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<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Three Impossible Theories</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>1</FirstPage>
			<LastPage>9</LastPage>
			<ELocationID EIdType="pii">1932</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.3085.1143</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Leonard </FirstName>
					<LastName>Susskind</LastName>
<Affiliation>Stanford Institute for Theoretical Physics and Department of Physics, Stanford University, Stanford, CA 94305-4060, USA and Google, Mountain View, CA</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>10</Month>
					<Day>06</Day>
				</PubDate>
			</History>
		<Abstract>I will begin by conjecturing a cosmological generalization of black hole complementarity (also known as the central dogma). I will then discuss three theories and argue that they are inconsistent with second law of thermodynamics if the cosmological version of the dogma is correct. The three theories are: the big rip; cyclic cosmology; and the Farhi-Guth-Guven mechanism for creating inflating universes behind black hole horizons.</Abstract>
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			<Param Name="value">Cosmology</Param>
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			<Object Type="keyword">
			<Param Name="value">Inflation</Param>
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<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_1932_7e68b1d2cddcb5273566ad6b64184291.pdf</ArchiveCopySource>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Categorical Symmetries and Fiber Functors from Multiple Gaugeable Homomorphisms from 6D N=(2,0) SCFTs</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>10</FirstPage>
			<LastPage>40</LastPage>
			<ELocationID EIdType="pii">1933</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.3062.1135</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Veronica </FirstName>
					<LastName>Pasquarella</LastName>
<Affiliation>Shanghai Institute for Mathematics and Interdisciplinary Sciences (SIMIS), Shanghai, 200433, China; Research Institute of Intelligent Complex Systems, Fudan University, Shanghai 
200433, China; Department of Applied Mathematics and Theoretical Physics (DAMTP), University of Cambridge, Wilberforce Road, CB3 0WA, Cambridge, UK</Affiliation>
<Identifier Source="ORCID">0000-0002-3276-0341</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>09</Month>
					<Day>17</Day>
				</PubDate>
			</History>
		<Abstract>Exploiting the symmetry topological field theory/topological order correspondence (SymTFT/TO), together with the higher-categorical structure of 6D N=(2,0) SCFTs, we prove that the total quantum dimension of the relative gaugeable algebra leading to intrinsic non-invertible symmetries between class S theories is greater with respect to the non-intrinsic case. From a higher-categorical perspective, this supports the idea that multiplicity is allowed to exceed unity in some superselection sectors.</Abstract>
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			<Param Name="value">higher categories</Param>
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			<Object Type="keyword">
			<Param Name="value">representation theory</Param>
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			<Param Name="value">relative QFTs</Param>
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			<Param Name="value">gauge theory</Param>
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<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_1933_67b34bc4c248f4c471f60b16a3fe614f.pdf</ArchiveCopySource>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>The EGUP-Induced Critical Radius: A New Holographic Scale for Quantum Gravity</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>41</FirstPage>
			<LastPage>59</LastPage>
			<ELocationID EIdType="pii">1949</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.2995.1124</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Sara </FirstName>
					<LastName>Motalebi</LastName>
<Affiliation>Department of Physics, School of Sciences, Tarbiat Modares University, P.O.Box 14155-4838, Tehran, Iran</Affiliation>
<Identifier Source="ORCID">0009-0006-6306-3115</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>07</Month>
					<Day>18</Day>
				</PubDate>
			</History>
		<Abstract>We present a unified framework incorporating both the Generalized and Extended Uncertainty Principles (GUP/EUP) in Anti-de Sitter space. This reveals a fundamental quantum gravity scale, the \textit{critical radius} $r_{\rm crit}=(\beta/\gamma)^{1/4}\sqrt{\ell_{P}L}$, which marks a phase transition where quantum gravitational ($\beta$) and AdS curvature ($\gamma$) effects equilibrate. At this scale, we demonstrate three interconnected phenomena: (i) a breakdown of the standard holographic duality, signaled by the exact vanishing of the boundary stress tensor $\langle T_{\mu\nu}\rangle=0$ under the self-duality condition $\partial_z g_{\mu\nu}|_{z=r_{\rm crit}}=0$; (ii) a topological transition manifested by the complexification of the central charge, $c_{\rm eff}=c\left(1+\frac{i}{2}\sqrt{\kappa}\ell_{P}^{2}\right)$ with $\kappa=(\beta/\gamma)^{1/4}\sqrt{\beta\gamma\ell_P/L}$; and (iii) a mechanism as a scenario for information paradox resolution, where information is recovered via topological storage in Chern-Simons states, modifying the Page curve with $\Delta S_{\rm recovery}&gt;0$. These effects establish a consistency condition $L&gt;\sqrt{\beta}\ell_{P}$ for a valid AdS/CFT correspondence and identify $r_{\rm crit}$ as the thermodynamic critical point where black holes transition to stringy remnants and information is topologically scrambled.</Abstract>
