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<ArticleSet>
<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>4</Issue>
				<PubDate PubStatus="epublish">
					<Year>2026</Year>
					<Month>05</Month>
					<Day>30</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Analytic Correspondence between Barrow Holographic Dark Energy and f(Q) Gravity</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>217</FirstPage>
			<LastPage>231</LastPage>
			<ELocationID EIdType="pii">2105</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2026.3208.1182</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Leila </FirstName>
					<LastName>Shahkarami</LastName>
<Affiliation>School of Physics, Damghan University, Damghan, P.O.Box 36716-45667, Iran.</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>28</Day>
				</PubDate>
			</History>
		<Abstract>We investigate Barrow holographic dark energy within the framework of symmetric teleparallel $f(Q)$ gravity at the homogeneous background level. Adopting a reconstruction viewpoint, we require the effective geometric energy density of $f(Q)$ gravity to reproduce the Barrow holographic scaling when the Hubble radius is chosen as the infrared cutoff. This condition uniquely determines a simple analytic power-law form for the nonmetricity scalar in the gravitational Lagrangian, with the Barrow deformation parameter directly fixing the exponent. The reconstructed action smoothly reduces to the symmetric teleparallel equivalent of general relativity in the limit of vanishing Barrow correction $\Delta$. We analyze the background cosmological behavior in the presence of pressureless matter and show that, for $0&lt;\Delta&lt;1$, the modified scaling admits an asymptotic de Sitter solution, while the standard $\Delta=0$ case does not yield self-acceleration with the Hubble cutoff. Our results establish a minimal analytic embedding of Barrow holographic dark energy into nonmetricity-based modified gravity and provide a transparent geometric interpretation of the Barrow deformation parameter.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Barrow Holographic Dark Energy</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">$f(Q)$ Gravity</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Symmetric Teleparallel Gravity</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Modified Gravity</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_2105_f49ab5e4eca3a4f55bfccd11d283daca.pdf</ArchiveCopySource>
</Article>
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