{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:5QZCAC6LAFCY3PGVOD5XWPTBMY","short_pith_number":"pith:5QZCAC6L","canonical_record":{"source":{"id":"1604.00373","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-29T11:51:27Z","cross_cats_sorted":[],"title_canon_sha256":"a3c0c239d71c12ddf3c09504785f989f0f512b0a4f844af4245746cb88a1f85b","abstract_canon_sha256":"03ad6ed260b347da1191d29c7b27654bc24c4070df3567c4880a50979d49e271"},"schema_version":"1.0"},"canonical_sha256":"ec32200bcb01458dbcd570fb7b3e6166244bcc950dc8681b73503d6668c90541","source":{"kind":"arxiv","id":"1604.00373","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.00373","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"arxiv_version","alias_value":"1604.00373v1","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.00373","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"pith_short_12","alias_value":"5QZCAC6LAFCY","created_at":"2026-05-18T12:30:01Z"},{"alias_kind":"pith_short_16","alias_value":"5QZCAC6LAFCY3PGV","created_at":"2026-05-18T12:30:01Z"},{"alias_kind":"pith_short_8","alias_value":"5QZCAC6L","created_at":"2026-05-18T12:30:01Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:5QZCAC6LAFCY3PGVOD5XWPTBMY","target":"record","payload":{"canonical_record":{"source":{"id":"1604.00373","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-29T11:51:27Z","cross_cats_sorted":[],"title_canon_sha256":"a3c0c239d71c12ddf3c09504785f989f0f512b0a4f844af4245746cb88a1f85b","abstract_canon_sha256":"03ad6ed260b347da1191d29c7b27654bc24c4070df3567c4880a50979d49e271"},"schema_version":"1.0"},"canonical_sha256":"ec32200bcb01458dbcd570fb7b3e6166244bcc950dc8681b73503d6668c90541","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:13:11.303130Z","signature_b64":"/SJ8lRRCp/CBMVrY3HDzokh7QQuMkK+nDjTOFQN+UMhG4nsy6z3QoDTWjV9zmv48CK6mlnCPzlTfy4RBzs2CDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ec32200bcb01458dbcd570fb7b3e6166244bcc950dc8681b73503d6668c90541","last_reissued_at":"2026-05-18T01:13:11.302792Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:13:11.302792Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1604.00373","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":"2026-05-18T01:13:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Gfnl31hfVz5A0dWrwiCuuNgMczxyrxVX1tP+4eV1FTx2ic57QAcM0Ed3gzZeSjlkWbkD9/8oVj7UtaOkpEVgDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-26T12:30:23.055910Z"},"content_sha256":"6955611a1716efce52f064246590dd8bf4c66291223e20f969622131bc1f8fb2","schema_version":"1.0","event_id":"sha256:6955611a1716efce52f064246590dd8bf4c66291223e20f969622131bc1f8fb2"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:5QZCAC6LAFCY3PGVOD5XWPTBMY","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The influence of outflow in supercritical accretion flows","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Amin Mosallanezhad, Fatemeh Zahra Zeraatgari, Shahram Abbassi","submitted_at":"2016-03-29T11:51:27Z","abstract_excerpt":"We solve the radiation-hydrodynamic (RHD) equations of supercritical accretion flows in the presence of radiation force and outflow by using self similar solutions. Compare with the pioneer works, in this paper we consider power-law function for mass inflow rate as $ \\dot{M} \\propto r^{s} $. We found that $ s = 1 $ when the radiative cooling term is included in the energy equation. Correspondingly, the effective temperature profile with respect to the radius was obtained as $ T_{\\text{eff}} \\varpropto r^{-1/2} $. In addition, we investigated the influence of the outflow on the dynamics of