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			<Object Type="keyword">
			<Param Name="value">Generalized Uncertainty Principle</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Extended Uncertainty Principle</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">AdS/CFT correspondence</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Black Hole/String Transition</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_1949_a5cfdd57fbedd8469d739b1807c7d077.pdf</ArchiveCopySource>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Hawking-Page Transition from Logarithmic Entropy in f(R) Gravity</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>60</FirstPage>
			<LastPage>81</LastPage>
			<ELocationID EIdType="pii">1950</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.3077.1142</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Sameer Ahmad </FirstName>
					<LastName>Mir</LastName>
<Affiliation>Department of Physics, Jamia Millia Islamia, New Delhi, 110025, India; Department of Computer Sciences, Asian School of Business, Uttar Pradesh, 210303, India</Affiliation>
<Identifier Source="ORCID">0000-0001-7528-1861</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>09</Month>
					<Day>28</Day>
				</PubDate>
			</History>
		<Abstract>We analyze the thermodynamics and phase structure of a static, spherically symmetric black hole that extends Schwarzschild within f(R) gravity. In the extended framework, we include a model-independent, one-loop-motivated logarithmic entropy correction with a free coefficient b. We derive closed-form expressions for temperature, enthalpy, corrected entropy, Gibbs free energy, and heat capacity to first order in the deformation parameter, and chart the Hawking-Page transition and local stability. A positive $b$ suppresses local stability for small black holes, while negative b enhances it. We also state the generalized first law with the f(R) coupling as a thermodynamic variable, providing a practical phenomenology for future microscopic determinations of b.</Abstract>
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			<Object Type="keyword">
			<Param Name="value">Black-hole thermodynamics</Param>
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			<Object Type="keyword">
			<Param Name="value">Gibbs free energy</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Logarithmic entropy correction</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">AdS black holes</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Phase structure and criticality</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Holographic implications</Param>
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<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_1950_90c236e24f8ce610b8f4f804a34273a2.pdf</ArchiveCopySource>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Holographic Dark Energy Models and Late Time Cosmic Acceleration in Light of Recent Observations</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>82</FirstPage>
			<LastPage>97</LastPage>
			<ELocationID EIdType="pii">1954</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.2988.1132</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Sonali </FirstName>
					<LastName>Borah</LastName>
<Affiliation>Department of Physics, Assam  University, Silchar-788011,Assam, India</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>08</Month>
					<Day>26</Day>
				</PubDate>
			</History>
		<Abstract>Holographic dark energy(HDE) models, based on the holographic principle, offer a quantum gravity-inspired explanation for the universe&#039;s late-time acceleration. In HDE models, the vacuum energy density relates to an infrared (IR) cutoff, determined by horizon scales. In this study, we performed parameter estimation using the latest observational data, including Type Ia Supernovae, GRBs, and observed Hubble parameters across various holographic dark energy models. We employ the Markov Chain Monte Carlo (MCMC) method to evaluate the viability of these models. Our results show that holographic dark energy models are consistent with existing data and provide insights into the dynamic nature of dark energy. This research highlights the deep connection between cosmological observations and quantum gravity concepts to enhance our understanding of cosmic acceleration.</Abstract>
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			<Object Type="keyword">
			<Param Name="value">Cosmic acceleration</Param>
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			<Object Type="keyword">
			<Param Name="value">Dark Energy</Param>
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			<Object Type="keyword">
			<Param Name="value">Holographic Principle</Param>
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			<Object Type="keyword">
			<Param Name="value">IR cutoff</Param>
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<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_1954_65b6eead17d6a65f86af162ec2f36af6.pdf</ArchiveCopySource>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Holographic and Thermodynamic Topological Perspectives on AdS Einstein-Power-Yang-Mills Black Holes with Generalized Entropy</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>98</FirstPage>
			<LastPage>125</LastPage>
			<ELocationID EIdType="pii">1996</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.3126.1156</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>N </FirstName>
					<LastName>Ramya</LastName>
<Affiliation>Department of Mathematics, Kongu Engineering College, Erode-638060, India</Affiliation>
