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<ArticleSet>
<Article>
<Journal>
				<PublisherName>The Physics Society of Iran</PublisherName>
				<JournalTitle>Iranian Journal of Physics Research</JournalTitle>
				<Issn>1682-6957</Issn>
				<Volume>26</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2026</Year>
					<Month>05</Month>
					<Day>22</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Photon sphere and shadow of dynamical Kottler black hole</ArticleTitle>
<VernacularTitle>Photon sphere and shadow of dynamical Kottler black hole</VernacularTitle>
			<FirstPage>55</FirstPage>
			<LastPage>60</LastPage>
			<ELocationID EIdType="pii">3789</ELocationID>
			
<ELocationID EIdType="doi">10.47176/ijpr.26.1.92192</ELocationID>
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName>Zahra</FirstName>
					<LastName>Allahyari Jalali</LastName>
<Affiliation>Tarbiat Modares University</Affiliation>

</Author>
<Author>
					<FirstName>Ali Akbar</FirstName>
					<LastName>Asgari</LastName>
<Affiliation>Tarbiat Modares University</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>09</Month>
					<Day>23</Day>
				</PubDate>
			</History>
		<Abstract>&lt;span&gt;In this paper, we analyze the shadow of a black hole immersed in a dynamic background reflecting the expansion of the universe due to the presence of dark energy. Using a time-dependent metric (the dynamic Kottler metric), we obtain the null (lightlike) geodesics of spacetime and calculate the effective potential for light rays. Our results show that the expansion of the universe causes the radius of the photon sphere, and consequently the black hole shadow, to decrease gradually over time. This phenomenon can be a way to determine cosmological parameters.&lt;/span&gt;</Abstract>
			<OtherAbstract Language="FA">&lt;span&gt;In this paper, we analyze the shadow of a black hole immersed in a dynamic background reflecting the expansion of the universe due to the presence of dark energy. Using a time-dependent metric (the dynamic Kottler metric), we obtain the null (lightlike) geodesics of spacetime and calculate the effective potential for light rays. Our results show that the expansion of the universe causes the radius of the photon sphere, and consequently the black hole shadow, to decrease gradually over time. This phenomenon can be a way to determine cosmological parameters.&lt;/span&gt;</OtherAbstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Kottler black hole</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Photon sphere</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Black hole shadow</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_3789_335d3d1cd7ef05ec77714a215134914c.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
