{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:I4LM2KI4ESRZC3GKL2674D7HYN","short_pith_number":"pith:I4LM2KI4","schema_version":"1.0","canonical_sha256":"4716cd291c24a3916cca5ebdfe0fe7c358143b262e857df6207739d4752563be","source":{"kind":"arxiv","id":"2412.03697","version":2},"attestation_state":"computed","paper":{"title":"The spectrum of near-BPS Kerr-Newman black holes and the ABJM mass gap","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Chiara Toldo, Matthew Heydeman","submitted_at":"2024-12-04T20:20:26Z","abstract_excerpt":"Supersymmetric rotating 1/16-BPS black holes in $AdS_4 \\times S^7$ are expected to capture the average degeneracy of BPS states in the dual ABJM superconformal theory for given fixed charges. This has been successfully demonstrated for the superconformal index using complexified black hole metrics, but a naive Gibbons-Hawking calculation of the actual degeneracies in the low temperature limit is invalid due to large quantum fluctuations of the near horizon $AdS_2$ metric. We argue that in a particular mixed grand/canonical ensemble, these fluctuations of the near-BPS Kerr-Newman black holes ar"},"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":"2412.03697","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-12-04T20:20:26Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"42d8938bdae0b631e352cde550c124395d762aaffcd82a642675f49fcc85517a","abstract_canon_sha256":"5ff96729cb81ee1a7f1db47bbbb98bcd8c4a35f04bfcac01369205c72bef2dcb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:59:04.133691Z","signature_b64":"ZuJ2VySxF/UGeFZ8qwt5ISiItWyIpxr2VGg+aNpVs7XLrYQJNkthB9LsW4NbCA4xf8OgKr46AA1aff/24Qc8DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4716cd291c24a3916cca5ebdfe0fe7c358143b262e857df6207739d4752563be","last_reissued_at":"2026-07-05T10:59:04.133202Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:59:04.133202Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The spectrum of near-BPS Kerr-Newman black holes and the ABJM mass gap","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Chiara Toldo, Matthew Heydeman","submitted_at":"2024-12-04T20:20:26Z","abstract_excerpt":"Supersymmetric rotating 1/16-BPS black holes in $AdS_4 \\times S^7$ are expected to capture the average degeneracy of BPS states in the dual ABJM superconformal theory for given fixed charges. This has been successfully demonstrated for the superconformal index using complexified black hole metrics, but a naive Gibbons-Hawking calculation of the actual degeneracies in the low temperature limit is invalid due to large quantum fluctuations of the near horizon $AdS_2$ metric. We argue that in a particular mixed grand/canonical ensemble, these fluctuations of the near-BPS Kerr-Newman black holes ar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.03697","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2412.03697/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2412.03697","created_at":"2026-07-05T10:59:04.133259+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.03697v2","created_at":"2026-07-05T10:59:04.133259+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.03697","created_at":"2026-07-05T10:59:04.133259+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4LM2KI4ESRZ","created_at":"2026-07-05T10:59:04.133259+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4LM2KI4ESRZC3GK","created_at":"2026-07-05T10:59:04.133259+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4LM2KI4","created_at":"2026-07-05T10:59:04.133259+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.23603","citing_title":"Two roads to fortuity in ABJM theory","ref_index":63,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23287","citing_title":"Chaos of Berry curvature for BPS microstates","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN","json":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN.json","graph_json":"https://pith.science/api/pith-number/I4LM2KI4ESRZC3GKL2674D7HYN/graph.json","events_json":"https://pith.science/api/pith-number/I4LM2KI4ESRZC3GKL2674D7HYN/events.json","paper":"https://pith.science/paper/I4LM2KI4"},"agent_actions":{"view_html":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN","download_json":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN.json","view_paper":"https://pith.science/paper/I4LM2KI4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.03697&json=true","fetch_graph":"https://pith.science/api/pith-number/I4LM2KI4ESRZC3GKL2674D7HYN/graph.json","fetch_events":"https://pith.science/api/pith-number/I4LM2KI4ESRZC3GKL2674D7HYN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN/action/storage_attestation","attest_author":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN/action/author_attestation","sign_citation":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN/action/citation_signature","submit_replication":"https://pith.science/pith/I4LM2KI4ESRZC3GKL2674D7HYN/action/replication_record"}},"created_at":"2026-07-05T10:59:04.133259+00:00","updated_at":"2026-07-05T10:59:04.133259+00:00"}