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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>21</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2021</Year>
					<Month>05</Month>
					<Day>22</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Quasinormal modes of black holes in dRGT massive gravity ‎
under electromagnetic perturbations</ArticleTitle>
<VernacularTitle>Quasinormal modes of black holes in dRGT massive gravity ‎
under electromagnetic perturbations</VernacularTitle>
			<FirstPage>213</FirstPage>
			<LastPage>218</LastPage>
			<ELocationID EIdType="pii">1688</ELocationID>
			
<ELocationID EIdType="doi">10.47176/ijpr.21.1.01144</ELocationID>
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName>S H</FirstName>
					<LastName>Hendi</LastName>
<Affiliation>Department of Physics, School of Science, Shiraz University, Shiraz, Iran; ‎
Biruni Observatory, School of Science, Shiraz University, Shiraz, Iran</Affiliation>
<Identifier Source="ORCID">0000-0002-4444-6579</Identifier>

</Author>
<Author>
					<FirstName>M</FirstName>
					<LastName>Momennia</LastName>
<Affiliation>Department of Physics, School of Science, Shiraz University, Shiraz, Iran; ‎
	Biruni Observatory, School of Science, Shiraz University, Shiraz, Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2020</Year>
					<Month>10</Month>
					<Day>24</Day>
				</PubDate>
			</History>
		<Abstract>Upon semi-analytical and numerical methods, the quasinormal frequencies of dRGT massive black holes under electromagnetic perturbation are calculated and the dynamical stability of these black holes is investigated. The effect of graviton’s mass on the frequencies is investigated and it is shown that the WKB approximation is valid not only for  but also only for low-mass gravitons.</Abstract>
			<OtherAbstract Language="FA">Upon semi-analytical and numerical methods, the quasinormal frequencies of dRGT massive black holes under electromagnetic perturbation are calculated and the dynamical stability of these black holes is investigated. The effect of graviton’s mass on the frequencies is investigated and it is shown that the WKB approximation is valid not only for  but also only for low-mass gravitons.</OtherAbstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Dynamic stability</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Quasinormal modes</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">massive gravity</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_1688_ae614c557843b1df326cb29c57225459.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
