{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:YSQQDKM4C32T76RAFB5OVYNU5Z","short_pith_number":"pith:YSQQDKM4","schema_version":"1.0","canonical_sha256":"c4a101a99c16f53ffa20287aeae1b4ee7b62fe0467ff66cf5e6a932cdbe73a36","source":{"kind":"arxiv","id":"1411.0883","version":2},"attestation_state":"computed","paper":{"title":"On the role of fast magnetic reconnection in accreting black hole sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. B. Singh, E.M. de Gouveia Dal Pino, L.H.S. Kadowaki","submitted_at":"2014-11-04T12:35:20Z","abstract_excerpt":"We attempt to explain the observed radio and gamma-ray emission produced in the surrounds of black holes by employing a magnetically-dominated accretion flow (MDAF) model and fast magnetic reconnection triggered by turbulence. In earlier work, standard disk model was used and we refine the model by focussing on the sub-Eddington regime to address the fundamental plane of black hole activity. The results do not change substantially with regard to previous work ensuring that the details of the accretion physics are not relevant in the magnetic reconnection process occurring in the corona. Rather"},"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":"1411.0883","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T12:35:20Z","cross_cats_sorted":[],"title_canon_sha256":"903a390e7181f3343c30735680dbe0c80b824ddc3dc35663128583dda9ab7429","abstract_canon_sha256":"7ccc0141a3c5915e3f68ffafe7424e0ed5ead8eef3579f56489a9df7b5b580f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:35.345400Z","signature_b64":"tfOmzEAUjYSC50NnVH2rwPNeWlUgryEe9wJyh9K7cPNLehssBPxQwe24hLKqlxDMQKU9GELwzVW3VCFuCsP2AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c4a101a99c16f53ffa20287aeae1b4ee7b62fe0467ff66cf5e6a932cdbe73a36","last_reissued_at":"2026-05-18T01:41:35.344710Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:35.344710Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the role of fast magnetic reconnection in accreting black hole sources","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. B. Singh, E.M. de Gouveia Dal Pino, L.H.S. Kadowaki","submitted_at":"2014-11-04T12:35:20Z","abstract_excerpt":"We attempt to explain the observed radio and gamma-ray emission produced in the surrounds of black holes by employing a magnetically-dominated accretion flow (MDAF) model and fast magnetic reconnection triggered by turbulence. In earlier work, standard disk model was used and we refine the model by focussing on the sub-Eddington regime to address the fundamental plane of black hole activity. The results do not change substantially with regard to previous work ensuring that the details of the accretion physics are not relevant in the magnetic reconnection process occurring in the corona. Rather"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0883","kind":"arxiv","version":2},"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":"1411.0883","created_at":"2026-05-18T01:41:35.344819+00:00"},{"alias_kind":"arxiv_version","alias_value":"1411.0883v2","created_at":"2026-05-18T01:41:35.344819+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.0883","created_at":"2026-05-18T01:41:35.344819+00:00"},{"alias_kind":"pith_short_12","alias_value":"YSQQDKM4C32T","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_16","alias_value":"YSQQDKM4C32T76RA","created_at":"2026-05-18T12:28:57.508820+00:00"},{"alias_kind":"pith_short_8","alias_value":"YSQQDKM4","created_at":"2026-05-18T12:28:57.508820+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/YSQQDKM4C32T76RAFB5OVYNU5Z","json":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z.json","graph_json":"https://pith.science/api/pith-number/YSQQDKM4C32T76RAFB5OVYNU5Z/graph.json","events_json":"https://pith.science/api/pith-number/YSQQDKM4C32T76RAFB5OVYNU5Z/events.json","paper":"https://pith.science/paper/YSQQDKM4"},"agent_actions":{"view_html":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z","download_json":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z.json","view_paper":"https://pith.science/paper/YSQQDKM4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1411.0883&json=true","fetch_graph":"https://pith.science/api/pith-number/YSQQDKM4C32T76RAFB5OVYNU5Z/graph.json","fetch_events":"https://pith.science/api/pith-number/YSQQDKM4C32T76RAFB5OVYNU5Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z/action/storage_attestation","attest_author":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z/action/author_attestation","sign_citation":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z/action/citation_signature","submit_replication":"https://pith.science/pith/YSQQDKM4C32T76RAFB5OVYNU5Z/action/replication_record"}},"created_at":"2026-05-18T01:41:35.344819+00:00","updated_at":"2026-05-18T01:41:35.344819+00:00"}