{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:H6XSHE6XLKE5S63OTZDSIBUTPV","short_pith_number":"pith:H6XSHE6X","schema_version":"1.0","canonical_sha256":"3faf2393d75a89d97b6e9e472406937d559b34ec7b0023240a1325e191bf44a8","source":{"kind":"arxiv","id":"1112.2018","version":1},"attestation_state":"computed","paper":{"title":"The nuclear symmetry energy, the inner crust, and global neutron star modeling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"Bao-An Li, Josh Hooker, Michael Gearheart, William G. Newton","submitted_at":"2011-12-09T04:50:26Z","abstract_excerpt":"The structure and composition of the inner crust of neutron stars, as well as global stellar properties such as radius and moment of inertia, have been shown to correlate with parameters characterizing the symmetry energy of nuclear matter such as its magnitude J and density dependence L at saturation density. It is thus mutually beneficial to nuclear physicists and astrophysicists to examine the combined effects of such correlations on potential neutron star observables in the light of recent experimental and theoretical constraints on J, L, and relationships between them. We review some basi"},"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":"1112.2018","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-12-09T04:50:26Z","cross_cats_sorted":["nucl-ex","nucl-th"],"title_canon_sha256":"b3b1c5acd407202ef69069351638e56b86d7bd7e75881d96c6612e219743c4de","abstract_canon_sha256":"718fd2fd79b4277c583006fb989e3169b7d442ae89168f53346cf74a89c4da41"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:06:44.349775Z","signature_b64":"ucku0ZVicmr6Vgqj+94urz46n8ZKSMMAOGj3xHbW7OSuqoqC/78d2Hom5jjA6nEqpcKbRjTsp1psAuXo5UUyCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3faf2393d75a89d97b6e9e472406937d559b34ec7b0023240a1325e191bf44a8","last_reissued_at":"2026-05-18T04:06:44.349219Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:06:44.349219Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The nuclear symmetry energy, the inner crust, and global neutron star modeling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"Bao-An Li, Josh Hooker, Michael Gearheart, William G. Newton","submitted_at":"2011-12-09T04:50:26Z","abstract_excerpt":"The structure and composition of the inner crust of neutron stars, as well as global stellar properties such as radius and moment of inertia, have been shown to correlate with parameters characterizing the symmetry energy of nuclear matter such as its magnitude J and density dependence L at saturation density. It is thus mutually beneficial to nuclear physicists and astrophysicists to examine the combined effects of such correlations on potential neutron star observables in the light of recent experimental and theoretical constraints on J, L, and relationships between them. We review some basi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1112.2018","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":"1112.2018","created_at":"2026-05-18T04:06:44.349305+00:00"},{"alias_kind":"arxiv_version","alias_value":"1112.2018v1","created_at":"2026-05-18T04:06:44.349305+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1112.2018","created_at":"2026-05-18T04:06:44.349305+00:00"},{"alias_kind":"pith_short_12","alias_value":"H6XSHE6XLKE5","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"H6XSHE6XLKE5S63O","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"H6XSHE6X","created_at":"2026-05-18T12:26:30.835961+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/H6XSHE6XLKE5S63OTZDSIBUTPV","json":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV.json","graph_json":"https://pith.science/api/pith-number/H6XSHE6XLKE5S63OTZDSIBUTPV/graph.json","events_json":"https://pith.science/api/pith-number/H6XSHE6XLKE5S63OTZDSIBUTPV/events.json","paper":"https://pith.science/paper/H6XSHE6X"},"agent_actions":{"view_html":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV","download_json":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV.json","view_paper":"https://pith.science/paper/H6XSHE6X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1112.2018&json=true","fetch_graph":"https://pith.science/api/pith-number/H6XSHE6XLKE5S63OTZDSIBUTPV/graph.json","fetch_events":"https://pith.science/api/pith-number/H6XSHE6XLKE5S63OTZDSIBUTPV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV/action/storage_attestation","attest_author":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV/action/author_attestation","sign_citation":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV/action/citation_signature","submit_replication":"https://pith.science/pith/H6XSHE6XLKE5S63OTZDSIBUTPV/action/replication_record"}},"created_at":"2026-05-18T04:06:44.349305+00:00","updated_at":"2026-05-18T04:06:44.349305+00:00"}