{"paper":{"title":"Special $N$-dimensional charged anti-de-Sitter black holes in $f(\\mathbb{Q})$ gravitational theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"G.G.L. Nashed","submitted_at":"2023-12-22T05:54:28Z","abstract_excerpt":"Due to the absence of spherically symmetric black hole solutions in $f(\\mathbb{Q})$ because of the constraint derived from its field equations, which yields either $\\mathbb{Q}=0 $ or $f_{\\mathbb{Q} \\mathbb{Q}}=0 $ \\cite{Heisenberg:2023lru,Maurya:2023muz}. We are going to introduce a tours solutions for charged anti-de-Sitter black holes in $N$-dimensions within the framework of the quadratic form of $f(\\mathbb{Q})$ gravity, where the coincident gauge condition is applied \\cite{Heisenberg:2023lru}. Here, $f(\\mathbb{Q})=\\mathbb{Q}+\\frac{1}2\\alpha \\mathbb{Q}^2-2\\Lambda$, and the condition $N \\geq"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.14451","kind":"arxiv","version":3},"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/2312.14451/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"}