Semiclassical one-loop analysis of solvable near-critical collapse solutions shows quantum corrections selecting a Boulware-like state and producing a growing mode that yields a finite mass gap and a transition to Type I behavior, enforcing weak cosmic censorship.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
fields
gr-qc 2verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
The Liouville solution in GR with scalar field and exponential potential describes spherically symmetric black hole formation with the horizon expanding at light speed from infinitesimal size at finite time, and mass proportional to time squared.
citing papers explorer
-
Black hole formation by a scalar field
The Liouville solution in GR with scalar field and exponential potential describes spherically symmetric black hole formation with the horizon expanding at light speed from infinitesimal size at finite time, and mass proportional to time squared.