{"paper":{"title":"Probing decoupled Throats of AdS$_{D}$ Black Holes in $D=6,7$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"Near-EVH geometries of AdS black holes in six and seven dimensions reduce to lower-dimensional black holes conformally related to EMMD gravity.","cross_cats":[],"primary_cat":"hep-th","authors_text":"Weichao Bu, Yang Lei","submitted_at":"2025-11-19T13:25:36Z","abstract_excerpt":"The Kerr/CFT correspondence establishes a relationship between extremal black holes in higher dimensions and a chiral conformal field theory (CFT) in their near-horizon limit. A generalization of this framework, known as the EVH/CFT correspondence, has been developed for four- and five-dimensional AdS black holes. It was further proposed in arXiv:1910.14293 that a generalized duality between $(D-2)$-dimensional geometry and $(D-3)$-dimensional field theory may emerge in AdS$_{D=6,7}$ black holes under a suitably defined extremal vanishing horizon (EVH) limit. In this work, we demonstrate that "},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"the near-EVH geometries arising in these AdS_{6,7} black hole models, under the EVH limit, reduce to lower-dimensional black hole solutions whose metrics are conformally related to configurations of Einstein-Maxwell-Maxwell-dilaton (EMMD) gravity.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"that the suitably defined EVH limit proposed in arXiv:1910.14293 produces a decoupled throat whose geometry is exactly conformally equivalent to an EMMD black hole solution.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Near-EVH limits of AdS6 and AdS7 black holes produce conformally related lower-dimensional black hole solutions in EMMD gravity, opening a potential path to microscopic entropy counting for non-AdS black holes via higher-dimensional AdS/CFT.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Near-EVH geometries of AdS black holes in six and seven dimensions reduce to lower-dimensional black holes conformally related to EMMD gravity.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"aec98ada7f8628f7b98bc51491f607344a7b32c9fcf51fd5bd4a1c3e799fa415"},"source":{"id":"2511.15426","kind":"arxiv","version":3},"verdict":{"id":"84acc4a0-bdbf-43e2-91e1-cbecd562be9e","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-17T20:38:02.340427Z","strongest_claim":"the near-EVH geometries arising in these AdS_{6,7} black hole models, under the EVH limit, reduce to lower-dimensional black hole solutions whose metrics are conformally related to configurations of Einstein-Maxwell-Maxwell-dilaton (EMMD) gravity.","one_line_summary":"Near-EVH limits of AdS6 and AdS7 black holes produce conformally related lower-dimensional black hole solutions in EMMD gravity, opening a potential path to microscopic entropy counting for non-AdS black holes via higher-dimensional AdS/CFT.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"that the suitably defined EVH limit proposed in arXiv:1910.14293 produces a decoupled throat whose geometry is exactly conformally equivalent to an EMMD black hole solution.","pith_extraction_headline":"Near-EVH geometries of AdS black holes in six and seven dimensions reduce to lower-dimensional black holes conformally related to EMMD gravity."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2511.15426/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":117,"sample":[{"doi":"","year":2020,"title":"Probing the EVH limit of supersymmetric AdS black holes,","work_id":"45e07944-5ab8-4296-b1ba-13c7b40e0e4a","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1972,"title":"S. W. Hawking,Black holes in general relativity,Commun. Math. Phys.25(1972) 152–166","work_id":"0a4fb036-ee57-4366-8725-e1e8a442043c","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":2025,"title":"Verification of the Black Hole Area Law with GW230814,","work_id":"ee5726ec-cfa6-4e66-b164-1498a060af64","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1998,"title":"Black Hole Entropy from Near-Horizon Microstates","work_id":"15208d9a-ff07-4fed-995d-9ec02d1457af","ref_index":4,"cited_arxiv_id":"hep-th/9712251","is_internal_anchor":true},{"doi":"","year":1999,"title":"The Extreme Kerr Throat Geometry: A Vacuum Analog of AdS_2 x S^2","work_id":"b46762fe-c3f9-4939-8855-68d334cf87bb","ref_index":5,"cited_arxiv_id":"hep-th/9905099","is_internal_anchor":true}],"resolved_work":117,"snapshot_sha256":"aba46d7bc291f589681a9213dc273abb6aeb32fe6582ec5b1f8ce3d7e89cf8bf","internal_anchors":65},"formal_canon":{"evidence_count":2,"snapshot_sha256":"f92c826286942a1fe894d7d7257a7881ddea69553f2a802bdcd2859c23971cbc"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}