{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:YTZRRUJZAXGZNLT4ZXDDY277IZ","short_pith_number":"pith:YTZRRUJZ","canonical_record":{"source":{"id":"1311.5565","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-21T21:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"a06e7b5c8fafb6845f62cbc1b7c12d566ab136d9f5626576f7dffb7a69a28a37","abstract_canon_sha256":"2f31bef4548316ab0ab6aebf573243f044b2f655388b63ed939316118dbe5c64"},"schema_version":"1.0"},"canonical_sha256":"c4f318d13905cd96ae7ccdc63c6bff4674afdae93c9a021943032c32b77980ae","source":{"kind":"arxiv","id":"1311.5565","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1311.5565","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"arxiv_version","alias_value":"1311.5565v1","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.5565","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"pith_short_12","alias_value":"YTZRRUJZAXGZ","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_16","alias_value":"YTZRRUJZAXGZNLT4","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_8","alias_value":"YTZRRUJZ","created_at":"2026-05-18T12:28:09Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:YTZRRUJZAXGZNLT4ZXDDY277IZ","target":"record","payload":{"canonical_record":{"source":{"id":"1311.5565","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-21T21:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"a06e7b5c8fafb6845f62cbc1b7c12d566ab136d9f5626576f7dffb7a69a28a37","abstract_canon_sha256":"2f31bef4548316ab0ab6aebf573243f044b2f655388b63ed939316118dbe5c64"},"schema_version":"1.0"},"canonical_sha256":"c4f318d13905cd96ae7ccdc63c6bff4674afdae93c9a021943032c32b77980ae","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:07.114450Z","signature_b64":"zzqaaG9Xw5EHw7qJoc7r73VJT5Wi9te56pWNljECr9sYDfgHFcM6wEc3QmqnRxcBRZhD9zAgg+fveHSz973WDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c4f318d13905cd96ae7ccdc63c6bff4674afdae93c9a021943032c32b77980ae","last_reissued_at":"2026-05-18T01:46:07.113854Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:07.113854Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1311.5565","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":"2026-05-18T01:46:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1yd+fbXEoZHZk0VJipj7uo7cHzVAuNhL5nXqpDGlgca6bQQEV3ip0/rgFVViJwsCXpspJsBqu6blYflNsbx8Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T15:48:56.531679Z"},"content_sha256":"791cd0e2beb6f22dd2a9eaa0978312bdfff9f658ef4114e4c9d7778cd5518942","schema_version":"1.0","event_id":"sha256:791cd0e2beb6f22dd2a9eaa0978312bdfff9f658ef4114e4c9d7778cd5518942"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:YTZRRUJZAXGZNLT4ZXDDY277IZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Physical Properties of the Inner Shocks in Hot, Tilted Black Hole Accretion Flows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aleksey Generozov, Ken B. Henisey, Omer Blaes, P. Chris Fragile","submitted_at":"2013-11-21T21:00:07Z","abstract_excerpt":"Simulations of hot, pressure supported, tilted black hole accretion flows, in which the angular momentum of the flow is misaligned with the black hole spin axis, can exhibit two non-axisymmetric shock structures in the inner regions of the flow. We analyze the strength and significance of these shock structures in simulations with tilt angles of 10 and 15 degrees. By integrating fluid trajectories in the simulations through the shocks, and tracking the variations of fluid quantities along these trajectories, we show that these shocks are strong, with substantial compression ratios, in contrast"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.5565","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:46:07Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"OUYWl0vxg14Zjq0rEJ1kSTby65Tuyx+/pQnzn05X0mg37oxlqWb8gA8F4Imkt0RqMS38qDnNhLm0J8OQDZPEAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T15:48:56.532339Z"},"content_sha256":"7a1efc313783fbd47cd679093b0607ceeab90ce4a5a78a58eb784e07cadf6cc9","schema_version":"1.0","event_id":"sha256:7a1efc313783fbd47cd679093b0607ceeab90ce4a5a78a58eb784e07cadf6cc9"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/bundle.json","state_url":"https://pith.science/