{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:1996:DPGJL3WUO5HCLERIVBZIPCFEZI","short_pith_number":"pith:DPGJL3WU","canonical_record":{"source":{"id":"astro-ph/9607019","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-03T19:50:02Z","cross_cats_sorted":[],"title_canon_sha256":"f64e38e73d96a56f4ddb997ae7f0575046307fa8394742b10d49666f93c080db","abstract_canon_sha256":"769b49a1dcd33a709bec5248efcee7c32d99e640688dc8fec656fb20c52ce8fb"},"schema_version":"1.0"},"canonical_sha256":"1bcc95eed4774e259228a8728788a4ca049eda75489f59b09263a8a58de33494","source":{"kind":"arxiv","id":"astro-ph/9607019","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9607019","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9607019v1","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9607019","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_12","alias_value":"DPGJL3WUO5HC","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_16","alias_value":"DPGJL3WUO5HCLERI","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_8","alias_value":"DPGJL3WU","created_at":"2026-07-04T16:00:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:1996:DPGJL3WUO5HCLERIVBZIPCFEZI","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/9607019","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-03T19:50:02Z","cross_cats_sorted":[],"title_canon_sha256":"f64e38e73d96a56f4ddb997ae7f0575046307fa8394742b10d49666f93c080db","abstract_canon_sha256":"769b49a1dcd33a709bec5248efcee7c32d99e640688dc8fec656fb20c52ce8fb"},"schema_version":"1.0"},"canonical_sha256":"1bcc95eed4774e259228a8728788a4ca049eda75489f59b09263a8a58de33494","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:00:10.640718Z","signature_b64":"viT8MWBU2p9oafH/tfh03Dww6dpd/v5aydj9ryBuEAZRc3tJwcPLggAHJqCfWYwBd4XzOnNfVovJg6gK9keoDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1bcc95eed4774e259228a8728788a4ca049eda75489f59b09263a8a58de33494","last_reissued_at":"2026-07-04T16:00:10.640292Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:00:10.640292Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/9607019","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:00:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"s4wUW0b1Wn0Kj8P2Omr3yYtjkCMU9IElQYDQEDpIzrq9b25b0jVS5skqY+OFiN1tY0gYHp1lbmcgGmqh3GbxBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-08T23:33:36.794649Z"},"content_sha256":"cf6dbb5baf53662be842dd70db86c9f73d78eb0fb0c822138d5ca77db1562012","schema_version":"1.0","event_id":"sha256:cf6dbb5baf53662be842dd70db86c9f73d78eb0fb0c822138d5ca77db1562012"},{"event_type":"graph_snapshot","subject_pith_number":"pith:1996:DPGJL3WUO5HCLERIVBZIPCFEZI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Global Structure and Dynamics of Advection-Dominated Accretion Flows Around Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Fumio Honma, Ramesh Narayan, Shoji Kato","submitted_at":"1996-07-03T19:50:02Z","abstract_excerpt":"We present global solutions that describe advection-dominated accretion flows around black holes. The solutions are obtained by numerically solving a set of coupled ordinary differential equations corresponding to a steady axisymmetric height-integrated flow. The solutions satisfy consistent boundary conditions at both ends. We obtain well-behaved transonic solutions for a wide range of values of the viscosity parameter $\\alpha$, from 0.001 to 0.3. We do not find any need for shocks in our solutions, and disagree with previous claims that viscous accretion flows with low values of $\\alpha$ mus"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9607019","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/astro-ph/9607019/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:00:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bkEOlQr3NeYEHT6Bd+csEdNacDts/dLayEfJzziLW7FB8OtnMA7R4+vXXuHbQb+nGsG4H3wceEqkDHKgc5o0DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-08T23:33:36.795142Z"},"content_sha256":"03d2ce2b1c67b08f05eb669edaffc455f243ea4a26253bc82edafce183084aad","schema_version":"1.0","event_id":"sha256:03d2ce2b1c67b08f05eb669edaffc455f243ea4a26253bc82edafce183084aad"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/bundle.json