{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.revision/1","content_sha256":"4a3725a178f7532d9d624a3dfa33871dc43647016bf97a2c63ad1e5d254ffae5","created":"2026-10-03T07:18:04Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":["5475cf5dc5b1a72283d26dc95dc6e00d7ea4e00096a7c6492e409a1816eeb011"],"salt":"2e39e1d345d3166aaf6780f3545580c0ed2f71028a2e8619404e47225e160cf1","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"revision"},"content":{"answer_type":"mechanism","assisted_by":[],"external_id":"grav.singularities-censorship.quantum-resolution","kind":"phenomenon","literature_status":"open","n":"1","parents":[],"plain":"General relativity predicts that everything inside a black hole ends at a singularity after a finite time. A quantum theory of gravity should replace this with something finite, but no calculation shows what.","posed_since":"","precise":"In a UV-complete framework, for example AdS/CFT for large AdS-Schwarzschild black holes, identify observables sensitive to the $r = 0$ spacelike singularity (such as the light-cone singularity of boundary correlators on a secondary sheet found by Fidkowski, Hubeny, Kleban and Shenker in 2004) and determine how finite-$N$ and finite-coupling effects modify them. An answer is an exact or controlled computation of such an observable showing whether the singularity is smoothed, replaced by a bounce, or remains an endpoint of semiclassical time.","problem_ref":null,"references":"","settled_by":"A non-perturbative computation of a boundary observable that probes the singularity, carried beyond leading order in 1/N.","status_note":"","title":"What replaces the Schwarzschild singularity in quantum gravity?","topic_ref":"8b19c125ce8ffc5355cad7a14e54dbe37cd8a883144325702998d078b535110b"},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"a8dcf6def711bf8e1e41f8e5102f6c4087952938994c345c63252683be7dc7c9","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"f36ced77bf8ea6bdd36f8b6ceec7cce0de2cba859b5080241cc2d2d3f03aa68f","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"HO_Pw8Z9zyFJrqGEaigul6vanKdNujsirIPB-wKMuNlbIoaH-qaMP_hIutdvGJ88FCDXbynrEUlvjt61CrOOCQ"},"schema":"pubphys.envelope/1"},"record_hash":"a8dcf6def711bf8e1e41f8e5102f6c4087952938994c345c63252683be7dc7c9","leaf_index":1505}