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<ArticleSet>
<Article>
<Journal>
				<PublisherName>The Physics Society of Iran</PublisherName>
				<JournalTitle>Iranian Journal of Physics Research</JournalTitle>
				<Issn>1682-6957</Issn>
				<Volume>3</Volume>
				<Issue>3</Issue>
				<PubDate PubStatus="epublish">
					<Year>2019</Year>
					<Month>11</Month>
					<Day>26</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Cosmological solutions of Brans-Dicke equations with cosmological constant</ArticleTitle>
<VernacularTitle>Cosmological solutions of Brans-Dicke equations with cosmological constant</VernacularTitle>
			<FirstPage>177</FirstPage>
			<LastPage>183</LastPage>
			<ELocationID EIdType="pii">682</ELocationID>
			
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName></FirstName>
					<LastName>I. Ahmadi-Azar</LastName>
<Affiliation></Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2019</Year>
					<Month>11</Month>
					<Day>26</Day>
				</PubDate>
			</History>
		<Abstract>  In this paper, the analytical solutions of Brans-Dicke (B-D) equations with cosmological constant are presented, in which the equation of state of the universe is P=mÙ° ρ , under the assumption φRn=c between the B-D field and the scale factor of the universe. The flat (K=0) Robertson- Walker metric has been considered for the metric of the universe. These solutions are rich in the sense that they include dust B-D theory with cosmological constant, Nariai Ù=° solutions, vacuum solutions of Ohanlen-Tupper and inflationary  Ù=° solutions.</Abstract>
			<OtherAbstract Language="FA">  In this paper, the analytical solutions of Brans-Dicke (B-D) equations with cosmological constant are presented, in which the equation of state of the universe is P=mÙ° ρ , under the assumption φRn=c between the B-D field and the scale factor of the universe. The flat (K=0) Robertson- Walker metric has been considered for the metric of the universe. These solutions are rich in the sense that they include dust B-D theory with cosmological constant, Nariai Ù=° solutions, vacuum solutions of Ohanlen-Tupper and inflationary  Ù=° solutions.</OtherAbstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">cosmological constant</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Brans-Dicke-theory</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">inflation</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_682_08d98638c6fcd194a4b1e6992063e944.pdf</ArchiveCopySource>
</Article>
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