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• W3098756074 abstract "We study the structure formation by investigating the spherical collapse model in the context of new agegraphic dark energy (NADE) model in flat FRW cosmology. We compute the perturbational quantities [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] for the NADE model and compare the results with those of EdS and [Formula: see text] models. We find that there is a dark energy-dominated universe at low redshifts and a matter-dominated universe at high redshifts in agreement with the observations. Also, the size of structures, the overdense spherical region, and the halo size in the NADE model are found to be smaller, denser, and larger than those of EdS and [Formula: see text] models. We compare our results with the results of tachyon scalar field and holographic dark energy models." @default.
• W3098756074 created "2020-11-23" @default.
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• W3098756074 date "2017-03-24" @default.
• W3098756074 modified "2023-09-23" @default.
• W3098756074 title "Evolution of spherical overdensities in new agegraphic dark energy model" @default.
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• W3098756074 doi "https://doi.org/10.1142/s0218271817501012" @default.
• W3098756074 hasPublicationYear "2017" @default.
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