{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OADIF2BKPLNBADNXWSG5WL3VRU","short_pith_number":"pith:OADIF2BK","schema_version":"1.0","canonical_sha256":"700682e82a7ada100db7b48ddb2f758d18ad25c1c2cde110516446d6e6b5665f","source":{"kind":"arxiv","id":"2403.15657","version":1},"attestation_state":"computed","paper":{"title":"The Non-triviality of Dynamical Chern-Simons Gravity and the Standard Model","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Cyril Creque-Sarbinowski, Heliudson Bernardo, Stephon Alexander","submitted_at":"2024-03-23T00:31:53Z","abstract_excerpt":"Given the growing interest in gravitational-wave and cosmological parity-violating effects in dynamical Chern-Simons (dCS) gravity, it is crucial to investigate whether the scalar-gravitational Pontryagin term in dCS persists when formulated in the context of the $\\text{U(1)}_{\\text{B}-\\text{L}}$ anomaly in the Standard Model (SM). In particular, it has been argued that dCS gravity can be reduced to Einstein gravity after ''rotating away'' the gravitational-Pontryagin coupling into the phase of the Weinberg operator $\\unicode{x2013}$ analogous to the rotation of the axion zero-mode into the qu"},"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":"2403.15657","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"hep-th","submitted_at":"2024-03-23T00:31:53Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ph"],"title_canon_sha256":"d7ec5810b96adf67c4c26dbb1144004c0b76e1ad3597bc88f6e3ffbe9a16f63c","abstract_canon_sha256":"9b95047a55b12f6614aca238b1069637431cf1ebdf0ea57f02a646d0fc71946c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:59:39.861691Z","signature_b64":"tpf0XV7mf8Ew9grYHGMjkn9u6IXGyWkltLp0uPQxS2lL5VBgFhQChsPafr8dmU9TZtvfv+Cr4zY43kCropSHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"700682e82a7ada100db7b48ddb2f758d18ad25c1c2cde110516446d6e6b5665f","last_reissued_at":"2026-07-05T07:59:39.861303Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:59:39.861303Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Non-triviality of Dynamical Chern-Simons Gravity and the Standard Model","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Cyril Creque-Sarbinowski, Heliudson Bernardo, Stephon Alexander","submitted_at":"2024-03-23T00:31:53Z","abstract_excerpt":"Given the growing interest in gravitational-wave and cosmological parity-violating effects in dynamical Chern-Simons (dCS) gravity, it is crucial to investigate whether the scalar-gravitational Pontryagin term in dCS persists when formulated in the context of the $\\text{U(1)}_{\\text{B}-\\text{L}}$ anomaly in the Standard Model (SM). In particular, it has been argued that dCS gravity can be reduced to Einstein gravity after ''rotating away'' the gravitational-Pontryagin coupling into the phase of the Weinberg operator $\\unicode{x2013}$ analogous to the rotation of the axion zero-mode into the qu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.15657","kind":"arxiv","version":1},"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/2403.15657/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":"2403.15657","created_at":"2026-07-05T07:59:39.861366+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.15657v1","created_at":"2026-07-05T07:59:39.861366+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.15657","created_at":"2026-07-05T07:59:39.861366+00:00"},{"alias_kind":"pith_short_12","alias_value":"OADIF2BKPLNB","created_at":"2026-07-05T07:59:39.861366+00:00"},{"alias_kind":"pith_short_16","alias_value":"OADIF2BKPLNBADNX","created_at":"2026-07-05T07:59:39.861366+00:00"},{"alias_kind":"pith_short_8","alias_value":"OADIF2BK","created_at":"2026-07-05T07:59:39.861366+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.00166","citing_title":"Cascading amplification of gravitational waves triggered by environment in dynamical Chern-Simons gravity","ref_index":69,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU","json":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU.json","graph_json":"https://pith.science/api/pith-number/OADIF2BKPLNBADNXWSG5WL3VRU/graph.json","events_json":"https://pith.science/api/pith-number/OADIF2BKPLNBADNXWSG5WL3VRU/events.json","paper":"https://pith.science/paper/OADIF2BK"},"agent_actions":{"view_html":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU","download_json":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU.json","view_paper":"https://pith.science/paper/OADIF2BK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.15657&json=true","fetch_graph":"https://pith.science/api/pith-number/OADIF2BKPLNBADNXWSG5WL3VRU/graph.json","fetch_events":"https://pith.science/api/pith-number/OADIF2BKPLNBADNXWSG5WL3VRU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU/action/storage_attestation","attest_author":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU/action/author_attestation","sign_citation":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU/action/citation_signature","submit_replication":"https://pith.science/pith/OADIF2BKPLNBADNXWSG5WL3VRU/action/replication_record"}},"created_at":"2026-07-05T07:59:39.861366+00:00","updated_at":"2026-07-05T07:59:39.861366+00:00"}