<Identifier Source="ORCID">0009-0005-1665-1996</Identifier>

</Author>
<Author>
					<FirstName>R </FirstName>
					<LastName>Tamilamuthan</LastName>
<Affiliation>Department of Electrical and Electronics Engineering, Assistant Professor, PERI Institute Of Technology, Chennai-600048, India</Affiliation>

</Author>
<Author>
					<FirstName>Hossein </FirstName>
					<LastName>Rashmanlou</LastName>
<Affiliation>Canadian Quantum Research Center, 106-460 Doyle Ave, Kelowna, British Columbia V1Y 0C2 Canada</Affiliation>
<Identifier Source="ORCID">0000-0001-8717-9530</Identifier>

</Author>
<Author>
					<FirstName>Farshid </FirstName>
					<LastName>Mofidnakhaei</LastName>
<Affiliation>Department of Physics, Sar. C., Islamic Azad University, Sari, Iran</Affiliation>
<Identifier Source="ORCID">0000-0002-2903-0428</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>11</Month>
					<Day>04</Day>
				</PubDate>
			</History>
		<Abstract>In this work, we explore the holographic and thermodynamic topology of Anti–de Sitter (AdS) Einstein–Power–Yang–Mills (EPYM) black holes using both the bulk–boundary correspondence and the restricted phase space (RPS) frameworks. The study employs several non-extensive entropy models, including Barrow, R´enyi, Sharma–Mittal, Kaniadakis, and Tsallis–Cirto entropies. Within the bulk–boundary formalism, we find that the free deformation parameters strongly influence the classification of topo‌logical charges w. For the Barrow entropy, two distinct topological charges w = +1 and w = −1 appear as the deformation parameter increases, closely resembling the Bekenstein–Hawking limit. The R´enyi entropy exhibits a transition from three charges w = (+1, 0, −1) to a single charge w = +1 as the non-extensive parameter rises, while setting the deformation parame‌ter to zero yields two symmetric charges w = ±1. In the Sharma–Mittal framework, three characteristic regions emerge: for higher parameter ra‌tios, w = +1; for balanced ratios, w = 0; and for lower ratios, w = −1. The Kaniadakis entropy generally shows w = ±1 for most admissible K values, except at K = 0, where only w = +1 remains. The Tsallis–Cirto entropy displays two topological charges w = ±1 for small deformation parameters and a single charge w = +1 as the parameter approaches 0.9. Extending the analysis to the RPS framework reveals that, for R´enyi, Sharma–Mittal, and Tsallis–Cirto entropies, the topological charge remains invariant at w = +1, regardless of parameter variation. However, in the Barrow and Kaniadakis cases, the topological configuration evolves with increasing non‌extensivity, leading to distinct topological transitions in w. These findings provide deeper insights into the holographic and thermodynamic structure of non-extensive AdS black holes and highlight their phase evolution under generalized entropy formulations. The present work differs by (i) an explicit bulk boundary holographic mapping that tracks how the EPYM power q modifies boundary central-charge and chemical potential variables, (ii) ad‌ditional analytic expansions and parameter-range scans for q and entropy deformation parameters, and (iii) the introduction of supplementary stabil‌ity diagnostics and response-function tests that probe the robustness of the topology classification.</Abstract>
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			<Param Name="value">Holography</Param>
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			<Object Type="keyword">
			<Param Name="value">thermodynamic</Param>
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			<Object Type="keyword">
			<Param Name="value">Black Holes</Param>
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			<Param Name="value">topology</Param>
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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Journal of Holography Applications in Physics</JournalTitle>
				<Issn>2783-4778</Issn>
				<Volume>6</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>12</Month>
					<Day>27</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Discussion on the Faizal–Krauss–Shabir–Marino Argument about the Theory of Everything</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>126</FirstPage>
			<LastPage>132</LastPage>
			<ELocationID EIdType="pii">2003</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2025.3160.1166</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Aatif Kaisar </FirstName>
					<LastName>Khan</LastName>
<Affiliation>Department of Physics, University of Florida, Gainesville, FL 32611-8440, USA</Affiliation>

</Author>
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				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>11</Month>
					<Day>21</Day>
				</PubDate>
			</History>
		<Abstract>In this note I comment on the article ``Consequences of Undecidability in Physics on the Theory of Everything&#039;&#039; by Faizal-Krauss-Shabir-Marino (FKSM). I first summarise what I take to be the central claims and contributions of the work, and then highlight why it is, in my view, a genuinely important step in the dialogue between mathematical logic and fundamental physics. I finally suggest a clarification concerning the status of non-algorithmic understanding in their framework, in order to avoid any appearance of human-centrism, and point out that their picture naturally invites an interpretation in which a consciousness-like, non-algorithmic form of understanding operates in a Platonic realm that generates the informational ``bit&#039;&#039; and, through it, the physical ``it&#039;&#039;.</Abstract>
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