{"id":"c4fe691b-6175-4a50-9cfb-c60808b85883","arxiv_id":"2504.12014","paper_version":2,"verdict":"REJECT","confidence":"HIGH","novelty_score":4.0,"correctness_risk":"high","formal_verification":"none","parameter_count":2,"one_line_summary":"Quantized horizon area with a step fixed by Landauer's principle yields logarithmic and inverse-area corrections to Hawking temperature and entropy for four black hole geometries.","lead":"This paper derives corrections to black hole temperature and entropy by assuming the event horizon area comes in discrete quantum steps, and fixes the step size using Landauer's principle from information theory. It applies the calculation to Schwarzschild, quantum-corrected Schwarzschild, charged, and rotating black holes, finding logarithmic and inverse-area entropy corrections.","discovery_kind":"extension","skeptic_critique":null,"referee_report":null,"author_rebuttal":null,"desk_editor":null,"rs_alignment":null,"lean_confirmation":null,"pith_extraction":null,"created_at":"2026-08-16T12:40:52.535858+00:00","model_set":{"reader":"deepseek-v4-flash"},"falsifier":null,"supporting_citations":[],"review_version":1}