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<Journal>
				<PublisherName>The Physics Society of Iran</PublisherName>
				<JournalTitle>Iranian Journal of Physics Research</JournalTitle>
				<Issn>1682-6957</Issn>
				<Volume>19</Volume>
				<Issue>3</Issue>
				<PubDate PubStatus="epublish">
					<Year>2020</Year>
					<Month>02</Month>
					<Day>02</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Spherically symmetric solutions in Ãber-gravity</ArticleTitle>
<VernacularTitle>Spherically symmetric solutions in Ãber-gravity</VernacularTitle>
			<FirstPage>565</FirstPage>
			<LastPage>570</LastPage>
			<ELocationID EIdType="pii">1539</ELocationID>
			
<ELocationID EIdType="doi">10.47176/ijpr.19.3.37461</ELocationID>
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName>N</FirstName>
					<LastName>Khosravi</LastName>
<Affiliation></Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2020</Year>
					<Month>02</Month>
					<Day>02</Day>
				</PubDate>
			</History>
		<Abstract>  &lt;br /&gt;In this paper, we introduce ubergravity based on the idea of the ensemble average theory of f (R) gravity models. This model has interesting properties including its universality. Another property of this model is its curvature dependency: In high curvatures, ubergravity is reduced to standard Einstein-Hilbert action, while in low curvatures, it vanishes. This transition happens at a scale of R0. It is possible to show that this dimensionful scale plays the role of the cosmological constant at late times. To consider the behavior of the non-linear structure formation, we need to start with the spherical collapse; hence, here we study the spherically symmetric solutions. We show that the radius dependency of these solutions is totally different from the Schwarzchild solution. Interestingly, the solutions looks like the Reissner-Nordstrom in the absence of any electrical charge.</Abstract>
			<OtherAbstract Language="FA">  &lt;br /&gt;In this paper, we introduce ubergravity based on the idea of the ensemble average theory of f (R) gravity models. This model has interesting properties including its universality. Another property of this model is its curvature dependency: In high curvatures, ubergravity is reduced to standard Einstein-Hilbert action, while in low curvatures, it vanishes. This transition happens at a scale of R0. It is possible to show that this dimensionful scale plays the role of the cosmological constant at late times. To consider the behavior of the non-linear structure formation, we need to start with the spherical collapse; hence, here we study the spherically symmetric solutions. We show that the radius dependency of these solutions is totally different from the Schwarzchild solution. Interestingly, the solutions looks like the Reissner-Nordstrom in the absence of any electrical charge.</OtherAbstract>
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			<Param Name="value">modified gravity</Param>
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			<Param Name="value">spherical solutions</Param>
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<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_1539_17e23e50bedc63b4095e3d8204ce063b.pdf</ArchiveCopySource>
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