{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:HZOCZQHG7Q7OOLZZB2PCIKVP2U","short_pith_number":"pith:HZOCZQHG","schema_version":"1.0","canonical_sha256":"3e5c2cc0e6fc3ee72f390e9e242aafd50ad11c8b2cd9e3d865443743dce20220","source":{"kind":"arxiv","id":"2302.14403","version":1},"attestation_state":"computed","paper":{"title":"On the Zeeman Effect in Magnetically-Arrested Disks","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Yoshiyuki Inoue","submitted_at":"2023-02-28T08:37:27Z","abstract_excerpt":"Magnetically arrested disk (MAD) has been argued as the key accretion phase to realize the formation of relativistic jets. However, due to the lack of magnetic field measurements of accreting systems, MAD has not been observationally confirmed yet. Here we propose that a strong magnetic field accompanied by MAD would induce the Zeeman splitting of relativistically broadened Fe K$\\alpha$ fluorescence lines in X-ray binaries and active galactic nuclei, where we consider a two-phase medium in the inner accretion disk, magnetically dominated hot corona and cold reflector. Such a geometrical config"},"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":"2302.14403","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-02-28T08:37:27Z","cross_cats_sorted":[],"title_canon_sha256":"6fca947bae508f83d6edfa3cbb866931a4a05b483d4240af5c40cba37e6fc11a","abstract_canon_sha256":"71011a3880aee99c2a3145fbebf48bac04ed902b752dd430163abc9481c9e622"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:58:09.254561Z","signature_b64":"KlRP6Y56xxH5wAdpf9LxXKU5aIhf1YhFXBzGpmyXaoh5HpSNiExXK+spK3pw2dUu2wWxhxJ9Am/Frt1j/nNDCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3e5c2cc0e6fc3ee72f390e9e242aafd50ad11c8b2cd9e3d865443743dce20220","last_reissued_at":"2026-07-05T05:58:09.253888Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:58:09.253888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Zeeman Effect in Magnetically-Arrested Disks","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Yoshiyuki Inoue","submitted_at":"2023-02-28T08:37:27Z","abstract_excerpt":"Magnetically arrested disk (MAD) has been argued as the key accretion phase to realize the formation of relativistic jets. However, due to the lack of magnetic field measurements of accreting systems, MAD has not been observationally confirmed yet. Here we propose that a strong magnetic field accompanied by MAD would induce the Zeeman splitting of relativistically broadened Fe K$\\alpha$ fluorescence lines in X-ray binaries and active galactic nuclei, where we consider a two-phase medium in the inner accretion disk, magnetically dominated hot corona and cold reflector. Such a geometrical config"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.14403","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/2302.14403/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":"2302.14403","created_at":"2026-07-05T05:58:09.254194+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.14403v1","created_at":"2026-07-05T05:58:09.254194+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.14403","created_at":"2026-07-05T05:58:09.254194+00:00"},{"alias_kind":"pith_short_12","alias_value":"HZOCZQHG7Q7O","created_at":"2026-07-05T05:58:09.254194+00:00"},{"alias_kind":"pith_short_16","alias_value":"HZOCZQHG7Q7OOLZZ","created_at":"2026-07-05T05:58:09.254194+00:00"},{"alias_kind":"pith_short_8","alias_value":"HZOCZQHG","created_at":"2026-07-05T05:58:09.254194+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/HZOCZQHG7Q7OOLZZB2PCIKVP2U","json":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U.json","graph_json":"https://pith.science/api/pith-number/HZOCZQHG7Q7OOLZZB2PCIKVP2U/graph.json","events_json":"https://pith.science/api/pith-number/HZOCZQHG7Q7OOLZZB2PCIKVP2U/events.json","paper":"https://pith.science/paper/HZOCZQHG"},"agent_actions":{"view_html":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U","download_json":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U.json","view_paper":"https://pith.science/paper/HZOCZQHG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.14403&json=true","fetch_graph":"https://pith.science/api/pith-number/HZOCZQHG7Q7OOLZZB2PCIKVP2U/graph.json","fetch_events":"https://pith.science/api/pith-number/HZOCZQHG7Q7OOLZZB2PCIKVP2U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U/action/storage_attestation","attest_author":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U/action/author_attestation","sign_citation":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U/action/citation_signature","submit_replication":"https://pith.science/pith/HZOCZQHG7Q7OOLZZB2PCIKVP2U/action/replication_record"}},"created_at":"2026-07-05T05:58:09.254194+00:00","updated_at":"2026-07-05T05:58:09.254194+00:00"}