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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>Nonstandard Lagrangian cosmology</ArticleTitle>
<VernacularTitle></VernacularTitle>
<FirstPage></FirstPage>
<LastPage></LastPage>
<ELocationID EIdType="doi">10.1186/2251-7235-7-58</ELocationID>
<Language>EN</Language>
<AuthorList>
<Author>
<FirstName>OICC</FirstName>
<LastName>Press Authors</LastName>
<Affiliation>Various OICC Press Authors</Affiliation>
<Identifier Source="ORCID"></Identifier>
</Author>
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<PublicationType>Journal Article</PublicationType>
<History>
<PubDate PubStatus="received">
<Year>2023</Year>
<Month>11</Month>
<Day>17</Day>
</PubDate>
</History>
<Abstract>AbstractWe show that many independent scenarios as the âaccelerated expansion of the universeâ, âeternal inflationâ, âeternally oscillating universeâ, ânonsingular oscillating universeâ, and âcollapse of an oscillating universeâ may occur without modifying the gravity theory or introducing scalar fields of any type. This is achieved by replacing the standard Lagrangian in the Friedmann-Robertson-Walker spacetime model by an exponentially nonstandard Lagrangian which modify the Euler-Lagrange equation although the standard variational approach is used.PACS45.20.Jj; 98.80.-k</Abstract>
<ObjectList>
<Object Type="keyword">
<Param Name="value">FRW cosmology</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Nonstandard Lagrangians</Param>
</Object>
<Object Type="keyword">
<Param Name="value">Spacetime model</Param>
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