{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:P2UMTAYZ65MF5ZZKINNV4S3OMI","short_pith_number":"pith:P2UMTAYZ","schema_version":"1.0","canonical_sha256":"7ea8c98319f7585ee72a435b5e4b6e622bee151e82e72df157d823432327ce91","source":{"kind":"arxiv","id":"gr-qc/9804058","version":1},"attestation_state":"computed","paper":{"title":"Quantum corrections to critical phenomena in gravitational collapse","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Adrian C Ottewill, Patrick R Brady","submitted_at":"1998-04-23T00:18:57Z","abstract_excerpt":"We investigate conformally coupled quantum matter fields on spherically symmetric, continuously self-similar backgrounds. By exploiting the symmetry associated with the self-similarity the general structure of the renormalized quantum stress-energy tensor can be derived. As an immediate application we consider a combination of classical, and quantum perturbations about exactly critical collapse. Generalizing the standard argument which explains the scaling law for black hole mass, $M \\propto |\\eta-\\eta^*|^\\beta$, we demonstrate the existence of a quantum mass gap when the classical critical ex"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"gr-qc/9804058","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1998-04-23T00:18:57Z","cross_cats_sorted":[],"title_canon_sha256":"1df8f92a9f8d6ddbc4ae62a6bfb2035b918c453a4af5c5b5e20bbbbe9d94b977","abstract_canon_sha256":"d601787faaf7c0c057967f13b7ec4ab00c6dabaedb2bba4a5bd589185a06f5f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:35:33.770477Z","signature_b64":"vFRJ+hevSc/fHHefBsQgR9AglGSZ5mZMGjQGAzCdlmc5lGw4Kk5r+qpPlJKz8ZIgUqD3UHlrKK3OGljUZ4wRDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7ea8c98319f7585ee72a435b5e4b6e622bee151e82e72df157d823432327ce91","last_reissued_at":"2026-05-18T04:35:33.769790Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:35:33.769790Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum corrections to critical phenomena in gravitational collapse","license":"","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Adrian C Ottewill, Patrick R Brady","submitted_at":"1998-04-23T00:18:57Z","abstract_excerpt":"We investigate conformally coupled quantum matter fields on spherically symmetric, continuously self-similar backgrounds. By exploiting the symmetry associated with the self-similarity the general structure of the renormalized quantum stress-energy tensor can be derived. As an immediate application we consider a combination of classical, and quantum perturbations about exactly critical collapse. Generalizing the standard argument which explains the scaling law for black hole mass, $M \\propto |\\eta-\\eta^*|^\\beta$, we demonstrate the existence of a quantum mass gap when the classical critical ex"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9804058","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"gr-qc/9804058","created_at":"2026-05-18T04:35:33.769900+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9804058v1","created_at":"2026-05-18T04:35:33.769900+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9804058","created_at":"2026-05-18T04:35:33.769900+00:00"},{"alias_kind":"pith_short_12","alias_value":"P2UMTAYZ65MF","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_16","alias_value":"P2UMTAYZ65MF5ZZK","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_8","alias_value":"P2UMTAYZ","created_at":"2026-05-18T12:25:49.038998+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2509.03584","citing_title":"Unveiling horizons in quantum critical collapse","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2509.03587","citing_title":"Quantum Critical Collapse Abhors a Naked Singularity","ref_index":26,"is_internal_anchor":true},{"citing_arxiv_id":"2509.03584","citing_title":"Unveiling horizons in quantum critical collapse","ref_index":69,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI","json":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI.json","graph_json":"https://pith.science/api/pith-number/P2UMTAYZ65MF5ZZKINNV4S3OMI/graph.json","events_json":"https://pith.science/api/pith-number/P2UMTAYZ65MF5ZZKINNV4S3OMI/events.json","paper":"https://pith.science/paper/P2UMTAYZ"},"agent_actions":{"view_html":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI","download_json":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI.json","view_paper":"https://pith.science/paper/P2UMTAYZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9804058&json=true","fetch_graph":"https://pith.science/api/pith-number/P2UMTAYZ65MF5ZZKINNV4S3OMI/graph.json","fetch_events":"https://pith.science/api/pith-number/P2UMTAYZ65MF5ZZKINNV4S3OMI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI/action/storage_attestation","attest_author":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI/action/author_attestation","sign_citation":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI/action/citation_signature","submit_replication":"https://pith.science/pith/P2UMTAYZ65MF5ZZKINNV4S3OMI/action/replication_record"}},"created_at":"2026-05-18T04:35:33.769900+00:00","updated_at":"2026-05-18T04:35:33.769900+00:00"}