{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:Z2H2CTUAUEZ56MN4CTCW6T7ARO","short_pith_number":"pith:Z2H2CTUA","schema_version":"1.0","canonical_sha256":"ce8fa14e80a133df31bc14c56f4fe08bba0d6bcc930c54012725207c77820267","source":{"kind":"arxiv","id":"1606.05997","version":3},"attestation_state":"computed","paper":{"title":"Mass and angular momentum of black holes in 3D gravity theories with first order formalism","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jong-Dae Park, Soonkeon Nam","submitted_at":"2016-06-20T07:30:46Z","abstract_excerpt":"We apply the Wald formalism to obtain masses and angular momenta of black holes in three dimensional gravity theories using the first order formalism. Wald formalism suggests that the entropy of a black hole can be defined by an integration of a conserved charge on the bifurcation horizon, and mass and angular momentum of a black hole as an integration of some charge variation form at spatial infinity. The action of three dimensional gravity theories can be represented by a form including some auxiliary fields. As well-known examples we have calculated masses and angular momenta of some black "},"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":"1606.05997","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2016-06-20T07:30:46Z","cross_cats_sorted":[],"title_canon_sha256":"3eb1aa5c5f0cd28a7e9c6f69b8cb16e65ca6e4e91b30a32a7607ebddeade85e3","abstract_canon_sha256":"4631d27deb6863d1f979f64834693b163688104ac743d6d4eeb9de4e3973ea00"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:29.077614Z","signature_b64":"6tGYbTrOCXiMn1A1Vbcg9SPmD++5ePoyZvKJPDRfff2fWww+UPOU1MaUzs87Za1SvI1/vnAz7jDZgCXGHpsQCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ce8fa14e80a133df31bc14c56f4fe08bba0d6bcc930c54012725207c77820267","last_reissued_at":"2026-05-18T00:11:29.077209Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:29.077209Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mass and angular momentum of black holes in 3D gravity theories with first order formalism","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Jong-Dae Park, Soonkeon Nam","submitted_at":"2016-06-20T07:30:46Z","abstract_excerpt":"We apply the Wald formalism to obtain masses and angular momenta of black holes in three dimensional gravity theories using the first order formalism. Wald formalism suggests that the entropy of a black hole can be defined by an integration of a conserved charge on the bifurcation horizon, and mass and angular momentum of a black hole as an integration of some charge variation form at spatial infinity. The action of three dimensional gravity theories can be represented by a form including some auxiliary fields. As well-known examples we have calculated masses and angular momenta of some black "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.05997","kind":"arxiv","version":3},"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":"1606.05997","created_at":"2026-05-18T00:11:29.077273+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.05997v3","created_at":"2026-05-18T00:11:29.077273+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.05997","created_at":"2026-05-18T00:11:29.077273+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z2H2CTUAUEZ5","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z2H2CTUAUEZ56MN4","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z2H2CTUA","created_at":"2026-05-18T12:30:53.716459+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.18062","citing_title":"Note on WAdS$_3$ black holes in extended BHT gravity","ref_index":35,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO","json":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO.json","graph_json":"https://pith.science/api/pith-number/Z2H2CTUAUEZ56MN4CTCW6T7ARO/graph.json","events_json":"https://pith.science/api/pith-number/Z2H2CTUAUEZ56MN4CTCW6T7ARO/events.json","paper":"https://pith.science/paper/Z2H2CTUA"},"agent_actions":{"view_html":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO","download_json":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO.json","view_paper":"https://pith.science/paper/Z2H2CTUA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.05997&json=true","fetch_graph":"https://pith.science/api/pith-number/Z2H2CTUAUEZ56MN4CTCW6T7ARO/graph.json","fetch_events":"https://pith.science/api/pith-number/Z2H2CTUAUEZ56MN4CTCW6T7ARO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO/action/storage_attestation","attest_author":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO/action/author_attestation","sign_citation":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO/action/citation_signature","submit_replication":"https://pith.science/pith/Z2H2CTUAUEZ56MN4CTCW6T7ARO/action/replication_record"}},"created_at":"2026-05-18T00:11:29.077273+00:00","updated_at":"2026-05-18T00:11:29.077273+00:00"}