{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:4KAPEYPO4ZK7QDWIDZQC5MXLNX","short_pith_number":"pith:4KAPEYPO","schema_version":"1.0","canonical_sha256":"e280f261eee655f80ec81e602eb2eb6deb089d54549dc02b76e30a59ef77df43","source":{"kind":"arxiv","id":"2211.16498","version":2},"attestation_state":"computed","paper":{"title":"Carrollian conformal scalar as flat-space singleton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrea Campoleoni, Simon Pekar, Xavier Bekaert","submitted_at":"2022-11-29T18:59:11Z","abstract_excerpt":"We show that, in any space-time dimension, the on-shell (electric) conformal Carrollian scalar can be interpreted as the flat-space limit of the singleton representation of the conformal algebra. In fact, a recently proposed higher-spin algebra for Minkowski spacetime amounts to the Poincar\\'e enveloping algebra on the corresponding module. This higher-spin algebra is a contraction of that entering Vasiliev's equations, which can be constructed analogously from the singleton representation of the conformal algebra. We also show that the higher-spin extension of the Poincar\\'e algebra we consid"},"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":"2211.16498","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-11-29T18:59:11Z","cross_cats_sorted":[],"title_canon_sha256":"daf1ae7dea82b349106293ebddfc46356bdb9145397cfe80fa5552bbcb1aaacf","abstract_canon_sha256":"e7ce331a1e905d67b197296098d5528720c60ecde138e1c54513c2c6471ad785"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:44:05.558263Z","signature_b64":"qNNpVCgKrqoIvXlCnEuV2bEDM/K2UyaIv9cmGNRE3oJ+gIaqdDuyms1Gzm54T9gQm2bw1sY6ld0kBXoQ9BmrBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e280f261eee655f80ec81e602eb2eb6deb089d54549dc02b76e30a59ef77df43","last_reissued_at":"2026-07-05T05:44:05.557791Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:44:05.557791Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Carrollian conformal scalar as flat-space singleton","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Andrea Campoleoni, Simon Pekar, Xavier Bekaert","submitted_at":"2022-11-29T18:59:11Z","abstract_excerpt":"We show that, in any space-time dimension, the on-shell (electric) conformal Carrollian scalar can be interpreted as the flat-space limit of the singleton representation of the conformal algebra. In fact, a recently proposed higher-spin algebra for Minkowski spacetime amounts to the Poincar\\'e enveloping algebra on the corresponding module. This higher-spin algebra is a contraction of that entering Vasiliev's equations, which can be constructed analogously from the singleton representation of the conformal algebra. We also show that the higher-spin extension of the Poincar\\'e algebra we consid"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.16498","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/2211.16498/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":"2211.16498","created_at":"2026-07-05T05:44:05.557848+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.16498v2","created_at":"2026-07-05T05:44:05.557848+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.16498","created_at":"2026-07-05T05:44:05.557848+00:00"},{"alias_kind":"pith_short_12","alias_value":"4KAPEYPO4ZK7","created_at":"2026-07-05T05:44:05.557848+00:00"},{"alias_kind":"pith_short_16","alias_value":"4KAPEYPO4ZK7QDWI","created_at":"2026-07-05T05:44:05.557848+00:00"},{"alias_kind":"pith_short_8","alias_value":"4KAPEYPO","created_at":"2026-07-05T05:44:05.557848+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06826","citing_title":"BMS$_3$ invariant field theories","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2606.03955","citing_title":"Flat from AdS: in any dimension and for any spin","ref_index":84,"is_internal_anchor":false},{"citing_arxiv_id":"2506.16164","citing_title":"The Carrollian Kaleidoscope","ref_index":73,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX","json":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX.json","graph_json":"https://pith.science/api/pith-number/4KAPEYPO4ZK7QDWIDZQC5MXLNX/graph.json","events_json":"https://pith.science/api/pith-number/4KAPEYPO4ZK7QDWIDZQC5MXLNX/events.json","paper":"https://pith.science/paper/4KAPEYPO"},"agent_actions":{"view_html":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX","download_json":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX.json","view_paper":"https://pith.science/paper/4KAPEYPO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.16498&json=true","fetch_graph":"https://pith.science/api/pith-number/4KAPEYPO4ZK7QDWIDZQC5MXLNX/graph.json","fetch_events":"https://pith.science/api/pith-number/4KAPEYPO4ZK7QDWIDZQC5MXLNX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX/action/storage_attestation","attest_author":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX/action/author_attestation","sign_citation":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX/action/citation_signature","submit_replication":"https://pith.science/pith/4KAPEYPO4ZK7QDWIDZQC5MXLNX/action/replication_record"}},"created_at":"2026-07-05T05:44:05.557848+00:00","updated_at":"2026-07-05T05:44:05.557848+00:00"}