{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:Y45DOD6HG65FWA7L2UEALJQW6G","short_pith_number":"pith:Y45DOD6H","schema_version":"1.0","canonical_sha256":"c73a370fc737ba5b03ebd50805a616f18f9c8efb24de92761f8fe7a5d5d10272","source":{"kind":"arxiv","id":"2309.00511","version":1},"attestation_state":"computed","paper":{"title":"Schwinger-Keldysh effective field theory for stable and causal relativistic hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.stat-mech","hep-ph","nucl-th","physics.flu-dyn"],"primary_cat":"hep-th","authors_text":"Akash Jain, Pavel Kovtun","submitted_at":"2023-09-01T14:59:05Z","abstract_excerpt":"We construct stable and causal effective field theories (EFTs) for describing statistical fluctuations in relativistic diffusion and relativistic hydrodynamics. These EFTs are fully non-linear, including couplings to background sources, and enable us to compute n-point time-ordered correlation functions including the effects of statistical fluctuations. The EFTs we construct are inspired by the Maxwell-Cattaneo model of relativistic diffusion and M\\\"uller-Israel-Stewart model of relativistic hydrodynamics respectively, and have been derived using both the Martin-Siggia-Rose and Schwinger-Keldy"},"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":"2309.00511","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-09-01T14:59:05Z","cross_cats_sorted":["cond-mat.stat-mech","hep-ph","nucl-th","physics.flu-dyn"],"title_canon_sha256":"c1d5c61fb8b3fffb1b9466768a871a04f52a4a9cade35cc8ccbf4667c1972c79","abstract_canon_sha256":"234ce5ae3352a32bd24c3c9353d5df4ad89ce5069fe4f4ec05a1878a3217e889"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:46:58.147622Z","signature_b64":"LRDRG2ydyNHAaba5Vw/DU9juWKIs+TtqdvCS2YqlWq4oA27972hx7tllAKC9SXpdKghIO24RfqJuag5gAOAUAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c73a370fc737ba5b03ebd50805a616f18f9c8efb24de92761f8fe7a5d5d10272","last_reissued_at":"2026-07-05T06:46:58.147131Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:46:58.147131Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Schwinger-Keldysh effective field theory for stable and causal relativistic hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.stat-mech","hep-ph","nucl-th","physics.flu-dyn"],"primary_cat":"hep-th","authors_text":"Akash Jain, Pavel Kovtun","submitted_at":"2023-09-01T14:59:05Z","abstract_excerpt":"We construct stable and causal effective field theories (EFTs) for describing statistical fluctuations in relativistic diffusion and relativistic hydrodynamics. These EFTs are fully non-linear, including couplings to background sources, and enable us to compute n-point time-ordered correlation functions including the effects of statistical fluctuations. The EFTs we construct are inspired by the Maxwell-Cattaneo model of relativistic diffusion and M\\\"uller-Israel-Stewart model of relativistic hydrodynamics respectively, and have been derived using both the Martin-Siggia-Rose and Schwinger-Keldy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.00511","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/2309.00511/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":"2309.00511","created_at":"2026-07-05T06:46:58.147187+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.00511v1","created_at":"2026-07-05T06:46:58.147187+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.00511","created_at":"2026-07-05T06:46:58.147187+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y45DOD6HG65F","created_at":"2026-07-05T06:46:58.147187+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y45DOD6HG65FWA7L","created_at":"2026-07-05T06:46:58.147187+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y45DOD6H","created_at":"2026-07-05T06:46:58.147187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06666","citing_title":"Effective Field Theories for Material Media","ref_index":115,"is_internal_anchor":true},{"citing_arxiv_id":"2606.02446","citing_title":"Cumulant dynamics in finite-memory diffusion","ref_index":83,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26941","citing_title":"Schwinger-Keldysh Path Integral for Gauge theories","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26941","citing_title":"Schwinger-Keldysh Path Integral for Gauge theories","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01807","citing_title":"Relativistic BDNK MHD Evolution in a Boost-Invariant Medium and Its Impact on Dilepton Production","ref_index":40,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G","json":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G.json","graph_json":"https://pith.science/api/pith-number/Y45DOD6HG65FWA7L2UEALJQW6G/graph.json","events_json":"https://pith.science/api/pith-number/Y45DOD6HG65FWA7L2UEALJQW6G/events.json","paper":"https://pith.science/paper/Y45DOD6H"},"agent_actions":{"view_html":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G","download_json":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G.json","view_paper":"https://pith.science/paper/Y45DOD6H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.00511&json=true","fetch_graph":"https://pith.science/api/pith-number/Y45DOD6HG65FWA7L2UEALJQW6G/graph.json","fetch_events":"https://pith.science/api/pith-number/Y45DOD6HG65FWA7L2UEALJQW6G/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G/action/storage_attestation","attest_author":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G/action/author_attestation","sign_citation":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G/action/citation_signature","submit_replication":"https://pith.science/pith/Y45DOD6HG65FWA7L2UEALJQW6G/action/replication_record"}},"created_at":"2026-07-05T06:46:58.147187+00:00","updated_at":"2026-07-05T06:46:58.147187+00:00"}