{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:3KEN6VL3H2FUZPEYMLP2ISZ4YR","short_pith_number":"pith:3KEN6VL3","schema_version":"1.0","canonical_sha256":"da88df557b3e8b4cbc9862dfa44b3cc45a7681a2531c2cdeb4b0274172a2b4ec","source":{"kind":"arxiv","id":"1109.0018","version":2},"attestation_state":"computed","paper":{"title":"Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Wynn C. G. Ho (University of Southampton)","submitted_at":"2011-08-31T20:04:04Z","abstract_excerpt":"Neutron stars accreting matter from low-mass binary companions are observed to undergo bursts of X-rays due to the thermonuclear explosion of material on the neutron star surface. We use recent results on superfluid and superconducting properties to show that the core temperature in these neutron stars may not be uniquely determined for a range of observed accretion rates. The degeneracy in inferred core temperatures could contribute to explaining the difference between neutron stars which have very short recurrence times between multiple bursts and those which have long recurrence times betwe"},"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":"1109.0018","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-08-31T20:04:04Z","cross_cats_sorted":["astro-ph.SR","hep-ph"],"title_canon_sha256":"8f096f8c60acb014ad3af52787480ed24daa3f4efbe8dbe2cb962d8a6023c409","abstract_canon_sha256":"2f3b3c0207e911208575fca0e3858d0ba7beadaed7bc66594da1123670a37fbd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:04:33.210027Z","signature_b64":"Vfs2OPBWj+59zZkQWo6pkgVK4/qP+b4RkQzg1EGWhLkN+jO5pU7buAXPVUBiZW3eUBytq848nh/82PDmNq1OAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"da88df557b3e8b4cbc9862dfa44b3cc45a7681a2531c2cdeb4b0274172a2b4ec","last_reissued_at":"2026-05-18T04:04:33.209339Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:04:33.209339Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Superfluid effects on gauging core temperatures of neutron stars in low-mass X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Wynn C. G. Ho (University of Southampton)","submitted_at":"2011-08-31T20:04:04Z","abstract_excerpt":"Neutron stars accreting matter from low-mass binary companions are observed to undergo bursts of X-rays due to the thermonuclear explosion of material on the neutron star surface. We use recent results on superfluid and superconducting properties to show that the core temperature in these neutron stars may not be uniquely determined for a range of observed accretion rates. The degeneracy in inferred core temperatures could contribute to explaining the difference between neutron stars which have very short recurrence times between multiple bursts and those which have long recurrence times betwe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.0018","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":"1109.0018","created_at":"2026-05-18T04:04:33.209429+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.0018v2","created_at":"2026-05-18T04:04:33.209429+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.0018","created_at":"2026-05-18T04:04:33.209429+00:00"},{"alias_kind":"pith_short_12","alias_value":"3KEN6VL3H2FU","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_16","alias_value":"3KEN6VL3H2FUZPEY","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_8","alias_value":"3KEN6VL3","created_at":"2026-05-18T12:26:18.847500+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/3KEN6VL3H2FUZPEYMLP2ISZ4YR","json":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR.json","graph_json":"https://pith.science/api/pith-number/3KEN6VL3H2FUZPEYMLP2ISZ4YR/graph.json","events_json":"https://pith.science/api/pith-number/3KEN6VL3H2FUZPEYMLP2ISZ4YR/events.json","paper":"https://pith.science/paper/3KEN6VL3"},"agent_actions":{"view_html":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR","download_json":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR.json","view_paper":"https://pith.science/paper/3KEN6VL3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.0018&json=true","fetch_graph":"https://pith.science/api/pith-number/3KEN6VL3H2FUZPEYMLP2ISZ4YR/graph.json","fetch_events":"https://pith.science/api/pith-number/3KEN6VL3H2FUZPEYMLP2ISZ4YR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR/action/storage_attestation","attest_author":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR/action/author_attestation","sign_citation":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR/action/citation_signature","submit_replication":"https://pith.science/pith/3KEN6VL3H2FUZPEYMLP2ISZ4YR/action/replication_record"}},"created_at":"2026-05-18T04:04:33.209429+00:00","updated_at":"2026-05-18T04:04:33.209429+00:00"}