Q stars in scalar-tensor gravitational theories in extra dimensions

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dc.contributor.author Prikas, A en
dc.date.accessioned 2014-03-01T01:24:54Z
dc.date.available 2014-03-01T01:24:54Z
dc.date.issued 2006 en
dc.identifier.issn 0022-2488 en
dc.identifier.uri http://hdl.handle.net/123456789/17504
dc.subject Extra Dimension en
dc.subject General Relativity en
dc.subject Anti De Sitter en
dc.subject brans dicke en
dc.subject.classification Physics, Mathematical en
dc.subject.other BOSON STARS en
dc.subject.other Q-BALLS en
dc.subject.other SOLITON STARS en
dc.subject.other GRAVITY en
dc.subject.other CONFIGURATIONS en
dc.subject.other STABILITY en
dc.subject.other EQUATION en
dc.subject.other STATE en
dc.subject.other GEON en
dc.title Q stars in scalar-tensor gravitational theories in extra dimensions en
heal.type journalArticle en
heal.identifier.primary 10.1063/1.2245208 en
heal.identifier.secondary http://dx.doi.org/10.1063/1.2245208 en
heal.identifier.secondary 082501 en
heal.language English en
heal.publicationDate 2006 en
heal.abstract We present Jordan-Brans-Dicke and general scalar-tensor gravitational theory in extra dimensions in an asymptotically flat or anti de Sitter spacetime. We consider a special gravitating, boson field configuration, a q star, in three, four, five, and six dimensions, within the framework of the above gravitational theory, and find that the parameters of the stable stars are a few percent different from the case of General Relativity. (c) 2006 American Institute of Physics. en
heal.publisher AMER INST PHYSICS en
heal.journalName Journal of Mathematical Physics en
dc.identifier.doi 10.1063/1.2245208 en
dc.identifier.isi ISI:000240237300016 en
dc.identifier.volume 47 en
dc.identifier.issue 8 en

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