{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:F2DSPIPFXXEBT6DB5Q7RKEFFXQ","short_pith_number":"pith:F2DSPIPF","schema_version":"1.0","canonical_sha256":"2e8727a1e5bdc819f861ec3f1510a5bc293002775e333a3c23e7c30cfc1476dd","source":{"kind":"arxiv","id":"2010.10101","version":1},"attestation_state":"computed","paper":{"title":"A unified accreting magnetar model for long-duration gamma-ray bursts and some stripped-envelope supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"L. J. Wang, W. L. Lin, X. F. Wang, Z. G. Dai","submitted_at":"2020-10-20T07:50:50Z","abstract_excerpt":"Both the long-duration gamma-ray bursts (LGRBs) and the Type I superluminous supernovae (SLSNe~I) have been proposed to be primarily powered by central magnetars. A correlation, proposed between the initial spin period ($P_0$) and the surface magnetic field ($B$) of the magnetars powering the X-ray plateaus in LGRB afterglows, indicates a possibility that the magnetars have reached an equilibrium spin period due to the fallback accretion. The corresponding accretion rates are inferred as $\\dot{M}\\approx10^{-4}-10^{-1}$ M$_\\odot$ s$^{-1}$, and this result holds for the cases of both isotropic a"},"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":"2010.10101","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-10-20T07:50:50Z","cross_cats_sorted":[],"title_canon_sha256":"dd1547bb513987b6dd0a9f0000251c7b2610911ea4124264316a6057a589a5f1","abstract_canon_sha256":"034da766b4ffd722f1e33f92169ecc634b8a1d97a47a87e00229e949da1a79ea"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:50:36.522092Z","signature_b64":"sh2XudsiBUaWRRghZxFR1v0AmtkzKKxM+GluKsXB/wH5kO6z2ZuB5YU4y1qc/lbWeP7JF60rB54WCETbWgG9AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e8727a1e5bdc819f861ec3f1510a5bc293002775e333a3c23e7c30cfc1476dd","last_reissued_at":"2026-07-05T01:50:36.521724Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:50:36.521724Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A unified accreting magnetar model for long-duration gamma-ray bursts and some stripped-envelope supernovae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"L. J. Wang, W. L. Lin, X. F. Wang, Z. G. Dai","submitted_at":"2020-10-20T07:50:50Z","abstract_excerpt":"Both the long-duration gamma-ray bursts (LGRBs) and the Type I superluminous supernovae (SLSNe~I) have been proposed to be primarily powered by central magnetars. A correlation, proposed between the initial spin period ($P_0$) and the surface magnetic field ($B$) of the magnetars powering the X-ray plateaus in LGRB afterglows, indicates a possibility that the magnetars have reached an equilibrium spin period due to the fallback accretion. The corresponding accretion rates are inferred as $\\dot{M}\\approx10^{-4}-10^{-1}$ M$_\\odot$ s$^{-1}$, and this result holds for the cases of both isotropic a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.10101","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/2010.10101/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":"2010.10101","created_at":"2026-07-05T01:50:36.521794+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.10101v1","created_at":"2026-07-05T01:50:36.521794+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.10101","created_at":"2026-07-05T01:50:36.521794+00:00"},{"alias_kind":"pith_short_12","alias_value":"F2DSPIPFXXEB","created_at":"2026-07-05T01:50:36.521794+00:00"},{"alias_kind":"pith_short_16","alias_value":"F2DSPIPFXXEBT6DB","created_at":"2026-07-05T01:50:36.521794+00:00"},{"alias_kind":"pith_short_8","alias_value":"F2DSPIPF","created_at":"2026-07-05T01:50:36.521794+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/F2DSPIPFXXEBT6DB5Q7RKEFFXQ","json":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ.json","graph_json":"https://pith.science/api/pith-number/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/graph.json","events_json":"https://pith.science/api/pith-number/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/events.json","paper":"https://pith.science/paper/F2DSPIPF"},"agent_actions":{"view_html":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ","download_json":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ.json","view_paper":"https://pith.science/paper/F2DSPIPF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.10101&json=true","fetch_graph":"https://pith.science/api/pith-number/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/graph.json","fetch_events":"https://pith.science/api/pith-number/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/action/storage_attestation","attest_author":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/action/author_attestation","sign_citation":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/action/citation_signature","submit_replication":"https://pith.science/pith/F2DSPIPFXXEBT6DB5Q7RKEFFXQ/action/replication_record"}},"created_at":"2026-07-05T01:50:36.521794+00:00","updated_at":"2026-07-05T01:50:36.521794+00:00"}