{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:VM5TUECWMSA6AUTCFBMNLNLYMW","short_pith_number":"pith:VM5TUECW","schema_version":"1.0","canonical_sha256":"ab3b3a10566481e052622858d5b578659d1f0e21aa6f2e29cc99f8e818cb4a84","source":{"kind":"arxiv","id":"2010.08834","version":1},"attestation_state":"computed","paper":{"title":"Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Claudia Ratti, Jacquelyn Noronha-Hostler, Jorge Noronha, Nicol\\'as Yunes, Veronica Dexheimer","submitted_at":"2020-10-17T17:52:19Z","abstract_excerpt":"With the computational power and algorithmic improvements available today, the ongoing STAR/RHIC and HADES/GSI experiments, the future FAIR and NICA facilities becoming operational, and the new precise measurements from NICER and LIGO/VIRGO, the high-energy nuclear physics and astrophysics communities are in the unique position to set very stringent constraints on the equation of state of strongly interacting matter. We review the state-of-the-art of different approaches used in the description of hot and ultradense baryonic matter in and out of equilibrium, and discuss the regions in the phas"},"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":"2010.08834","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2020-10-17T17:52:19Z","cross_cats_sorted":["astro-ph.HE","gr-qc","hep-ph","nucl-ex"],"title_canon_sha256":"4474cfbd47913dbcb508affa5e696b034dc006e380b772f1fa0e4085638812cd","abstract_canon_sha256":"0524f0508c962a4f8838f16306b8e1491c28c44b07fa2e4d20fd70566a0742ec"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:55:34.106999Z","signature_b64":"iowvS9PRDsoRPQR8rmgyMMmzWNd3zpXZ7+8NiKFZWyV0T2Dxd+q2gSF/+W3FiNq2w7oFhOGJtesHRia7VWBlDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ab3b3a10566481e052622858d5b578659d1f0e21aa6f2e29cc99f8e818cb4a84","last_reissued_at":"2026-07-05T02:55:34.106497Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:55:34.106497Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Claudia Ratti, Jacquelyn Noronha-Hostler, Jorge Noronha, Nicol\\'as Yunes, Veronica Dexheimer","submitted_at":"2020-10-17T17:52:19Z","abstract_excerpt":"With the computational power and algorithmic improvements available today, the ongoing STAR/RHIC and HADES/GSI experiments, the future FAIR and NICA facilities becoming operational, and the new precise measurements from NICER and LIGO/VIRGO, the high-energy nuclear physics and astrophysics communities are in the unique position to set very stringent constraints on the equation of state of strongly interacting matter. We review the state-of-the-art of different approaches used in the description of hot and ultradense baryonic matter in and out of equilibrium, and discuss the regions in the phas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.08834","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/2010.08834/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":"2010.08834","created_at":"2026-07-05T02:55:34.106548+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.08834v1","created_at":"2026-07-05T02:55:34.106548+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.08834","created_at":"2026-07-05T02:55:34.106548+00:00"},{"alias_kind":"pith_short_12","alias_value":"VM5TUECWMSA6","created_at":"2026-07-05T02:55:34.106548+00:00"},{"alias_kind":"pith_short_16","alias_value":"VM5TUECWMSA6AUTC","created_at":"2026-07-05T02:55:34.106548+00:00"},{"alias_kind":"pith_short_8","alias_value":"VM5TUECW","created_at":"2026-07-05T02:55:34.106548+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.26326","citing_title":"Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine","ref_index":4,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW","json":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW.json","graph_json":"https://pith.science/api/pith-number/VM5TUECWMSA6AUTCFBMNLNLYMW/graph.json","events_json":"https://pith.science/api/pith-number/VM5TUECWMSA6AUTCFBMNLNLYMW/events.json","paper":"https://pith.science/paper/VM5TUECW"},"agent_actions":{"view_html":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW","download_json":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW.json","view_paper":"https://pith.science/paper/VM5TUECW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.08834&json=true","fetch_graph":"https://pith.science/api/pith-number/VM5TUECWMSA6AUTCFBMNLNLYMW/graph.json","fetch_events":"https://pith.science/api/pith-number/VM5TUECWMSA6AUTCFBMNLNLYMW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW/action/storage_attestation","attest_author":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW/action/author_attestation","sign_citation":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW/action/citation_signature","submit_replication":"https://pith.science/pith/VM5TUECWMSA6AUTCFBMNLNLYMW/action/replication_record"}},"created_at":"2026-07-05T02:55:34.106548+00:00","updated_at":"2026-07-05T02:55:34.106548+00:00"}