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.
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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.
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Unveiling horizons in quantum critical collapse
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.
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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.