{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:MVDV22TWSTJGMQFFZFOIMCRYV2","short_pith_number":"pith:MVDV22TW","schema_version":"1.0","canonical_sha256":"65475d6a7694d26640a5c95c860a38aeb34b1c62e0e285eb464d853406885e00","source":{"kind":"arxiv","id":"1307.1566","version":1},"attestation_state":"computed","paper":{"title":"Core-crust transition pressure for relativistic slowly rotating neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"J. L. Bl\\'azquez-Salcedo, L. M. Gonz\\'alez-Romero","submitted_at":"2013-07-05T09:49:50Z","abstract_excerpt":"We study the influence of core-\\textit{crust} transition pressure changes on the general dynamical properties of neutron star configurations. First we study the matching conditions in core-\\textit{crust} transition pressure region, where phase transitions in the equation of state causes energy density jumps. Then using a surface \\textit{crust} approximation, we can construct configurations where the matter is described by the equation of state of the core of the star and the core-\\textit{crust} transition pressure. We will consider neutron stars in the slow rotation limit, considering perturba"},"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":"1307.1566","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2013-07-05T09:49:50Z","cross_cats_sorted":[],"title_canon_sha256":"136393531b5e18f9809507c84c3d14045c7488391def35e05fb81268dcf4d1c1","abstract_canon_sha256":"7c8049f58a4eb3f786115ec42aa6b123b505fde138d08762f020b0df6dbea6fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:19:12.530810Z","signature_b64":"TymRYXDaMeDsdHTY+YL9NOvoKef+Nr251MQ6LF9Sk7UuL1O+7GgABuX6Hg1lHKlA9HBHAHpXDqLuTraJneaFCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65475d6a7694d26640a5c95c860a38aeb34b1c62e0e285eb464d853406885e00","last_reissued_at":"2026-05-18T03:19:12.530237Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:19:12.530237Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Core-crust transition pressure for relativistic slowly rotating neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"J. L. Bl\\'azquez-Salcedo, L. M. Gonz\\'alez-Romero","submitted_at":"2013-07-05T09:49:50Z","abstract_excerpt":"We study the influence of core-\\textit{crust} transition pressure changes on the general dynamical properties of neutron star configurations. First we study the matching conditions in core-\\textit{crust} transition pressure region, where phase transitions in the equation of state causes energy density jumps. Then using a surface \\textit{crust} approximation, we can construct configurations where the matter is described by the equation of state of the core of the star and the core-\\textit{crust} transition pressure. We will consider neutron stars in the slow rotation limit, considering perturba"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1307.1566","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":"1307.1566","created_at":"2026-05-18T03:19:12.530322+00:00"},{"alias_kind":"arxiv_version","alias_value":"1307.1566v1","created_at":"2026-05-18T03:19:12.530322+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1307.1566","created_at":"2026-05-18T03:19:12.530322+00:00"},{"alias_kind":"pith_short_12","alias_value":"MVDV22TWSTJG","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_16","alias_value":"MVDV22TWSTJGMQFF","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_8","alias_value":"MVDV22TW","created_at":"2026-05-18T12:27:52.871228+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/MVDV22TWSTJGMQFFZFOIMCRYV2","json":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2.json","graph_json":"https://pith.science/api/pith-number/MVDV22TWSTJGMQFFZFOIMCRYV2/graph.json","events_json":"https://pith.science/api/pith-number/MVDV22TWSTJGMQFFZFOIMCRYV2/events.json","paper":"https://pith.science/paper/MVDV22TW"},"agent_actions":{"view_html":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2","download_json":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2.json","view_paper":"https://pith.science/paper/MVDV22TW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1307.1566&json=true","fetch_graph":"https://pith.science/api/pith-number/MVDV22TWSTJGMQFFZFOIMCRYV2/graph.json","fetch_events":"https://pith.science/api/pith-number/MVDV22TWSTJGMQFFZFOIMCRYV2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2/action/storage_attestation","attest_author":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2/action/author_attestation","sign_citation":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2/action/citation_signature","submit_replication":"https://pith.science/pith/MVDV22TWSTJGMQFFZFOIMCRYV2/action/replication_record"}},"created_at":"2026-05-18T03:19:12.530322+00:00","updated_at":"2026-05-18T03:19:12.530322+00:00"}