{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:5XQ5BEW4RDRSB5MLNGCC3CHARF","short_pith_number":"pith:5XQ5BEW4","schema_version":"1.0","canonical_sha256":"ede1d092dc88e320f58b69842d88e0894d8aeee898cf4dada92aef0f4be1e9f2","source":{"kind":"arxiv","id":"2211.06628","version":3},"attestation_state":"computed","paper":{"title":"Higher derivative invariants in four dimensional N=3 Poincare supergravity","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Bindusar Sahoo, Debangshu Mukherjee, Madhu Mishra, Subramanya Hegde","submitted_at":"2022-11-12T10:35:03Z","abstract_excerpt":"In this paper, we use the superconformal approach to derive the higher derivative action for N = 3 Poincare supergravity in four space-time dimensions. We first study the coupling of N = 3 vector multiplets to conformal supergravity. Thereafter we combine it with the pure N = 3 conformal supergravity action and use a minimum of three vector multiplets as compensators to arrive at Poincare supergravity with higher derivative corrections. We give a general prescription on how to eliminate the auxiliary fields in an iterative manner and obtain the supergravity action order by order in derivatives"},"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":"2211.06628","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"hep-th","submitted_at":"2022-11-12T10:35:03Z","cross_cats_sorted":[],"title_canon_sha256":"cae310bb1981b1dfe0f2125f7087520cfc2292c8f502256f6db7b84aa56a7143","abstract_canon_sha256":"b7565e0f77cc5aec3ee96cdc7ca436f78de414352bd45eb6dff4fe26541bf3b2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:53:05.984593Z","signature_b64":"jAGCyaqhqFoVPOpZVQG8yiNunT2cTe4GZxaLSeEggssr/ODtWe/MPuS9W27r1ZMTZdy+dw+pee8EnRMoZHRYCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ede1d092dc88e320f58b69842d88e0894d8aeee898cf4dada92aef0f4be1e9f2","last_reissued_at":"2026-07-05T05:53:05.984176Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:53:05.984176Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higher derivative invariants in four dimensional N=3 Poincare supergravity","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Bindusar Sahoo, Debangshu Mukherjee, Madhu Mishra, Subramanya Hegde","submitted_at":"2022-11-12T10:35:03Z","abstract_excerpt":"In this paper, we use the superconformal approach to derive the higher derivative action for N = 3 Poincare supergravity in four space-time dimensions. We first study the coupling of N = 3 vector multiplets to conformal supergravity. Thereafter we combine it with the pure N = 3 conformal supergravity action and use a minimum of three vector multiplets as compensators to arrive at Poincare supergravity with higher derivative corrections. We give a general prescription on how to eliminate the auxiliary fields in an iterative manner and obtain the supergravity action order by order in derivatives"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.06628","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2211.06628/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":"2211.06628","created_at":"2026-07-05T05:53:05.984234+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.06628v3","created_at":"2026-07-05T05:53:05.984234+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.06628","created_at":"2026-07-05T05:53:05.984234+00:00"},{"alias_kind":"pith_short_12","alias_value":"5XQ5BEW4RDRS","created_at":"2026-07-05T05:53:05.984234+00:00"},{"alias_kind":"pith_short_16","alias_value":"5XQ5BEW4RDRSB5ML","created_at":"2026-07-05T05:53:05.984234+00:00"},{"alias_kind":"pith_short_8","alias_value":"5XQ5BEW4","created_at":"2026-07-05T05:53:05.984234+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2505.00638","citing_title":"Only Flat Spacetime is Full BPS in Four Dimensional N=3 and N=4 Supergravity","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF","json":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF.json","graph_json":"https://pith.science/api/pith-number/5XQ5BEW4RDRSB5MLNGCC3CHARF/graph.json","events_json":"https://pith.science/api/pith-number/5XQ5BEW4RDRSB5MLNGCC3CHARF/events.json","paper":"https://pith.science/paper/5XQ5BEW4"},"agent_actions":{"view_html":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF","download_json":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF.json","view_paper":"https://pith.science/paper/5XQ5BEW4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.06628&json=true","fetch_graph":"https://pith.science/api/pith-number/5XQ5BEW4RDRSB5MLNGCC3CHARF/graph.json","fetch_events":"https://pith.science/api/pith-number/5XQ5BEW4RDRSB5MLNGCC3CHARF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF/action/storage_attestation","attest_author":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF/action/author_attestation","sign_citation":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF/action/citation_signature","submit_replication":"https://pith.science/pith/5XQ5BEW4RDRSB5MLNGCC3CHARF/action/replication_record"}},"created_at":"2026-07-05T05:53:05.984234+00:00","updated_at":"2026-07-05T05:53:05.984234+00:00"}