Reconstruction of modified Gauss–Bonnet gravity for emergent universe

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dc.contributor.authorPaul, B. C.
dc.contributor.authorMaharaj, S. D.
dc.contributor.authorBeesham, A
dc.date.accessioned2023-05-17T13:23:25Z
dc.date.available2023-05-17T13:23:25Z
dc.date.issued2022
dc.descriptionReconstruction of modified Gauss–Bonnet gravity for emergent universe
dc.description.abstractWe present a flat emergent universe model in modified Gauss–Bonnet gravity in four dimensions. The emergent universe model is free from a big-bang singularity and also describes the observed universe fairly well. It is assumed that the present universe emerged from a static Einstein universe phase that exists in the infinite past. To obtain the flat emergent universe model, we reconstruct mimetic modified f(G)-gravity (G representing Gauss–Bonnet terms). The functional form of f(G)-gravity is determined with or without matter, and can accommodate the early inflation and late accelerating phases satisfactorily. In contrast, in Einstein’s general theory of relativity, a flat emergent universe was obtained within the modified matter sector.
dc.identifier.citationPaul, B.C., Maharaj, S.D. and Beesham, A., 2022. Reconstruction of modified Gauss–Bonnet gravity for emergent universe. International Journal of Modern Physics D, 31(06), p.2250045.
dc.identifier.issn0218-2718
dc.identifier.urihttps://uzspace.unizulu.ac.za/handle/10530/2323
dc.language.isoen
dc.publisherUniversity of Zululand
dc.titleReconstruction of modified Gauss–Bonnet gravity for emergent universe
dc.typeArticle
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