{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:ABN7VDWM2UTFX5WVTU4FYZ5E4E","short_pith_number":"pith:ABN7VDWM","schema_version":"1.0","canonical_sha256":"005bfa8eccd5265bf6d59d385c67a4e13a871ada968c1ed32dbebb1457ee9050","source":{"kind":"arxiv","id":"1410.8745","version":1},"attestation_state":"computed","paper":{"title":"Super-Eddington accretion in ultra-luminous neutron star binary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maxim Lyutikov (Purdue)","submitted_at":"2014-10-31T14:21:25Z","abstract_excerpt":"We discuss properties of the ultra-luminous $X$-ray source in the galaxy M82, NuSTAR J095551+6940.8, containing an accreting neutron star. The neutron star has surface magnetic field $ B_{NS} \\approx 1.4 \\times 10^{13 } \\, {\\rm G}$ and experiences accretion rate of $9 \\times 10^{-7} M_\\odot {\\rm \\, yr}^{-1} $. The magnetospheric radius, close to the corotation radius, is $\\sim 2 \\times 10^8$ cm. The accretion torque on the neutron star is reduce well below what is expected in a simple magnetospheric accretion due to effective penetration of the stellar magnetic field into the disk beyond the c"},"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":"1410.8745","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-10-31T14:21:25Z","cross_cats_sorted":[],"title_canon_sha256":"9c61d514e0726b4520eca43a4f5eb2ce355a8b81347ea46391e86f321886c1b3","abstract_canon_sha256":"10b9e189de2558f30f786e1f791d054861cdccf967ee487eace01d6f2871074f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:38:53.793253Z","signature_b64":"gsPLYKtcYQ2akUVsXjSi/UWrDofeNfu+TxywYDOiaJcVNz0sg7hOX1RFEeKBB7agU3BS0QXn3THIebqTplOGBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"005bfa8eccd5265bf6d59d385c67a4e13a871ada968c1ed32dbebb1457ee9050","last_reissued_at":"2026-05-18T02:38:53.792859Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:38:53.792859Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Super-Eddington accretion in ultra-luminous neutron star binary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maxim Lyutikov (Purdue)","submitted_at":"2014-10-31T14:21:25Z","abstract_excerpt":"We discuss properties of the ultra-luminous $X$-ray source in the galaxy M82, NuSTAR J095551+6940.8, containing an accreting neutron star. The neutron star has surface magnetic field $ B_{NS} \\approx 1.4 \\times 10^{13 } \\, {\\rm G}$ and experiences accretion rate of $9 \\times 10^{-7} M_\\odot {\\rm \\, yr}^{-1} $. The magnetospheric radius, close to the corotation radius, is $\\sim 2 \\times 10^8$ cm. The accretion torque on the neutron star is reduce well below what is expected in a simple magnetospheric accretion due to effective penetration of the stellar magnetic field into the disk beyond the c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.8745","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":"1410.8745","created_at":"2026-05-18T02:38:53.792934+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.8745v1","created_at":"2026-05-18T02:38:53.792934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.8745","created_at":"2026-05-18T02:38:53.792934+00:00"},{"alias_kind":"pith_short_12","alias_value":"ABN7VDWM2UTF","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_16","alias_value":"ABN7VDWM2UTFX5WV","created_at":"2026-05-18T12:28:19.803747+00:00"},{"alias_kind":"pith_short_8","alias_value":"ABN7VDWM","created_at":"2026-05-18T12:28:19.803747+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/ABN7VDWM2UTFX5WVTU4FYZ5E4E","json":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E.json","graph_json":"https://pith.science/api/pith-number/ABN7VDWM2UTFX5WVTU4FYZ5E4E/graph.json","events_json":"https://pith.science/api/pith-number/ABN7VDWM2UTFX5WVTU4FYZ5E4E/events.json","paper":"https://pith.science/paper/ABN7VDWM"},"agent_actions":{"view_html":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E","download_json":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E.json","view_paper":"https://pith.science/paper/ABN7VDWM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.8745&json=true","fetch_graph":"https://pith.science/api/pith-number/ABN7VDWM2UTFX5WVTU4FYZ5E4E/graph.json","fetch_events":"https://pith.science/api/pith-number/ABN7VDWM2UTFX5WVTU4FYZ5E4E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E/action/storage_attestation","attest_author":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E/action/author_attestation","sign_citation":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E/action/citation_signature","submit_replication":"https://pith.science/pith/ABN7VDWM2UTFX5WVTU4FYZ5E4E/action/replication_record"}},"created_at":"2026-05-18T02:38:53.792934+00:00","updated_at":"2026-05-18T02:38:53.792934+00:00"}