{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:VB3RNSCFFWOB2VV6UT3KLTZBOW","short_pith_number":"pith:VB3RNSCF","schema_version":"1.0","canonical_sha256":"a87716c8452d9c1d56bea4f6a5cf217598eba54b946ddec6ee87644a8fa99545","source":{"kind":"arxiv","id":"2608.10733","version":1},"attestation_state":"computed","paper":{"title":"Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aleksei V. Kuzin, Alexander A. Mushtukov, Alexander Salganik, Andrey S. Tavleev, Galina Lipunova, Juri Poutanen, Sergey S. Tsygankov, Sofia V. Forsblom, Valery F. Suleimanov","submitted_at":"2026-08-11T09:53:11Z","abstract_excerpt":"The final stages of outbursts in transient X-ray pulsars (XRPs), which are characterised by a significant decline in the mass accretion rate, provide valuable insight into the physics of the accretion disc and its interaction with the strong magnetic field of the neutron star (NS). In particular, the `propeller effect', or centrifugal inhibition of accretion, has been proposed as a key mechanism governing both the onset luminosity and the timescale of the rapid transition to the quiescent state. In addition, it offers an independent method for estimating the magnetic field strength of the NS. "},"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":"2608.10733","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-08-11T09:53:11Z","cross_cats_sorted":[],"title_canon_sha256":"8b95661cff0c28e29d06ffae9b3f7171155b5bc19a421e80867067a96463a072","abstract_canon_sha256":"96393b6d235f7953622af70ebebf85c82420fea54018b1a0e71ab6667c6e8035"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-12T01:23:09.396096Z","signature_b64":"i9u7xLRNmTE+QPP1QV17Swm5xsgs4/zKLpbP/2jD/xlmKszehjnn8Yzelt7eJLAcdsTeiikcu5TuZrCc4iHiDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a87716c8452d9c1d56bea4f6a5cf217598eba54b946ddec6ee87644a8fa99545","last_reissued_at":"2026-08-12T01:23:09.394518Z","signature_status":"signed_v1","first_computed_at":"2026-08-12T01:23:09.394518Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aleksei V. Kuzin, Alexander A. Mushtukov, Alexander Salganik, Andrey S. Tavleev, Galina Lipunova, Juri Poutanen, Sergey S. Tsygankov, Sofia V. Forsblom, Valery F. Suleimanov","submitted_at":"2026-08-11T09:53:11Z","abstract_excerpt":"The final stages of outbursts in transient X-ray pulsars (XRPs), which are characterised by a significant decline in the mass accretion rate, provide valuable insight into the physics of the accretion disc and its interaction with the strong magnetic field of the neutron star (NS). In particular, the `propeller effect', or centrifugal inhibition of accretion, has been proposed as a key mechanism governing both the onset luminosity and the timescale of the rapid transition to the quiescent state. In addition, it offers an independent method for estimating the magnetic field strength of the NS. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2608.10733","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/2608.10733/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":"2608.10733","created_at":"2026-08-12T01:23:09.398332+00:00"},{"alias_kind":"arxiv_version","alias_value":"2608.10733v1","created_at":"2026-08-12T01:23:09.398332+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2608.10733","created_at":"2026-08-12T01:23:09.398332+00:00"},{"alias_kind":"pith_short_12","alias_value":"VB3RNSCFFWOB","created_at":"2026-08-12T01:23:09.398332+00:00"},{"alias_kind":"pith_short_16","alias_value":"VB3RNSCFFWOB2VV6","created_at":"2026-08-12T01:23:09.398332+00:00"},{"alias_kind":"pith_short_8","alias_value":"VB3RNSCF","created_at":"2026-08-12T01:23:09.398332+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/VB3RNSCFFWOB2VV6UT3KLTZBOW","json":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW.json","graph_json":"https://pith.science/api/pith-number/VB3RNSCFFWOB2VV6UT3KLTZBOW/graph.json","events_json":"https://pith.science/api/pith-number/VB3RNSCFFWOB2VV6UT3KLTZBOW/events.json","paper":"https://pith.science/paper/VB3RNSCF"},"agent_actions":{"view_html":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW","download_json":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW.json","view_paper":"https://pith.science/paper/VB3RNSCF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2608.10733&json=true","fetch_graph":"https://pith.science/api/pith-number/VB3RNSCFFWOB2VV6UT3KLTZBOW/graph.json","fetch_events":"https://pith.science/api/pith-number/VB3RNSCFFWOB2VV6UT3KLTZBOW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW/action/storage_attestation","attest_author":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW/action/author_attestation","sign_citation":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW/action/citation_signature","submit_replication":"https://pith.science/pith/VB3RNSCFFWOB2VV6UT3KLTZBOW/action/replication_record"}},"created_at":"2026-08-12T01:23:09.398332+00:00","updated_at":"2026-08-12T01:23:09.398332+00:00"}