{"paper":{"title":"A New Interpretation for the Hot Corona in Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jian-Min Wang, Yan-Rong Li, Yu Zhao","submitted_at":"2025-02-01T17:52:05Z","abstract_excerpt":"This work attempts to provide a new interpretation for the hot corona in active galactic nuclei (AGNs). A thin\n  parabolic magnetic reconnection layer, anchored at the innermost disk and extending along the boundary of the\n  magnetic tower for a few tens of gravitational radii, serves as a hard-X-ray source above the disk. Within this\n  reconnection layer, the tearing instability leads to the formation of a chain of plasmoids, which contain relativistic\n  electrons that generate X-ray radiation through inverse-Compton (IC) scattering of soft photons emitted by the\n  accretion disk. Based on pr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.00504","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/2502.00504/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"}