{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:LDDFAEXI6DLEXG76ET3RHSBNMW","short_pith_number":"pith:LDDFAEXI","schema_version":"1.0","canonical_sha256":"58c65012e8f0d64b9bfe24f713c82d65b0c592ffcaaf1032b5f01d726c4947a7","source":{"kind":"arxiv","id":"nucl-th/9804058","version":1},"attestation_state":"computed","paper":{"title":"Equation of State, Spectra and Composition of Hot and Dense Infinite Hadronic Matter in a Microscopic Transport Model","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"C. Spieles, H. Stoecker, H. Weber, J. Konopka, L. Bravina, L. Neise, M. Belkacem, M. Bleicher, M. Brandstetter, M. I. Gorenstein, S. A. Bass, S. Soff, W. Greiner","submitted_at":"1998-04-23T12:58:19Z","abstract_excerpt":"Equilibrium properties of infinite relativistic hadron matter are investigated using the Ultrarelativistic Quantum Molecular Dynamics (UrQMD) model. The simulations are performed in a box with periodic boundary conditions. Equilibration times depend critically on energy and baryon densities. Energy spectra of various hadronic species are shown to be isotropic and consistent with a single temperature in equilibrium. The variation of energy density versus temperature shows a Hagedorn-like behavior with a limiting temperature of 130$\\pm$10 MeV. Comparison of abundances of different particle speci"},"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/9804058","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"1998-04-23T12:58:19Z","cross_cats_sorted":[],"title_canon_sha256":"2ec907bd51c0973b1037f1dfea22b5d1089a2d5dc6a91e1eb6e7659b4db43c06","abstract_canon_sha256":"e2f29ec61bf97774c5a171f67882639ec7e4c8abe9af3d566aa7673e422c34e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:23:27.747549Z","signature_b64":"9Qkcrkj/ldjZOaMQ8GqQi0507TBZVlO5LGPWmVQiAGz7lwVqbd9SPfCw1FhccmPhaC8QRdTe2nJW4aaii9JyDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"58c65012e8f0d64b9bfe24f713c82d65b0c592ffcaaf1032b5f01d726c4947a7","last_reissued_at":"2026-07-04T15:23:27.747114Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:23:27.747114Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Equation of State, Spectra and Composition of Hot and Dense Infinite Hadronic Matter in a Microscopic Transport Model","license":"","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"C. Spieles, H. Stoecker, H. Weber, J. Konopka, L. Bravina, L. Neise, M. Belkacem, M. Bleicher, M. Brandstetter, M. I. Gorenstein, S. A. Bass, S. Soff, W. Greiner","submitted_at":"1998-04-23T12:58:19Z","abstract_excerpt":"Equilibrium properties of infinite relativistic hadron matter are investigated using the Ultrarelativistic Quantum Molecular Dynamics (UrQMD) model. The simulations are performed in a box with periodic boundary conditions. Equilibration times depend critically on energy and baryon densities. Energy spectra of various hadronic species are shown to be isotropic and consistent with a single temperature in equilibrium. The variation of energy density versus temperature shows a Hagedorn-like behavior with a limiting temperature of 130$\\pm$10 MeV. Comparison of abundances of different particle speci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/9804058","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/nucl-th/9804058/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/9804058","created_at":"2026-07-04T15:23:27.747180+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/9804058v1","created_at":"2026-07-04T15:23:27.747180+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/9804058","created_at":"2026-07-04T15:23:27.747180+00:00"},{"alias_kind":"pith_short_12","alias_value":"LDDFAEXI6DLE","created_at":"2026-07-04T15:23:27.747180+00:00"},{"alias_kind":"pith_short_16","alias_value":"LDDFAEXI6DLEXG76","created_at":"2026-07-04T15:23:27.747180+00:00"},{"alias_kind":"pith_short_8","alias_value":"LDDFAEXI","created_at":"2026-07-04T15:23:27.747180+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW","json":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW.json","graph_json":"https://pith.science/api/pith-number/LDDFAEXI6DLEXG76ET3RHSBNMW/graph.json","events_json":"https://pith.science/api/pith-number/LDDFAEXI6DLEXG76ET3RHSBNMW/events.json","paper":"https://pith.science/paper/LDDFAEXI"},"agent_actions":{"view_html":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW","download_json":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW.json","view_paper":"https://pith.science/paper/LDDFAEXI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/9804058&json=true","fetch_graph":"https://pith.science/api/pith-number/LDDFAEXI6DLEXG76ET3RHSBNMW/graph.json","fetch_events":"https://pith.science/api/pith-number/LDDFAEXI6DLEXG76ET3RHSBNMW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW/action/storage_attestation","attest_author":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW/action/author_attestation","sign_citation":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW/action/citation_signature","submit_replication":"https://pith.science/pith/LDDFAEXI6DLEXG76ET3RHSBNMW/action/replication_record"}},"created_at":"2026-07-04T15:23:27.747180+00:00","updated_at":"2026-07-04T15:23:27.747180+00:00"}