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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>4</Volume>
				<Issue>3</Issue>
				<PubDate PubStatus="epublish">
					<Year>2024</Year>
					<Month>09</Month>
					<Day>25</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Nonextensive Statistical Mechanics and Black Hole Thermodynamics: Tsallis and Kaniadakis Entropies</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>63</FirstPage>
			<LastPage>92</LastPage>
			<ELocationID EIdType="pii">419</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2024.833.1086</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Rusul H. </FirstName>
					<LastName>Alsaedi</LastName>
<Affiliation>Department of Theoretical Physics, Faculty of Basic Sciences, University of Mazandaran, 47416-95447, Babolsar, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Tahereh </FirstName>
					<LastName>Azizi</LastName>
<Affiliation>Department of Theoretical Physics, Faculty of  Basic Sciences, University of Mazandaran, 47416-95447, Babolsar, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Jafar </FirstName>
					<LastName>Sadeghi</LastName>
<Affiliation>Department of Theoretical Physics, Faculty of  Basic Sciences, University of Mazandaran, 47416-95447, Babolsar, Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2024</Year>
					<Month>06</Month>
					<Day>08</Day>
				</PubDate>
			</History>
		<Abstract>We study the impact of nonextensive entropy on the thermodynamics of various black hole configurations, utilizing both Tsallis and Kaniadakis statistical frameworks. Additionally, we explore the stability of these black holes using the framework of nonextensivity. Our analysis reveals that the nonextensive Kaniadakis entropy does not result in any stability for the black holes. In contrast, the nonextensive Tsallis entropy ensures the stability of various black hole configurations.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Classical statistical mechanics</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">General Relativity</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">nonextensive entropies</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_419_88b10b18a1d003dc4e823e5b4b07da9d.pdf</ArchiveCopySource>
</Article>
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