can account for a variable gravitational condensate with the vacuum dark energy equation of state ,…
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 · Relativity and Gravitational Theory · Noncommutative and Quantum Gravity Theories
