{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LA3ABHUE2HC4SQ6MMPCWSE24LH","short_pith_number":"pith:LA3ABHUE","schema_version":"1.0","canonical_sha256":"5836009e84d1c5c943cc63c569135c59cbab5bb0bcae712939419b3ebd297037","source":{"kind":"arxiv","id":"1606.00016","version":1},"attestation_state":"computed","paper":{"title":"Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"A. F. Fantina, C. Ducoin, J. M. Pearson, N. Chamel, N. G\\\"urlebeck, T. Delsate","submitted_at":"2016-05-31T20:00:22Z","abstract_excerpt":"Giant pulsar frequency glitches as detected in the emblematic Vela pulsar have long been thought to be the manifestation of a neutron superfluid permeating the inner crust of a neutron star. However, this superfluid has been recently found to be entrained by the crust, and as a consequence it does not carry enough angular momentum to explain giant glitches. The extent to which pulsar-timing observations can be reconciled with the standard vortex-mediated glitch theory is studied considering the current uncertainties on dense-matter properties. To this end, the crustal moment of inertia of glit"},"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":"1606.00016","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-05-31T20:00:22Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"39dfa5d7edf707845c442f88e470fcc698b3c1d01c941374a0a4ec70c57412ae","abstract_canon_sha256":"4d27481bd5eff44cc1d3597338bf263fa36413f03d58a5441dd22c1c2c2520e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:24.173866Z","signature_b64":"ZWg3xpdb78HQeiXJ8tAp3cpkqeA2UKHWk2eWelfsoP92nr1sOzNHUvCSAasNlCFzkZPl1ytDY78H1J0YSe0SAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5836009e84d1c5c943cc63c569135c59cbab5bb0bcae712939419b3ebd297037","last_reissued_at":"2026-05-18T01:10:24.173383Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:24.173383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Giant Pulsar Glitches and the Inertia of Neutron-Star Crusts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"A. F. Fantina, C. Ducoin, J. M. Pearson, N. Chamel, N. G\\\"urlebeck, T. Delsate","submitted_at":"2016-05-31T20:00:22Z","abstract_excerpt":"Giant pulsar frequency glitches as detected in the emblematic Vela pulsar have long been thought to be the manifestation of a neutron superfluid permeating the inner crust of a neutron star. However, this superfluid has been recently found to be entrained by the crust, and as a consequence it does not carry enough angular momentum to explain giant glitches. The extent to which pulsar-timing observations can be reconciled with the standard vortex-mediated glitch theory is studied considering the current uncertainties on dense-matter properties. To this end, the crustal moment of inertia of glit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.00016","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":"1606.00016","created_at":"2026-05-18T01:10:24.173464+00:00"},{"alias_kind":"arxiv_version","alias_value":"1606.00016v1","created_at":"2026-05-18T01:10:24.173464+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.00016","created_at":"2026-05-18T01:10:24.173464+00:00"},{"alias_kind":"pith_short_12","alias_value":"LA3ABHUE2HC4","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LA3ABHUE2HC4SQ6M","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LA3ABHUE","created_at":"2026-05-18T12:30:29.479603+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.16929","citing_title":"Properties of the neutron star crust informed by nuclear structure data","ref_index":78,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH","json":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH.json","graph_json":"https://pith.science/api/pith-number/LA3ABHUE2HC4SQ6MMPCWSE24LH/graph.json","events_json":"https://pith.science/api/pith-number/LA3ABHUE2HC4SQ6MMPCWSE24LH/events.json","paper":"https://pith.science/paper/LA3ABHUE"},"agent_actions":{"view_html":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH","download_json":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH.json","view_paper":"https://pith.science/paper/LA3ABHUE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1606.00016&json=true","fetch_graph":"https://pith.science/api/pith-number/LA3ABHUE2HC4SQ6MMPCWSE24LH/graph.json","fetch_events":"https://pith.science/api/pith-number/LA3ABHUE2HC4SQ6MMPCWSE24LH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH/action/storage_attestation","attest_author":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH/action/author_attestation","sign_citation":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH/action/citation_signature","submit_replication":"https://pith.science/pith/LA3ABHUE2HC4SQ6MMPCWSE24LH/action/replication_record"}},"created_at":"2026-05-18T01:10:24.173464+00:00","updated_at":"2026-05-18T01:10:24.173464+00:00"}