{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:BEUXFX26T6SWKDYAGNUK22VXQG","short_pith_number":"pith:BEUXFX26","schema_version":"1.0","canonical_sha256":"092972df5e9fa5650f003368ad6ab781bb1e848bed3bac3d10301d92bfc416b1","source":{"kind":"arxiv","id":"1706.01489","version":1},"attestation_state":"computed","paper":{"title":"The Dynamics of Truncated Black Hole Accretion Disks I: Viscous, Hydrodynamic Case","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Christopher S. Reynolds, J. Drew Hogg","submitted_at":"2017-06-05T18:37:30Z","abstract_excerpt":"Truncated accretion disks are commonly invoked to explain the spectro-temporal variability from accreting black holes in both small systems, i.e. state transitions in galactic black hole binaries (GBHBs), and large systems, i.e. low-luminosity active galactic nuclei (LLAGNs). In the canonical truncated disk model of moderately low accretion rate systems, gas in the inner region of the accretion disk occupies a hot, radiatively inefficient phase, which leads to a geometrically thick disk, while the gas in the outer region occupies a cooler, radiatively efficient phase that resides in the standa"},"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":"1706.01489","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-05T18:37:30Z","cross_cats_sorted":[],"title_canon_sha256":"a7bf2bf92116f89f291892f468efe9ca9a23c343ed08b608821534d5d20e0019","abstract_canon_sha256":"5908189f3e9317e6b9d5d77971e25bb6230d098f64b94b5db7486561af8f8ebc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:40:03.184038Z","signature_b64":"XC31NA3xbtJmbkGAox/cP29xNOHTCqHgV3FbJqDR0o47HCc2Jyj+byWajFRIIcyTY53+PfULFBKDtfM+ZWJVAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"092972df5e9fa5650f003368ad6ab781bb1e848bed3bac3d10301d92bfc416b1","last_reissued_at":"2026-05-18T00:40:03.183640Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:40:03.183640Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Dynamics of Truncated Black Hole Accretion Disks I: Viscous, Hydrodynamic Case","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Christopher S. Reynolds, J. Drew Hogg","submitted_at":"2017-06-05T18:37:30Z","abstract_excerpt":"Truncated accretion disks are commonly invoked to explain the spectro-temporal variability from accreting black holes in both small systems, i.e. state transitions in galactic black hole binaries (GBHBs), and large systems, i.e. low-luminosity active galactic nuclei (LLAGNs). In the canonical truncated disk model of moderately low accretion rate systems, gas in the inner region of the accretion disk occupies a hot, radiatively inefficient phase, which leads to a geometrically thick disk, while the gas in the outer region occupies a cooler, radiatively efficient phase that resides in the standa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.01489","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":"1706.01489","created_at":"2026-05-18T00:40:03.183696+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.01489v1","created_at":"2026-05-18T00:40:03.183696+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.01489","created_at":"2026-05-18T00:40:03.183696+00:00"},{"alias_kind":"pith_short_12","alias_value":"BEUXFX26T6SW","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_16","alias_value":"BEUXFX26T6SWKDYA","created_at":"2026-05-18T12:31:08.081275+00:00"},{"alias_kind":"pith_short_8","alias_value":"BEUXFX26","created_at":"2026-05-18T12:31:08.081275+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/BEUXFX26T6SWKDYAGNUK22VXQG","json":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG.json","graph_json":"https://pith.science/api/pith-number/BEUXFX26T6SWKDYAGNUK22VXQG/graph.json","events_json":"https://pith.science/api/pith-number/BEUXFX26T6SWKDYAGNUK22VXQG/events.json","paper":"https://pith.science/paper/BEUXFX26"},"agent_actions":{"view_html":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG","download_json":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG.json","view_paper":"https://pith.science/paper/BEUXFX26","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.01489&json=true","fetch_graph":"https://pith.science/api/pith-number/BEUXFX26T6SWKDYAGNUK22VXQG/graph.json","fetch_events":"https://pith.science/api/pith-number/BEUXFX26T6SWKDYAGNUK22VXQG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG/action/storage_attestation","attest_author":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG/action/author_attestation","sign_citation":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG/action/citation_signature","submit_replication":"https://pith.science/pith/BEUXFX26T6SWKDYAGNUK22VXQG/action/replication_record"}},"created_at":"2026-05-18T00:40:03.183696+00:00","updated_at":"2026-05-18T00:40:03.183696+00:00"}