{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:FIGAMOCKHSK32TBBX2XGKWT4QO","short_pith_number":"pith:FIGAMOCK","schema_version":"1.0","canonical_sha256":"2a0c06384a3c95bd4c21beae655a7c83a0b165009662331eff477203ce67c46f","source":{"kind":"arxiv","id":"2201.13150","version":2},"attestation_state":"computed","paper":{"title":"Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"nucl-th","authors_text":"Anton Motornenko, Elias R. Most, Horst Stoecker, Jan Steinheimer, Luciano Rezzolla, Matthias Hanauske, Veronica Dexheimer","submitted_at":"2022-01-31T11:51:19Z","abstract_excerpt":"Binary neutron-star mergers and heavy-ion collisions are related through the properties of the hot and dense nuclear matter formed during these extreme events. In particular, low-energy heavy-ion collisions offer exciting prospects to recreate such {extreme} conditions in the laboratory. However, it remains unexplored to what degree those collisions can actually reproduce hot and dense matter formed in binary neutron star mergers. As a way to understand similarities and differences between these systems, we {discuss their geometry and }perform a direct numerical comparison of the thermodynamic"},"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":"2201.13150","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2022-01-31T11:51:19Z","cross_cats_sorted":["astro-ph.HE","gr-qc"],"title_canon_sha256":"6f18c590f7fd5215868129e0eaab03d4a02940cb95bfdfa3a2eef336bb3b48f6","abstract_canon_sha256":"774c5397295ba98e9153f7c4842d9ad236a9b5153f996d2e001e2c0c50454d42"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:57:10.375400Z","signature_b64":"ZDacHuT/32PjmTdlwRbnuM4RlVJCjOJpH896nWLw5aXB3rmGBKVjd3DZ6UGaLxjQg6VgUBXoc9RTjLvX7Mc+Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2a0c06384a3c95bd4c21beae655a7c83a0b165009662331eff477203ce67c46f","last_reissued_at":"2026-07-05T05:57:10.374887Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:57:10.374887Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing neutron-star matter in the lab: similarities and differences between binary mergers and heavy-ion collisions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"nucl-th","authors_text":"Anton Motornenko, Elias R. Most, Horst Stoecker, Jan Steinheimer, Luciano Rezzolla, Matthias Hanauske, Veronica Dexheimer","submitted_at":"2022-01-31T11:51:19Z","abstract_excerpt":"Binary neutron-star mergers and heavy-ion collisions are related through the properties of the hot and dense nuclear matter formed during these extreme events. In particular, low-energy heavy-ion collisions offer exciting prospects to recreate such {extreme} conditions in the laboratory. However, it remains unexplored to what degree those collisions can actually reproduce hot and dense matter formed in binary neutron star mergers. As a way to understand similarities and differences between these systems, we {discuss their geometry and }perform a direct numerical comparison of the thermodynamic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.13150","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/2201.13150/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":"2201.13150","created_at":"2026-07-05T05:57:10.374946+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.13150v2","created_at":"2026-07-05T05:57:10.374946+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.13150","created_at":"2026-07-05T05:57:10.374946+00:00"},{"alias_kind":"pith_short_12","alias_value":"FIGAMOCKHSK3","created_at":"2026-07-05T05:57:10.374946+00:00"},{"alias_kind":"pith_short_16","alias_value":"FIGAMOCKHSK32TBB","created_at":"2026-07-05T05:57:10.374946+00:00"},{"alias_kind":"pith_short_8","alias_value":"FIGAMOCK","created_at":"2026-07-05T05:57:10.374946+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"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":3,"is_internal_anchor":false},{"citing_arxiv_id":"2606.08522","citing_title":"Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08584","citing_title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","ref_index":66,"is_internal_anchor":false},{"citing_arxiv_id":"2411.04969","citing_title":"Systematic study of flow of protons and light clusters in intermediate-energy heavy-ion collisions with momentum-dependent potentials","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2510.09104","citing_title":"Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2602.02654","citing_title":"Dynamical response of twin stars to perturbations","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08584","citing_title":"The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover","ref_index":66,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO","json":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO.json","graph_json":"https://pith.science/api/pith-number/FIGAMOCKHSK32TBBX2XGKWT4QO/graph.json","events_json":"https://pith.science/api/pith-number/FIGAMOCKHSK32TBBX2XGKWT4QO/events.json","paper":"https://pith.science/paper/FIGAMOCK"},"agent_actions":{"view_html":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO","download_json":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO.json","view_paper":"https://pith.science/paper/FIGAMOCK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.13150&json=true","fetch_graph":"https://pith.science/api/pith-number/FIGAMOCKHSK32TBBX2XGKWT4QO/graph.json","fetch_events":"https://pith.science/api/pith-number/FIGAMOCKHSK32TBBX2XGKWT4QO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO/action/storage_attestation","attest_author":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO/action/author_attestation","sign_citation":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO/action/citation_signature","submit_replication":"https://pith.science/pith/FIGAMOCKHSK32TBBX2XGKWT4QO/action/replication_record"}},"created_at":"2026-07-05T05:57:10.374946+00:00","updated_at":"2026-07-05T05:57:10.374946+00:00"}