{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:SW5GHEGZFD6RFAU472A3C4JISY","short_pith_number":"pith:SW5GHEGZ","schema_version":"1.0","canonical_sha256":"95ba6390d928fd12829cfe81b17128963c976766b98bb0dc007e89d117ef0e15","source":{"kind":"arxiv","id":"1005.4811","version":1},"attestation_state":"computed","paper":{"title":"Thermodynamics of dense hadronic matter in a parity doublet model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Chihiro Sasaki, Igor Mishustin","submitted_at":"2010-05-26T13:44:02Z","abstract_excerpt":"We study thermodynamics of nuclear matter in a two-flavored parity doublet model within the mean field approximation. Parameters of the model are chosen to reproduce correctly the properties of the nuclear ground state. The model predicts two phase transitions in nuclear matter, a liquid-gas phase transition at normal nuclear density and a chiral transition at higher density. At finite temperature the pion decay constant exhibits a considerable reduction at intermediate values of chemical potential, which is traced back to the presence of the liquid-gas transition, and approaches zero at highe"},"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":"1005.4811","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-05-26T13:44:02Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"0ac5caa3b8746d8c067ca5e10e2cd543e7059bbe615267afb3c89265ae8fbf68","abstract_canon_sha256":"69b99aa47aa5bd6756b4623b2fbe07e266f9d2217e31bbf8131403cb092a394d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:33:23.929760Z","signature_b64":"OjVgf8oJvrVCsZE94WjiSzKvuV67k9g10YHej4EoUenzA66IIOj8XDXUSet7Ew7IdPKC9N7hhXlttW0IE8BZCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"95ba6390d928fd12829cfe81b17128963c976766b98bb0dc007e89d117ef0e15","last_reissued_at":"2026-05-18T02:33:23.929157Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:33:23.929157Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamics of dense hadronic matter in a parity doublet model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Chihiro Sasaki, Igor Mishustin","submitted_at":"2010-05-26T13:44:02Z","abstract_excerpt":"We study thermodynamics of nuclear matter in a two-flavored parity doublet model within the mean field approximation. Parameters of the model are chosen to reproduce correctly the properties of the nuclear ground state. The model predicts two phase transitions in nuclear matter, a liquid-gas phase transition at normal nuclear density and a chiral transition at higher density. At finite temperature the pion decay constant exhibits a considerable reduction at intermediate values of chemical potential, which is traced back to the presence of the liquid-gas transition, and approaches zero at highe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.4811","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":""},"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":"1005.4811","created_at":"2026-05-18T02:33:23.929261+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.4811v1","created_at":"2026-05-18T02:33:23.929261+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.4811","created_at":"2026-05-18T02:33:23.929261+00:00"},{"alias_kind":"pith_short_12","alias_value":"SW5GHEGZFD6R","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"SW5GHEGZFD6RFAU4","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"SW5GHEGZ","created_at":"2026-05-18T12:26:13.927090+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.05921","citing_title":"Matter And Gravitation In Collisions of heavy ions and neutron stars: equation of state","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY","json":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY.json","graph_json":"https://pith.science/api/pith-number/SW5GHEGZFD6RFAU472A3C4JISY/graph.json","events_json":"https://pith.science/api/pith-number/SW5GHEGZFD6RFAU472A3C4JISY/events.json","paper":"https://pith.science/paper/SW5GHEGZ"},"agent_actions":{"view_html":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY","download_json":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY.json","view_paper":"https://pith.science/paper/SW5GHEGZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.4811&json=true","fetch_graph":"https://pith.science/api/pith-number/SW5GHEGZFD6RFAU472A3C4JISY/graph.json","fetch_events":"https://pith.science/api/pith-number/SW5GHEGZFD6RFAU472A3C4JISY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY/action/storage_attestation","attest_author":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY/action/author_attestation","sign_citation":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY/action/citation_signature","submit_replication":"https://pith.science/pith/SW5GHEGZFD6RFAU472A3C4JISY/action/replication_record"}},"created_at":"2026-05-18T02:33:23.929261+00:00","updated_at":"2026-05-18T02:33:23.929261+00:00"}