Gravitational collapses and Hilbertian repulsion
A. Loinger, T. Marsico

TL;DR
This paper explores how incorporating Hilbertian gravitational repulsion alters the classical understanding of gravitational collapse, suggesting that collapsing dust spheres may form finite-sized bodies instead of singularities.
Contribution
It introduces the concept of Hilbertian gravitational repulsion into collapse models, proposing a finite outcome for dust sphere collapse.
Findings
Collapse results in finite-sized bodies due to repulsion
Hilbertian repulsion prevents singularity formation
Revises classical collapse models
Abstract
If we take into account the Hilbertian gravitational repulsion, even a dust sphere with a zero fluido-dynamical pressure collapses to a body of a comparatively small, finite, volume.
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 · Quantum Electrodynamics and Casimir Effect
