{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SMFDN3BFREZUTVT2FZ4EIDHGHU","short_pith_number":"pith:SMFDN3BF","schema_version":"1.0","canonical_sha256":"930a36ec25893349d67a2e78440ce63d2ad6d64ed297d839483330823ac17edf","source":{"kind":"arxiv","id":"1308.5403","version":2},"attestation_state":"computed","paper":{"title":"The compressibility of rotating black holes in D-dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Brian P. Dolan","submitted_at":"2013-08-25T12:54:55Z","abstract_excerpt":"Treating the cosmological constant as a pressure, in the context of black hole thermodynamics, a thermodynamic volume for the black hole can be defined as being the thermodynamic variable conjugate to the pressure, in the sense of a Legendre transform. The thermodynamic volume is explicitly calculated, as the Legendre transform of the pressure in the enthalpy for a rotating asymptotically anti-de Sitter Myers-Perry black hole in D space-time dimensions. The volume obtained is shown to agree with previous calculations using the Smarr relation. The compressibility is calculated and shown to be n"},"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":"1308.5403","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2013-08-25T12:54:55Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"902314071f2fa2969825feab1abb3fa798bb0b3ac8603146d395935390388fb1","abstract_canon_sha256":"da07b868afea3ec9da70def779080cf5e34c8fe8590a91b178cba78cf92ad902"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:58.829825Z","signature_b64":"/TCOkB2AU4ncodjncoJfzgSHS+7BSOlZJAvzta2Zd5v2qRIcqf2rm46wl2nyZG5+iGqR4piglnWFhahhHgreCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"930a36ec25893349d67a2e78440ce63d2ad6d64ed297d839483330823ac17edf","last_reissued_at":"2026-05-18T01:47:58.829168Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:58.829168Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The compressibility of rotating black holes in D-dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Brian P. Dolan","submitted_at":"2013-08-25T12:54:55Z","abstract_excerpt":"Treating the cosmological constant as a pressure, in the context of black hole thermodynamics, a thermodynamic volume for the black hole can be defined as being the thermodynamic variable conjugate to the pressure, in the sense of a Legendre transform. The thermodynamic volume is explicitly calculated, as the Legendre transform of the pressure in the enthalpy for a rotating asymptotically anti-de Sitter Myers-Perry black hole in D space-time dimensions. The volume obtained is shown to agree with previous calculations using the Smarr relation. The compressibility is calculated and shown to be n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.5403","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":""},"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":"1308.5403","created_at":"2026-05-18T01:47:58.829265+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.5403v2","created_at":"2026-05-18T01:47:58.829265+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.5403","created_at":"2026-05-18T01:47:58.829265+00:00"},{"alias_kind":"pith_short_12","alias_value":"SMFDN3BFREZU","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SMFDN3BFREZUTVT2","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SMFDN3BF","created_at":"2026-05-18T12:27:59.945178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1608.06147","citing_title":"Black hole chemistry: thermodynamics with Lambda","ref_index":117,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU","json":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU.json","graph_json":"https://pith.science/api/pith-number/SMFDN3BFREZUTVT2FZ4EIDHGHU/graph.json","events_json":"https://pith.science/api/pith-number/SMFDN3BFREZUTVT2FZ4EIDHGHU/events.json","paper":"https://pith.science/paper/SMFDN3BF"},"agent_actions":{"view_html":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU","download_json":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU.json","view_paper":"https://pith.science/paper/SMFDN3BF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.5403&json=true","fetch_graph":"https://pith.science/api/pith-number/SMFDN3BFREZUTVT2FZ4EIDHGHU/graph.json","fetch_events":"https://pith.science/api/pith-number/SMFDN3BFREZUTVT2FZ4EIDHGHU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU/action/storage_attestation","attest_author":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU/action/author_attestation","sign_citation":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU/action/citation_signature","submit_replication":"https://pith.science/pith/SMFDN3BFREZUTVT2FZ4EIDHGHU/action/replication_record"}},"created_at":"2026-05-18T01:47:58.829265+00:00","updated_at":"2026-05-18T01:47:58.829265+00:00"}