2019
DOI: 10.1007/s12036-019-9591-4
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Hypersurface-homogeneous modified holographic Ricci dark energy cosmological model by hybrid expansion law in Saez–Ballester theory of gravitation

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Cited by 18 publications
(3 citation statements)
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“…At the bouncing epoch, the jerk parameter has a singular value because of the vanishing nature of the Hubble rate at bounce. At a large cosmic time away from the bounce, the jerk parameter decreases to small values close to one, which was outlined in our earlier work [58,59].…”
Section: Stability Factorsupporting
confidence: 62%
“…At the bouncing epoch, the jerk parameter has a singular value because of the vanishing nature of the Hubble rate at bounce. At a large cosmic time away from the bounce, the jerk parameter decreases to small values close to one, which was outlined in our earlier work [58,59].…”
Section: Stability Factorsupporting
confidence: 62%
“…We also believe that this gravity theory provides an adequate description of the weak fields and a solution of missing matter cosmological problem in non-flat cosmology. Various authors including our own peer research group have constructed models of the universe in Sáez-Ballester theory and published fruitful results [11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%
“…We also believe that this gravity theory provides an adequate description of the weak fields and a solution of missing matter cosmological problem in non-flat cosmology. Various authors including our own peer research group have constructed models of the universe in Sáez-Ballester theory and published fruitful results [11][12][13][14][15][16][17].…”
Section: Introductionmentioning
confidence: 99%