{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QXTZ7EONG3IHECF7VVPVFFB3BA","short_pith_number":"pith:QXTZ7EON","schema_version":"1.0","canonical_sha256":"85e79f91cd36d07208bfad5f52943b0839da9574f111bc01cb194d97fc5596d3","source":{"kind":"arxiv","id":"2306.04693","version":2},"attestation_state":"computed","paper":{"title":"Following Black Hole States","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Harish Murali, Kasia Budzik, Pedro Vieira","submitted_at":"2023-06-07T18:00:17Z","abstract_excerpt":"We study $\\mathcal{N}=4$ SYM at non-integer number of colours. By varying $N$ we can continuously follow states all the way from $N=\\infty$ where integrability reigns to finite $N$ where quantum gravity effects dominate. As an application we consider classically $1/16$ BPS states. Quantum mechanically, these states are generically non-supersymmetric but some special states - at special values of $N$ - become super-symmetric at the quantum level as well. They are the so-called quantum black hole states studied recently using cohomology. We write down the form of the lightest BH state at $N=2$ -"},"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":"2306.04693","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-06-07T18:00:17Z","cross_cats_sorted":[],"title_canon_sha256":"8ebb8620a5443bf343979300e51d8a7106e49b17a0bf5195543ef8677b08d382","abstract_canon_sha256":"706be6a29a7890fb1b8013caa5fd95032456730a2db9160cb3375b3f4ccc4797"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:50:40.692520Z","signature_b64":"XL4T40+JyQnzB5Xq71APqqC5WyaqS6i87wQPVq0J+ry8gnO0Q+Heu9LCcUGiyHaZTJBpUzZnyvdybckHDxErDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"85e79f91cd36d07208bfad5f52943b0839da9574f111bc01cb194d97fc5596d3","last_reissued_at":"2026-07-05T06:50:40.691996Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:50:40.691996Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Following Black Hole States","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Harish Murali, Kasia Budzik, Pedro Vieira","submitted_at":"2023-06-07T18:00:17Z","abstract_excerpt":"We study $\\mathcal{N}=4$ SYM at non-integer number of colours. By varying $N$ we can continuously follow states all the way from $N=\\infty$ where integrability reigns to finite $N$ where quantum gravity effects dominate. As an application we consider classically $1/16$ BPS states. Quantum mechanically, these states are generically non-supersymmetric but some special states - at special values of $N$ - become super-symmetric at the quantum level as well. They are the so-called quantum black hole states studied recently using cohomology. We write down the form of the lightest BH state at $N=2$ -"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.04693","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/2306.04693/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":"2306.04693","created_at":"2026-07-05T06:50:40.692059+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.04693v2","created_at":"2026-07-05T06:50:40.692059+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.04693","created_at":"2026-07-05T06:50:40.692059+00:00"},{"alias_kind":"pith_short_12","alias_value":"QXTZ7EONG3IH","created_at":"2026-07-05T06:50:40.692059+00:00"},{"alias_kind":"pith_short_16","alias_value":"QXTZ7EONG3IHECF7","created_at":"2026-07-05T06:50:40.692059+00:00"},{"alias_kind":"pith_short_8","alias_value":"QXTZ7EON","created_at":"2026-07-05T06:50:40.692059+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.27955","citing_title":"Quantum black hole cohomologies","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30725","citing_title":"Constrained particle on a group: from propagators to correlators","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2606.27955","citing_title":"Quantum black hole cohomologies","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2605.25560","citing_title":"Finite-$N$ BMN index across all vacuum sectors","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2512.23603","citing_title":"Two roads to fortuity in ABJM theory","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18725","citing_title":"Signatures of Quantum Chaos in the D1D5 System","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2603.18138","citing_title":"The Resolved Elliptic Genus and the D1-D5 CFT","ref_index":75,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23287","citing_title":"Chaos of Berry curvature for BPS microstates","ref_index":139,"is_internal_anchor":false},{"citing_arxiv_id":"2604.20663","citing_title":"Towering Gravitons in AdS$_3$/CFT$_2$","ref_index":17,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA","json":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA.json","graph_json":"https://pith.science/api/pith-number/QXTZ7EONG3IHECF7VVPVFFB3BA/graph.json","events_json":"https://pith.science/api/pith-number/QXTZ7EONG3IHECF7VVPVFFB3BA/events.json","paper":"https://pith.science/paper/QXTZ7EON"},"agent_actions":{"view_html":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA","download_json":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA.json","view_paper":"https://pith.science/paper/QXTZ7EON","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.04693&json=true","fetch_graph":"https://pith.science/api/pith-number/QXTZ7EONG3IHECF7VVPVFFB3BA/graph.json","fetch_events":"https://pith.science/api/pith-number/QXTZ7EONG3IHECF7VVPVFFB3BA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA/action/storage_attestation","attest_author":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA/action/author_attestation","sign_citation":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA/action/citation_signature","submit_replication":"https://pith.science/pith/QXTZ7EONG3IHECF7VVPVFFB3BA/action/replication_record"}},"created_at":"2026-07-05T06:50:40.692059+00:00","updated_at":"2026-07-05T06:50:40.692059+00:00"}