{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:3Y3W2KULT3COPTT2TAX4P4HBCY","short_pith_number":"pith:3Y3W2KUL","schema_version":"1.0","canonical_sha256":"de376d2a8b9ec4e7ce7a982fc7f0e11618754f0228e75421fae49035aecd97c9","source":{"kind":"arxiv","id":"nucl-th/0403074","version":2},"attestation_state":"computed","paper":{"title":"Indication of quark deconfinement and evidence for a Hubble flow in 130 and 200 GeV Au+Au collisions","license":"","headline":"","cross_cats":["hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"A. Ster, B. Lorstad, M. Csanad, T. Csorgo","submitted_at":"2004-03-24T18:07:06Z","abstract_excerpt":"Buda-Lund hydro model fits are compared to BRAHMS, PHENIX, PHOBOS and STAR data on identified particle spectra, two-particle Bose-Einstein or HBT correlations, charged particle pseudorapidity distributions and pseudorapidity as well as p_t dependent elliptic flow in sqrt(s_NN) = 130 and 200 GeV Au+Au collisions at RHIC. Preliminary results indicate that 7/8-th of the particle emitting volume is rather cold, with surface temperature of 105 MeV, but the temperature has a distribution and the most central 1/8-th of the volume is superheated to temperatures above the critical value, T(x) > T_c = 1"},"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/0403074","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"nucl-th","submitted_at":"2004-03-24T18:07:06Z","cross_cats_sorted":["hep-ph","nucl-ex"],"title_canon_sha256":"f5ff5e3d35919a19159a0ed4664a3c55faf9d3e7ccc1ab97726cec12bd259bfe","abstract_canon_sha256":"7156f5ee18599fc6391f8c07bd6b8a3675282f429a7b96edfca91ba3a6cc23b2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:37:34.137463Z","signature_b64":"vb2KV86Guaq9kp04aRYa8iH/C6zNX66tXHHw2SZ3NHoW2uE/mVFiOuYsFVy1dCD837ixfPKfp//2GLFxvfzjCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de376d2a8b9ec4e7ce7a982fc7f0e11618754f0228e75421fae49035aecd97c9","last_reissued_at":"2026-07-04T15:37:34.137072Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:37:34.137072Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Indication of quark deconfinement and evidence for a Hubble flow in 130 and 200 GeV Au+Au collisions","license":"","headline":"","cross_cats":["hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"A. Ster, B. Lorstad, M. Csanad, T. Csorgo","submitted_at":"2004-03-24T18:07:06Z","abstract_excerpt":"Buda-Lund hydro model fits are compared to BRAHMS, PHENIX, PHOBOS and STAR data on identified particle spectra, two-particle Bose-Einstein or HBT correlations, charged particle pseudorapidity distributions and pseudorapidity as well as p_t dependent elliptic flow in sqrt(s_NN) = 130 and 200 GeV Au+Au collisions at RHIC. Preliminary results indicate that 7/8-th of the particle emitting volume is rather cold, with surface temperature of 105 MeV, but the temperature has a distribution and the most central 1/8-th of the volume is superheated to temperatures above the critical value, T(x) > T_c = 1"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-th/0403074","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/0403074/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/0403074","created_at":"2026-07-04T15:37:34.137130+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-th/0403074v2","created_at":"2026-07-04T15:37:34.137130+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-th/0403074","created_at":"2026-07-04T15:37:34.137130+00:00"},{"alias_kind":"pith_short_12","alias_value":"3Y3W2KULT3CO","created_at":"2026-07-04T15:37:34.137130+00:00"},{"alias_kind":"pith_short_16","alias_value":"3Y3W2KULT3COPTT2","created_at":"2026-07-04T15:37:34.137130+00:00"},{"alias_kind":"pith_short_8","alias_value":"3Y3W2KUL","created_at":"2026-07-04T15:37:34.137130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1909.02498","citing_title":"A simple family of solutions of relativistic viscous hydrodynamics for fireballs with Hubble flow and ellipsoidal symmetry","ref_index":41,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY","json":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY.json","graph_json":"https://pith.science/api/pith-number/3Y3W2KULT3COPTT2TAX4P4HBCY/graph.json","events_json":"https://pith.science/api/pith-number/3Y3W2KULT3COPTT2TAX4P4HBCY/events.json","paper":"https://pith.science/paper/3Y3W2KUL"},"agent_actions":{"view_html":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY","download_json":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY.json","view_paper":"https://pith.science/paper/3Y3W2KUL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-th/0403074&json=true","fetch_graph":"https://pith.science/api/pith-number/3Y3W2KULT3COPTT2TAX4P4HBCY/graph.json","fetch_events":"https://pith.science/api/pith-number/3Y3W2KULT3COPTT2TAX4P4HBCY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY/action/storage_attestation","attest_author":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY/action/author_attestation","sign_citation":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY/action/citation_signature","submit_replication":"https://pith.science/pith/3Y3W2KULT3COPTT2TAX4P4HBCY/action/replication_record"}},"created_at":"2026-07-04T15:37:34.137130+00:00","updated_at":"2026-07-04T15:37:34.137130+00:00"}