{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:SSV6PI64JRAWTX5EUQGHY3LYXM","short_pith_number":"pith:SSV6PI64","schema_version":"1.0","canonical_sha256":"94abe7a3dc4c4169dfa4a40c7c6d78bb074a88544f672349e482f1321966bbf0","source":{"kind":"arxiv","id":"2008.08610","version":4},"attestation_state":"computed","paper":{"title":"Constraining momentum space correlators using slightly broken higher spin symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Renjan Rajan John, Sachin Jain, Vinay Malvimat","submitted_at":"2020-08-19T18:03:10Z","abstract_excerpt":"In this work, building up on [1] we present momentum space Ward identities related to broken higher spin symmetry as an alternate approach to computing correlators of spinning operators in interacting theories such as the quasi-fermionic and quasi-bosonic theories. The direct Feynman diagram approach to computing correlation functions is intricate and in general has been performed only in specific kinematic regimes. We use higher spin equations to obtain the parity even and parity odd contributions to two-, three- and four-point correlators involving spinning and scalar operators in a general "},"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":"2008.08610","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2020-08-19T18:03:10Z","cross_cats_sorted":[],"title_canon_sha256":"66c143ec4a6c12a40974f6075f7d996f6285cedf52c3b02f865f15d43d7e1b4d","abstract_canon_sha256":"6bdd098fa9b04d2f7ac5ed2eb62695b28790e552f69231d72cbc87dbc6ab0690"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:00:45.999162Z","signature_b64":"qONPbqziF2Iz4A+B2fEYWU8pR6HOLIjvhvWgQncWag8t2W/Uk+xxaj0f0zIBESaO9/EB3hTw5Zd+eE9cCGG5BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"94abe7a3dc4c4169dfa4a40c7c6d78bb074a88544f672349e482f1321966bbf0","last_reissued_at":"2026-07-05T03:00:45.998763Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:00:45.998763Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining momentum space correlators using slightly broken higher spin symmetry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Renjan Rajan John, Sachin Jain, Vinay Malvimat","submitted_at":"2020-08-19T18:03:10Z","abstract_excerpt":"In this work, building up on [1] we present momentum space Ward identities related to broken higher spin symmetry as an alternate approach to computing correlators of spinning operators in interacting theories such as the quasi-fermionic and quasi-bosonic theories. The direct Feynman diagram approach to computing correlation functions is intricate and in general has been performed only in specific kinematic regimes. We use higher spin equations to obtain the parity even and parity odd contributions to two-, three- and four-point correlators involving spinning and scalar operators in a general "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2008.08610","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2008.08610/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":"2008.08610","created_at":"2026-07-05T03:00:45.998829+00:00"},{"alias_kind":"arxiv_version","alias_value":"2008.08610v4","created_at":"2026-07-05T03:00:45.998829+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2008.08610","created_at":"2026-07-05T03:00:45.998829+00:00"},{"alias_kind":"pith_short_12","alias_value":"SSV6PI64JRAW","created_at":"2026-07-05T03:00:45.998829+00:00"},{"alias_kind":"pith_short_16","alias_value":"SSV6PI64JRAWTX5E","created_at":"2026-07-05T03:00:45.998829+00:00"},{"alias_kind":"pith_short_8","alias_value":"SSV6PI64","created_at":"2026-07-05T03:00:45.998829+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26623","citing_title":"Central charges $C_J$ and $C_T$ in QED$_d$-GNY model and scalar QED$_d$","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07503","citing_title":"Super-Grassmannians for $\\mathcal{N}=2$ to $4$ SCFT$_3$: From AdS$_4$ Correlators to $\\mathcal{N}=4$ SYM scattering Amplitudes","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07446","citing_title":"The $\\mathcal{N}=1$ Super-Grassmannian for CFT$_3$ and a Foray on AdS and Cosmological Correlators","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM","json":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM.json","graph_json":"https://pith.science/api/pith-number/SSV6PI64JRAWTX5EUQGHY3LYXM/graph.json","events_json":"https://pith.science/api/pith-number/SSV6PI64JRAWTX5EUQGHY3LYXM/events.json","paper":"https://pith.science/paper/SSV6PI64"},"agent_actions":{"view_html":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM","download_json":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM.json","view_paper":"https://pith.science/paper/SSV6PI64","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2008.08610&json=true","fetch_graph":"https://pith.science/api/pith-number/SSV6PI64JRAWTX5EUQGHY3LYXM/graph.json","fetch_events":"https://pith.science/api/pith-number/SSV6PI64JRAWTX5EUQGHY3LYXM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM/action/storage_attestation","attest_author":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM/action/author_attestation","sign_citation":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM/action/citation_signature","submit_replication":"https://pith.science/pith/SSV6PI64JRAWTX5EUQGHY3LYXM/action/replication_record"}},"created_at":"2026-07-05T03:00:45.998829+00:00","updated_at":"2026-07-05T03:00:45.998829+00:00"}