{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:PHMHNTTP5GRNU7IFG7JJS7GB4X","short_pith_number":"pith:PHMHNTTP","schema_version":"1.0","canonical_sha256":"79d876ce6fe9a2da7d0537d2997cc1e5e4ab5f43d190ad9a1436bbbfefe1fcbd","source":{"kind":"arxiv","id":"1902.00825","version":1},"attestation_state":"computed","paper":{"title":"Quasilocal Smarr relations for static black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"F. D. Villalba, P. Bargue\\~no","submitted_at":"2019-02-03T01:25:32Z","abstract_excerpt":"Generalized Smarr relations in terms of quasilocal variables are obtained for Schwarzschild and Reissner-Nordstr\\\"om black holes. The approach is based on gravitational path integrals with finite boundaries on which, following Brown and York, thermodynamic variables are identified through a Hamilton-Jacobi analysis of the action. The resulting expressions allow us to construct the relation between the quasilocal energy obtained in this setting and the Komar and Misner-Sharp energies, which are regarded as thermodynamical internal energy in other approaches. The quasilocal Smarr relation is obt"},"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":"1902.00825","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-02-03T01:25:32Z","cross_cats_sorted":[],"title_canon_sha256":"ef3d7cdaa28ecf2c5b546d5c0d4df7a70170ee1683cda3818e152b1a3e520792","abstract_canon_sha256":"bfd04d6fd8270218eb858c0db0deef62bfff97b0253a80d80736e8e5ed7c90f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:53:41.068904Z","signature_b64":"WsSqJ803B2LYSvW++2GL+Gg9Y7KVlMTLOj+7RezYuhFhH2e6eFT+kNRe140Z9pOTY93wzW8sbwUEbHetVzUwDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79d876ce6fe9a2da7d0537d2997cc1e5e4ab5f43d190ad9a1436bbbfefe1fcbd","last_reissued_at":"2026-05-17T23:53:41.068461Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:53:41.068461Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasilocal Smarr relations for static black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"F. D. Villalba, P. Bargue\\~no","submitted_at":"2019-02-03T01:25:32Z","abstract_excerpt":"Generalized Smarr relations in terms of quasilocal variables are obtained for Schwarzschild and Reissner-Nordstr\\\"om black holes. The approach is based on gravitational path integrals with finite boundaries on which, following Brown and York, thermodynamic variables are identified through a Hamilton-Jacobi analysis of the action. The resulting expressions allow us to construct the relation between the quasilocal energy obtained in this setting and the Komar and Misner-Sharp energies, which are regarded as thermodynamical internal energy in other approaches. The quasilocal Smarr relation is obt"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1902.00825","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":"1902.00825","created_at":"2026-05-17T23:53:41.068531+00:00"},{"alias_kind":"arxiv_version","alias_value":"1902.00825v1","created_at":"2026-05-17T23:53:41.068531+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1902.00825","created_at":"2026-05-17T23:53:41.068531+00:00"},{"alias_kind":"pith_short_12","alias_value":"PHMHNTTP5GRN","created_at":"2026-05-18T12:33:24.271573+00:00"},{"alias_kind":"pith_short_16","alias_value":"PHMHNTTP5GRNU7IF","created_at":"2026-05-18T12:33:24.271573+00:00"},{"alias_kind":"pith_short_8","alias_value":"PHMHNTTP","created_at":"2026-05-18T12:33:24.271573+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.07236","citing_title":"Black holes at a finite distance: Quasi-local restricted phase space formalism","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X","json":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X.json","graph_json":"https://pith.science/api/pith-number/PHMHNTTP5GRNU7IFG7JJS7GB4X/graph.json","events_json":"https://pith.science/api/pith-number/PHMHNTTP5GRNU7IFG7JJS7GB4X/events.json","paper":"https://pith.science/paper/PHMHNTTP"},"agent_actions":{"view_html":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X","download_json":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X.json","view_paper":"https://pith.science/paper/PHMHNTTP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1902.00825&json=true","fetch_graph":"https://pith.science/api/pith-number/PHMHNTTP5GRNU7IFG7JJS7GB4X/graph.json","fetch_events":"https://pith.science/api/pith-number/PHMHNTTP5GRNU7IFG7JJS7GB4X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X/action/storage_attestation","attest_author":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X/action/author_attestation","sign_citation":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X/action/citation_signature","submit_replication":"https://pith.science/pith/PHMHNTTP5GRNU7IFG7JJS7GB4X/action/replication_record"}},"created_at":"2026-05-17T23:53:41.068531+00:00","updated_at":"2026-05-17T23:53:41.068531+00:00"}