Revisiting the semiclassical gravity scenario for gravitational collapse
C. Barcelo, S. Liberati, S. Sonego, M. Visser

TL;DR
This paper explores whether observed dark, compact objects are true black holes by revisiting semiclassical gravity, proposing alternative collapse outcomes that could replace classical black holes.
Contribution
It introduces a revised semiclassical collapse scenario suggesting the formation of alternative compact objects instead of traditional black holes.
Findings
Alternative objects could form from stellar collapse.
These objects may explain observations without classical black hole issues.
Revises understanding of gravitational collapse in semiclassical gravity.
Abstract
The existence of extremely dark and compact astronomical bodies is by now a well established observational fact. On the other hand, classical General Relativity predicts the existence of black holes which fit very well with the observations, but do lead to important conceptual problems. In this contribution we ask ourselves the straightforward question: Are the dark and compact objects that we have observational evidence for black holes in the sense of General Relativity? By revising the semiclassical scenario of stellar collapse we find out that as the result of a collapse some alternative objects could be formed which might supplant black holes.
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.
