Mass (re)distribution for quantum dust cores of black holes
L. Gallerani, A. Mentrelli, A. Giusti, R. Casadio

TL;DR
This paper refines the quantum dust core model of black holes by deriving a mass distribution that incorporates quantum superpositions, resulting in a more accurate and physically consistent description of the black hole's internal structure.
Contribution
It introduces a new mass distribution model that accounts for quantum superpositions across layers, improving upon previous linear profiles and maintaining metric regularity.
Findings
Mass distribution becomes nearly parabolic with quantum superpositions
The refined model shows a non-vanishing tension in the core
Regularity of the metric and causal structure is preserved
Abstract
The collective ground state for a spherical symmetric dust ball has been investigated recently in [R. Casadio, Phys. Lett. B 843 (2023) 138055]. In this study, we refine that model by obtaining a mass distribution that accounts for the superposition of wavefunctions across different layers. The refined mass distribution shows significant deviations from the approximation without quantum superpositions. Specifically, the new nearly parabolic distribution replaces the linear mass profile of the original work, featuring an overall downward concavity, which leads to a non-vanishing tension. Notably, the regularity of the metric and causal structure are preserved in the refined analysis.
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.
