{"paper":{"title":"A systematic study of the condensation of the corona and the application for $\\Gamma_{\\rm 2-10keV}-L_{\\rm bol}/L_{\\rm Edd}$ correlation in luminous active galactic nuclei","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"B.F. Liu, Erlin Qiao","submitted_at":"2018-03-09T03:48:24Z","abstract_excerpt":"In this paper, we explained the observed $\\Gamma_{\\rm 2-10keV}-L_{\\rm bol}/L_{\\rm Edd}$ correlation in luminous active galactic nuclei within the framework of the condensation of the corona around a supermassive black hole (Liu et al. 2015; Qiao & Liu 2017). Specifically, we systemically test the effects of black hole mass $M$, the viscosity parameter $\\alpha$, and the magnetic parameter $\\beta$ (with magnetic pressure $p_{\\rm m}=B^2/{8\\pi}=(1-\\beta)p_{\\rm tot}$, $p_{\\rm tot}=p_{\\rm gas}+p_{\\rm m}$) on the structure of the accretion disc and the corona, as well as the corresponding emergent sp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.03375","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"}