{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:UQBD7HH6V6CL5IIOIU3ALD327X","short_pith_number":"pith:UQBD7HH6","schema_version":"1.0","canonical_sha256":"a4023f9cfeaf84bea10e4536058f7afdcd59005e924755fa3913030197576cc9","source":{"kind":"arxiv","id":"astro-ph/9804189","version":1},"attestation_state":"computed","paper":{"title":"Neutron superfluidity in strongly magnetic interiors of neutron stars and its effect on thermal evolution","license":"","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph","authors_text":"Ch. Schaab, F. Weber, M. K. Weigel (University of Munich)","submitted_at":"1998-04-20T11:14:03Z","abstract_excerpt":"The possibility of a neutron m=2-superfluid in the interior of neutron stars is investigated. This pairing state is energetically favoured in strong magnetic fields ($H\\sim 10^{16}-10^{17}$ G). Because of the node in the angular-dependent energy gap along the field direction the neutrino emissivity is only suppressed polynomially as function in $T/T_{c}$ instead of exponentially, as it is obtained for a nodeless pairing state. The effect of this pairing state on the thermal evolution of neutron stars is studied, and its outcome is compared with the evolution of ``normal'', i.e. nodeless, super"},"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":"astro-ph/9804189","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1998-04-20T11:14:03Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"e46d5f880004bca8867186d7ec76feb8a53d8bd2b4a7d3ab61dac1e14b3a139b","abstract_canon_sha256":"8656f5d381b639b5985fa01c9490ba0bb582265156b903953cfb4eb78d9643cb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:37.585177Z","signature_b64":"5xy1dgmq/WC0v5GRYIlbiZvKkVW15oKtnUcpLjTiOdS08wHApcIfFKquwosIUtA5Ihc3Mt9fr+AjoEjD8XEbCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a4023f9cfeaf84bea10e4536058f7afdcd59005e924755fa3913030197576cc9","last_reissued_at":"2026-05-18T01:07:37.584562Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:37.584562Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutron superfluidity in strongly magnetic interiors of neutron stars and its effect on thermal evolution","license":"","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph","authors_text":"Ch. Schaab, F. Weber, M. K. Weigel (University of Munich)","submitted_at":"1998-04-20T11:14:03Z","abstract_excerpt":"The possibility of a neutron m=2-superfluid in the interior of neutron stars is investigated. This pairing state is energetically favoured in strong magnetic fields ($H\\sim 10^{16}-10^{17}$ G). Because of the node in the angular-dependent energy gap along the field direction the neutrino emissivity is only suppressed polynomially as function in $T/T_{c}$ instead of exponentially, as it is obtained for a nodeless pairing state. The effect of this pairing state on the thermal evolution of neutron stars is studied, and its outcome is compared with the evolution of ``normal'', i.e. nodeless, super"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9804189","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":"astro-ph/9804189","created_at":"2026-05-18T01:07:37.584663+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9804189v1","created_at":"2026-05-18T01:07:37.584663+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9804189","created_at":"2026-05-18T01:07:37.584663+00:00"},{"alias_kind":"pith_short_12","alias_value":"UQBD7HH6V6CL","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_16","alias_value":"UQBD7HH6V6CL5IIO","created_at":"2026-05-18T12:25:49.038998+00:00"},{"alias_kind":"pith_short_8","alias_value":"UQBD7HH6","created_at":"2026-05-18T12:25:49.038998+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/UQBD7HH6V6CL5IIOIU3ALD327X","json":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X.json","graph_json":"https://pith.science/api/pith-number/UQBD7HH6V6CL5IIOIU3ALD327X/graph.json","events_json":"https://pith.science/api/pith-number/UQBD7HH6V6CL5IIOIU3ALD327X/events.json","paper":"https://pith.science/paper/UQBD7HH6"},"agent_actions":{"view_html":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X","download_json":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X.json","view_paper":"https://pith.science/paper/UQBD7HH6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9804189&json=true","fetch_graph":"https://pith.science/api/pith-number/UQBD7HH6V6CL5IIOIU3ALD327X/graph.json","fetch_events":"https://pith.science/api/pith-number/UQBD7HH6V6CL5IIOIU3ALD327X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X/action/storage_attestation","attest_author":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X/action/author_attestation","sign_citation":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X/action/citation_signature","submit_replication":"https://pith.science/pith/UQBD7HH6V6CL5IIOIU3ALD327X/action/replication_record"}},"created_at":"2026-05-18T01:07:37.584663+00:00","updated_at":"2026-05-18T01:07:37.584663+00:00"}