","state_url":"https://pith.science/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-08T23:33:36Z","links":{"resolver":"https://pith.science/pith/DPGJL3WUO5HCLERIVBZIPCFEZI","bundle":"https://pith.science/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/bundle.json","state":"https://pith.science/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/DPGJL3WUO5HCLERIVBZIPCFEZI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:1996:DPGJL3WUO5HCLERIVBZIPCFEZI","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"769b49a1dcd33a709bec5248efcee7c32d99e640688dc8fec656fb20c52ce8fb","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-03T19:50:02Z","title_canon_sha256":"f64e38e73d96a56f4ddb997ae7f0575046307fa8394742b10d49666f93c080db"},"schema_version":"1.0","source":{"id":"astro-ph/9607019","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9607019","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9607019v1","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9607019","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_12","alias_value":"DPGJL3WUO5HC","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_16","alias_value":"DPGJL3WUO5HCLERI","created_at":"2026-07-04T16:00:10Z"},{"alias_kind":"pith_short_8","alias_value":"DPGJL3WU","created_at":"2026-07-04T16:00:10Z"}],"graph_snapshots":[{"event_id":"sha256:03d2ce2b1c67b08f05eb669edaffc455f243ea4a26253bc82edafce183084aad","target":"graph","created_at":"2026-07-04T16:00:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/9607019/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We present global solutions that describe advection-dominated accretion flows around black holes. The solutions are obtained by numerically solving a set of coupled ordinary differential equations corresponding to a steady axisymmetric height-integrated flow. The solutions satisfy consistent boundary conditions at both ends. We obtain well-behaved transonic solutions for a wide range of values of the viscosity parameter $\\alpha$, from 0.001 to 0.3. We do not find any need for shocks in our solutions, and disagree with previous claims that viscous accretion flows with low values of $\\alpha$ mus","authors_text":"Fumio Honma, Ramesh Narayan, Shoji Kato","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"1996-07-03T19:50:02Z","title":"Global Structure and Dynamics of Advection-Dominated Accretion Flows Around Black Holes"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9607019","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:cf6dbb5baf53662be842dd70db86c9f73d78eb0fb0c822138d5ca77db1562012","target":"record","created_at":"2026-07-04T16:00:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"769b49a1dcd33a709bec5248efcee7c32d99e640688dc8fec656fb20c52ce8fb","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"1996-07-03T19:50:02Z","title_canon_sha256":"f64e38e73d96a56f4ddb997ae7f0575046307fa8394742b10d49666f93c080db"},"schema_version":"1.0","source":{"id":"astro-ph/9607019","kind":"arxiv","version":1}},"canonical_sha256":"1bcc95eed4774e259228a8728788a4ca049eda75489f59b09263a8a58de33494","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"1bcc95eed4774e259228a8728788a4ca049eda75489f59b09263a8a58de33494","first_computed_at":"2026-07-04T16:00:10.640292Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:00:10.640292Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"viT8MWBU2p9oafH/tfh03Dww6dpd/v5aydj9ryBuEAZRc3tJwcPLggAHJqCfWYwBd4XzOnNfVovJg6gK9keoDw==","signature_status":"signed_v1","signed_at":"2026-07-04T16:00:10.640718Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/9607019","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:cf6dbb5baf53662be842dd70db86c9f73d78eb0fb0c822138d5ca77db1562012","sha256:03d2ce2b1c67b08f05eb669edaffc455f243ea4a26253bc82edafce183084aad"],"state_sha256":"4c5a71aa2ba48bd378d49a6e507f9675057db2c6f08e67ec6d2f32f99d352d00"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"asmmFUTbBOOPZyfPR3WL9QNUFUkE9XAtDrifbVhvuPWUNxt5BxPUVjvMaYv3T6F03YVA2HgoSbAMhfbAM8TeDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-08T23:33:36.799569Z","bundle_sha256":"be8e1f4c8c023b873c6bbd3ad99601b96a035cf1e43b2ff3baba4b837ef5cebc"}}