{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:45DNQY757WOUS5FSEXHBUHJOSD","short_pith_number":"pith:45DNQY75","schema_version":"1.0","canonical_sha256":"e746d863fdfd9d4974b225ce1a1d2e90e402512a18ae40754448e0193948288e","source":{"kind":"arxiv","id":"1705.05383","version":3},"attestation_state":"computed","paper":{"title":"An extremization principle for the entropy of rotating BPS black holes in AdS$_5$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alberto Zaffaroni, Kiril Hristov, Seyed Morteza Hosseini","submitted_at":"2017-05-15T18:00:03Z","abstract_excerpt":"We show that the Bekenstein-Hawking entropy of a class of BPS electrically charged rotating black holes in AdS$_5\\times S^5$ can be obtained by a simple extremization principle. We expect that this extremization corresponds to the attractor mechanism for BPS rotating black holes in five-dimensional gauged supergravity, which is still unknown. The expression to be extremized has a suggestive resemblance to anomaly polynomials and the supersymmetric Casimir energy recently studied for $\\mathcal{N}=4$ super Yang-Mills."},"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":"1705.05383","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-05-15T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"fd502fd1cf711a37686dcc2220bd77e5bd18f05aeb4d6e0dfec1b551e2877c38","abstract_canon_sha256":"f266147e9930c4c36755a90e4157af92efbd836442155c7422d7d6407c5d48be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:39:12.174810Z","signature_b64":"8DmvSI7Y42HuKZHtxodljKOwoj3M9pp4RH3AVO2PIJ8MG/8w1tVlJUZjWB67VuBEAfQv5I/BX4txEIuNMTatCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e746d863fdfd9d4974b225ce1a1d2e90e402512a18ae40754448e0193948288e","last_reissued_at":"2026-05-18T00:39:12.174115Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:39:12.174115Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An extremization principle for the entropy of rotating BPS black holes in AdS$_5$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alberto Zaffaroni, Kiril Hristov, Seyed Morteza Hosseini","submitted_at":"2017-05-15T18:00:03Z","abstract_excerpt":"We show that the Bekenstein-Hawking entropy of a class of BPS electrically charged rotating black holes in AdS$_5\\times S^5$ can be obtained by a simple extremization principle. We expect that this extremization corresponds to the attractor mechanism for BPS rotating black holes in five-dimensional gauged supergravity, which is still unknown. The expression to be extremized has a suggestive resemblance to anomaly polynomials and the supersymmetric Casimir energy recently studied for $\\mathcal{N}=4$ super Yang-Mills."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.05383","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":"1705.05383","created_at":"2026-05-18T00:39:12.174217+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.05383v3","created_at":"2026-05-18T00:39:12.174217+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.05383","created_at":"2026-05-18T00:39:12.174217+00:00"},{"alias_kind":"pith_short_12","alias_value":"45DNQY757WOU","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"45DNQY757WOUS5FS","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"45DNQY75","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2512.23603","citing_title":"Two roads to fortuity in ABJM theory","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2508.05322","citing_title":"Explorations of Universality in the Entropy and Hawking Radiation of Non-Extremal Kerr AdS$_4$ Black Holes","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2508.08207","citing_title":"Equivariant localization for $D=5$ gauged supergravity","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2511.15426","citing_title":"Probing decoupled Throats of AdS$_{D}$ Black Holes in $D=6,7$","ref_index":56,"is_internal_anchor":true},{"citing_arxiv_id":"2605.00987","citing_title":"A gravity interpretation for the complex Euclidean saddles of the ABJM index","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09490","citing_title":"The superconformal index and localizing higher derivative supergravity","ref_index":11,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD","json":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD.json","graph_json":"https://pith.science/api/pith-number/45DNQY757WOUS5FSEXHBUHJOSD/graph.json","events_json":"https://pith.science/api/pith-number/45DNQY757WOUS5FSEXHBUHJOSD/events.json","paper":"https://pith.science/paper/45DNQY75"},"agent_actions":{"view_html":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD","download_json":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD.json","view_paper":"https://pith.science/paper/45DNQY75","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.05383&json=true","fetch_graph":"https://pith.science/api/pith-number/45DNQY757WOUS5FSEXHBUHJOSD/graph.json","fetch_events":"https://pith.science/api/pith-number/45DNQY757WOUS5FSEXHBUHJOSD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD/action/storage_attestation","attest_author":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD/action/author_attestation","sign_citation":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD/action/citation_signature","submit_replication":"https://pith.science/pith/45DNQY757WOUS5FSEXHBUHJOSD/action/replication_record"}},"created_at":"2026-05-18T00:39:12.174217+00:00","updated_at":"2026-05-18T00:39:12.174217+00:00"}