{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:KNYC6U7GO33QELZINREXZUD3RN","short_pith_number":"pith:KNYC6U7G","schema_version":"1.0","canonical_sha256":"53702f53e676f7022f286c497cd07b8b728477feef2ce367ce52fcc256d558f6","source":{"kind":"arxiv","id":"hep-th/9806236","version":3},"attestation_state":"computed","paper":{"title":"Higher-Spin Gauge Interactions for Massive Matter Fields in 3D AdS Space-Time","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Mikhail Vasiliev (Lebedev Physics Institute), Sergey Prokushkin","submitted_at":"1998-06-29T19:26:14Z","abstract_excerpt":"A remarkable feature of the models with interactions exhibiting higher-spin (HS) gauge symmetries in $d>2$ is that their most symmetric vacua require (anti)-de Sitter (AdS) geometry rather than the flat one. In striking parallelism to what might be expected of M theory HS gauge theories describe infinite towers of fields of all spins and possess naturally space-time SUSY and Chan-Paton type inner symmetries. In this paper, we analyze at the level of the equations of motion the simplest non-trivial HS model which describes HS gauge interactions (on the top of the usual supergravitational and (C"},"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":"hep-th/9806236","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1998-06-29T19:26:14Z","cross_cats_sorted":[],"title_canon_sha256":"402e73fcbe5e8c5181687e14ca96fc0ab6382e6360b8c02b2e939ae167683501","abstract_canon_sha256":"70709523908892315061e708449dcca94651f75535005bad1aabe14ccdde35de"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:16:23.615296Z","signature_b64":"hWCcA7KMI0cur/b7/ezdJuZmXECPRth9xw3lSnC9KpSDNNJeCRWWB//LWkIMTUAmkyDr70DJtkEQbVL4uki5Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"53702f53e676f7022f286c497cd07b8b728477feef2ce367ce52fcc256d558f6","last_reissued_at":"2026-05-18T04:16:23.614818Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:16:23.614818Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higher-Spin Gauge Interactions for Massive Matter Fields in 3D AdS Space-Time","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Mikhail Vasiliev (Lebedev Physics Institute), Sergey Prokushkin","submitted_at":"1998-06-29T19:26:14Z","abstract_excerpt":"A remarkable feature of the models with interactions exhibiting higher-spin (HS) gauge symmetries in $d>2$ is that their most symmetric vacua require (anti)-de Sitter (AdS) geometry rather than the flat one. In striking parallelism to what might be expected of M theory HS gauge theories describe infinite towers of fields of all spins and possess naturally space-time SUSY and Chan-Paton type inner symmetries. In this paper, we analyze at the level of the equations of motion the simplest non-trivial HS model which describes HS gauge interactions (on the top of the usual supergravitational and (C"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9806236","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":"hep-th/9806236","created_at":"2026-05-18T04:16:23.614894+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9806236v3","created_at":"2026-05-18T04:16:23.614894+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9806236","created_at":"2026-05-18T04:16:23.614894+00:00"},{"alias_kind":"pith_short_12","alias_value":"KNYC6U7GO33Q","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_16","alias_value":"KNYC6U7GO33QELZI","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_8","alias_value":"KNYC6U7G","created_at":"2026-05-18T12:25:49.038998+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2508.11500","citing_title":"Differential Contracting Homotopy in the Linearized 3d Higher-Spin Theory","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2603.21822","citing_title":"Self-dual gravity from higher-spin theory","ref_index":40,"is_internal_anchor":true},{"citing_arxiv_id":"2604.27068","citing_title":"Holographic realization of higher-spin Carrollian free fields","ref_index":19,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN","json":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN.json","graph_json":"https://pith.science/api/pith-number/KNYC6U7GO33QELZINREXZUD3RN/graph.json","events_json":"https://pith.science/api/pith-number/KNYC6U7GO33QELZINREXZUD3RN/events.json","paper":"https://pith.science/paper/KNYC6U7G"},"agent_actions":{"view_html":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN","download_json":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN.json","view_paper":"https://pith.science/paper/KNYC6U7G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9806236&json=true","fetch_graph":"https://pith.science/api/pith-number/KNYC6U7GO33QELZINREXZUD3RN/graph.json","fetch_events":"https://pith.science/api/pith-number/KNYC6U7GO33QELZINREXZUD3RN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN/action/storage_attestation","attest_author":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN/action/author_attestation","sign_citation":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN/action/citation_signature","submit_replication":"https://pith.science/pith/KNYC6U7GO33QELZINREXZUD3RN/action/replication_record"}},"created_at":"2026-05-18T04:16:23.614894+00:00","updated_at":"2026-05-18T04:16:23.614894+00:00"}