{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1994:P5ZICKLPY5O42PSO72TQR3GKCG","short_pith_number":"pith:P5ZICKLP","schema_version":"1.0","canonical_sha256":"7f7281296fc75dcd3e4efea708ecca1189b91a83179b41839daaf0eae5442f1e","source":{"kind":"arxiv","id":"gr-qc/9405024","version":2},"attestation_state":"computed","paper":{"title":"The Path Integral Formulation of Gravitational Thermodynamics","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"J.D. Brown, J.W. York","submitted_at":"1994-05-09T21:02:34Z","abstract_excerpt":"The first objective of this article is to show that the black hole partition function can be placed on a firm logical foundation by enclosing the black hole in a spatially finite \"box\" or boundary. The presence of the box has the effect of stabilizing the black hole and yields a system with a positive heat capacity. The second objective of this article is to explore the origin of black hole entropy. This is accomplished through the construction of a path integral expression for the density matrix for the gravitational field, and through an analysis of the connection between the density matrix "},"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/9405024","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1994-05-09T21:02:34Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"2ee4c7f31dd209794a77ca1e2ba932242933490f167043c00825014cbfae57f8","abstract_canon_sha256":"461e461b7b464718a5b583fe84b3efda8630c0a8e14a7883340fe37dfa942a74"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:07:25.316276Z","signature_b64":"LGGaZ2oMRS+ZEAUrPc4qVnushO21CUL4Kfr+r2nX7XaU1+GWd+nfCq2ISOP4xK08hqJ4F49whOliKCsa29DdBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7f7281296fc75dcd3e4efea708ecca1189b91a83179b41839daaf0eae5442f1e","last_reissued_at":"2026-07-04T15:07:25.315838Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:07:25.315838Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Path Integral Formulation of Gravitational Thermodynamics","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"J.D. Brown, J.W. York","submitted_at":"1994-05-09T21:02:34Z","abstract_excerpt":"The first objective of this article is to show that the black hole partition function can be placed on a firm logical foundation by enclosing the black hole in a spatially finite \"box\" or boundary. The presence of the box has the effect of stabilizing the black hole and yields a system with a positive heat capacity. The second objective of this article is to explore the origin of black hole entropy. This is accomplished through the construction of a path integral expression for the density matrix for the gravitational field, and through an analysis of the connection between the density matrix "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9405024","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/gr-qc/9405024/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":"gr-qc/9405024","created_at":"2026-07-04T15:07:25.315926+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9405024v2","created_at":"2026-07-04T15:07:25.315926+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9405024","created_at":"2026-07-04T15:07:25.315926+00:00"},{"alias_kind":"pith_short_12","alias_value":"P5ZICKLPY5O4","created_at":"2026-07-04T15:07:25.315926+00:00"},{"alias_kind":"pith_short_16","alias_value":"P5ZICKLPY5O42PSO","created_at":"2026-07-04T15:07:25.315926+00:00"},{"alias_kind":"pith_short_8","alias_value":"P5ZICKLP","created_at":"2026-07-04T15:07:25.315926+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.03469","citing_title":"Thermodynamics in space-times without horizons","ref_index":17,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG","json":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG.json","graph_json":"https://pith.science/api/pith-number/P5ZICKLPY5O42PSO72TQR3GKCG/graph.json","events_json":"https://pith.science/api/pith-number/P5ZICKLPY5O42PSO72TQR3GKCG/events.json","paper":"https://pith.science/paper/P5ZICKLP"},"agent_actions":{"view_html":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG","download_json":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG.json","view_paper":"https://pith.science/paper/P5ZICKLP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9405024&json=true","fetch_graph":"https://pith.science/api/pith-number/P5ZICKLPY5O42PSO72TQR3GKCG/graph.json","fetch_events":"https://pith.science/api/pith-number/P5ZICKLPY5O42PSO72TQR3GKCG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG/action/storage_attestation","attest_author":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG/action/author_attestation","sign_citation":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG/action/citation_signature","submit_replication":"https://pith.science/pith/P5ZICKLPY5O42PSO72TQR3GKCG/action/replication_record"}},"created_at":"2026-07-04T15:07:25.315926+00:00","updated_at":"2026-07-04T15:07:25.315926+00:00"}