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/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":"2026-05-28T15:48:56Z","links":{"resolver":"https://pith.science/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ","bundle":"https://pith.science/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/bundle.json","state":"https://pith.science/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/YTZRRUJZAXGZNLT4ZXDDY277IZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:YTZRRUJZAXGZNLT4ZXDDY277IZ","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":"2f31bef4548316ab0ab6aebf573243f044b2f655388b63ed939316118dbe5c64","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-21T21:00:07Z","title_canon_sha256":"a06e7b5c8fafb6845f62cbc1b7c12d566ab136d9f5626576f7dffb7a69a28a37"},"schema_version":"1.0","source":{"id":"1311.5565","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1311.5565","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"arxiv_version","alias_value":"1311.5565v1","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.5565","created_at":"2026-05-18T01:46:07Z"},{"alias_kind":"pith_short_12","alias_value":"YTZRRUJZAXGZ","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_16","alias_value":"YTZRRUJZAXGZNLT4","created_at":"2026-05-18T12:28:09Z"},{"alias_kind":"pith_short_8","alias_value":"YTZRRUJZ","created_at":"2026-05-18T12:28:09Z"}],"graph_snapshots":[{"event_id":"sha256:7a1efc313783fbd47cd679093b0607ceeab90ce4a5a78a58eb784e07cadf6cc9","target":"graph","created_at":"2026-05-18T01:46:07Z","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"},"paper":{"abstract_excerpt":"Simulations of hot, pressure supported, tilted black hole accretion flows, in which the angular momentum of the flow is misaligned with the black hole spin axis, can exhibit two non-axisymmetric shock structures in the inner regions of the flow. We analyze the strength and significance of these shock structures in simulations with tilt angles of 10 and 15 degrees. By integrating fluid trajectories in the simulations through the shocks, and tracking the variations of fluid quantities along these trajectories, we show that these shocks are strong, with substantial compression ratios, in contrast","authors_text":"Aleksey Generozov, Ken B. Henisey, Omer Blaes, P. Chris Fragile","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-21T21:00:07Z","title":"Physical Properties of the Inner Shocks in Hot, Tilted Black Hole Accretion Flows"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.5565","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":"sha256:791cd0e2beb6f22dd2a9eaa0978312bdfff9f658ef4114e4c9d7778cd5518942","target":"record","created_at":"2026-05-18T01:46:07Z","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":"2f31bef4548316ab0ab6aebf573243f044b2f655388b63ed939316118dbe5c64","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-21T21:00:07Z","title_canon_sha256":"a06e7b5c8fafb6845f62cbc1b7c12d566ab136d9f5626576f7dffb7a69a28a37"},"schema_version":"1.0","source":{"id":"1311.5565","kind":"arxiv","version":1}},"canonical_sha256":"c4f318d13905cd96ae7ccdc63c6bff4674afdae93c9a021943032c32b77980ae","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c4f318d13905cd96ae7ccdc63c6bff4674afdae93c9a021943032c32b77980ae","first_computed_at":"2026-05-18T01:46:07.113854Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:46:07.113854Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"zzqaaG9Xw5EHw7qJoc7r73VJT5Wi9te56pWNljECr9sYDfgHFcM6wEc3QmqnRxcBRZhD9zAgg+fveHSz973WDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:46:07.114450Z","signed_message":"canonical_sha256_bytes"},"source_id":"1311.5565","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:791cd0e2beb6f22dd2a9eaa0978312bdfff9f658ef4114e4c9d7778cd5518942","sha256:7a1efc313783fbd47cd679093b0607ceeab90ce4a5a78a58eb784e07cadf6cc9"],"state_sha256":"8a0d6518aa80271f4d6c8ea18ad83e1081a23b8db39a5940b00a21f47364026e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YAk4KJ5zyDLBFRhBWkKQ18gh7uHYKXy52itvP1wJmQK2HbF3Kb+VtO3eWy6uco3VGaaoqmMM8g0gpj9Xis3PCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T15:48:56.535294Z","bundle_sha256":"654f11a3534812a046c3538461b925a2a57db8a22f9d003860849ca42f28bca2"}}