{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:DK5K6N3L73MK52GHOBGPHSL5EP","short_pith_number":"pith:DK5K6N3L","schema_version":"1.0","canonical_sha256":"1abaaf376bfed8aee8c7704cf3c97d23c2f83849a2cb33b7f36076fbdebca41a","source":{"kind":"arxiv","id":"2402.16529","version":1},"attestation_state":"computed","paper":{"title":"Black hole in a combined magnetic field: ionized accretion disks in the jetlike and looplike configurations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Arman Tursunov, Martin Kolo\\v{s}, Saken Toktarbay, Saltanat Kenzhebayeva","submitted_at":"2024-02-26T12:25:56Z","abstract_excerpt":"Magnetic fields surrounding black holes are responsible for various astrophysical phenomena related to accretion processes and relativistic jets. Depending on the source, the configuration of the field lines may differ significantly, affecting the trajectories of charged particles and the corresponding observables. Usually, the magnetic fields around black holes are modeled within a single source or current generating the field. However, magnetic fields can have more than a single origin, being a combination of different fields, such as, e.g., that of an accretion disk and external large-scale"},"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":"2402.16529","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-02-26T12:25:56Z","cross_cats_sorted":["astro-ph.GA","gr-qc"],"title_canon_sha256":"bbcafc91effe580643123403ff1118b6fc7e56278842504c8ee37680fc731914","abstract_canon_sha256":"1afba2840beae6244a456b996f36066f09bc4e17312c5b949221ebb80d128602"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:56:03.295411Z","signature_b64":"irovxrGdHFlj5d8JfgHC7Q2mDtQMtWMCTXJFbB4TeVn8qxxYwBMkvqCkFLlBEAQURx9HkG+JXcptSDvrP3T9CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1abaaf376bfed8aee8c7704cf3c97d23c2f83849a2cb33b7f36076fbdebca41a","last_reissued_at":"2026-07-05T07:56:03.294941Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:56:03.294941Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole in a combined magnetic field: ionized accretion disks in the jetlike and looplike configurations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Arman Tursunov, Martin Kolo\\v{s}, Saken Toktarbay, Saltanat Kenzhebayeva","submitted_at":"2024-02-26T12:25:56Z","abstract_excerpt":"Magnetic fields surrounding black holes are responsible for various astrophysical phenomena related to accretion processes and relativistic jets. Depending on the source, the configuration of the field lines may differ significantly, affecting the trajectories of charged particles and the corresponding observables. Usually, the magnetic fields around black holes are modeled within a single source or current generating the field. However, magnetic fields can have more than a single origin, being a combination of different fields, such as, e.g., that of an accretion disk and external large-scale"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.16529","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/2402.16529/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":"2402.16529","created_at":"2026-07-05T07:56:03.295002+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.16529v1","created_at":"2026-07-05T07:56:03.295002+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.16529","created_at":"2026-07-05T07:56:03.295002+00:00"},{"alias_kind":"pith_short_12","alias_value":"DK5K6N3L73MK","created_at":"2026-07-05T07:56:03.295002+00:00"},{"alias_kind":"pith_short_16","alias_value":"DK5K6N3L73MK52GH","created_at":"2026-07-05T07:56:03.295002+00:00"},{"alias_kind":"pith_short_8","alias_value":"DK5K6N3L","created_at":"2026-07-05T07:56:03.295002+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/DK5K6N3L73MK52GHOBGPHSL5EP","json":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP.json","graph_json":"https://pith.science/api/pith-number/DK5K6N3L73MK52GHOBGPHSL5EP/graph.json","events_json":"https://pith.science/api/pith-number/DK5K6N3L73MK52GHOBGPHSL5EP/events.json","paper":"https://pith.science/paper/DK5K6N3L"},"agent_actions":{"view_html":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP","download_json":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP.json","view_paper":"https://pith.science/paper/DK5K6N3L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.16529&json=true","fetch_graph":"https://pith.science/api/pith-number/DK5K6N3L73MK52GHOBGPHSL5EP/graph.json","fetch_events":"https://pith.science/api/pith-number/DK5K6N3L73MK52GHOBGPHSL5EP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP/action/storage_attestation","attest_author":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP/action/author_attestation","sign_citation":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP/action/citation_signature","submit_replication":"https://pith.science/pith/DK5K6N3L73MK52GHOBGPHSL5EP/action/replication_record"}},"created_at":"2026-07-05T07:56:03.295002+00:00","updated_at":"2026-07-05T07:56:03.295002+00:00"}