{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,27]],"date-time":"2025-10-27T05:08:25Z","timestamp":1761541705381,"version":"build-2065373602"},"reference-count":78,"publisher":"MDPI AG","issue":"2","license":[{"start":{"date-parts":[[2024,2,11]],"date-time":"2024-02-11T00:00:00Z","timestamp":1707609600000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>Given the AdS\/CFT relationship, the study of higher-dimensional AdS black holes is extremely important. Furthermore, since the restriction derived from\u00a0f(Q)\u2019s field equations prevents it from deriving spherically symmetric black hole solutions, the result is either\u00a0Q\u2032=0\u00a0or\u00a0fQQ=0. Utilizing the cylindrical coordinate system within the context the cubic form of\u00a0f(Q)\u00a0theory while imposing the condition of a coincident gauge, we establish the existence of static solutions in D-dimensions. The power-law ansatz, which is the most practical based on observations, will be used in this study, where\u00a0f(Q)=Q+12\u03b3Q2+13\u03b3Q3\u22122\u039b\u00a0and the condition\u00a0D\u22654\u00a0are met. These solutions belong to a new solution class, the properties of which are derived only from the non-metricity Q modification, since they do not have a general relativity limit. We examine the singularities present in the solutions by calculating the non-metricity and curvature invariant values. In conclusion, we compute thermodynamic parameters such as Gibbs free energy, Hawking temperature, and entropy. These thermodynamic calculations confirm that our model is stable.<\/jats:p>","DOI":"10.3390\/sym16020219","type":"journal-article","created":{"date-parts":[[2024,2,12]],"date-time":"2024-02-12T04:47:45Z","timestamp":1707713265000},"page":"219","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":4,"title":["Solutions with a Flat Horizon in D Dimensions within the Cubic Form of f(Q) Gravity"],"prefix":"10.3390","volume":"16","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-5544-1119","authenticated-orcid":false,"given":"Gamal Gergess Lamee","family":"Nashed","sequence":"first","affiliation":[{"name":"Centre for Theoretical Physics, The British University in Egypt, P.O. Box 43, El Sherouk City, Cairo 11837, Egypt"},{"name":"Center for Space Research, North-West University, Potchefstroom 2520, South Africa"}]}],"member":"1968","published-online":{"date-parts":[[2024,2,11]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"175","DOI":"10.1086\/377226","article-title":"First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters","volume":"148","author":"Spergel","year":"2003","journal-title":"Astrophys. J. Suppl."},{"key":"ref_2","doi-asserted-by":"crossref","first-page":"565","DOI":"10.1086\/307221","article-title":"Measurements of \u03a9 and \u039b from 42 high redshift supernovae","volume":"517","author":"Perlmutter","year":"1999","journal-title":"Astrophys. 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