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EXACT SOLUTION IN A SCALE INVARIANT MODEL WITH VANISHING COSMOLOGICAL CONSTANT

dc.citation.epage6en_US
dc.citation.issue1en_US
dc.citation.spage1en_US
dc.citation.volume29en_US
dc.citation.woscount3
dc.contributor.authorKAO, WFen_US
dc.contributor.department交大名義發表zh_TW
dc.contributor.department電子物理學系zh_TW
dc.contributor.departmentNational Chiao Tung Universityen_US
dc.contributor.departmentDepartment of Electrophysicsen_US
dc.date.accessioned2014-12-08T15:05:20Z
dc.date.available2014-12-08T15:05:20Z
dc.date.issued1991-02-01en_US
dc.description.abstractWe analyze a special scale invariant effective theory with vanishing cosmological constant. We show that, in this theory, the spatial-independence of the inflation is implied by the equation of motion incorporated with the Robertson-Walker metric. Furthermore, we find that this theory can be solved exactly for k = O Robertson-Walker spaces. We also find almost exact solution in k not-equal 0 spaces.en_US
dc.identifier.issn0577-9073en_US
dc.identifier.journalCHINESE JOURNAL OF PHYSICSen_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/3870
dc.identifier.wosnumberWOS:A1991EX77500001
dc.language.isoen_USen_US
dc.titleEXACT SOLUTION IN A SCALE INVARIANT MODEL WITH VANISHING COSMOLOGICAL CONSTANTen_US
dc.typeArticleen_US

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