the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.00373","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":"2026-05-18T01:13:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"RnHDGujygpzrogC3GuCiRGupGcbFz+YCSOrxlPmnzfM+8n9ixIWdNgAqL8qcgSDScfbHxPe9fyEJt8waQIMkCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-26T12:30:23.056257Z"},"content_sha256":"7b48d17decf2afa1d78d8b1e9a403172074e914a0b13ee84361ea40325ad1b11","schema_version":"1.0","event_id":"sha256:7b48d17decf2afa1d78d8b1e9a403172074e914a0b13ee84361ea40325ad1b11"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/bundle.json","state_url":"https://pith.science/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/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":"2026-06-26T12:30:23Z","links":{"resolver":"https://pith.science/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY","bundle":"https://pith.science/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/bundle.json","state":"https://pith.science/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5QZCAC6LAFCY3PGVOD5XWPTBMY/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:5QZCAC6LAFCY3PGVOD5XWPTBMY","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":"03ad6ed260b347da1191d29c7b27654bc24c4070df3567c4880a50979d49e271","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-29T11:51:27Z","title_canon_sha256":"a3c0c239d71c12ddf3c09504785f989f0f512b0a4f844af4245746cb88a1f85b"},"schema_version":"1.0","source":{"id":"1604.00373","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1604.00373","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"arxiv_version","alias_value":"1604.00373v1","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.00373","created_at":"2026-05-18T01:13:11Z"},{"alias_kind":"pith_short_12","alias_value":"5QZCAC6LAFCY","created_at":"2026-05-18T12:30:01Z"},{"alias_kind":"pith_short_16","alias_value":"5QZCAC6LAFCY3PGV","created_at":"2026-05-18T12:30:01Z"},{"alias_kind":"pith_short_8","alias_value":"5QZCAC6L","created_at":"2026-05-18T12:30:01Z"}],"graph_snapshots":[{"event_id":"sha256:7b48d17decf2afa1d78d8b1e9a403172074e914a0b13ee84361ea40325ad1b11","target":"graph","created_at":"2026-05-18T01:13:11Z","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":"We solve the radiation-hydrodynamic (RHD) equations of supercritical accretion flows in the presence of radiation force and outflow by using self similar solutions. Compare with the pioneer works, in this paper we consider power-law function for mass inflow rate as $ \\dot{M} \\propto r^{s} $. We found that $ s = 1 $ when the radiative cooling term is included in the energy equation. Correspondingly, the effective temperature profile with respect to the radius was obtained as $ T_{\\text{eff}} \\varpropto r^{-1/2} $. In addition, we investigated the influence of the outflow on the dynamics of the ","authors_text":"Amin Mosallanezhad, Fatemeh Zahra Zeraatgari, Shahram Abbassi","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-29T11:51:27Z","title":"The influence of outflow in supercritical accretion flows"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.00373","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":"sha256:6955611a1716efce52f064246590dd8bf4c66291223e20f969622131bc1f8fb2","target":"record","created_at":"2026-05-18T01:13:11Z","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":"03ad6ed260b347da1191d29c7b27654bc24c4070df3567c4880a50979d49e271","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-29T11:51:27Z","title_canon_sha256":"a3c0c239d71c12ddf3c09504785f989f0f512b0a4f844af4245746cb88a1f85b"},"schema_version":"1.0","source":{"id":"1604.00373","kind":"arxiv","version":1}},"canonical_sha256":"ec32200bcb01458dbcd570fb7b3e6166244bcc950dc8681b73503d6668c90541","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ec32200bcb01458dbcd570fb7b3e6166244bcc950dc8681b73503d6668c90541","first_computed_at":"2026-05-18T01:13:11.302792Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:13:11.302792Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"/SJ8lRRCp/CBMVrY3HDzokh7QQuMkK+nDjTOFQN+UMhG4nsy6z3QoDTWjV9zmv48CK6mlnCPzlTfy4RBzs2CDg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:13:11.303130Z","signed_message":"canonical_sha256_bytes"},"source_id":"1604.00373","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6955611a1716efce52f064246590dd8bf4c66291223e20f969622131bc1f8fb2","sha256:7b48d17decf2afa1d78d8b1e9a403172074e914a0b13ee84361ea40325ad1b11"],"state_sha256":"f4412b05ca77ae1ff14afd39c8db7c85b2b09c188bb00a85962199bb59681f7c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lp0/IiKjK9WmoTNu846RRysQ0/Uej/+rENqNJi8v5/lCPJJ29uKF4zKHpLX9hw9AN0eAPFk9ms2yJ8/fZzApBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-26T12:30:23.058386Z","bundle_sha256":"c18c3121f7a1d760b494256889ec9a4456fa69fc642ad263148a6e5388d1b7c3"}}