{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:DLDLTT7YS4E74RFSDNFUC3KXKO","short_pith_number":"pith:DLDLTT7Y","schema_version":"1.0","canonical_sha256":"1ac6b9cff89709fe44b21b4b416d5753b7305b099194f8c60fb0fbd9f01f7cfb","source":{"kind":"arxiv","id":"1809.05310","version":3},"attestation_state":"computed","paper":{"title":"Gauged Wess-Zumino terms for a general coset space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","cond-mat.supr-con","hep-ph"],"primary_cat":"hep-th","authors_text":"Helena Kolesova, Tomas Brauner","submitted_at":"2018-09-14T08:59:31Z","abstract_excerpt":"The low-energy physics of systems with spontaneously broken continuous symmetry is dominated by the ensuing Nambu-Goldstone bosons. It has been known for half a century how to construct invariant Lagrangian densities for the low-energy effective theory of Nambu-Goldstone bosons. Contributions, invariant only up to a surface term -- also known as the Wess-Zumino (WZ) terms -- are more subtle, and as a rule are topological in nature. Although WZ terms have been studied intensively in theoretically oriented literature, explicit expressions do not seem to be available in sufficient generality in a"},"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":"1809.05310","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2018-09-14T08:59:31Z","cross_cats_sorted":["cond-mat.str-el","cond-mat.supr-con","hep-ph"],"title_canon_sha256":"3721d5e8652b1afb28a4b05823cdc3374eac4661fc7d5506a133827ee41b6895","abstract_canon_sha256":"b01263b3f1bec65f0e060fcf7a4230bca4eba1af1ded180e5b3f0f65a3f61732"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:42:52.229208Z","signature_b64":"bT4H/ZsUj8EwsnWng4ZkOKwAA+gXZ3HvS3wDkMkXORS0dOz2s/8bzH6x1/coKKKgS2b+D9VN6T/4TnF628eGAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ac6b9cff89709fe44b21b4b416d5753b7305b099194f8c60fb0fbd9f01f7cfb","last_reissued_at":"2026-07-05T04:42:52.228786Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:42:52.228786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gauged Wess-Zumino terms for a general coset space","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.str-el","cond-mat.supr-con","hep-ph"],"primary_cat":"hep-th","authors_text":"Helena Kolesova, Tomas Brauner","submitted_at":"2018-09-14T08:59:31Z","abstract_excerpt":"The low-energy physics of systems with spontaneously broken continuous symmetry is dominated by the ensuing Nambu-Goldstone bosons. It has been known for half a century how to construct invariant Lagrangian densities for the low-energy effective theory of Nambu-Goldstone bosons. Contributions, invariant only up to a surface term -- also known as the Wess-Zumino (WZ) terms -- are more subtle, and as a rule are topological in nature. Although WZ terms have been studied intensively in theoretically oriented literature, explicit expressions do not seem to be available in sufficient generality in a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.05310","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/1809.05310/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":"1809.05310","created_at":"2026-07-05T04:42:52.228844+00:00"},{"alias_kind":"arxiv_version","alias_value":"1809.05310v3","created_at":"2026-07-05T04:42:52.228844+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.05310","created_at":"2026-07-05T04:42:52.228844+00:00"},{"alias_kind":"pith_short_12","alias_value":"DLDLTT7YS4E7","created_at":"2026-07-05T04:42:52.228844+00:00"},{"alias_kind":"pith_short_16","alias_value":"DLDLTT7YS4E74RFS","created_at":"2026-07-05T04:42:52.228844+00:00"},{"alias_kind":"pith_short_8","alias_value":"DLDLTT7Y","created_at":"2026-07-05T04:42:52.228844+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.07102","citing_title":"NLO observables for QCD-like theories and application to pion dark matter","ref_index":88,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO","json":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO.json","graph_json":"https://pith.science/api/pith-number/DLDLTT7YS4E74RFSDNFUC3KXKO/graph.json","events_json":"https://pith.science/api/pith-number/DLDLTT7YS4E74RFSDNFUC3KXKO/events.json","paper":"https://pith.science/paper/DLDLTT7Y"},"agent_actions":{"view_html":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO","download_json":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO.json","view_paper":"https://pith.science/paper/DLDLTT7Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1809.05310&json=true","fetch_graph":"https://pith.science/api/pith-number/DLDLTT7YS4E74RFSDNFUC3KXKO/graph.json","fetch_events":"https://pith.science/api/pith-number/DLDLTT7YS4E74RFSDNFUC3KXKO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO/action/storage_attestation","attest_author":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO/action/author_attestation","sign_citation":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO/action/citation_signature","submit_replication":"https://pith.science/pith/DLDLTT7YS4E74RFSDNFUC3KXKO/action/replication_record"}},"created_at":"2026-07-05T04:42:52.228844+00:00","updated_at":"2026-07-05T04:42:52.228844+00:00"}