{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:AF52X3SNHWD7THAIM5KGC3JXFV","short_pith_number":"pith:AF52X3SN","schema_version":"1.0","canonical_sha256":"017babee4d3d87f99c086754616d372d660e90fb6c4647f01379e4ab5550c559","source":{"kind":"arxiv","id":"2607.07784","version":1},"attestation_state":"computed","paper":{"title":"The SANE, the MAD, and the Chimera","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"George N. Wong, James M. Stone","submitted_at":"2026-07-08T18:00:00Z","abstract_excerpt":"Non-radiative black hole accretion flows are commonly classified by their magnetic flux state, with standard and normal evolution (SANE) disks and magnetically arrested disks (MADs) marking the usual weak- and strong-flux regimes. We compare three-dimensional general relativistic magnetohydrodynamics simulations of a weakly magnetized SANE flow, a standard MAD, and a Chimera flow fed by a different reservoir of mass, angular momentum, and coherent magnetic flux. The Chimera reaches a MAD-level horizon magnetic flux and launches a powerful electromagnetic jet during an extended non-eruptive int"},"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":"2607.07784","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-07-08T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"8347728afba9c3ed6a6e57355500f2eafddd8be098de2bc780cb737f92c335f7","abstract_canon_sha256":"27b269f57fa122a098da208e2cc7c5fd7cbfd6d4cb77accde47c73f4e46e5fb1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-10T00:18:59.152623Z","signature_b64":"hQYGLArrtVP355thnG55LqdUQhYvq3fRrA+ojcOWZRFUWj8R4fm0kade+JqD9WK91IgNI4J+MV8AVaRgi2tgBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"017babee4d3d87f99c086754616d372d660e90fb6c4647f01379e4ab5550c559","last_reissued_at":"2026-07-10T00:18:59.152214Z","signature_status":"signed_v1","first_computed_at":"2026-07-10T00:18:59.152214Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The SANE, the MAD, and the Chimera","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"George N. Wong, James M. Stone","submitted_at":"2026-07-08T18:00:00Z","abstract_excerpt":"Non-radiative black hole accretion flows are commonly classified by their magnetic flux state, with standard and normal evolution (SANE) disks and magnetically arrested disks (MADs) marking the usual weak- and strong-flux regimes. We compare three-dimensional general relativistic magnetohydrodynamics simulations of a weakly magnetized SANE flow, a standard MAD, and a Chimera flow fed by a different reservoir of mass, angular momentum, and coherent magnetic flux. The Chimera reaches a MAD-level horizon magnetic flux and launches a powerful electromagnetic jet during an extended non-eruptive int"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2607.07784","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/2607.07784/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":"2607.07784","created_at":"2026-07-10T00:18:59.152271+00:00"},{"alias_kind":"arxiv_version","alias_value":"2607.07784v1","created_at":"2026-07-10T00:18:59.152271+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2607.07784","created_at":"2026-07-10T00:18:59.152271+00:00"},{"alias_kind":"pith_short_12","alias_value":"AF52X3SNHWD7","created_at":"2026-07-10T00:18:59.152271+00:00"},{"alias_kind":"pith_short_16","alias_value":"AF52X3SNHWD7THAI","created_at":"2026-07-10T00:18:59.152271+00:00"},{"alias_kind":"pith_short_8","alias_value":"AF52X3SN","created_at":"2026-07-10T00:18:59.152271+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/AF52X3SNHWD7THAIM5KGC3JXFV","json":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV.json","graph_json":"https://pith.science/api/pith-number/AF52X3SNHWD7THAIM5KGC3JXFV/graph.json","events_json":"https://pith.science/api/pith-number/AF52X3SNHWD7THAIM5KGC3JXFV/events.json","paper":"https://pith.science/paper/AF52X3SN"},"agent_actions":{"view_html":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV","download_json":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV.json","view_paper":"https://pith.science/paper/AF52X3SN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2607.07784&json=true","fetch_graph":"https://pith.science/api/pith-number/AF52X3SNHWD7THAIM5KGC3JXFV/graph.json","fetch_events":"https://pith.science/api/pith-number/AF52X3SNHWD7THAIM5KGC3JXFV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV/action/storage_attestation","attest_author":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV/action/author_attestation","sign_citation":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV/action/citation_signature","submit_replication":"https://pith.science/pith/AF52X3SNHWD7THAIM5KGC3JXFV/action/replication_record"}},"created_at":"2026-07-10T00:18:59.152271+00:00","updated_at":"2026-07-10T00:18:59.152271+00:00"}