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<ArticleSet>
<Article>
<Journal>
<PublisherName>OICC Press</PublisherName>
<JournalTitle>Journal of Theoretical and Applied Physics</JournalTitle>
<Issn>2251-7235</Issn>
<Volume>7</Volume>
<Issue>1</Issue>
<PubDate PubStatus="epublish">
<Year>2023</Year>
<Month>11</Month>
<Day>17</Day>
</PubDate>
</Journal>
<ArticleTitle>Reconstruction of modified holographic Ricci dark energy in El-Nabulsi fractional action cosmology</ArticleTitle>
<VernacularTitle></VernacularTitle>
<FirstPage></FirstPage>
<LastPage></LastPage>
<ELocationID EIdType="doi">10.1186/2251-7235-7-22</ELocationID>
<Language>EN</Language>
<AuthorList>
<Author>
<FirstName>OICC</FirstName>
<LastName>Press Authors</LastName>
<Affiliation>Various OICC Press Authors</Affiliation>
<Identifier Source="ORCID"></Identifier>
</Author>
</AuthorList>
<PublicationType>Journal Article</PublicationType>
<History>
<PubDate PubStatus="received">
<Year>2023</Year>
<Month>11</Month>
<Day>17</Day>
</PubDate>
</History>
<Abstract>AbstractIn this work, we discussed the âmodified holographic Ricci dark energyâ cosmological model based on El-Nabulsi fractional action cosmology. corresponding related cosmological parameters have been reconstructed. It has been observed that the equation of state parameter behaves like quintessence. Finally, through a test by the squared speed of sound, the proposed reconstruction model is found to be classically unstable.PACS 95.36.+x, 95.35.+d

&amp;nbsp;

&amp;nbsp;</Abstract>
<ObjectList>
<Object Type="keyword">
<Param Name="value">Cosmological parameters</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Fractional action cosmology</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Modified holographic Ricci dark energy</Param>
</Object>
</ObjectList>
</Article>
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