{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:GX6RFFQUVWDCEBOVKU2YLPCWWZ","short_pith_number":"pith:GX6RFFQU","schema_version":"1.0","canonical_sha256":"35fd129614ad862205d5553585bc56b647952c53bd8187e74d095d1baca66e81","source":{"kind":"arxiv","id":"1406.5302","version":2},"attestation_state":"computed","paper":{"title":"Stability of the $\\beta$-equilibrated dense matter and core-crust transition in neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Debasis Atta, D.N. Basu","submitted_at":"2014-06-20T08:03:13Z","abstract_excerpt":"The stability of the $\\beta$-equilibrated dense nuclear matter is analyzed with respect to the thermodynamic stability conditions. Based on the density dependent M3Y effective nucleon-nucleon interaction, the effects of the nuclear incompressibility on the proton fraction in neutron stars and the location of the inner edge of their crusts and core-crust transition density and pressure are investigated. The high-density behavior of symmetric and asymmetric nuclear matter satisfies the constraints from the observed flow data of heavy-ion collisions. The neutron star properties studied using $\\be"},"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":"1406.5302","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2014-06-20T08:03:13Z","cross_cats_sorted":[],"title_canon_sha256":"0abf260a96eb7bcce4c77e81f6d6168c812874bf6c4306b6e596bcddf298e3a6","abstract_canon_sha256":"a0cf71d6f92433e2866701e800c223f0a0708e4390b380f73e0f00664cc71b83"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:43:34.895734Z","signature_b64":"ctB5usuKDo733+3WgRmkk17R1MRYTvWOfQla0Trkyxmt/jovhVjOWDHtuZe9nb9WVg90VKDLDfBbfLVA9w7QAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"35fd129614ad862205d5553585bc56b647952c53bd8187e74d095d1baca66e81","last_reissued_at":"2026-05-18T02:43:34.895239Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:43:34.895239Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stability of the $\\beta$-equilibrated dense matter and core-crust transition in neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Debasis Atta, D.N. Basu","submitted_at":"2014-06-20T08:03:13Z","abstract_excerpt":"The stability of the $\\beta$-equilibrated dense nuclear matter is analyzed with respect to the thermodynamic stability conditions. Based on the density dependent M3Y effective nucleon-nucleon interaction, the effects of the nuclear incompressibility on the proton fraction in neutron stars and the location of the inner edge of their crusts and core-crust transition density and pressure are investigated. The high-density behavior of symmetric and asymmetric nuclear matter satisfies the constraints from the observed flow data of heavy-ion collisions. The neutron star properties studied using $\\be"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.5302","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":""},"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":"1406.5302","created_at":"2026-05-18T02:43:34.895307+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.5302v2","created_at":"2026-05-18T02:43:34.895307+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.5302","created_at":"2026-05-18T02:43:34.895307+00:00"},{"alias_kind":"pith_short_12","alias_value":"GX6RFFQUVWDC","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"GX6RFFQUVWDCEBOV","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"GX6RFFQU","created_at":"2026-05-18T12:28:30.664211+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/GX6RFFQUVWDCEBOVKU2YLPCWWZ","json":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ.json","graph_json":"https://pith.science/api/pith-number/GX6RFFQUVWDCEBOVKU2YLPCWWZ/graph.json","events_json":"https://pith.science/api/pith-number/GX6RFFQUVWDCEBOVKU2YLPCWWZ/events.json","paper":"https://pith.science/paper/GX6RFFQU"},"agent_actions":{"view_html":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ","download_json":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ.json","view_paper":"https://pith.science/paper/GX6RFFQU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.5302&json=true","fetch_graph":"https://pith.science/api/pith-number/GX6RFFQUVWDCEBOVKU2YLPCWWZ/graph.json","fetch_events":"https://pith.science/api/pith-number/GX6RFFQUVWDCEBOVKU2YLPCWWZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ/action/storage_attestation","attest_author":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ/action/author_attestation","sign_citation":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ/action/citation_signature","submit_replication":"https://pith.science/pith/GX6RFFQUVWDCEBOVKU2YLPCWWZ/action/replication_record"}},"created_at":"2026-05-18T02:43:34.895307+00:00","updated_at":"2026-05-18T02:43:34.895307+00:00"}