{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:S7JFFDCKZK5INQUSQJOWK2KNMB","short_pith_number":"pith:S7JFFDCK","schema_version":"1.0","canonical_sha256":"97d2528c4acaba86c292825d65694d604eba5abfd83ebe34f618f75af0ce8fbd","source":{"kind":"arxiv","id":"2407.19387","version":4},"attestation_state":"computed","paper":{"title":"BPS Chaos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Henry W. Lin, Stephen H. Shenker, Yiming Chen","submitted_at":"2024-07-28T04:08:11Z","abstract_excerpt":"Black holes are chaotic quantum systems that are expected to exhibit random matrix statistics in their finite energy spectrum. Lin, Maldacena, Rozenberg and Shan (LMRS) have proposed a related characterization of chaos for the ground states of BPS black holes with finite area horizons. On a separate front, the \"fuzzball program\" has uncovered large families of horizon-free geometries that account for the entropy of holographic BPS systems, but only in situations with sufficient supersymmetry to exclude finite area horizons. The highly structured, non-random nature of these solutions seems in t"},"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":"2407.19387","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-07-28T04:08:11Z","cross_cats_sorted":[],"title_canon_sha256":"3207485f3d9a0101a00ec1d9d4f4c9e02f425cb09da33a428ad244cf51e6a626","abstract_canon_sha256":"186993604af2bdce3006081695db5ab52ba3d7d2e4298a9c49982ddd7e01a000"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-26T02:03:46.840388Z","signature_b64":"dR/HJBZW0WUYW0KZWr0JpWrTd+DTtTfzogoKOMyleA9MVuCgoi736jWJlDkuhAegXb5iDD++40VrwHA7QAYQBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"97d2528c4acaba86c292825d65694d604eba5abfd83ebe34f618f75af0ce8fbd","last_reissued_at":"2026-05-26T02:03:46.839501Z","signature_status":"signed_v1","first_computed_at":"2026-05-26T02:03:46.839501Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"BPS Chaos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Henry W. Lin, Stephen H. Shenker, Yiming Chen","submitted_at":"2024-07-28T04:08:11Z","abstract_excerpt":"Black holes are chaotic quantum systems that are expected to exhibit random matrix statistics in their finite energy spectrum. Lin, Maldacena, Rozenberg and Shan (LMRS) have proposed a related characterization of chaos for the ground states of BPS black holes with finite area horizons. On a separate front, the \"fuzzball program\" has uncovered large families of horizon-free geometries that account for the entropy of holographic BPS systems, but only in situations with sufficient supersymmetry to exclude finite area horizons. The highly structured, non-random nature of these solutions seems in t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.19387","kind":"arxiv","version":4},"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/2407.19387/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":"2407.19387","created_at":"2026-05-26T02:03:46.839615+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.19387v4","created_at":"2026-05-26T02:03:46.839615+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.19387","created_at":"2026-05-26T02:03:46.839615+00:00"},{"alias_kind":"pith_short_12","alias_value":"S7JFFDCKZK5I","created_at":"2026-05-26T02:03:46.839615+00:00"},{"alias_kind":"pith_short_16","alias_value":"S7JFFDCKZK5INQUS","created_at":"2026-05-26T02:03:46.839615+00:00"},{"alias_kind":"pith_short_8","alias_value":"S7JFFDCK","created_at":"2026-05-26T02:03:46.839615+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":8,"sample":[{"citing_arxiv_id":"2605.20913","citing_title":"Chaos-Integrability Transition in the BPS Subspace of the $\\mathcal{N}=2$ SYK Model","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2605.16254","citing_title":"Fortuity and Complexity in a Simple Quark Model","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18725","citing_title":"Signatures of Quantum Chaos in the D1D5 System","ref_index":62,"is_internal_anchor":true},{"citing_arxiv_id":"2603.18138","citing_title":"The Resolved Elliptic Genus and the D1-D5 CFT","ref_index":59,"is_internal_anchor":true},{"citing_arxiv_id":"2603.29443","citing_title":"Cosmological brick walls & quantum chaotic dynamics of de Sitter horizons","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"2604.23287","citing_title":"Chaos of Berry curvature for BPS microstates","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2605.06465","citing_title":"Non-planar corrections in the symmetric orbifold","ref_index":44,"is_internal_anchor":true},{"citing_arxiv_id":"2605.08085","citing_title":"Fermionic trace relations and supersymmetric indices at finite $N$","ref_index":35,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB","json":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB.json","graph_json":"https://pith.science/api/pith-number/S7JFFDCKZK5INQUSQJOWK2KNMB/graph.json","events_json":"https://pith.science/api/pith-number/S7JFFDCKZK5INQUSQJOWK2KNMB/events.json","paper":"https://pith.science/paper/S7JFFDCK"},"agent_actions":{"view_html":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB","download_json":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB.json","view_paper":"https://pith.science/paper/S7JFFDCK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.19387&json=true","fetch_graph":"https://pith.science/api/pith-number/S7JFFDCKZK5INQUSQJOWK2KNMB/graph.json","fetch_events":"https://pith.science/api/pith-number/S7JFFDCKZK5INQUSQJOWK2KNMB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB/action/storage_attestation","attest_author":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB/action/author_attestation","sign_citation":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB/action/citation_signature","submit_replication":"https://pith.science/pith/S7JFFDCKZK5INQUSQJOWK2KNMB/action/replication_record"}},"created_at":"2026-05-26T02:03:46.839615+00:00","updated_at":"2026-05-26T02:03:46.839615+00:00"}