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<Article>
<Journal>
				<PublisherName>The Physics Society of Iran</PublisherName>
				<JournalTitle>Iranian Journal of Physics Research</JournalTitle>
				<Issn>1682-6957</Issn>
				<Volume>22</Volume>
				<Issue>4</Issue>
				<PubDate PubStatus="epublish">
					<Year>2023</Year>
					<Month>02</Month>
					<Day>20</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Study of corrections on the holographic zero sound</ArticleTitle>
<VernacularTitle>Study of corrections on the holographic zero sound</VernacularTitle>
			<FirstPage>773</FirstPage>
			<LastPage>782</LastPage>
			<ELocationID EIdType="pii">3322</ELocationID>
			
<ELocationID EIdType="doi">10.47176/ijpr.22.4.21381</ELocationID>
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName>Seyed Mohammad Reza</FirstName>
					<LastName>Mirabbasi</LastName>
<Affiliation>Department of Physics University of Kashan, Kashan, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Kazem</FirstName>
					<LastName>Bitaghsir Fadafan</LastName>
<Affiliation>Faculty of Physics, Shahrood University of Technology, Shahrood, Iran</Affiliation>
<Identifier Source="ORCID">0000-0001-9835-7128</Identifier>

</Author>
<Author>
					<FirstName>Majid</FirstName>
					<LastName>Monem Zadeh</LastName>
<Affiliation>Department of Physics University of Kashan, Kashan, Iran</Affiliation>
<Identifier Source="ORCID">0000-0001-6636-9458</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2021</Year>
					<Month>12</Month>
					<Day>22</Day>
				</PubDate>
			</History>
		<Abstract>In a holographic compressible quantum matter, we calculate the sound mode using holography. For this purpose, we consider a structure of D&lt;sub&gt;3&lt;/sub&gt;-D&lt;sub&gt;7&lt;/sub&gt; branes that corresponds to this holographic compressible quantum matter. In this system, the sound mode is called the zero sound mode. In Gauss-Bonnet gravitational field geometry, we calculate the corrections entered at zero sound and show that the attenuation rate decreases.
&lt;em&gt; &lt;/em&gt;</Abstract>
			<OtherAbstract Language="FA">In a holographic compressible quantum matter, we calculate the sound mode using holography. For this purpose, we consider a structure of D&lt;sub&gt;3&lt;/sub&gt;-D&lt;sub&gt;7&lt;/sub&gt; branes that corresponds to this holographic compressible quantum matter. In this system, the sound mode is called the zero sound mode. In Gauss-Bonnet gravitational field geometry, we calculate the corrections entered at zero sound and show that the attenuation rate decreases.
&lt;em&gt; &lt;/em&gt;</OtherAbstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">AdS/CFT correspondence</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Holography</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">branes</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">zero sound</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Gauss</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Bonnet</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_3322_f7cfdde9db36af8e0d9a6d123d5c385e.pdf</ArchiveCopySource>
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