{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:KDJH4HOYPHYB4BJSQ362GE4QNF","short_pith_number":"pith:KDJH4HOY","schema_version":"1.0","canonical_sha256":"50d27e1dd879f01e053286fda31390695bf6e3f37d672fcdcd3f44f2a4de93e6","source":{"kind":"arxiv","id":"2211.17225","version":2},"attestation_state":"computed","paper":{"title":"Weak Cosmic Censorship and Second Law of Black Hole Thermodynamics in Higher Derivative Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Bo Ning, Feng-Li Lin, Yanbei Chen","submitted_at":"2022-11-30T18:27:09Z","abstract_excerpt":"Infalling matter may destroy a black hole and expose the naked singularity. Thus, Penrose proposed the weak cosmic censorship conjecture to avoid such a possibility. On the other hand, if the black hole is not destroyed by infalling matter, from the second law of black hole thermodynamics, the black hole entropy should increase due to the information carried by the infalling matter. In this work, we demonstrate by examples of perturbative near-extremal black holes in higher derivative gravity theories that the second law implies weak cosmic censorship. We also compare our proposal to the one d"},"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":"2211.17225","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-11-30T18:27:09Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"74d2c0e8d284d8012f66bf0cc612defeabe2f490e46d1e3359da63e087d9d870","abstract_canon_sha256":"84122636e7cd8ad842f03103637f7cba2eeae8980bfae9e5530354a5dea7d54c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:34:21.881626Z","signature_b64":"K/Bzg9QGvUeG1IfGVqgz3ZmPzGGicSY6NmHZQbYVqKKJOhtXBtSicBdo0wTg6kyiGowWOq1N4fqceoaFGeLoDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50d27e1dd879f01e053286fda31390695bf6e3f37d672fcdcd3f44f2a4de93e6","last_reissued_at":"2026-07-05T06:34:21.881137Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:34:21.881137Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Weak Cosmic Censorship and Second Law of Black Hole Thermodynamics in Higher Derivative Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Bo Ning, Feng-Li Lin, Yanbei Chen","submitted_at":"2022-11-30T18:27:09Z","abstract_excerpt":"Infalling matter may destroy a black hole and expose the naked singularity. Thus, Penrose proposed the weak cosmic censorship conjecture to avoid such a possibility. On the other hand, if the black hole is not destroyed by infalling matter, from the second law of black hole thermodynamics, the black hole entropy should increase due to the information carried by the infalling matter. In this work, we demonstrate by examples of perturbative near-extremal black holes in higher derivative gravity theories that the second law implies weak cosmic censorship. We also compare our proposal to the one d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.17225","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2211.17225/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2211.17225","created_at":"2026-07-05T06:34:21.881195+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.17225v2","created_at":"2026-07-05T06:34:21.881195+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.17225","created_at":"2026-07-05T06:34:21.881195+00:00"},{"alias_kind":"pith_short_12","alias_value":"KDJH4HOYPHYB","created_at":"2026-07-05T06:34:21.881195+00:00"},{"alias_kind":"pith_short_16","alias_value":"KDJH4HOYPHYB4BJS","created_at":"2026-07-05T06:34:21.881195+00:00"},{"alias_kind":"pith_short_8","alias_value":"KDJH4HOY","created_at":"2026-07-05T06:34:21.881195+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.19535","citing_title":"The First Law and Weak Cosmic Censorship for de Sitter Black Holes","ref_index":72,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF","json":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF.json","graph_json":"https://pith.science/api/pith-number/KDJH4HOYPHYB4BJSQ362GE4QNF/graph.json","events_json":"https://pith.science/api/pith-number/KDJH4HOYPHYB4BJSQ362GE4QNF/events.json","paper":"https://pith.science/paper/KDJH4HOY"},"agent_actions":{"view_html":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF","download_json":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF.json","view_paper":"https://pith.science/paper/KDJH4HOY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.17225&json=true","fetch_graph":"https://pith.science/api/pith-number/KDJH4HOYPHYB4BJSQ362GE4QNF/graph.json","fetch_events":"https://pith.science/api/pith-number/KDJH4HOYPHYB4BJSQ362GE4QNF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF/action/storage_attestation","attest_author":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF/action/author_attestation","sign_citation":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF/action/citation_signature","submit_replication":"https://pith.science/pith/KDJH4HOYPHYB4BJSQ362GE4QNF/action/replication_record"}},"created_at":"2026-07-05T06:34:21.881195+00:00","updated_at":"2026-07-05T06:34:21.881195+00:00"}