{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:2SEHJ6W72TPUMW2X6H4FJGU6LX","short_pith_number":"pith:2SEHJ6W7","schema_version":"1.0","canonical_sha256":"d48874fadfd4df465b57f1f8549a9e5dc50c32219a1cc56064a0d1ca8b1e8f6a","source":{"kind":"arxiv","id":"1307.6243","version":3},"attestation_state":"computed","paper":{"title":"AdS Dyonic Black Hole and its Thermodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"C.N. Pope, H. Lu, Y. Pang","submitted_at":"2013-07-23T20:48:55Z","abstract_excerpt":"We obtain spherically-symmetric and $\\R^2$-symmetric dyonic black holes that are asymptotic to anti-de Sitter space-time (AdS), which are solutions in maximal gauged four-dimensional supergravity, with just one of the U(1) fields carrying both the electric and magnetic charges $(Q,P)$. We study the thermodynamics, and find that the usually-expected first law does not hold unless P=0, Q=0 or P=Q. For general values of the charges, we find that the first law requires a modification with a new pair of thermodynamic conjugate variables. We show that they describe the scalar hair that breaks some o"},"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":"1307.6243","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-07-23T20:48:55Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"3f5be87e0e4354b3cfa520a8acae7ca60d4ed4b42017c5bdd149afcd3a178a84","abstract_canon_sha256":"fd86e04d5d99c7e7433af3fdf0ec619072c2309afd33a0cff4c123a420e237c9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:07:54.432872Z","signature_b64":"cOCW5ubSEaW6jhC3KYQAkKBJ3FOOc34FPSd0iV4LddZGu0DJ+3SZ/JgfFOGUyrUIUiGWoOv87FXoJl34C48BAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d48874fadfd4df465b57f1f8549a9e5dc50c32219a1cc56064a0d1ca8b1e8f6a","last_reissued_at":"2026-05-18T03:07:54.432037Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:07:54.432037Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"AdS Dyonic Black Hole and its Thermodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"C.N. Pope, H. Lu, Y. Pang","submitted_at":"2013-07-23T20:48:55Z","abstract_excerpt":"We obtain spherically-symmetric and $\\R^2$-symmetric dyonic black holes that are asymptotic to anti-de Sitter space-time (AdS), which are solutions in maximal gauged four-dimensional supergravity, with just one of the U(1) fields carrying both the electric and magnetic charges $(Q,P)$. We study the thermodynamics, and find that the usually-expected first law does not hold unless P=0, Q=0 or P=Q. For general values of the charges, we find that the first law requires a modification with a new pair of thermodynamic conjugate variables. We show that they describe the scalar hair that breaks some o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.6243","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":"1307.6243","created_at":"2026-05-18T03:07:54.432144+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.6243v3","created_at":"2026-05-18T03:07:54.432144+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.6243","created_at":"2026-05-18T03:07:54.432144+00:00"},{"alias_kind":"pith_short_12","alias_value":"2SEHJ6W72TPU","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"2SEHJ6W72TPUMW2X","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"2SEHJ6W7","created_at":"2026-05-18T12:27:32.513160+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2311.00550","citing_title":"Holographic renormalization and the variational problem for mixed boundary conditions via a solution-dependent superpotential-like function","ref_index":11,"is_internal_anchor":true},{"citing_arxiv_id":"2511.19926","citing_title":"Revisiting black holes and their thermodynamics in Einstein-Kalb-Ramond gravity","ref_index":23,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX","json":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX.json","graph_json":"https://pith.science/api/pith-number/2SEHJ6W72TPUMW2X6H4FJGU6LX/graph.json","events_json":"https://pith.science/api/pith-number/2SEHJ6W72TPUMW2X6H4FJGU6LX/events.json","paper":"https://pith.science/paper/2SEHJ6W7"},"agent_actions":{"view_html":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX","download_json":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX.json","view_paper":"https://pith.science/paper/2SEHJ6W7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.6243&json=true","fetch_graph":"https://pith.science/api/pith-number/2SEHJ6W72TPUMW2X6H4FJGU6LX/graph.json","fetch_events":"https://pith.science/api/pith-number/2SEHJ6W72TPUMW2X6H4FJGU6LX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX/action/storage_attestation","attest_author":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX/action/author_attestation","sign_citation":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX/action/citation_signature","submit_replication":"https://pith.science/pith/2SEHJ6W72TPUMW2X6H4FJGU6LX/action/replication_record"}},"created_at":"2026-05-18T03:07:54.432144+00:00","updated_at":"2026-05-18T03:07:54.432144+00:00"}