{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:IPQJAK4P3WEQHCN4CSXY3BAKZO","short_pith_number":"pith:IPQJAK4P","schema_version":"1.0","canonical_sha256":"43e0902b8fdd890389bc14af8d840acb875e5864357f9728ff162d52780c7f07","source":{"kind":"arxiv","id":"nucl-th/0309055","version":2},"attestation_state":"computed","paper":{"title":"Causal Theories of Dissipative Relativistic Fluid Dynamics for Nuclear Collisions","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Azwinndini Muronga","submitted_at":"2003-09-22T08:18:17Z","abstract_excerpt":"Non-equilibrium fluid dynamics derived from the extended irreversible thermodynamics of the causal M\\\"uller--Israel--Stewart theory of dissipative processes in relativistic fluids based on Grad's moment method is applied to the study of the dynamics of hot matter produced in ultra--relativistic heavy ion collisions. The temperature, energy density and entropy evolution are investigated in the framework of the Bjorken boost--invariant scaling limit. The results of these second order theories are compared to those of first order theories due to Eckart and to Landau and Lifshitz and those of zero"},"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":"nucl-th/0309055","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"2003-09-22T08:18:17Z","cross_cats_sorted":[],"title_canon_sha256":"2375dcb969c7119b56c23e930baf03c93ee52ee45be9bca0d1816197af7ae058","abstract_canon_sha256":"12ae6d41d519d537f055e8a4e94a73f86b087ca7fd922ea709b9f6e18a2d8605"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:26:53.955493Z","signature_b64":"Jgqz5dFLJoQz3Y2L1CbsV7VtCyxx85msHKoeFK5YiizicMcTJhVl+bFxGMlw7Tyzh0LLygLjO5HwGUl7JJpXBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"43e0902b8fdd890389bc14af8d840acb875e5864357f9728ff162d52780c7f07","last_reissued_at":"2026-07-04T15:26:53.955082Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:26:53.955082Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Causal Theories of Dissipative Relativistic Fluid Dynamics for Nuclear Collisions","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Azwinndini Muronga","submitted_at":"2003-09-22T08:18:17Z","abstract_excerpt":"Non-equilibrium fluid dynamics derived from the extended irreversible thermodynamics of the causal M\\\"uller--Israel--Stewart theory of dissipative processes in relativistic fluids based on Grad's moment method is applied to the study of the dynamics of hot matter produced in ultra--relativistic heavy ion collisions. The temperature, energy density and entropy evolution are investigated in the framework of the Bjorken boost--invariant scaling limit. The results of these second order theories are compared to those of first order theories due to Eckart and to Landau and Lifshitz and those of zero"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/0309055","kind":"arxiv","version":2},"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/nucl-th/0309055/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":"nucl-th/0309055","created_at":"2026-07-04T15:26:53.955132+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/0309055v2","created_at":"2026-07-04T15:26:53.955132+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/0309055","created_at":"2026-07-04T15:26:53.955132+00:00"},{"alias_kind":"pith_short_12","alias_value":"IPQJAK4P3WEQ","created_at":"2026-07-04T15:26:53.955132+00:00"},{"alias_kind":"pith_short_16","alias_value":"IPQJAK4P3WEQHCN4","created_at":"2026-07-04T15:26:53.955132+00:00"},{"alias_kind":"pith_short_8","alias_value":"IPQJAK4P","created_at":"2026-07-04T15:26:53.955132+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.31749","citing_title":"Finite-Density Dynamics of Chemically Equilibrating QGP in Conformal Gubser Flow and Hard Thermal Photon Production","ref_index":9,"is_internal_anchor":true},{"citing_arxiv_id":"2512.04011","citing_title":"Freeze-out and spectral running of primordial gravitational waves in viscous cosmology","ref_index":49,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO","json":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO.json","graph_json":"https://pith.science/api/pith-number/IPQJAK4P3WEQHCN4CSXY3BAKZO/graph.json","events_json":"https://pith.science/api/pith-number/IPQJAK4P3WEQHCN4CSXY3BAKZO/events.json","paper":"https://pith.science/paper/IPQJAK4P"},"agent_actions":{"view_html":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO","download_json":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO.json","view_paper":"https://pith.science/paper/IPQJAK4P","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/0309055&json=true","fetch_graph":"https://pith.science/api/pith-number/IPQJAK4P3WEQHCN4CSXY3BAKZO/graph.json","fetch_events":"https://pith.science/api/pith-number/IPQJAK4P3WEQHCN4CSXY3BAKZO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO/action/storage_attestation","attest_author":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO/action/author_attestation","sign_citation":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO/action/citation_signature","submit_replication":"https://pith.science/pith/IPQJAK4P3WEQHCN4CSXY3BAKZO/action/replication_record"}},"created_at":"2026-07-04T15:26:53.955132+00:00","updated_at":"2026-07-04T15:26:53.955132+00:00"}