{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:O3AE2UY4LRXJKHE4Z6JCXRPPU5","short_pith_number":"pith:O3AE2UY4","schema_version":"1.0","canonical_sha256":"76c04d531c5c6e951c9ccf922bc5efa746b8a0e2a109aca9d497df1e8ecf803a","source":{"kind":"arxiv","id":"1102.0179","version":2},"attestation_state":"computed","paper":{"title":"Kinetic description of quasi-stationary axisymmetric collisionless accretion disk plasmas with arbitrary magnetic field configurations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Claudio Cremaschini, John C. Miller, Massimo Tessarotto","submitted_at":"2011-02-01T15:24:51Z","abstract_excerpt":"A kinetic treatment is developed for collisionless magnetized plasmas occurring in high-temperature, low-density astrophysical accretion disks, such as are thought to be present in some radiatively-inefficient accretion flows onto black holes. Quasi-stationary configurations are investigated, within the framework of a Vlasov-Maxwell description. The plasma is taken to be axisymmetric and subject to the action of slowly time-varying gravitational and electromagnetic fields. The magnetic field is assumed to be characterized by a family of locally nested but open magnetic surfaces. The slow colli"},"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":"1102.0179","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-02-01T15:24:51Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"ef5a8bdbec256e48eee43ac79dcf15d3bf4bc271ff6e5293722c11026674cca8","abstract_canon_sha256":"00a7c8532ce1996d886b5497a1938c8760f45d4e594e026f053c5e30bf48e2ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:18.086441Z","signature_b64":"o8ffXmzy3UQU7pKT8yaiWUwGA4gDrsxU0DR2F28vuQ7er064kv5HSxdKZmkW4y+jVYrQH69c2myZpLAtKTMbDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"76c04d531c5c6e951c9ccf922bc5efa746b8a0e2a109aca9d497df1e8ecf803a","last_reissued_at":"2026-05-18T02:03:18.085846Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:18.085846Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinetic description of quasi-stationary axisymmetric collisionless accretion disk plasmas with arbitrary magnetic field configurations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Claudio Cremaschini, John C. Miller, Massimo Tessarotto","submitted_at":"2011-02-01T15:24:51Z","abstract_excerpt":"A kinetic treatment is developed for collisionless magnetized plasmas occurring in high-temperature, low-density astrophysical accretion disks, such as are thought to be present in some radiatively-inefficient accretion flows onto black holes. Quasi-stationary configurations are investigated, within the framework of a Vlasov-Maxwell description. The plasma is taken to be axisymmetric and subject to the action of slowly time-varying gravitational and electromagnetic fields. The magnetic field is assumed to be characterized by a family of locally nested but open magnetic surfaces. The slow colli"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.0179","kind":"arxiv","version":2},"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":"1102.0179","created_at":"2026-05-18T02:03:18.085944+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.0179v2","created_at":"2026-05-18T02:03:18.085944+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.0179","created_at":"2026-05-18T02:03:18.085944+00:00"},{"alias_kind":"pith_short_12","alias_value":"O3AE2UY4LRXJ","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_16","alias_value":"O3AE2UY4LRXJKHE4","created_at":"2026-05-18T12:26:37.096874+00:00"},{"alias_kind":"pith_short_8","alias_value":"O3AE2UY4","created_at":"2026-05-18T12:26:37.096874+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/O3AE2UY4LRXJKHE4Z6JCXRPPU5","json":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5.json","graph_json":"https://pith.science/api/pith-number/O3AE2UY4LRXJKHE4Z6JCXRPPU5/graph.json","events_json":"https://pith.science/api/pith-number/O3AE2UY4LRXJKHE4Z6JCXRPPU5/events.json","paper":"https://pith.science/paper/O3AE2UY4"},"agent_actions":{"view_html":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5","download_json":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5.json","view_paper":"https://pith.science/paper/O3AE2UY4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.0179&json=true","fetch_graph":"https://pith.science/api/pith-number/O3AE2UY4LRXJKHE4Z6JCXRPPU5/graph.json","fetch_events":"https://pith.science/api/pith-number/O3AE2UY4LRXJKHE4Z6JCXRPPU5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5/action/storage_attestation","attest_author":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5/action/author_attestation","sign_citation":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5/action/citation_signature","submit_replication":"https://pith.science/pith/O3AE2UY4LRXJKHE4Z6JCXRPPU5/action/replication_record"}},"created_at":"2026-05-18T02:03:18.085944+00:00","updated_at":"2026-05-18T02:03:18.085944+00:00"}