Superposition of FLRW universes

buir.contributor.authorGürses, Metin
buir.contributor.authorYaghoub, Heydarzade
dc.citation.epage12en_US
dc.citation.issueNumber6en_US
dc.citation.spage1en_US
dc.citation.volumeNumber2020en_US
dc.contributor.authorGürses, Metin
dc.contributor.authorYaghoub, Heydarzade
dc.contributor.authorTekin, B.
dc.date.accessioned2021-02-12T10:40:56Z
dc.date.available2021-02-12T10:40:56Z
dc.date.issued2020
dc.departmentDepartment of Mathematicsen_US
dc.description.abstractWe show that (1) the Einstein field equations with a perfect fluid source admit a nonlinear superposition of two distinct homogenous Friedman-Lemaitre-Robertson-Walker (FLRW) metrics as a solution, (2) the superposed solution is an inhomogeneous geometry in general, (3) it reduces to a homogeneous one in the two asymptotes which are the early and the late stages of the universe as described by two different FLRW metrics, (4) the solution possesses a scale factor inversion symmetry and (5) the solution implies two kinds of topology changes: one during the time evolution of the superposed universe and the other occurring in the asymptotic region of space.en_US
dc.identifier.doi10.1088/1475-7516/2020/06/060en_US
dc.identifier.issn1475-7516
dc.identifier.urihttp://hdl.handle.net/11693/55108
dc.language.isoEnglishen_US
dc.publisherInstitute of Physics Publishingen_US
dc.relation.isversionofhttps://dx.doi.org/10.1088/1475-7516/2020/06/060en_US
dc.source.titleJournal of Cosmology and Astroparticle Physicsen_US
dc.subjectCosmic singularityen_US
dc.subjectCosmological phase transitionsen_US
dc.subjectCosmology of theories beyond the SMen_US
dc.subjectDark energy theoryen_US
dc.titleSuperposition of FLRW universesen_US
dc.typeArticleen_US

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