{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:R27J2XGFPSY7P24VS4HSENOZ73","short_pith_number":"pith:R27J2XGF","schema_version":"1.0","canonical_sha256":"8ebe9d5cc57cb1f7eb95970f2235d9fee4c004987d99b569195537e2fd5d0ae5","source":{"kind":"arxiv","id":"1405.3967","version":1},"attestation_state":"computed","paper":{"title":"Towards an effective action for relativistic dissipative hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","nucl-th"],"primary_cat":"hep-ph","authors_text":"Guy D. Moore, Paul Romatschke, Pavel Kovtun","submitted_at":"2014-05-15T19:45:55Z","abstract_excerpt":"We propose an effective action for first order relativistic dissipative hydrodynamics that can be used to evaluate n-point symmetrized correlation functions, taking into account thermal fluctuations of the hydrodynamic variables."},"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":"1405.3967","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-05-15T19:45:55Z","cross_cats_sorted":["hep-th","nucl-th"],"title_canon_sha256":"6aaa02b3f7091bebda7cc6a904f37fa1a5de9b5ad8dbe7cf658ae59c5551aa41","abstract_canon_sha256":"fac30d96dc6c2efb1ce8110babb868c1210ff2f6a5a1225ec2edcf2978005057"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:11.972806Z","signature_b64":"aFZD3zrZVS52lAHkGLZiUGGlSKGPNddOlHmhZvDeGl8FKeDEnoEs7B6SzXdn55gAlGDykDHJZVTQMRmV+BLWCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8ebe9d5cc57cb1f7eb95970f2235d9fee4c004987d99b569195537e2fd5d0ae5","last_reissued_at":"2026-05-18T01:43:11.972186Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:11.972186Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Towards an effective action for relativistic dissipative hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","nucl-th"],"primary_cat":"hep-ph","authors_text":"Guy D. Moore, Paul Romatschke, Pavel Kovtun","submitted_at":"2014-05-15T19:45:55Z","abstract_excerpt":"We propose an effective action for first order relativistic dissipative hydrodynamics that can be used to evaluate n-point symmetrized correlation functions, taking into account thermal fluctuations of the hydrodynamic variables."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.3967","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":""},"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":"1405.3967","created_at":"2026-05-18T01:43:11.972284+00:00"},{"alias_kind":"arxiv_version","alias_value":"1405.3967v1","created_at":"2026-05-18T01:43:11.972284+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.3967","created_at":"2026-05-18T01:43:11.972284+00:00"},{"alias_kind":"pith_short_12","alias_value":"R27J2XGFPSY7","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"R27J2XGFPSY7P24V","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"R27J2XGF","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.18346","citing_title":"Schwinger-Keldysh effective theory of charge transport: redundancies and systematic $\\omega/T$ expansion","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2604.27730","citing_title":"Non-Gaussian hydrodynamic fluctuations in an expanding relativistic fluid","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73","json":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73.json","graph_json":"https://pith.science/api/pith-number/R27J2XGFPSY7P24VS4HSENOZ73/graph.json","events_json":"https://pith.science/api/pith-number/R27J2XGFPSY7P24VS4HSENOZ73/events.json","paper":"https://pith.science/paper/R27J2XGF"},"agent_actions":{"view_html":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73","download_json":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73.json","view_paper":"https://pith.science/paper/R27J2XGF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1405.3967&json=true","fetch_graph":"https://pith.science/api/pith-number/R27J2XGFPSY7P24VS4HSENOZ73/graph.json","fetch_events":"https://pith.science/api/pith-number/R27J2XGFPSY7P24VS4HSENOZ73/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73/action/storage_attestation","attest_author":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73/action/author_attestation","sign_citation":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73/action/citation_signature","submit_replication":"https://pith.science/pith/R27J2XGFPSY7P24VS4HSENOZ73/action/replication_record"}},"created_at":"2026-05-18T01:43:11.972284+00:00","updated_at":"2026-05-18T01:43:11.972284+00:00"}