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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>3</Volume>
				<Issue>3</Issue>
				<PubDate PubStatus="epublish">
					<Year>2023</Year>
					<Month>09</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Holographic baryons, dense matter and neutron star mergers</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>1</FirstPage>
			<LastPage>22</LastPage>
			<ELocationID EIdType="pii">338</ELocationID>
			
<ELocationID EIdType="doi">10.22128/jhap.2023.695.1054</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Matti </FirstName>
					<LastName>Jarvinen</LastName>
<Affiliation>Asia Pacific Center for Theoretical Physics, Pohang, 37673, Korea</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2023</Year>
					<Month>06</Month>
					<Day>28</Day>
				</PubDate>
			</History>
		<Abstract>The gauge/gravity duality, combined with information from lattice QCD, nuclear theory, and perturbative QCD, can be used to constrain the equation of state of hot and dense QCD. I discuss an approach based on the holographic V-QCD model. I start by reviewing the results from the construction of the V-QCD baryon as a soliton of the gauge fields in the model.&lt;br /&gt;&lt;br /&gt;Then I discuss implementing nuclear matter in the model by using a homogeneous approach. The model predicts a strongly first order phase transition from nuclear to quark matter with a critical endpoint. By using the model in state-of-the-art simulations of neutron star binaries with parameters consistent with GW170817, I study the formation of quark matter during the merger process.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Holography</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">QCD</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Neutron stars</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jhap.du.ac.ir/article_338_ea7ec6e26dab23cea4da43e138bb8017.pdf</ArchiveCopySource>
</Article>
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