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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Iranian Journal of Astronomy and Astrophysics</JournalTitle>
				<Issn>2322-4924</Issn>
				<Volume>9</Volume>
				<Issue>2</Issue>
				<PubDate PubStatus="epublish">
					<Year>2022</Year>
					<Month>10</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Central AdS Generalized Ay{\'o}n-Beato-Garc{\'\i}a Black Holes and Joule-Thomson Expansion</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>109</FirstPage>
			<LastPage>119</LastPage>
			<ELocationID EIdType="pii">336</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2022.631.1132</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Elham </FirstName>
					<LastName>Ghasemi</LastName>
<Affiliation>Faculty of Physics, Semnan university, semnan, iran</Affiliation>

</Author>
<Author>
					<FirstName>Hossein </FirstName>
					<LastName>Ghaffarnejad</LastName>
<Affiliation>Faculty of Physics, Semnan Universiy, Semnan, Iran, 35131-19111</Affiliation>
<Identifier Source="ORCID">0000-0002-0438-6452</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2022</Year>
					<Month>12</Month>
					<Day>01</Day>
				</PubDate>
			</History>
		<Abstract>In this paper, the Joule-Thomson (JT) adiabatic expansion is&lt;br /&gt;&lt;br /&gt;investigated for generalized Ayon-Beato-Garcia (ABG)&lt;br /&gt;&lt;br /&gt;\textcolor[rgb]{0.00,0.00,1.00}{regular} black hole. It has a&lt;br /&gt;&lt;br /&gt;magnetic charge which makes central region of the black hole&lt;br /&gt;&lt;br /&gt;metric to be AdS spacetime and so become non singular.&lt;br /&gt;&lt;br /&gt;\textcolor[rgb]{0.00,0.00,1.00}{Thus we not need to use an&lt;br /&gt;&lt;br /&gt;additional cosmological parameter coming from ADS/CFT&lt;br /&gt;&lt;br /&gt;correspondence for production of pressure coordinate in the black&lt;br /&gt;&lt;br /&gt;hole equation of state. Form this point of view our work is a new&lt;br /&gt;&lt;br /&gt;approach versus to conventional methods which are addressed in the&lt;br /&gt;&lt;br /&gt;references of this paper. However we will see important behavior&lt;br /&gt;&lt;br /&gt;of parameters of this modified ABG black hole on possibility of&lt;br /&gt;&lt;br /&gt;being of JT adiabatic expansion.} This black hole is characterized&lt;br /&gt;&lt;br /&gt;by five parameters including mass $m$, magnetic charge $q$, and&lt;br /&gt;&lt;br /&gt;three \textcolor[rgb]{0.00,0.00,1.00}{other} parameters related to&lt;br /&gt;&lt;br /&gt;form of used nonlinear electromagnetic interaction fields.&lt;br /&gt;&lt;br /&gt;\textcolor[rgb]{0.00,0.00,1.00}{Inversion points are in fact a&lt;br /&gt;&lt;br /&gt;particular T-P curve at constant enthalpy and it separates cooling&lt;br /&gt;&lt;br /&gt;and heating phase of the modified AdS ABG black hole.}</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Nonsingular black holes</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Magnetic charge</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Phase transition</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">black hole thermodynamic</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Joule Thomson, Anti de Sitter</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_336_2e61986f0ed47bbfb13ce1b4b29cd3b2.pdf</ArchiveCopySource>
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