{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:7LM2HH2ET6ZYT2UI4CXNLGJGIT","short_pith_number":"pith:7LM2HH2E","schema_version":"1.0","canonical_sha256":"fad9a39f449fb389ea88e0aed5992644faa9d63865eff966b1313ea012f68877","source":{"kind":"arxiv","id":"1008.4579","version":3},"attestation_state":"computed","paper":{"title":"Nonlinear W(infinity) Algebra as Asymptotic Symmetry of Three-Dimensional Higher Spin Anti-de Sitter Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Marc Henneaux, Soo-Jong Rey","submitted_at":"2010-08-26T20:00:00Z","abstract_excerpt":"We investigate the asymptotic symmetry algebra of (2+1)-dimensional higher spin, anti-de Sitter gravity. We use the formulation of the theory as a Chern-Simons gauge theory based on the higher spin algebra hs(1,1). Expanding the gauge connection around asymptotically anti-de Sitter spacetime, we specify consistent boundary conditions on the higher spin gauge fields. We then study residual gauge transformation, the corresponding surface terms and their Poisson bracket algebra. We find that the asymptotic symmetry algebra is a nonlinearly deformed W(infinity) algebra with classical central charg"},"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":"1008.4579","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2010-08-26T20:00:00Z","cross_cats_sorted":["gr-qc","math-ph","math.MP"],"title_canon_sha256":"03503ba418722ca158bdc5e893571861c9f3408577546d2830ec88ae60890bce","abstract_canon_sha256":"8220a6698fcc9356871755d637df29b53d1452637ba22aa0a45b6afd42991cd6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:33:59.716793Z","signature_b64":"8/ELrE4v28gH4/z6LiwDC3/q1DzLh0k95LUp2eFigpJGxim+KUULeoweAg3yGlUrvBqpPQZfe5ZKMXRhcIilAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fad9a39f449fb389ea88e0aed5992644faa9d63865eff966b1313ea012f68877","last_reissued_at":"2026-05-18T04:33:59.716267Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:33:59.716267Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonlinear W(infinity) Algebra as Asymptotic Symmetry of Three-Dimensional Higher Spin Anti-de Sitter Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Marc Henneaux, Soo-Jong Rey","submitted_at":"2010-08-26T20:00:00Z","abstract_excerpt":"We investigate the asymptotic symmetry algebra of (2+1)-dimensional higher spin, anti-de Sitter gravity. We use the formulation of the theory as a Chern-Simons gauge theory based on the higher spin algebra hs(1,1). Expanding the gauge connection around asymptotically anti-de Sitter spacetime, we specify consistent boundary conditions on the higher spin gauge fields. We then study residual gauge transformation, the corresponding surface terms and their Poisson bracket algebra. We find that the asymptotic symmetry algebra is a nonlinearly deformed W(infinity) algebra with classical central charg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.4579","kind":"arxiv","version":3},"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":"1008.4579","created_at":"2026-05-18T04:33:59.716363+00:00"},{"alias_kind":"arxiv_version","alias_value":"1008.4579v3","created_at":"2026-05-18T04:33:59.716363+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.4579","created_at":"2026-05-18T04:33:59.716363+00:00"},{"alias_kind":"pith_short_12","alias_value":"7LM2HH2ET6ZY","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"7LM2HH2ET6ZYT2UI","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"7LM2HH2E","created_at":"2026-05-18T12:26:04.259169+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2506.16164","citing_title":"The Carrollian Kaleidoscope","ref_index":155,"is_internal_anchor":true},{"citing_arxiv_id":"2602.20037","citing_title":"The asymptotic charges of Curtright dual graviton and Curtright extensions of BMS algebra","ref_index":76,"is_internal_anchor":true},{"citing_arxiv_id":"2603.21822","citing_title":"Self-dual gravity from higher-spin theory","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2604.27068","citing_title":"Holographic realization of higher-spin Carrollian free fields","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24873","citing_title":"Amplitudes in self-dual (higher-spin) theories","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT","json":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT.json","graph_json":"https://pith.science/api/pith-number/7LM2HH2ET6ZYT2UI4CXNLGJGIT/graph.json","events_json":"https://pith.science/api/pith-number/7LM2HH2ET6ZYT2UI4CXNLGJGIT/events.json","paper":"https://pith.science/paper/7LM2HH2E"},"agent_actions":{"view_html":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT","download_json":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT.json","view_paper":"https://pith.science/paper/7LM2HH2E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1008.4579&json=true","fetch_graph":"https://pith.science/api/pith-number/7LM2HH2ET6ZYT2UI4CXNLGJGIT/graph.json","fetch_events":"https://pith.science/api/pith-number/7LM2HH2ET6ZYT2UI4CXNLGJGIT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT/action/storage_attestation","attest_author":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT/action/author_attestation","sign_citation":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT/action/citation_signature","submit_replication":"https://pith.science/pith/7LM2HH2ET6ZYT2UI4CXNLGJGIT/action/replication_record"}},"created_at":"2026-05-18T04:33:59.716363+00:00","updated_at":"2026-05-18T04:33:59.716363+00:00"}