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Friedmann equation and stability of inflationary higher derivative gravity

dc.citation.epage0en_US
dc.citation.issue12en_US
dc.citation.spage0en_US
dc.citation.volume63en_US
dc.citation.woscount9en_US
dc.contributor.authorKao, WFen_US
dc.contributor.authorPen, ULen_US
dc.contributor.authorZhang, PJen_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.date.accessioned2019-04-03T06:39:24Z
dc.date.available2019-04-03T06:39:24Z
dc.date.issued2001-06-15en_US
dc.description.abstractA stability analysis of the de Sitter universe in pure gravity theory is known to be useful in many aspects. We first show how to complete the proof of an earlier argument based on a redundant field equation. It is shown further that the stability condition applies to k not equal 0 Friedmann-Robertson-Walker spaces based on the nonredundant Friedmann equation derived from a simple effective Lagrangian. We show how to derive this expression for the Friedmann equation of pure gravity theory. This expression is also generalized to include scalar field interactions.en_US
dc.identifier.doi10.1103/PhysRevD.63.127301en_US
dc.identifier.issn0556-2821en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.63.127301en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/29567
dc.identifier.wosnumberWOS:000169288400079en_US
dc.language.isoen_USen_US
dc.titleFriedmann equation and stability of inflationary higher derivative gravityen_US
dc.typeArticleen_US

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