REVIEW 2 cited by
Black Holes at Exp-time
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Classical GR governs the evolution of black holes for a long time, but at some exponentially large time it must break down. The breakdown, and what comes after it, is not well understood. In this paper I'll discuss the problem using concepts drawn from complexity geometry. In particular the geometric concept of cut locus plays a key role.
Forward citations
Cited by 2 Pith papers
-
Tight bounds on recurrence time in closed quantum systems
For any finite-dimensional Hamiltonian and initial pure state, the first recurrence time obeys t_rec ≤ t_exit (4π/ε)^{d-1}, with an explicit inverse quantum speed limit bound on t_exit.
-
Evaporating Black Hole Interior and Complexity Evolution
In JT gravity with an end-of-the-world brane, the renormalized interior length — read as subsystem complexity — grows linearly, peaks around the Page time, and then decays exponentially, with growing relative fluctuat...
Discussion (0). Continue with ORCID to comment.