{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:NGZLRNZXGSDWLETZSA532LZQE3","short_pith_number":"pith:NGZLRNZX","schema_version":"1.0","canonical_sha256":"69b2b8b7373487659279903bbd2f3026e041eb18b3f949c5a49f07513b47a610","source":{"kind":"arxiv","id":"1812.00923","version":2},"attestation_state":"computed","paper":{"title":"Wilson Surface Central Charge from Holographic Entanglement Entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andy O'Bannon, Brandon Robinson, Darya Krym, John Estes, Ronnie Rodgers","submitted_at":"2018-12-03T17:28:12Z","abstract_excerpt":"We use entanglement entropy to define a central charge associated to a two-dimensional defect or boundary in a conformal field theory (CFT). We present holographic calculations of this central charge for several maximally supersymmetric CFTs dual to eleven-dimensional supergravity in Anti-de Sitter space, namely the M5-brane theory with a Wilson surface defect and three-dimensional CFTs related to the M2-brane theory with a boundary. Our results for the central charge depend on a partition of the number of M2-branes, $N$, ending on the number of M5-branes, $M$. For the Wilson surface, the part"},"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":"1812.00923","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2018-12-03T17:28:12Z","cross_cats_sorted":[],"title_canon_sha256":"9113a58c707dfb4e56ab4641d1da48a031c8de3736a3dc649d8cf8f28c5a96cf","abstract_canon_sha256":"049ebb4fd7e8370f8742205fdcc30244716f37c04ea653fb475d92224902d867"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:40:49.378627Z","signature_b64":"OYm/VEyFAua1c8y7X5BjArcVaENDBupTB9p/aW18GUu3QPteJ8z5XuutSn094X/1E5dH8PCzbE+ViL+99zicCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"69b2b8b7373487659279903bbd2f3026e041eb18b3f949c5a49f07513b47a610","last_reissued_at":"2026-05-17T23:40:49.377919Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:40:49.377919Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wilson Surface Central Charge from Holographic Entanglement Entropy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andy O'Bannon, Brandon Robinson, Darya Krym, John Estes, Ronnie Rodgers","submitted_at":"2018-12-03T17:28:12Z","abstract_excerpt":"We use entanglement entropy to define a central charge associated to a two-dimensional defect or boundary in a conformal field theory (CFT). We present holographic calculations of this central charge for several maximally supersymmetric CFTs dual to eleven-dimensional supergravity in Anti-de Sitter space, namely the M5-brane theory with a Wilson surface defect and three-dimensional CFTs related to the M2-brane theory with a boundary. Our results for the central charge depend on a partition of the number of M2-branes, $N$, ending on the number of M5-branes, $M$. For the Wilson surface, the part"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.00923","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":""},"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":"1812.00923","created_at":"2026-05-17T23:40:49.378036+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.00923v2","created_at":"2026-05-17T23:40:49.378036+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.00923","created_at":"2026-05-17T23:40:49.378036+00:00"},{"alias_kind":"pith_short_12","alias_value":"NGZLRNZXGSDW","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_16","alias_value":"NGZLRNZXGSDWLETZ","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_8","alias_value":"NGZLRNZX","created_at":"2026-05-18T12:32:40.477152+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.09498","citing_title":"From Weyl Anomaly to Defect Supersymmetric R\\'enyi Entropy and Casimir Energy","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3","json":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3.json","graph_json":"https://pith.science/api/pith-number/NGZLRNZXGSDWLETZSA532LZQE3/graph.json","events_json":"https://pith.science/api/pith-number/NGZLRNZXGSDWLETZSA532LZQE3/events.json","paper":"https://pith.science/paper/NGZLRNZX"},"agent_actions":{"view_html":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3","download_json":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3.json","view_paper":"https://pith.science/paper/NGZLRNZX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.00923&json=true","fetch_graph":"https://pith.science/api/pith-number/NGZLRNZXGSDWLETZSA532LZQE3/graph.json","fetch_events":"https://pith.science/api/pith-number/NGZLRNZXGSDWLETZSA532LZQE3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3/action/storage_attestation","attest_author":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3/action/author_attestation","sign_citation":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3/action/citation_signature","submit_replication":"https://pith.science/pith/NGZLRNZXGSDWLETZSA532LZQE3/action/replication_record"}},"created_at":"2026-05-17T23:40:49.378036+00:00","updated_at":"2026-05-17T23:40:49.378036+00:00"}