{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:SPDCBKX3GPR5GQ5R34RDQL3F6V","short_pith_number":"pith:SPDCBKX3","schema_version":"1.0","canonical_sha256":"93c620aafb33e3d343b1df22382f65f54d1921c7387c40f04a8bdc7dda95ddaa","source":{"kind":"arxiv","id":"1306.4338","version":4},"attestation_state":"computed","paper":{"title":"Wilson Lines and Entanglement Entropy in Higher Spin Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alejandra Castro, Martin Ammon, Nabil Iqbal","submitted_at":"2013-06-18T20:10:40Z","abstract_excerpt":"Holographic entanglement entropy provides a direct connection between classical geometry and quantum entanglement; however the usual prescription does not apply to theories of higher spin gravity, where standard notions of geometry are no longer gauge invariant. We present a proposal for the holographic computation of entanglement entropy in field theories dual to higher spin theories of gravity in AdS3. These theories have a Chern-Simons description, and our proposal involves a Wilson line in an infinite-dimensional representation of the bulk gauge group. In the case of spin-2 gravity such Wi"},"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":"1306.4338","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2013-06-18T20:10:40Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"e059d3a32a31e54d1d40e55e0b94638caaf5e3c7732d79b219ee0e4e2ed692ef","abstract_canon_sha256":"0d4aefa7d971bd721b128d3d092f5b2519d10b5cc326d60847b0bcdd7e68a6eb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:19:35.522142Z","signature_b64":"2OTqRP2Ggg1J3yUZuIxG/R5ZIIMwqU0c9u5VX4eJRs+s4CE5N0uRE9lV0klV4RsB79y0X4sIshK2/KNEZownDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"93c620aafb33e3d343b1df22382f65f54d1921c7387c40f04a8bdc7dda95ddaa","last_reissued_at":"2026-05-18T01:19:35.521517Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:19:35.521517Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wilson Lines and Entanglement Entropy in Higher Spin Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alejandra Castro, Martin Ammon, Nabil Iqbal","submitted_at":"2013-06-18T20:10:40Z","abstract_excerpt":"Holographic entanglement entropy provides a direct connection between classical geometry and quantum entanglement; however the usual prescription does not apply to theories of higher spin gravity, where standard notions of geometry are no longer gauge invariant. We present a proposal for the holographic computation of entanglement entropy in field theories dual to higher spin theories of gravity in AdS3. These theories have a Chern-Simons description, and our proposal involves a Wilson line in an infinite-dimensional representation of the bulk gauge group. In the case of spin-2 gravity such Wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.4338","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":""},"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":"1306.4338","created_at":"2026-05-18T01:19:35.521618+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.4338v4","created_at":"2026-05-18T01:19:35.521618+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.4338","created_at":"2026-05-18T01:19:35.521618+00:00"},{"alias_kind":"pith_short_12","alias_value":"SPDCBKX3GPR5","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"SPDCBKX3GPR5GQ5R","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"SPDCBKX3","created_at":"2026-05-18T12:27:59.945178+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.16164","citing_title":"The Carrollian Kaleidoscope","ref_index":175,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V","json":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V.json","graph_json":"https://pith.science/api/pith-number/SPDCBKX3GPR5GQ5R34RDQL3F6V/graph.json","events_json":"https://pith.science/api/pith-number/SPDCBKX3GPR5GQ5R34RDQL3F6V/events.json","paper":"https://pith.science/paper/SPDCBKX3"},"agent_actions":{"view_html":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V","download_json":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V.json","view_paper":"https://pith.science/paper/SPDCBKX3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.4338&json=true","fetch_graph":"https://pith.science/api/pith-number/SPDCBKX3GPR5GQ5R34RDQL3F6V/graph.json","fetch_events":"https://pith.science/api/pith-number/SPDCBKX3GPR5GQ5R34RDQL3F6V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V/action/storage_attestation","attest_author":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V/action/author_attestation","sign_citation":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V/action/citation_signature","submit_replication":"https://pith.science/pith/SPDCBKX3GPR5GQ5R34RDQL3F6V/action/replication_record"}},"created_at":"2026-05-18T01:19:35.521618+00:00","updated_at":"2026-05-18T01:19:35.521618+00:00"}