{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:UUKT2ME3JSHOXITET75XBCHJZT","short_pith_number":"pith:UUKT2ME3","schema_version":"1.0","canonical_sha256":"a5153d309b4c8eeba2649ffb7088e9ccf340d02e9f34c4f9a1d0c6f7d5b7bfa1","source":{"kind":"arxiv","id":"2106.03590","version":2},"attestation_state":"computed","paper":{"title":"Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"nucl-th","authors_text":"Aziz Rabhi, Constan\\c{c}a Provid\\^encia, M\\'arcio Ferreira","submitted_at":"2021-06-07T13:16:30Z","abstract_excerpt":"The effect of temperature on the crust-core transition of a magnetar is studied. The thermodynamical spinodals are used to calculate the transition region within a relativistic mean-field approach for the equation of state. Magnetic fields with intensities $5\\times 10^{16}$ G and $5\\times 10 ^{17}$ G are considered. It is shown that the effect on the extension of the crust-core transition is washed away for temperatures above $10^{9}$ K for magnetic field intensities $ \\lesssim 5\\times 10^{16}$ G but may still persist if a magnetic field as high as $5\\times 10 ^{17}$G is considered. For temper"},"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":"2106.03590","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2021-06-07T13:16:30Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"980f7a9ea53ae727eaf56cfae59b7a32bd158532c90371f12fa47854d1da665e","abstract_canon_sha256":"832728987dcfd61752fe351c7f07fd05b18db8ca7f186552eb39eb2adaadcb29"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:12:38.994118Z","signature_b64":"CXcJED96ljWEmOMEMrqnKhi474Qs97zXYnfQXic3RoWn9bL1V8LuR+RIlGVwnsDHbh24Ktt2lyhZKcBvuQzHDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a5153d309b4c8eeba2649ffb7088e9ccf340d02e9f34c4f9a1d0c6f7d5b7bfa1","last_reissued_at":"2026-07-05T03:12:38.993703Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:12:38.993703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Crust-core transition of a neutron star: effect of the temperature under strong magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"nucl-th","authors_text":"Aziz Rabhi, Constan\\c{c}a Provid\\^encia, M\\'arcio Ferreira","submitted_at":"2021-06-07T13:16:30Z","abstract_excerpt":"The effect of temperature on the crust-core transition of a magnetar is studied. The thermodynamical spinodals are used to calculate the transition region within a relativistic mean-field approach for the equation of state. Magnetic fields with intensities $5\\times 10^{16}$ G and $5\\times 10 ^{17}$ G are considered. It is shown that the effect on the extension of the crust-core transition is washed away for temperatures above $10^{9}$ K for magnetic field intensities $ \\lesssim 5\\times 10^{16}$ G but may still persist if a magnetic field as high as $5\\times 10 ^{17}$G is considered. For temper"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2106.03590","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2106.03590/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":"2106.03590","created_at":"2026-07-05T03:12:38.993768+00:00"},{"alias_kind":"arxiv_version","alias_value":"2106.03590v2","created_at":"2026-07-05T03:12:38.993768+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2106.03590","created_at":"2026-07-05T03:12:38.993768+00:00"},{"alias_kind":"pith_short_12","alias_value":"UUKT2ME3JSHO","created_at":"2026-07-05T03:12:38.993768+00:00"},{"alias_kind":"pith_short_16","alias_value":"UUKT2ME3JSHOXITE","created_at":"2026-07-05T03:12:38.993768+00:00"},{"alias_kind":"pith_short_8","alias_value":"UUKT2ME3","created_at":"2026-07-05T03:12:38.993768+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/UUKT2ME3JSHOXITET75XBCHJZT","json":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT.json","graph_json":"https://pith.science/api/pith-number/UUKT2ME3JSHOXITET75XBCHJZT/graph.json","events_json":"https://pith.science/api/pith-number/UUKT2ME3JSHOXITET75XBCHJZT/events.json","paper":"https://pith.science/paper/UUKT2ME3"},"agent_actions":{"view_html":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT","download_json":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT.json","view_paper":"https://pith.science/paper/UUKT2ME3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2106.03590&json=true","fetch_graph":"https://pith.science/api/pith-number/UUKT2ME3JSHOXITET75XBCHJZT/graph.json","fetch_events":"https://pith.science/api/pith-number/UUKT2ME3JSHOXITET75XBCHJZT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT/action/storage_attestation","attest_author":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT/action/author_attestation","sign_citation":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT/action/citation_signature","submit_replication":"https://pith.science/pith/UUKT2ME3JSHOXITET75XBCHJZT/action/replication_record"}},"created_at":"2026-07-05T03:12:38.993768+00:00","updated_at":"2026-07-05T03:12:38.993768+00:00"}