{"paper":{"title":"Black hole Near Horizons through the Looking Glass","arxiv_id":"2602.20267","primary_cat":"hep-th","submitted_at":"2026-02-23T19:00:19+00:00","version_compiled":"v2"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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spacetime.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.68,"main_claim_p":0.11,"quantitative":true,"quantitative_p":0.5,"role_probabilities":{"gap":0.0,"method":0.04,"result":0.74,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.18,"interpretation":0.04}},{"i":2,"p":0.98,"id":"s2","own":true,"role":"contribution","text":"We launch a detailed study of probes in this geometry.","hedge":{"p":0.65,"label":"asserted"},"own_p":0.88,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.98,"interpretation":0.0}},{"i":3,"p":0.86,"id":"s3","own":true,"role":"contribution","text":"We study particle geodesics and scalar fields.","hedge":{"p":0.79,"label":"asserted"},"own_p":0.92,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.0,"method":0.14,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.86,"interpretation":0.0}},{"i":4,"p":0.69,"id":"s4","own":true,"role":"method","text":"The first part of the paper constructs geodesics and probe scalar fields directly in the SC geometry.","hedge":{"p":0.93,"label":"asserted"},"own_p":0.93,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.1,"role_probabilities":{"gap":0.0,"method":0.69,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.31,"interpretation":0.0}},{"i":5,"p":0.61,"id":"s5","own":true,"role":"contribution","text":"We then look at a wide class of examples, including the Schwarzschild BH and the Kerr BH in asymptotically flat spacetimes, the BTZ BH and the black brane in AdS spacetimes, as well as Lifshitz black holes and construct the explicit maps to the SC geometry to obtain results specific to each case.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.93,"main_claim_p":0.08,"quantitative":false,"quantitative_p":0.11,"role_probabilities":{"gap":0.0,"method":0.38,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.61,"interpretation":0.0}},{"i":6,"p":0.77,"id":"s6","own":true,"role":"result","text":"These results are reproduced by considering the probe particles and fields in the original BH background and taking the near-horizon limit of the solutions.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.87,"main_claim_p":0.13,"quantitative":false,"quantitative_p":0.17,"role_probabilities":{"gap":0.0,"method":0.16,"result":0.77,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.03,"interpretation":0.04}},{"i":7,"p":0.54,"id":"s7","own":true,"role":"interpretation","text":"Our encyclopedia of examples establishes the notion of SC geometries as near-horizon geometries of 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