{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:BNUH3ZZYQOKWQE3HFA27VVC4QD","short_pith_number":"pith:BNUH3ZZY","schema_version":"1.0","canonical_sha256":"0b687de73883956813672835fad45c80c6a9b3e3eb6e9c781689412c152253ab","source":{"kind":"arxiv","id":"2402.15548","version":1},"attestation_state":"computed","paper":{"title":"General predictions of neutron star properties using unified relativistic mean-field equations of state","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-th","authors_text":"Francesca Gulminelli, Helena Pais, Luigi Scurto","submitted_at":"2024-02-23T15:31:46Z","abstract_excerpt":"In this work we present general predictions for the static observables of neutron stars (NSs) under the hypothesis of a purely nucleonic composition of the ultra-dense baryonic matter, using Bayesian inference on a very large parameter space conditioned by both astrophysical and nuclear physics constraints. The equation of states are obtained using a unified approach of the NS core and inner crust within a fully covariant treatment based on a relativistic mean-field Lagrangian density with density dependent couplings. The posterior distributions are well compatible with the ones obtained by se"},"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":"2402.15548","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"nucl-th","submitted_at":"2024-02-23T15:31:46Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"ba35d9d2659aa94167221d1aafde41c5f0ff730cee1653dd95538e0bfc3398a5","abstract_canon_sha256":"ac79f2200dd54a3076b4319f1340f6b9e389ecbaec9308f40bb962532b03e63e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:49:37.607803Z","signature_b64":"bopl7G965sRPogW3JNikTlpBgQXBk+FVPywaBiWjFMit3B1dw+oH6J/VmUIMImVvuurO8XDyN3mKNIBn4ZGTAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b687de73883956813672835fad45c80c6a9b3e3eb6e9c781689412c152253ab","last_reissued_at":"2026-07-05T07:49:37.607385Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:49:37.607385Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"General predictions of neutron star properties using unified relativistic mean-field equations of state","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-th","authors_text":"Francesca Gulminelli, Helena Pais, Luigi Scurto","submitted_at":"2024-02-23T15:31:46Z","abstract_excerpt":"In this work we present general predictions for the static observables of neutron stars (NSs) under the hypothesis of a purely nucleonic composition of the ultra-dense baryonic matter, using Bayesian inference on a very large parameter space conditioned by both astrophysical and nuclear physics constraints. The equation of states are obtained using a unified approach of the NS core and inner crust within a fully covariant treatment based on a relativistic mean-field Lagrangian density with density dependent couplings. The posterior distributions are well compatible with the ones obtained by se"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.15548","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/2402.15548/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":"2402.15548","created_at":"2026-07-05T07:49:37.607447+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.15548v1","created_at":"2026-07-05T07:49:37.607447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.15548","created_at":"2026-07-05T07:49:37.607447+00:00"},{"alias_kind":"pith_short_12","alias_value":"BNUH3ZZYQOKW","created_at":"2026-07-05T07:49:37.607447+00:00"},{"alias_kind":"pith_short_16","alias_value":"BNUH3ZZYQOKWQE3H","created_at":"2026-07-05T07:49:37.607447+00:00"},{"alias_kind":"pith_short_8","alias_value":"BNUH3ZZY","created_at":"2026-07-05T07:49:37.607447+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.01503","citing_title":"Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Influences of parametrizations of density dependent couplings","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD","json":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD.json","graph_json":"https://pith.science/api/pith-number/BNUH3ZZYQOKWQE3HFA27VVC4QD/graph.json","events_json":"https://pith.science/api/pith-number/BNUH3ZZYQOKWQE3HFA27VVC4QD/events.json","paper":"https://pith.science/paper/BNUH3ZZY"},"agent_actions":{"view_html":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD","download_json":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD.json","view_paper":"https://pith.science/paper/BNUH3ZZY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.15548&json=true","fetch_graph":"https://pith.science/api/pith-number/BNUH3ZZYQOKWQE3HFA27VVC4QD/graph.json","fetch_events":"https://pith.science/api/pith-number/BNUH3ZZYQOKWQE3HFA27VVC4QD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD/action/storage_attestation","attest_author":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD/action/author_attestation","sign_citation":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD/action/citation_signature","submit_replication":"https://pith.science/pith/BNUH3ZZYQOKWQE3HFA27VVC4QD/action/replication_record"}},"created_at":"2026-07-05T07:49:37.607447+00:00","updated_at":"2026-07-05T07:49:37.607447+00:00"}