{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:CSMZ4OB4FXDHOYC7ZX6MEUFOAM","short_pith_number":"pith:CSMZ4OB4","schema_version":"1.0","canonical_sha256":"14999e383c2dc677605fcdfcc250ae030b42ea5d2d4fc578f781a5ad1b25fd54","source":{"kind":"arxiv","id":"1912.01265","version":1},"attestation_state":"computed","paper":{"title":"Crystallization of the inner crust of a neutron star and the influence of shell effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"A. F. Fantina, F. Gulminelli, J. M. Pearson, N. Chamel, T. Carreau","submitted_at":"2019-12-03T09:51:49Z","abstract_excerpt":"Context. In the cooling process of a non-accreting neutron star, the composition and properties of the crust are thought to be fixed at the finite temperature where nuclear reactions fall out of equilibrium. A lower estimation for this temperature is given by the crystallization temperature, which can be as high as $\\approx 7\\times 10^9$ K in the inner crust, potentially leading to sizeable differences with respect to the simplifying cold-catalyzed matter hypothesis. Aims. We extend the recent work by Fantina et al. (2019) on the outer crust, to the study of the crystallization of the inner cr"},"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":"1912.01265","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-12-03T09:51:49Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"78c459d0a09c5306a332a4f16fea60d7c51f6ae41b6a7010b0cbd379d00dcf37","abstract_canon_sha256":"f543e426ba9bb9c47251b84d319a062442767d623ee7f42d24c5c1ae568213ea"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:46:53.844543Z","signature_b64":"pXMhF98MohTbJ/a0t9zxZrwLE9Bc9tqazQbMp43zvwvsB7MW6K6WHiiG3ALFZ+BSo4LsPgSC8ONmmmVp3oB3Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14999e383c2dc677605fcdfcc250ae030b42ea5d2d4fc578f781a5ad1b25fd54","last_reissued_at":"2026-07-05T00:46:53.844069Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:46:53.844069Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Crystallization of the inner crust of a neutron star and the influence of shell effects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"A. F. Fantina, F. Gulminelli, J. M. Pearson, N. Chamel, T. Carreau","submitted_at":"2019-12-03T09:51:49Z","abstract_excerpt":"Context. In the cooling process of a non-accreting neutron star, the composition and properties of the crust are thought to be fixed at the finite temperature where nuclear reactions fall out of equilibrium. A lower estimation for this temperature is given by the crystallization temperature, which can be as high as $\\approx 7\\times 10^9$ K in the inner crust, potentially leading to sizeable differences with respect to the simplifying cold-catalyzed matter hypothesis. Aims. We extend the recent work by Fantina et al. (2019) on the outer crust, to the study of the crystallization of the inner cr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.01265","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1912.01265/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":"1912.01265","created_at":"2026-07-05T00:46:53.844120+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.01265v1","created_at":"2026-07-05T00:46:53.844120+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.01265","created_at":"2026-07-05T00:46:53.844120+00:00"},{"alias_kind":"pith_short_12","alias_value":"CSMZ4OB4FXDH","created_at":"2026-07-05T00:46:53.844120+00:00"},{"alias_kind":"pith_short_16","alias_value":"CSMZ4OB4FXDHOYC7","created_at":"2026-07-05T00:46:53.844120+00:00"},{"alias_kind":"pith_short_8","alias_value":"CSMZ4OB4","created_at":"2026-07-05T00:46:53.844120+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2505.16929","citing_title":"Properties of the neutron star crust informed by nuclear structure data","ref_index":64,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM","json":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM.json","graph_json":"https://pith.science/api/pith-number/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/graph.json","events_json":"https://pith.science/api/pith-number/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/events.json","paper":"https://pith.science/paper/CSMZ4OB4"},"agent_actions":{"view_html":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM","download_json":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM.json","view_paper":"https://pith.science/paper/CSMZ4OB4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.01265&json=true","fetch_graph":"https://pith.science/api/pith-number/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/graph.json","fetch_events":"https://pith.science/api/pith-number/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/action/storage_attestation","attest_author":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/action/author_attestation","sign_citation":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/action/citation_signature","submit_replication":"https://pith.science/pith/CSMZ4OB4FXDHOYC7ZX6MEUFOAM/action/replication_record"}},"created_at":"2026-07-05T00:46:53.844120+00:00","updated_at":"2026-07-05T00:46:53.844120+00:00"}