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<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>Fractional action cosmology: some dark energy models in emergent, logamediate, and intermediate scenarios of the universe</ArticleTitle>
<VernacularTitle></VernacularTitle>
<FirstPage></FirstPage>
<LastPage></LastPage>
<ELocationID EIdType="doi">10.1186/2251-7235-7-25</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 the framework of fractional action cosmology, we have reconstructed the scalar potentials and scalar fields, namely, quintessence, phantom, tachyon, k-essence, Dirac-Born-Infeld-essence, hessence, dilaton field, and Yang-Mills field. To get more physical picture of the variation of the scalar field and potential with time, we express a scale factor in emergent, logamediate, and intermediate scenarios, under which the universe expands differently.PACS98.80.Cq, 95.36.+x</Abstract>
<ObjectList>
<Object Type="keyword">
<Param Name="value">Dark energy</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Emergent</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Fractional action cosmology</Param>
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<Object Type="keyword">
<Param Name="value">Intermediate</Param>
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<Object Type="keyword">
<Param Name="value">Logamediate</Param>
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<Object Type="keyword">
<Param Name="value">Universe</Param>
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