{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:O73RLRIEUNENGGO2L4PPFOIGKH","short_pith_number":"pith:O73RLRIE","schema_version":"1.0","canonical_sha256":"77f715c504a348d319da5f1ef2b90651d32fbf14c4350ffe4833fdb8c8a2f7ff","source":{"kind":"arxiv","id":"1204.2644","version":1},"attestation_state":"computed","paper":{"title":"Optimization of relativistic mean field model for finite nuclei to neutron star matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"A. Sulaksono, B. K. Agrawal, P. -G. Reinhard","submitted_at":"2012-04-12T07:43:05Z","abstract_excerpt":"We have optimized the parameters of extended relativistic mean-field model using a selected set of global observables which includes binding energies and charge radii for nuclei along several isotopic and isotonic chains and the iso-scalar giant monopole resonance energies for the $^{90}$Zr and $^{208}$Pb nuclei. The model parameters are further constrained by the available informations on the energy per neutron for the dilute neutron matter and bounds on the equations of state of the symmetric and asymmetric nuclear matter at supra-nuclear densities. Two new parameter sets BSP and IUFSU* are "},"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":"1204.2644","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2012-04-12T07:43:05Z","cross_cats_sorted":[],"title_canon_sha256":"fcabd786e611bce167212c544b855b57ce5f7b5bd264ed7e7fb01389f180eabe","abstract_canon_sha256":"8f1bff0ce0ba637f4de043f6b680841cc581203809e9ddf1c9a212df5376f7e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:53.249342Z","signature_b64":"v2nUikfGNpdKMyz8wEor0ertk8Liowv1t3vzxcpS3APpwWjiyv/FHnwX/q2TAR4pWOLBUP5QWSFBfs8TLqYlBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77f715c504a348d319da5f1ef2b90651d32fbf14c4350ffe4833fdb8c8a2f7ff","last_reissued_at":"2026-05-18T01:57:53.248892Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:53.248892Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Optimization of relativistic mean field model for finite nuclei to neutron star matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"A. Sulaksono, B. K. Agrawal, P. -G. Reinhard","submitted_at":"2012-04-12T07:43:05Z","abstract_excerpt":"We have optimized the parameters of extended relativistic mean-field model using a selected set of global observables which includes binding energies and charge radii for nuclei along several isotopic and isotonic chains and the iso-scalar giant monopole resonance energies for the $^{90}$Zr and $^{208}$Pb nuclei. The model parameters are further constrained by the available informations on the energy per neutron for the dilute neutron matter and bounds on the equations of state of the symmetric and asymmetric nuclear matter at supra-nuclear densities. Two new parameter sets BSP and IUFSU* are "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.2644","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":"1204.2644","created_at":"2026-05-18T01:57:53.248954+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.2644v1","created_at":"2026-05-18T01:57:53.248954+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.2644","created_at":"2026-05-18T01:57:53.248954+00:00"},{"alias_kind":"pith_short_12","alias_value":"O73RLRIEUNEN","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_16","alias_value":"O73RLRIEUNENGGO2","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_8","alias_value":"O73RLRIE","created_at":"2026-05-18T12:27:16.716162+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH","json":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH.json","graph_json":"https://pith.science/api/pith-number/O73RLRIEUNENGGO2L4PPFOIGKH/graph.json","events_json":"https://pith.science/api/pith-number/O73RLRIEUNENGGO2L4PPFOIGKH/events.json","paper":"https://pith.science/paper/O73RLRIE"},"agent_actions":{"view_html":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH","download_json":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH.json","view_paper":"https://pith.science/paper/O73RLRIE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.2644&json=true","fetch_graph":"https://pith.science/api/pith-number/O73RLRIEUNENGGO2L4PPFOIGKH/graph.json","fetch_events":"https://pith.science/api/pith-number/O73RLRIEUNENGGO2L4PPFOIGKH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH/action/storage_attestation","attest_author":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH/action/author_attestation","sign_citation":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH/action/citation_signature","submit_replication":"https://pith.science/pith/O73RLRIEUNENGGO2L4PPFOIGKH/action/replication_record"}},"created_at":"2026-05-18T01:57:53.248954+00:00","updated_at":"2026-05-18T01:57:53.248954+00:00"}